The
Subsoil of Naples —
a new translation for this
website, Naples: Life, Death &
Miracles.
[This is a
translation of Il Sottosuolo di Napoli (The
Subsoil of Naples), commissioned and published
by the city of Naples in 1967. The entire
500-page work in the original Italian was
scanned and made available in .pdf format on
the website of Napoli Underground
(NUg). A complete English translation by
myself and Larry Ray appeared in May 2010 and
appeared on that same website. THAT IS NO
LONGER THE CASE (!) as that website has gone
off-line. I hope to make The Subsoil of
Naples available here. It will take some
time.
The
original Il Sottosuolo di Napoli from
1967 had three parts: the first one is
essentially an explanation of why the book was
written. That section is directly below on
this page (yes, I know it's a screen --humor
me) and starts after the next paragraph. It
runs about halfway down the page. The second
part then starts (on this page). It is all
technical geology but a lot of it is
accessible even to me (!) and is worthwhile.
Of that second part, all 9 sections are now
complete (as of 30 October 2019). The first
chapter is also on this page. A link is at the
bottom to move to the next page). Be patient.
The original book had a part 3 to it of graphs
and maps, which may not be available.
The Subsoil of Naples is about building and overbuilding in Naples. It was and remains an exhaustive compendium of general geology, the geology of Naples, urbanology and social commentary. Though The Subsoil of Naples is more than 50 years old, it is by no means dated and bears careful reading with respect to the things that have changed and, above all, have not changed since it was written. —Jeff Matthews
[For
other
material on the topic of Underground Naples,
see that portal
index.]
This is part 1 Part 2 starts below, here
-
continues here
- then here -
last pages
(complete)
(complete-part 2,
ch.1)
(complete-part 2,
ch.2) (complete-part 2, ch. 3-6)
(7,8,9 all
complete)
1. Introduction (directly below) 2.
Table of Contents 3. Formation of Commission,
Results & Conclusion
introduction
The Subsoil of Naples
A flood of houses has submerged Naples to an incredible degree. The hills have been assaulted, the greenery destroyed, the entire area victim of building speculators. Whoever now views Naples from the sea stares at a giant cement presepe* clinging to a desolate tuffaceous* cliff.This is Naples today, the city that nurtured Virgil, the city praised by Goethe. It is a Naples that in the 18th century, driven by the sensational discoveries at Pompeii and Herculaneum, blossomed in its role as capital. Naples then expanded slowly with a few villas along the Chiaia, first towards Posillipo, then still a wooded area, and then with villas towards the green and open plain leading to Portici. Then, in 1812 Murat broke the enchanted silence of Posillipo and her villages and created the now “must see” path, the panoramic road from Villa Donn’Anna to the Cape. The luxuriant woods and vineyards, a sweeter and more human Naples, where an outing into the countryside of San Giacomo dei Capri [an area in the Vomero section of Naples] meant leaving the populated areas of the city behind. All that is still within living memory.
But if reason, a sense of civic duty,
and a love of Naples have failed at all levels of
responsibility to halt this violent
spread of housing
speculation, there is a new, decisive element in the
problems of Naples that makes it necessary to
change the way we
have done things in the past. As this report make clears,
we absolutely cannot delay this; it has to
do with the safety of our people and
how what lies below the surface of
our city affects their safety.
We now know, based on this scientific study of great
technical importance, that a great overload, both static
and
hydraulic, weighs upon the ancient
(or inadequate) infrastructure of Naples due to
irrational, chaotic urban expansion
over the last twenty years. We now
know with certainty that the tipping point, at least in
some areas that have been in balance,
is not far off. Earth slides, cave-ins and sink-holes
are unfortunately not new here, but their alarming
frequency over the last few years and
the nature of these episodes, especially in the hill
areas, comes from a
progressive deterioration of the
supporting subsoil. The underground cavities of all
shapes and sizes that have been well
identified in parts of the city aggravate this
precarious balance, but they are not, in general, the
primary cause.
This
alarming diagnosis has been formulated with scientific
rigor by the Commission for the Study of the Subsoil of
Naples; the commission has passed on to the city
administration important technical and urbanological
recommendations. The final report by
the Commission will be of great interest to specialists
both in Italy and abroad,
but for everyone the report is a
valuable lesson and a grave warning.
It seems obvious that the remedies
for the damage caused by past errors, thoughtlessness
and abuse, are not to be
found simply in regulations and
public works aimed at restoring conditions of safety to
the city. Those remedies have to be
undertaken within the vaster context of an urban
restructuring of the city, which the center-left city
administration has
been cautiously working out. Anyone can see that most of
the problems are due to the persistent lack of modern
and functional
urban regulation. That regulation goes back to 1939 and
will no longer do.
That basic evaluation sums up
precisely the present conditions and the situation we
find ourselves in. This investigation
of the subsoil of Naples was promoted and carried out by
the center-left administration of the city, and work
towards a new regulatory plan is well
underway. All of the material, appropriately
coordinated, should be finished in the first
months of the coming year. We emphasize that these plans
are a clear about-face with respect to how these
problems have been dealt with in the
past. Correct, responsible administrative action will
finally assure the city of decent urban,
economic and social development based
on a cohesive view of the problems and their solutions.
It is time to move from planning to getting the
job done. Naples has to be restructured for
coming generations. We
must give back to Naples her
safety, her breath, her greenery and prestige.
It will require collective commitment by
cultural
and technical forces and the forces of labor, as
well as decisive will power of politicians.
The valiant technicians who gave us
this study of the subsoil dedicate it to the coming
generation of the 1980s, those
on the frontier of civilization and
progress. As head of the commission and as a Neapolitan,
I speak for the entire
citizenry when I
express my gratitude to them. This work will not be
canceled by time or by men but shall remain a
secure guide to
the rebuilding the city and shall serve to warn the
future as well as accuse the past.
Naples, October
1967,
[Signed]
Bruno
Romano
The Subsoil of Naples
The digitizing of the original Italian volume was done
by Napoli Underground (NUg). Authorization for it was
granted to NUg by the Director General of the City of
Naples, Doctor Vincenzo Mossetti as directed by the
mayor of Naples, the Honorable Rosa Russo Iervolino, and
was granted as Project No. 170, dated March 9th, 2010.
Special thanks go to City Councilman Salvatore Parisi
without whom this project would not have been possible.
The original translation was done in March and April,
2010 by Jeff Matthews and Larry Ray.
The term "subsoil" as used here means the various strata
of different kinds of soils and rock that cover
thousands of square meters of interconnected man-made
cavities beneath the city. These cavities include
aqueducts, sewer mains, tunnels and the gigantic tuff
sandstone quarries that honeycomb areas beneath the
city. The Subsoil of Naples is about the
problems of building and overbuilding. This report was
and remains an exhaustive compendium of general geology,
the geology of Naples, urbanology and social commentary.
The Subsoil of Naples is more than 50 years old,
[ed. note: this was written in 1967] but is by no means
outdated. It bears careful reading as to the things that
have changed and, above all, have not changed
since it was written. Occasional comments have been
added as “translator’s notes,” [which are bracketed like
this]. The editors appreciate comments and corrections.
The translation notes and introduction are at the top of this page.
to top of this page
TABLE OF CONTENTS:
Translation Notes & 1967 Introduction by Bruno Romano
PART ONE - above
Formation of the Commission, report and conclusions
PART TWO
Chapter 1:
Geological considerations - BELOW ON THIS PAGE
Chapter 2:
Geological overview: the city of Naples
Chapter 3:
How mining and underground structures make subsoil shift
Chapter 4:
The distribution of cavities in the urban area
Chapter 5:
Underground waters
Chapter 6: A
geotechnical description of the urban territory
Chapter
7: The aqueduct and the subsoil
Chapter
8: The city sewage system, defects and remedies
Chapter
9: Causes of movement
Municipal
Building Code proposals, test procedures, and other
detail-specific data, Commission proposals and soil
testing parameters, etc. will be presented in a very
abbreviated form following Chapter 9.
(original
p.9) FORMATION OF COMMISSION, REPORT AND
CONCLUSIONS
(A)
Formation of Commission. On March 14, 1966, the
city council accepted the proposal of public works
commissioner, Bruno Romano, to appoint a commission to
determine the origins and characteristics of the subsoil
of Naples.
Member of the
Commission (also, hereafter in text, "We"):
President: Hon. Dr. Bruno Romano,
Assessor of Public Works
Dr. Ing. Lelio Saccani, Head Engineer
of the City of Napoli
Dr. Ing. Mario Sgarrella, Head, Dept.
of Civil engineering of Napoli
Dr. Ing. Francesco Saverio Verde,
Head, Fire Department of Napoli
Dr. Ing. Sabattino Meneganti, Dir.
Naples District, State Dept of Mining
Prof. Ing. Arrigo Croce, Full
Professor, Technical Univ. Geotechnology
Prof. Ing. Vincenzo Franciosi,
Professor, Construction Science
Prof. Ing. Pasquale Nicotera, Full
professor of Applied Geology
Dr. Ing. Dante Bardi, Inspector
General, State Dept. of Mining
Prof. Ing. Roberto Di Stefano,
University Professor, Expert
Prof. Pietro Parenzan, President,
Southern Italy Speleological Center
Dr. Ing. Carlo Galateri, Asst. to
Technical University Chair, Foundations
Secretary: Dr. Ing. Guido Vinaccia,
Official, Technical Office
Besides these members, we called upon the following
experts for occasional opinions and analyses:
Prof. Ing. Luigi Adriani; Prof. Ing. Corrado Beguinot;
Prof. Ing. Renato di Martino; Prof. Ing. Paolo Ferrari;
Dottor Guido Martene; Prof. Ing. Giuseppe Paolella;
Prof. Ing. Giovanni Sapio; Dottor Ing. Silvio
Terracciano; Prof. Ing. Carlo Viparelli. These people
participated in the final meeting of the commission and
assisted in drawing up the concluding report, especially
as regards the section on the causes of movement and
settling in the subsoil.
B) Commission Goals
We were required to turn out a
detailed report
a. with
systematic historical data and bibliography;
b. that
included appropriate external agencies as sources;
c. with
accurate topographical surveys of both surface and
subsoil;
d. with
appropriate drawings and cartographic materials;
e. with
details of appropriate laboratory work undertaken;
f. that
reflected an orderly and complete geotechnical
investigation of the subsoil.
All of this was in order to determine
a. the
quality and quantity of materials beneath the urban
surface, with special reference to the boundaries of
yellow tuff near the surface;
b. the
movement of underground water;
c. the
location and state of all cavities in the rock and in
loose soil above it, with graphics and descriptions;
d.
relevant geological and archaeological data.
(C) How the work proceeded:
The commission was convened by the mayor, Prof. Giovanni
Principe, on 16 April 1966. At the first meeting, we
decided to divide the work into two phases; first, a
historical and bibliographic study and collecting data
and findings from various agencies and societies,
including cartographic material; second, coordinating
these materials.
(C-1) Collecting data
At the meeting on 13 May 1966, we subdivided the first phase
into these parallel sectors:
a. collecting and classifying
geological and geotechnical material about the subsoil
(given to Prof. P. Nicotera);
b. collecting data on
existing cavities and on underground hydrology (given to
engineer, D. Bardi);
c. collating and preparing
graphics of the above material (given to Prof. R. Di
Stefano);
Also, since there had been recent collapses of retaining
structures, we turned our attention not only to the
subsoil but to surface foundations; this was given to
Prof. V. Franciosi, who would draw up plans for
constructing retaining walls.
Furthermore,
since there had already been a collapse of the
containing wall along the street, via Catullo, and since
the city public works commission had already appointed a
technical staff to investigate the static conditions in
the hill sections, this earlier subsoil commission gave
us data from their own work by contacting professors
Nicotera, Franciosi and Croce on 31 May 1966. As will be
seen, these investigations gave us an entire overview of
the Posillipo hill. The city public works commission
then independently gave us a copy of its findings, with
graphics.
(C-2) Determining the Cavities
For the second phase (C-1b, above) of our work
(collecting data on existing cavities), the job of
preparing that report was given to Prof. P. Parenzan and
S. Meneganti, engineer and chief of the Naples Mining
District. Two research squads were formed with Prof.
Tempra, vice-president of the Speleological Center, as
chief.
The report, “Means and Organization of Surveying the
Subsoil of Naples,” was given to us on 31 May 1966 by
engineer Menegante. It was the basis for our survey and
detailed what had to be done and the time it would take
to do it.
(See part 3 for the text of that report)
Then, within our commission, we formed a sub-group to
organize the diagnostic phase of the work. Thus, a first
temporary nucleus of the Office of Subsoil was set up
under the auspices of the Institute of Applied Geology
of the Engineering Department of Naples, directed by
Prof. P. Nicotera. Above all, we paid attention to
preparing cartographic materials of city territory with
as much geological data as possible. We note that each
member of the commission collected data and made other
contributions on his own behalf or that of the agency he represented.
We made requests to the following agencies, who provided
materials as indicated:
1. The State Railway: we requested the lay-outs
of rail routes and elevation of the underground rail
system with relevant documentation from the construction
of that system. No data were provided;
2. S.E.P.S.A. [the narrow-gauge Cumana train line]: request made, 26 May 1966 ; eight graphics received, 8 Feb 1967;
3. Central cable-car: request, 26 May 1966; received survey data on the route of that facility;
4. Mergellina cable-car: request, 26 May 1966; no response. Later request, 1 Feb 1967; received 5 fotostatic copes of the tunnel plans of that facility;
5. Secondary Vomero Railways: request, 16 May 1967; received, 28 May 1966, all materials in their possession;
6. Pneumatic postal agency: request on 26 May 1966; answered 7 June 1966. They had no useful data;
7. Naples Gas Company: request on 26 May 1966; they had no useful data since gas lines are on or at the surface but gave us subsoil specifications from the construction of a newer gas line;
8.
Superintendent of Monuments: request on 26 May 1966 (for
data on ancient cavities of historic interest,
catacombs, the Seiano Grotto, etc.). No answer.
Follow-up request on 1 Feb 1967; received lay-out and
technical subsoil details for the area beneath via
Egiziaca a Pizzofalcone;
9. Superintendent of Antiquities: request on 26 May 1966; no relevant data available;
10. A.M.A.N: [ Aqueduct Agency] request, 26 May 1966; reply, 7 June 1966 with available data.
(C-3)
Core Sampling
For terrain above the tuff we collected stratigraphic
data through 500 core samples from SAF (Fondedile),
SAMCEF, engineer Contardi, as well as from the
Geotechnical Institute of the Engineering Dept. and from
the city of Naples. We studied and evaluated the
material carefully and arranged it topographically for
later reference.
(C-4) Ordering the material
We kept separate files: i.e. for core samples,
underground cavities, bibliography. We evaluated all material for
reliability and relevance. Thus, the first documentation
of the subsoil was ready and the surveying proceeded.
That complex initial work produced the following
grouping of cavities:
1. those with uncertain location of access;
2. those with sufficiently
approximate location of access;
3. those already described
approximately by existing schematics;
4. those described in good
detail by existing schematics;
5. street and railway tunnels
running straight between two known and well-defined
openings.
Further
subdivisions might occur within each group as data were
refined as to, for example, access locations or
reliability of diagrams, etc.
We draw attention at the outset to those cavities in the
second group, those with sufficiently approximate
location of access. The Subsoil Commission was able to
use the services of workers from the City Roads
Division, who, on site, gave us precise locations, ease
of access, physical condition of the sites and property
ownership. A regularly updated “personal registry” of
each cavity was kept for the legal and administrative
purposes of gaining access to properties.
(C-5) Survey
operations
From the outset we found a net difference (which we had
anticipated) between the ancient tufa quarries and those
cavities that had been the sites of water storage for
the ancient city. In almost all cases, the former are
still used and negotiable, while the latter are either
clogged with refuse or otherwise completely blocked.
Other noteworthy difficulties had to do with the apathy
or suspicions on the part of property owners or tenants,
or with unclear relations between landlords and tenants,
or by the splintered subdivisions of the property,
itself.1 Those difficulties
conditioned or modified our early work in various
quarters of the city.
{1In some
cases, areas within the same grotto belonged to, or were
rented by, different parties, and subdivided by various
walled off areas creating many small sections, each
requiring its own separate legal procedures.}
From our work, still going on, a number of cases have
emerged of cavities that are totally inaccessible or not
negotiable. These sites cannot be dealt with in this
first phase of operations due to the high cost of
clearing and cleaning them as well as to resistance
(both active and passive) from property owners and
tenants. In cases where the commission or the city
administration cannot resolve this, other solutions,
including court orders, will be necessary.
From the beginning, Prof. Patenzan provided the Subsoil
Commission with men and material from the Center for
Speleology in the South (Naples section), about 20 young
speleologists with proper equipment. Alongside of them,
from March 1967, there was also a team under the
direction of Dr. Armando Falangola; this group went to
work immediately under the guidance of the Subsoil
Commission.
By 30 September 1967, about 140,000 sq. meters had been
surveyed underground; precisely 21,000 sq. meters of
underground cavities and 119,000 sq. meters of excavated
quarry voids. All of this has meant a great degree of
determination in dealing with the problems of deep
cavities, particularly given the enormous and complex
difficulties in accessing this type of underground
structure. This objective (reached in less than a year,
if you consider that the first
months were involved with organization and start-up)
surpasses the commission’s original, optimistic
predictions of 100,000 sq. meters per year.
Our system for representing graphically the cavities
seems particularly useful. Besides two-dimensional maps,
drawings showed both transverse and, in many case, axial
sections with a series of topographical cross sections.
A report, often with photos, was drawn up for each
survey.
(C-6) Examining the surveys and reported
(unconfirmed) locations
We conclude with the topographical surveys. The last
phase of work for each cavity was an examination of the
underground area, noting the existence of possible
static or hydrologic shifting, the state of repair of
retaining structures, the presence of otherwise
particular geological characteristics (such as, for
example, soils weakened physically or chemically,
tectonic phenomena, etc.)
We brought cases that were causes for alarm to the
attention of the Safety Office of the city
administration, whose job, as we know, is to make
appropriate repairs. The time limit for our work had
been set at 18 months, which was up on 16 October 1967.
Even after such a short time and even with the
difficulties we encountered (stemming from both the
particular nature of the work and, above all, from the
skimpy participation of public and private agencies), we
feel we can now make the following report to the city
administration.
D) Results
We know that a systematic study of subsoil in a case as
complex as Naples is not a matter of just a few months;
it takes constant determination to research and update.
Yet we now feel able to furnish the most ample
documentation and most exhaustive statement possible on
the subsoil of Naples, given our current state of
knowledge.
The bibliography (in part III of this report) lists 478
sources regarding surveys of the subsoil of Naples; they
are the principle sources of information in the field.
Of special interest are those from the VIII National
Geotechnical Congress, held in Cagliari in February
1967, on “The Subsoil of Big Cities.” Based on its
investigations, we have been able to identify (as of 30
September 1967) 366 cavities, divided as follows:
—203 cavities (or cavity entryways) at levels beneath
their relative entrances at the surface;
—163 cavities (or cavity entryways) on the same level as
their relative entrances at the surface;
In the first group we count those voids that have been,
or are currently, facilities for some purpose; that is,
the Claudio, Bolla, and Carmignano aqueducts; local
systems of water storage (the areas in the high city);
chambers used in the past for storing supplies; tuff
caves beneath factories; and old, abandoned sewers.
Entrance to those cavities is by way of well shafts or
well shafts and stairs; the stairs were put in during
the war so the structures could serve as air-raid
shelters.
In the second group are the voids resulting from
quarrying stone for construction material (with the
voids, often going from the street-level entrances back
beneath prominent tufaceous masses for a considerable
distance); street tunnels, both ancient and modern;
railway tunnels; modern aqueducts; underground Bourbon
passageways; and, finally, a good part of the catacombs.
As noted, the Commission identified the best way to
survey the cavities within the approximate limits
considered in the best technical and practical interests
of the city, indicating the presence of such cavities
and with the understanding that more detailed studies
would follow either by those agencies or those
individuals directly interested in individual areas. Our
surveys showed this methodology to be the best one.
to top of this page
Part III
of this report lists the cavities and gives an overview
plus some examples of the actual files that we prepared.
There are also descriptive monographs on cavities that
detail the stratigraphy of the 185 core samples.
This material is the first nucleus of what we have
gathered about the subsoil; it is material that should
then be continuously developed and kept current in the
“Special Section for Subsoil” of the Municipal Technical
Office, freely available for consultation and serving as
an easy and rapid guide for practical use.
Furthermore (see map, below), a geological-technical
chart for Naples on a scale of 1:10,000 was prepared; it
contains indications for geology, curve of the uppermost
level of the yellow tuff strata; location of core
samples; and location of cavities. There is also an
isopach chart (on a scale of 1:10,000) of the loose
terrain covering the yellow tuff.
Chapter 2 of part II of this report describes how those
charts were prepared and contains general observations
on the eastern and western parts of the city and on the
Posillipo hill. All of the cavities with a known
configuration have been represented on a scale of
1:10,000 on the tables corresponding to the Topographic
Survey Department, STR, of the urban surface. Some of
those tables are also included in this report.
The Commission, in keeping with the goals it set for
itself at the outset, has also prepared a detailed study
of the nature and genesis of the subsoil of Naples; that
is found in chapter 1 of part II. We also felt it proper
to describe (see chapter 3 of part II) ancient and
modern methods of excavating building material in
Naples.
On the basis of what we have gathered and presented in
this report, we were able to follow the evolution of
cavities in relation to urban development over time;
that is, we could trace the actual path and chronology
of their distribution (see chapter 3 of part II). For
material on the course of underground water and
variations over time in strata, see chapter 5 of part
II.
The geotechnical features of the urban territory is the
subject of chapter 6 of part II. We deal with the
stratum of subsoil considered technically significant in
relation to buildings on the surface and how their
foundations are affected. Urban areas are identified
that present particular geotechnical problems.
We also deal with both ancient and modern construction
and how it has been affected by earth movement resulting
from water seeping into the subsoil or by cavities
either in the tuff or in the loose soil above the tuff;
we look at hillside construction (where the surface is
naturally sloped or where it has been terraced for
building on properties that are vertically adjacent on
the slope), and, finally, with buildings placed on voids
built up with artificial landfill.
We have also noted the most recent studies on surveying
and building road-beds. We noted with interest the
phenomenon of earth movements in the tunnels of Naples,
both modern and ancient Roman. These studies gave us
indications of how to build such structures in the
future. The general situation as to the aqueducts and
sewage system was the object of intense scrutiny by the
Commission. These two items are dealt with,
respectively, in chapters 7 and 8 of part II.
We note the work by an earlier commission on the
condition and stability of retaining walls in the hill
sections, in particular the Posillipo hill (as covered
in the SPEME convention) [SREME refers to the 1926
convention that founded a corporation to build a new
quarter of Naples on the Posillipo hill.] Our report and
the main graphic material are in part III.
The Commission used studies by Prof. Franciosi, for the
design of restraining walls in urban centers (see part
III).
The Commission, though not required to do by its
founding charter, reserves the right, to express further
views in particular cases. We have used chapter 9 of
part II to express our views on the main causes of the
frequent earth movements that Naples is subject to. We
find that our conclusions do not differ substantially
from those of the Commission that preceded us [i.e. the
S.P.E.M.E study] and hope that they will now attract
attention and action.
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this page
Conclusions
On the basis of its work, the Commission herewith
presents its conclusions to the city administration:
(1) General recommendations
— 1-1. Urban plans and programs. We recommend
that urban plans for restructuring the city (road
building both on the surface and underground, new urban
settlements, etc.) be verified not just with the usual
environmental and geological criteria, but with detailed
analyses of factors relevant to the subsoil, especially
those contained in this report.
With that recommendation, the Commission stresses the
difficulty of such verification and notes that in Naples
and elsewhere much construction is not done in
accordance with such criteria. Taking these technical
factors into consideration can substantially reduce
problems in construction and help produce solutions to
our urban problems.
image 2
We invite the administration to give this report to the
zoning commission quickly so our subsoil can be made safe.
—1-2. With utmost urgency we recommend that the
city stop terracing, rock cutting, filling, medium- and
large-scale earth moving, and construction of retaining
walls unless those works are authorized by the Special
Section for Subsoil. We stress that building licenses and
authorizations of habitability be granted only after
technical reports on the safety of the foundations and
sewer systems of the buildings in question. Those licenses
shall be granted by taking into account not just the
serviceability of private sewage lines and roads, but the
certified capacity of public sewage system, public roads,
and retaining walls in the areas that handle the
additional load.
We thus recommend that the city not permit new housing
settlements in the greater urban area unless work on
appropriate sewer lines that are to serve those
settlements are completed both for new lines as well as
upgrading existing ones. We also note that in the new
settlement that is to go up in Secondigliano (in
accordance with Law 167), that there are no rainwater
catchment basins and that work needs to be done to upgrade
the facilities that channel off waste water. The
Ponticelli settlement likewise needs upgrades to the
existing channels.
As to the areas of the high Vomero, Arenella, Pigna, S.
Giacomo dei Capri, Camaldoli, and the slope of the Vomero
hill descending from the ridge-line of via Cilea-Corso
Europa-via Tasso towards the Corso Vittorio Emanuele: that
slope is already heavily urbanized, and run-off already
flows into insufficient collectors along via Tasso, via
Aniello Falcone, and Corso Vittorio Emanuele. The
Commission recommends that the city restrict building in
that area and not issue further building licenses until
these deficiencies are corrected
The Commission recommends once again (see Part III) to the
city council that until appropriate maintenance is done on
retaining walls, sewer lines and other problems, no
further building licenses be issued for the areas covered
by the SPEME convention, nor should already authorized
terracing, rock cutting, and filling be allowed to go
forward.
image 3. The areas
marked A through F are referenced in Recommendations
1-3.
image 3
Finally we recommend, in any case, that no new buildings
overload the existing collectors and sewer lines of the
city.
—1-3. The Commission recommends that detailed
plans be drawn up for the urban renewal of the following
sections of the
city as indicated by letters A-F in
image 3, above:
a. The area of Materdei –
Vergini – Sanità, bounded by via Foria (the Botanical
Gardens), the Miradois hill (from the
Astronomical Observatory to the
Capodimonte Palace), the Capodimonte hill (along the
line of the new Tangenziale
highway, the
Materdei hill and S. Maria degli Sacalzi to via Foria;
b. The historic center of the city, bounded by via Foria, via Cesare Rossaroll, Castel Capuano, Rettifilo, via Sanfelice, via Roma, via Pessina;
c. The area of Montesanto – Ventaglieri, bounded by via Roma, the rise at via S. Rosa, the slopes of the Vomero hill to Piazza Leonardo, the military hospital and via Settedolori;
d. The Spanish Quarters, consisting of the slope (to via Giovanni Nicotera and via Chiaia) rising from via Roma to the Corso Vittorio Emanuele;
e. The Pizzofalcone Hill, bounded by via Chiaia, Chiatamone and Santa Lucia;
f. The area of Chiaia, bounded by via G. Nicotera,
via Chiaia, via dei Mille, via Crispi, Corso V.Emanuele,
from the
Cumana station the central cable-car
station.
The plans to renew these areas should include not just
the surface, but the subsoil, as well.
We recommend renewing the surface strata in these areas,
including strips along the base of the Vomero and
Posillipo hills, and slopes above via Chiaia,
Piedigrotta, Mergellina, and Posillipo as far as via
Tasso and via Manzoni.
—1-4. As to the efficient maintenance of the
sewer system, the Commission recognizes the absolute
necessity, in the interest of public health, of
immediate intervention by the city administration.
There is much to be done that simply cannot be put off, both in the interest of public health as well as urban stability; nevertheless, in setting up priorities, we stress giving precedence to restoring balance to the city’s water supply.
We
recommend that the city, where possible, provide access
shafts that permit underground work (particularly on the
aqueducts) without interfering with normal services and
the damages that might ensue. We call attention to the
importance of shielding metal conduits, actively or
passively, from stray electrical currents. Public
transport agencies should take care not to ground
current directly into the subsoil.
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(2) Recommendation for regulations
—2-1. The Commission strongly recommends
regulations for the planning, building and testing of:
a. quarries, both open-air and
underground; excavations that expose subsoil or
tufaceous material; land-fills
(incorporating surveys and reports
from excavations in major projects);
b. walls and sustaining
structures;
c. foundations of buildings,
particularly those on tufaceous cavities or recent
land-fill;
These regulations should, as we detail in Part III,
comply with instructions from the Upper Council of the
Department of Public Works; regulations shall apply both
to private concerns and to public agencies in the city.
We recommend that the administration speedily meet its
obligation to have property owners, builders and
contractors provide reports on special issues regarding
foundations, and, indeed, on any matter relevant to the
condition of the subsoil; these reports should be made
to the Special Section for Subsoil.
—2-2. The Commission finds the regulations in the
Regolamento Comunale (approved in 1942 and still
in effect) regarding sewer lines in private buildings to
be largely outmoded and no longer valid, especially for
these sections: S. Giovanni, Barra, Ponticelli,
Poggioreale and the Industrial Zone, which are to be
served by an autonomous network with a new water
purification facility, now almost complete, located at
S. Giovanni a Teduccio.
We thus urge the speedy adoption of a modern, efficient
Code that contains, among other things, precise
regulations for the planning, building and testing of
private and public sewage systems.
(3) Particular Recommendations
—3-1. We know that applyimg these recommendations
will take effort from an organizational standpoint as
well as a practical one. We thus recommend to the
Administration that it hasten to set up an Ufficio
Tecnico del Comune (City Technical Office) to
handle existing problems and those that crop up in the
future. We draw attention to the need for adequate
personnel for construction, surveillance, and
maintenance of new sewer lines.
—3-2. We hold indispensable a “Special Section
for Subsoil.” That section shall work along the
following lines:
a. it shall continue our work
and keep collection and updating data on the subsoil;
b. it shall continue to verify the dynamic condition of roads, both public and private, using existing data as well as complaints or other reports regarding the stability of sustaining walls;
c. in building licenses or permits, the “Special
Section for Subsoil” shall make its own decision on
whether or not the
code for the construction of
foundations is being followed;
—3-3. The Commission urgently recommends to the
city that it continue with ongoing studies of the
stability of the hill areas and provide for the speedy
completion of projects, particularly those regarding
maintenance of quarry walls and sustaining walls, and
with particular emphasis on those sewer lines subject to
earth movement since they present a special problem for
the stability of the urban infrastructure.
—3-4. The Commission urgently recommends to the
Administration that it provide the City with valid,
up-to-date maps and charts of the urban territory. The
current cartographic documents are insufficient and, in
some case, even wrong.
THIS IS THE END OF
PART 1 OF The Subsoil of Naples.
PART 2, Chapter 1 is
compete. IMMEDIATELY BELOW.
PART 2, Chapter 2 is complete.
(Oct 16, 2019)
to portal for underground
Naples
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PART TWO:
complete table of contents:
Chapter 1:
Geological considerations DIRECTLY BELOW
Chapter 2: Geological
overview: the city of Naples
Chapter 3: How mining and
underground structures make subsoil shift
Chapter 4: The distribution of
cavities in the urban area
Chapter 5: Underground waters
Chapter 6: A geotechnical
description of the urban territory
Chapter 7: The
aqueduct and the subsoil
Chapter 8: The city
sewer system, defects and remedies
Chapter
9: Causes of movement
PART TWO: Chapter One
Geological Make-Up
by Engineering Profs. P.
Nicotera and P. Lucira
Beyond the Premise and
Overview, DIRECTLY BELOW, this long, highly
technical "Geological
Make-Up"
has these
13 subheadings (in this
order, as they
appear in the text.) You may
link to them
individually here:
THE ANCIENT ERUPTIVE CYCLE IN THE
CAMPI FLEGREI
RECENT
ERUPTIVE CYCLES OF THE CAMPI FLEGREI
VOLCANIC
ACTIVITY OF SOMMA-VESUVIUS
NATURE AND
GENESIS OF THE TERRAIN IN THE SUBSOIL OF NAPLES
LAVAS
LAPIDEOUS
PYRCOCLASTIC MATERIALS
GREY
CAMPANIAN TUFF
PIPERNO
STRATIFIED
YELLOW TUFF
CHAOTIC
YELLOW TUFF
LOOSE
PYROCLASTIC MATERIALS
UNDISTURBED
MATERIALS
DISTURBED MATERIALS
PREMISE
The urban and
outlying areas of Naples are spread in the center of
an extremely complex and characteristic volcanic
region that
includes the Somma-Vesuvius crater complex in the east
to the dozens of craters in the volcanic district of
the Campi Flegrei in the west.
Almost all of the urban conglomerate is on land formed
by the volcanic activity of the
Campi Flegrei, while the outlying
areas, though also connected
in large part to the Campi Flegrei, also extend
to the
east, to Somma-Vesuvius and have their origins
in activity of that volcano.
In speaking of the subsoil of the city of
Naples, whether urban problems or hydraulic and
geotechnical problems in a
broader sense, we need to
know the geological history of the area. It is
only by reconstructing the causes and
chronology
of geological phenomena and petrogenesis that
have formed this region that we can understand
the
technical
implications in given situations as well as
understand the physical, chemical and mechanical
properties of the rock and
soil in the region.
The goal of this chapter is
to contribute to a more useful understanding of
the technical problems related to the subsoil
of Naples. We have thus tried
to outline the geological history of Naples and
the surrounding area.
We first describe the
geological history of the Flegrean volcanoes and
Somma-Vesuvius; then, we describe the
characteristics of their geological products and
the main phenomena that accompanied the origins
of these volcanic
complexes.
OVERVIEW OF THE GEOLOGICAL HISTORY OF THE
FLEGREAN-NEAPOLITAN AREA
The beginning of the volcanic
activity that formed the area now occupied by
the city of Naples and the surrounding area
goes back to the end of the
Pliocene period or the beginning of the
Quaternary. Various studies place the beginning
of
Flegrean volcanic activity at
the 4th glaciation; that is after the beginning
of Ischian volcanic activity but before the
Somma-Vesuvian activity.
Following the dropping of the
“Tirrenide” continental area in the Tyrrhenian
Sea, regional fracturing occurred of the kind
known as Tyrrhenian and
Appennine. That led to the upwelling of a
basaltic magma that, before reaching the
surface,
produced various laccoliths, each one of which
formed isolated magma basins, themselves. These
were, because of
varying local conditions,
then subject in turn to their own particular
processes of magmatic evolution. These were the
original
kernels of the more or less complex volcanic
structures that
then developed.
Relatively large and shallow
magma basins thus formed at Ischia, the Campi
Flegrei and Somma-Vesuvius. Each of
these
basins developed autonomously, depending on
local conditions (tectonics, stratigraphy,
depth, etc.).
The magma basin of the Campi
Flegrei, judging from the largely
alkalitrachtytic make-up of Flegrean geological
products,
probably derives from a trachyte-basalt magma
intrusion noticeably extended vertically,
permitting the
build-up
of large masses of light magma and
differentiated in the higher parts of the basin.
On the other hand, the
extreme
scarcity of weakly leucitic lava suggests that
the roof of the basin is not formed of mesozoic
limestone and that the magma
took its position, at a later time, in Tertiary
sediments.
De Lorenzo subdivides past
activity of the Phlegrean area into three
phases: the first and oldest produced the
Breccia
Museo [trans. note: that is the term also used
in English. It is defined in various sources as
“a pyroclastic deposit
produced
during an eruptive event that occurred in the
southwestern sector of the Campi Flegrei about
20,000 years
ago.” Apparently, the first
use of the term is in Johnston-Lavis. See
bibliography] and piperno; the second, yellow
tuff; and the third,
pyroclastic products, partially mixed (in part
pozzolana) formed by volcanic activity after the
formation of yellow tuff.
image 4
More recent studies have
produced a slightly different picture, including
a cycle of activity before the period set by De
Lorenzo, defined as the
archiflegrean eruptive cycle, which corresponds
to the first and second De Lorenzo periods and
which concludes with the
formation of chaotic yellow tuff (known as
typical yellow Neapolitan tuff), and, finally,
includes a last cycle known
as the recent eruptive cycle of the Campi
Flegrei, which corresponds to the third of De
Lorenzo’s
ancient subdivisions. Each cycle of activity
thus identified is progressively more explosive
within each cycle although
that pattern has attenuated
over time.
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THE
ARCHIFLEGREAN ERUPTIVE CYCLE
Activity in the Campi
Flegrei started with a long series of
eruptions of primarily trachytic nature, the
tuff and lava from which
formed a composite volcano (or perhaps a
series of such volcanoes) of the kind and size
of Somma-Vesuvius.
After a long period of
quiet, during which there was constant and
progressive build-up of pressure from gasses
in the
magma basin, there followed an exceptionally
violent eruption that was the origin of grey
Campanian tuff, putting an
end to the activity of this
Archiflegrean volcano. As a result of the
partialemptying of the Archiflegrean magma
basin,
there followed a caldera collapse of the central
part of the volcano complex.
The boundaries of the large
Archiflegrean caldera collapse are not well
defined, either because the caldera was
deformed
by other and later local collapses or because
the caldera was filled and buried by the
activity of at least forty
spin-off volcanoes that later formed over a
long period of time within the caldera. In any
event, the products of later
volcanic
activity deposited on the prominent,
preexisting features of the caldera have not
erased the traces of the
ancient
form; they can still be seen. We can thus see
visible traces of the wall in the east that truncated
the Monte di
Procida promontory, from
Miliscola to Torregaveta, then on the rather
steep southern slope of Mt. San Severino to
the north-east of Cuma,
then on the northern and eastern edges of the
Quarto Plain, on the sunken edges of Pianura
and
Soccavo, and, finally, on the northern slope
of the Posillipo hill. The form of the eastern
region of the Campi Flegrei, to
the east of Camaldoli, is
determined by the ancient surfaces of the
Archiflegrean complex, largely unaltered even
by the products of later
eruptions.
THE ANCIENT ERUPTIVE CYCLE IN THE CAMPI
FLEGREI
After the Archiflegrean
caldera collapse, a number of preexisting,
buried tectonic faults were reactivated by the
rejuvenation of some Tyrrhenian faults, which,
besides submerging the northern section of the
caldera (the Miseno and
Palumbo shallows), facilitated the rise of
magma within the caldera and in the
surrounding area, now occupied by the
city of
Naples. The peripheral and radial fractures of
the Archiflegrean caldera were then
superimposed on these
preexisting but rejuvenated tectonic
lines, making the entire volcanic-tectonic
structure of the Campi Flegrei extremely
complex and often
undecipherable.
Because of the outgassing
of magma following the great eruptive
explosion of grey Campanian tuff, the
Archiflegrean
caldera resumed activity at
first with effusive eruptions of smaller
volcanoes that led to the formation of flows,
lava
domes and scoriae. Most of the volcanic
complex of this period was destroyed by later
activity or buried by later
eruptions; the only
remaining, visible traces are the ruins of the
Miliscola volcano and the alkili-trachytic
dome of S.
Martino (both at Monte di
Procida).
With the progressive,
thermically retrograde increase of vapor
pressure, larger volcanic complexes were
gradually
formed,
and activity became mixed between effusive and
explosive (composite volcanoes) such as the
now largely
sunken
volcano at Torregaveta of which the only
remains are the tuffs and lava flows at the
northwest base of Monte di
Proicida.
From composite volcanoes of
mixed activity, there follows, by way of
afurther increase in eruptive energy, a series
of
eruptions marked by a rapid succession of
explosions that emit a large quantity of ash
and pumice mixed with little
stones
and large blocks spewed upward; Thus,
composite yellow tuff volcanoes were born and
are different from those
that one still sees at Capo Miseno, Porto
Miseono, Bacoli, “Archaverno,” Nisida,
Coroglio and Trentaremi. In these
explosive and rhythmic
eruptions, the pyroclastic material, still hot
and rich with gas that falling near the
crateric center underwent
rapid diagenesis, whereas the material falling
farther away fell cooler in well-defined
layers of ash, pumice
and varying sizes of
lapilli or small stones. Thus the same
eruption produced simultaneous formation of
stratified mixed rocky tuff
and looser pyroclastic materials laterally
mixed and gradually turning from one into the
other.
At the end of this eruptive
cycle, due to the general build-up of gas in
cooling magma, the explosive activity
culminated in a series of
extremely violent eruptions that emitted a
enormous amount of ash, pumice, and sand in
the form of hot, falling
clouds, thus forming chaotic, yellow tuff or
typical Neapolitan yellow tuff. Among the
chaotic yellow tuff
complexes that are
recognizable today, we note the Chiaia
volcano, the Fuorigrotta volcano, and the
volcanoes of
Mofete, Girolomini,
and Gauro, which is certainly the most recent.
At the same time as yellow
chaotic tuff —or, more precisely— in the
interval between two eruptions of yellow tuff,
there was activity at the
volcanoes of Soccavo and Pianura (at the base
of Camaldoli, on the rim of the Flegrean
caldera); the first of
these produced the well-known piperno and the
so-called “Breccia Museo,” while the second
deposited a whitish
ash-pumice-like semi-coherent tuff. The
eruptions at Soccavo and Pianure were followed
by earth slides on the walls of
the two emptied volcanic
conduits with subsequent chipping of the Flegrean
Caldera.
The eruptions of the
chaotic yellow tuff volcanoes should have
extinguished after a single violent eruption
but frequently followed by
extended collapses; however, these were
different in kind from the ones at Soccavo and
Pianura because, rather
than simple steepenings of the walls of the
volcanic conduits, they were true
volcanic-tectonic collapses, that is,
collapses of the dome of
the magma basin divided into a number of
clumps by radial and peripheral faults such as
to cause
regional collapses such as, for example, the
collapse in the Gulf of Pozzuoli all the way
to the Quarto Plain with
the lowering, as a single
block, of the entire volcanic complex at
Gauro.
After the eruptions of
chaotic yellow tuff volcanoes, which went on
for an extended period (though broken by
periods of stasis, the
magma beca me poor in gas and no longer
capable of explosive activity. At the end of
the ancient
Campiflegrean eruptive cycle, there were only
a few effusions of largely viscous trachytic
lavas rising along some of the
collapse faults, which led
to the formation of some lava domes such as
that of Mt. Olibano.
Due to the collapses caused
by the yellow tuff eruptions, the end of the
ancient Campiflegrean eruptive cycle then
saw the sea invade a
large part of the central area of the Campi
Flegrei, from the Gulf of Pozzuoli to the
Quarto Plain, to
Piano, Soccavo and the
Fuorigrotta flatland. Out of that sea rose
only Monte di Procida and the rest of the
volcanic
complexes of Archiaverno,
Mofete, Gerolomini, Gauro, Camaldoli and the
Posillipo spine joined to the Vomero hill and
Capodimonte hill to the
northeast.
RECENT ERUPTIVE CYCLES OF THE CAMPI FLEGREI
A long period of inactivity
then gradually gave the magma time to build up
explosive energy; at that point, volcanic
activity
in the Campi Flegrei reawakened with a new
cycle of explosive and mixed eruptions.
One of the first eruptions
of that cycle was that at Baiai, followed
perhaps at short intervals by those at
Minopoli near
Soccavo and, gradually,
many others, the chronology of which is
difficult to establish, such as the volcanoes
on the Baia sea-bottom, the
Gallo-Russo volcano, and then the eruptions,
broken by long periods of quiescence, of the
volcanoes at Montagna
Spaccata, Pisani andAgnano.
After the violent Agnano
eruption, there must have followed a
particularly long period of quiescence, during
which time the volcanic
complexes were set upon by the strong forces
of erosion (the crater walls had already
broken in places due to the
most recent landslides or eruptions). Much
material was thus removed or rearranged and
the morphology of the area
changed to a considerable degree.
Eruptions picked up then
with renewed violence at Solfatara, followed
by the eruptions at Cigliano, Averno, and the
prehistoric eruptions of the Astroni (in the
Neolithic, c. 1500 BC), finally ending with
the less explosive eruption marked
by strong ejections of
scoriae or vesicular basaltic lava at Fossa
Lupara and Monte Nuovo (the latter was in 1538
AD).
Most of the pyroclastic
products were not particularly coherent and
are partially known as “pozzolano". They
blanket
almost the entire Flegrean area with chaotic
yellow tuff, are due to the recent Flegrean
eruptive cycle.
The historic eruption of
Mt. Nuovo, the bradisismic movements of single
huge blocks (for example, in Pozzuoli), and
the hydrothermal and
fumarole activity that still persists in
Baiai, Pozzuoli, Solfatara and Agnano (that
is, along a fault line in
the direction of the Tyrrhenian) attest to
volcanic activity still very much alive, if a
bit sluggish, and are evidence that
the current basin still
contains noteworthy amounts of magma
undergoing cooling and solidification.
VOLCANIC ACTIVITY OF SOMMA-VESUVIUS
According to Rittman, who
reconstructed the history of Somma-Vesuvius in
minute detail, endogenous forces had been
keeping volcanic activity
in the Campi Flegrei alive for some time when,
about 12,000 years ago, the area beneath the
current Somma-Vesuvius was
punctured for the first time by a violent
explosion, no doubt facilitated by the
fracturing generated by the
sinking of the Campanian basin.
The new volcano that formed
is called Somma Primordiale and must
have been the site of impressive eruptions as
evidenced by the great
amount of ash thrown up in a short period of
time. The basin feeding this eruptive center
must have had an origin
analogous to that feeding volcanism in the
Campi Flegrei and Flegrean islands; that is,
an
ascent of differentiated
acidic magma through a Tyrrhenian fracture to
almost beneath the Mesozoic sediments, thus
creating an independent
magma hot-spot over a time that can be
subdivided into four periods, which we here
briefly
review.
The products of Somma
Primordiale were totally trachytic in nature,
as were those of the Flegrean volcanoes. Domes
of very viscous lava formed
in the crater of this new volcano only to be
fractured and removed by violent explosions
that alternated with
effusions until a dome finally formed that was
strong enough to resist. That plugged the
conduit and
condemned the volcano to a
long period of inactivity. Yet, while Somma
was pausing, powerful explosions of the
Flegrean volcanoes
were spewing up great amounts of ash and
pumice in the form of hot clouds that then
settled on
sleeping Somma to solidify
as yellow Neapolitan tuff.
In the meantime, the entire
Campanian plain was shifting up and down in a
series of movements by separate and
opposing blocks,
carryingthe Somma Primordial below sea level
along with the yellow tuff that had covered
it. Speaking of blocks
moving, it should be noted that because of
that, in historic times, the land on the
western coast of southern
Italy took on a noticeable
inward tilt (i.e. away from the sea); waters
flowing on the surface then stagnated near the
coast,
producing a number of marshes such as Pianura
Pontina, Basso Volturno, and the area of
Pesto. The same thing would
have happened at the mouth of the Sarno river
if Somma had not reawakened and filled in the
land just as it was tilting
away from the sea. This reawakening of Somma
took place in around 6,000 BC and was followed
by a long series of
cumulative eruptions of the powerful volcanic
complex referred to as Somma Antico, the
products of which covered the
ruins of Somma Primordiale.
Images 5-6 (top 2, l
& r) - Cavity beneath #59
via Montesanto showing
a section of
the
Carmignano
aqueduct
successively
enlarged by the extraction of quarried
tuff sandstone.
![]() |
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![]() |
![]() |
Images
7-8 (bottom 2, l & r) Cavity beneath #18
via Broggia, detail of access to the vault.
[translator's note - the debris piles seen in these photos are typical. Well shafts were used for quick debris removal from WWII bombings and block many cavities. Unfortunately, shafts and other openings are still used to dump trash and all matter of waste material into the cavities below the city.]
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page
to top of Part Two
Petrographic studies
of the Somma Antico lavas (defined as
orvietites—i.e. leucititic trachybasalts with
leucite) show
that the magma basin
continued to rise slowly, reaching the
Triassicdolomite that was then absorbed by the
magma with
a subsequent change in the progressively deeper
and more intense chemical activity of the ejecta
from the
volcano.
After another long pause, volcanic activity
started again with an emission of “octavianites”
(leucititic tefrite
basaltoids) and the formation
of the prehistoric volcano we call Somma Recente
(or YoungSomma).
Somma Recente, a typical
composite volcano, reached a height of about
2000 meters; after activity in prehistoric
times, it was quiescent phase
for many centuries and permitted the growth and
development on the slopes and summit
of luxuriant wooded
vegetation until 79 AD when the volcano suddenly
came to life again.
The eruption of that year,
which destroyed the flourishing cites of
Pompeii, Herculaneum and Stabiae, marked the
birth of Vesuvius and was
initially one of “obstructed conduit” (called a
Plinian eruption, from the majestic description
of the event given to us in
two letters written to Tacitus by Pliny the
Younger, who witnessed the eruption.) From that
first
eruption down to our own times, Vesuvius has had
periods of intense activity alternating with
calm intervals, some of
them centuries long. The
products of the volcano are petrographically
termed “Vesuvites (that is, leucititic
plagioclase) and constitute a
great amount of ash and lapilli as well as
copious lava flows that snake down the slopes.
NATURE AND GENESIS OF THE TERRAIN IN THE
SUBSOIL OF NAPLES
After this summary of the chronology of tectonic
and volcanic events over geologic time that
formed the region
now occupied by the city of
Naples and environs, we move to a short
description of the various formations that make
up the subsoil of this
region. We examine them from the standpoint of
genesis and chemical-mineralogy in order to
clarify their technical
characteristics both in sito and as
construction material.
We have noted that the area is made up almost solely of volcanic products of the two eruptive centers, the Campi Flegrei and Somma-Vesuvius; in fact, even the alluvial deposits and sand are largely modifications of the same ejecta. In the material that makes up the subsoil of Naples and environs, whether Flegrean or Somma-Vesuvian, whether deposited directly on the surface or from alluvial or marine sources, we have made petrographic and geotechnical distinctions in order to provide a classification that better fits the goals outlined at the beginning of this report.
Thus we have classified the
materials under consideration into three large
groups: lavas, pyroclastic lapideous material,
and loose pyroclastic
materials. In turn, these groups have their own
further subdivisions.
As far as lavas are concerned, we find it useful
to distinguish between those of Flegrean origin
and those of
Somma-Vesuvian origin. That distinction fits our
purposes, although from a strictly petrographic
point of view, it may
seem a bit simplistic.
For the pyroclastic lapideous material, all exclusively of Flegrean origin, we need to make the following distinctions: Campanian yellow tuff, piperno, stratified yellow tuff, and chaotic yellow tuff. For loose pyroclastic materials, the classification becomes somewhat more complex, whether due to the extreme heterogeneous origin of these materials or to the many factors that may have intervened over time to change the original characteristics.
To avoid a laborious, complex
and not very useful classification, we use a
very schematic one. Even if this misses some
of the fine points, it is
immediately useful. We see the necessary
distinction in loose pyroclastic materials to be
between
disturbed and undisturbed. [Lava remaining where
it was first ejected would be undisturbed; that
same
material moved or broken up
by earthquake or landslide is disturbed.]
Disturbed loose pyroclastic materials are
further subdivided, based on
genesis and granulometrics, into breccia and
scoriae; pumice; lapilli and sand; ash and
pozzolano, other divisions
into provenance (Flegrean or Somma-Vesuvian) are
also possible. For disturbed loose pyroclastic
materials,
further subdivisionsmust use granulometrics. For
these materials, there is no further need to
distinguish their genesis
that might significantly influence their
geotechnical characteristics.
This classification (like
all, and perhaps more than some) is forced on us
by the need for simplicity; we shall see that
there are
materials of uncertain origin, for example,
between pyroclastic lapideous materials and
loose materials, or
between lavas and pyroclastic
lapideous materials; there is no way around that
inconvenience given the origin and
nature of the materials. We
must remember the processes at the origin of
these materials and remember our goal,
which is
practical and technical.
As noted, the lavas of
Flegrean origin are mostly trachytic, while
those of Somma-Vesuvian origin are essentailly
tefritic or plagifloiditic
(most of which are ejecta of Vesuvius after the
eruption of 79 AD). Vesuvian lava (also referred
to locally as “pietrarsa”) is
a characteristic building material in Naples; it
is used as street pavement, as cut stone,
masonry
units, fill rubble, and even as breakwater
blocks. The main centers of extraction are in
Portici, Resina, and
Torre del Greco where lava
flows from various epochs are "cultivated”
(primarily the flows of 1631 and 1760): the best
blocks are obtained at the
center of the flow near the wall called “pietre
del pedicino” [an old local reference to the
hardest ‘heart’ or center
core of a lava stream], while blocks from the
upper part of the “cima” [summit] flow are of
lesser
quality due to many vacuoles and general
irregularities. The significant physical and
mechanical characteristics
are: apparent specific
weight= 2.70 – 2.78; wear index (thickness in mm
of the abraded surface under a load of 0.1
Kg/cm2 and
after a course of 1 Km) = 1.10; breaking load to
crushing = 1200 Kg/cm2 (min. 600, max. 1800).
Rocks of Vesuvian lava are
very good for construction blocks, but mot as a
base to build on; the lava hides an
insidious
danger in the vast and extended cavities at the
base of the flow where the sand-scoriae of the
bed of the flow have been
washed away by underground waters. Before
building on a lava bed, it is good to check the
thickness of the lava for
possible cavities. Trachytic Flegrean lavas are
much less widespread; they are found at Mt.
Olibano and at
Solfatara,
at the base of Mt. Spina, at the Astroni, at the
Punta Marmolite of Quarto, at Mt. Cuma and at
some stretches of Monte di
Procida. Of these outcroppings, only those at
Quarto and Mt. Olibano have been used to harvest
construction materials: the
Quarto trachyphonolites, clearly fluidic, were
used by the ancient Romans as road surfacing,
the alkalitrachyte of Mt.
Olibano was also used by the Romans in the
Pozzuoli amphitheater and also in more recent
times in
various Neapolitan monument buildings (Castel
Nuovo, S. Francesco di Paola, etc.) and for a
number of
maintenance buildings along the Naples-Roma
rapid train line and many highways. The known
physical and mechanical
properties of these rock types are: Quarto
trachyphonolite, apparent specific weight=2.55;
breaking load to crushing =
1200-1900 Kg/cm2; Pozzuoli, apparent specific
weight=2.50; resistance to crushing = 400-800
Kg/cm2;
trachytic.
More important than the
surface outcroppings of Flegrean trachyticlavas
that at these sites are those amassed
beneath
the ejecta of later eruptions and that have
often been found in the course of underground
work in Naples.
Among
these, we note the two trachytic masses found
during the building of the Cumana railway tunnel
at Montesanto, the trachyte
at Piazza Amedeo at the upper sewage collector
and the rainwater run-off collector; the
trachyte masses
found in the Posillipo hill
at the Naples city sewer effluents of Cuma and
Coroglio; and finally the trachytic masses found
in building the urban stretch
of the Diretissima [rapid train]
tunnel.
Some reports in technical
literature say that all of these lava masses
result from effusions before those that produced
yellow
Neapolitan tuff. In our view that must be taken
with some reservation since there is no longer
any doubt that in the
intervals between some eruptions of yellow tuff
there were also other particular ones that
produced piperno; thus, the
intrusion of trachytic domes could easily have
taken place. In any event, whatever the age and
position of the
trachytic
masses, it is important to keep in mind for very
practical reasons that they can be found
anywhere in the
urban
area, even in those areas that we view as
exclusively given over toyellow tuff formations.
LAPIDEOUS PYRCOCLASTIC MATERIALS
As noted earlier, lapideous
pyroclastic materials in the area of Naples
(even outside of the city limits) are all of
Flegrean origin. That is not
surprising since diagenesis (that is,
lapidification) of pyroclastic materials is
strictly linked to the
eruptions
that produce them. That is, lapidification is
not a secondary process that may or may not
occur after
pyroclastic materials are
deposited. Lapidifcation doesn’t depend on
environmental conditions independently of the
phenomena that produced those
deposits in the first place, such as, for
example, an elevated degree of amassing from
an overlying load of
materials, or the infiltration of water, or the
influence of a marine environment.
Lapidification is not due to
the particular state of subdivision or the lack
of uniformity in the pyroclastic products.
Rather, the diagenesis of
Neapolitan pyroclastic materials can be
exclusively attributed to the particular
conditions present at the moment of the
eruption and precisely to the
phenomena of autometamorphism (autopneumatolysis
and autohydrothermalization) from
gasses escaping from the mass
of deposited and still hot and volatile
pyroclastic materials. Only some particular
eruptive activity (described
later) has deposited masses of hot pyroclastic
materials, rich in gasses, and only in those
cases has
lapidification occurred. Somma-Vesuvius has
never had eruptions of the type that permit that
depositing of
hot, gas-rich, pyroclastic
materials. That is why its pyroclastic products
have never undergone diagenesis and have
remained
loose.
The degree of diagenesis
depends, above all, on the temperature and the
contents in the form of gasses of the
materials
at the moment of sedimentation; that explains
the shaded, gradual change, both vertically and
laterally, of
lapideous pyroclastic
materials into other semicoherent and, again,
into completely loose pyroclastic materials.
According to the most recent
views, this tuff is said to be the product of a
powerful explosive eruption that put an end
to the original of all
Flegrean volcanoes, the great composite volcano
called Archiflegreo. In the wake of the powerful
eruption,
the central part of Archiflegreo collapsed,
producing the Archiflegrean Caldera
[images
9-13 below] are all of the Cavity beneath #18
via Broggia; a tunnel in inconsistent soils in
the zone
beneath Piazza Dante
showing examples of various solutions for
upper cover reinforcement.
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Two
Since
this tuff is one of the most ancient
products of volcanic activity in the
Campi Flegrei, we don't see it
cropping up in
its original area where it is buried
beneath the products of later
eruptions. It is found only at a
notable distance from
the Campi Flegrei
proper; that is, in the Campanian
basin, from Capua to the plains of
Angri and Nocera, and on the
Sorrento plain.
Normally, the tuff is grey, often
shading over to grey-brown,
occasionally tending to yellow, and,
more rarely,
reddish or violet. The compactness
varies; sometimes it can be easily
crumbled by hand; other times it is
lithoid. It is
characterized by the abundant
presence of pumice and small black
scoriae in a cineritic mass
generally lighter in
color, and the
tuff sometimes displays very large
scoriae that are foamlike, fragile
and irregular. In some zones it has
a flame structure
very similar to that of piperno,
which has led to it also being
called pipernoid grey tuff.
The eruption of
grey Campanian tuff must have taken
place in a rhythmic succession of
violent explosions sending up
great quantities
of mixed ash and lava shreds, with
large quantities of gasses, creating
a dense and hot suspension
that settled in a
chaotic state and then lapidified
through autometamorphism. Every so
often, the rhythm of the
explosions must
have slowed, allowing for a
dispersion of gasses and the cooling
of ash and scoriae ejected in those
intervals, which
then settled under conditions no
longer favorable to complete
diagenesis.
This explains the
subtle and gradual changes we see in
some zones across the entire series
of grey Campanian tuff. In
effect, when you
speak of grey Campanian tuff, the
boundaries between lapideous
materials and semicoherent
materials or
completely loose materials are not
precise, so refined is the change
from one to the other. In some zones
the lapedeous
facies reaches a considerable width
(20 to 30 meters and more), while
the semicoherent facies is
reduced to a few
meters and less at the wall and roof
of the bank. In some zones you have
lapideous banks repeatedly
alternating with
semicoherent or loose banks only
inches thick or, at the most, a few
meters, with gradual changes from
one type to
another but without appreciable
differences that you would notice in
the structure of the entire mass or
in the size or
frequency of scoriae and pumice.
That is why we
define “grey Campanian tuff” in
terms of how it was formed
geologically rather than by
lithologic type,
thus including in the definition all
of the materials emitted during the
eruption of this tuff. Then we
specify, if
necessary, how
consistency and cohesive the
material is at a given spot. For
geotechnical purposes, it is
important to keep
in mind that grey Campanian tuff
often has very weak cohesion that,
however, still permits the
opening of
excavations and almost vertical
banks even tens of meters high
without the danger of collapse.
Likewise,
underground
digging is possible without the need
for sustaining structures. If,
however, you try to extract from one
of the
excavations a block that has been
cut to a regular shape, that may not
be possible because the material
will
crumble into an
incoherent mass of very fine and
ashlike mixture of scoriae and
pumice; once the cohesion is
destroyed, it is
impossible to restore or
reconstitute the material to its
original density.
That particular
behavior of semicoherent grey
Campanian tuff is often the source
of mistakes by those who lack
sufficient
knowledge of this formation or lack
experience working with it. Thus,
for example, you might have a core
sample pass
through the material and give
readings such as “ash with scoriae
and pumice” or even “fine sands,
slightly silty
with pebbles and coarse sand”. The
consequences of such a
misinterpretation of a core sample
are obvious,
especially if you
are laying out the path of a tunnel,
for example.
On the other
hand, it is also evident that the
weak cohesion of some varieties of
grey Campanian tuff cannot always
guarantee
stability and safety, especially in
certain kinds of leveling work or
excavation. To avoid the potential
for
disaster, you
really do need a case by case
analysis by an expert.
The lapideous
variety of grey Campanian tuff is
widely used as construction
material, especially in many towns
north of Naples,
in the area of Caserta, in the areas
of Angri and Nocera, and in the area
of Sorrento. The physical and
mechanical
characteristics of the material vary
from place to place and even within
the same general area. On the
average, however,
the characteristics vary within the
following values: apparent specific
weight= 1.20-1.60; imbibition
coefficient in
reference to weight= 30-50%;
breaking load to crushing= 25-60
Kg/cm2. Some Salernitan grey tuffs
have been found
that have a value for breaking load
to crushing as high as 150 Kg/cm2.
One of the most
characteristic volcanic products in
Campania is piperno. It has
been widely used by Neapolitan
architects over
the centuries and lends air of
patrician elegance of many older
Neapolitan buildings.
Piperno has a
lapideous look and feel to it. The
bulk is typically gray with darker
bits scattered throughout, called
“flames”, They
are lens-shaped and distributed in
roughly parallel fashion. The
lapideous consistency of piperno and
its almost
fluidic structure have caused
various scholars in the past (Von
Buch, Zambonini, De Lorenzo) to hold
that
piperno was a
lava —that is, an effusive
rock— but more recent studies
no longer leave any doubt that it is
volcanic tuff —
that is, trachytic pyroclastic rock
caused by a particular type of
eruptive activity known as a “lava
lake”. This occurs
when deep magma
rises in the volcanic conduit and
invades the crater, but doesn’t
overflow, thus creating a fluid and
incandescent lake
of lava within the crater. From this
outgassed, fluid and very hot lava
lake, spray and fountains then
shoot up while
new, deep and much more viscous
magma rises, is pulverized by
escaping gasses and ejects in the
form of a fine
ash. You thus have, all around the
crater, a rain of ash and doughy
lava bits that release gasses
contained
within them (or
from deeper sources) and solidify by
pneumatolysis into a single rough
mass of lapideous consistency.
The consensus of
opinion is that piperno was the
product of a single volcano in the
Campi Flegrei, the so-called Soccavo
volcano on the
edge of the Archiflegrean Caldera at
the foot of the Camaldoli hill. The
piperno eruption of Soccavo,
contrary to De
Lorenzo’s view, occurred in the
interval between two eruptions of
chaotic yellow tuff and is thus much
more recent than
the eruptions of grey Campanian
tuff, which piperno has nothing in
common with. The formation of
piperno in
Soccavo was accompanied by a coarse
and characteristic pyroclastic
formation called “breccia museo.”
That formation
lies above the piperno bank and was
the product of a violent explosion
of the Soccavo volcano after the
collapse of part
of the volcanic conduit and walls of
the crater.
Other than at the
base of Camaldoli, piperno has been
found elsewhere in the urban area of
Naples, particularly in the
area of Piazza
Amedeo/Parco Grifeo, along the
extension of via Palizzi and in the
Diretissima [train] tunnel
(still near
Piazza Amedeo).
Stratigraphically, the piperno
masses are between two formations of
chaotic yellow tuff and, according
to Rittmann, must
be from the same eruption that
produced the Camaldoli piperno—that
is, the Soccavo eruption.
More recently,
however, we have found other pockets
of piperno in the urban area, even
at some distance from the
eruptive center
at Soccavo. We thus
hypothesize that piperno, rather
than the product of a single
volcano, is more
likely from a
particular type of eruptive activity
of various volcanoes in the course
of eruptions that produced chaotic
yellow tuff. We
do not yet have enough evidence to
prove that hypothesis, but it is
good to keep it in mind for future
studies of the
Neapolitan subsoil. Various
underground quarries on the
Camaldoli slopes with entrances at
Soccavo and
Pianura mined this material in the
past; these quarries today are
almost all abandoned and dangerous.
Extraction of
piperno from them
is limited to rare cases when the
material is for restoration.
Although this
material was widely used in times
past in Naples, there are no solid
data on its physical and mechanical
characteristics.
Two studies from 1820 and 1869 put
values of 592 Kg/cm2 and 151 Kg/
cm2, respectively, for breaking
load to crushing.
The first type showed an apparent
specific weight of 2.60; the second
showed 2.28 (which explains
the low values
for resistance to crushing).
This tuff came
fron explosive eruptions during the
ancient eruptive cycle of the Campei
Flegrei before the beginnings of
chaotic yellow
tuff eruptions. The distinction
between stratified yellow tuff and
chaotic yellow tuff is very
important
because it lets
us define chronological points of
reference useful in reconstructing
the stratigraphy and tectonics of
the region. The
eruptive centers, still
recognizable, that produced
stratified yellow tuff are the
volcanoes at Capo Miseno,
Bacoli, and Porto
Miseno, plus the volcanoes at Nisdia,
Coroglio, and
Trentaremi at
the extreme end of the Posillipo
hill. In
general, stratified yellow tuff
shows a lot of pumice and scoriae,
mostly small (although at Nisida
there are some
very frothy
scoriae that reach one meter in
size). Besides the stratification,
this formation also shows noticeable
granulometric
differences in the strata and in
color and in distinct
characteristics that differentiate
this tuff from chaotic
yellow tuff
(which, as we shall see, even at the
roof and wall can sometimes be
clearly stratified). Higher up,
stratified yellow
tuff gradually shades into a clear
grey color, is semi-coherent
and contains numerous bits of pumice
and light,
frothy scoriae.
The eruptions
that produced stratified yellow tuff
must have been a series of
explosions in rapid succession that
threw up large
amounts of pumice and ash mixed with
scoriae. At the end, the rhythm of
the eruptions slowed, extinguishing
in a few last
isolated explosions. The rapid
depositing of pyroclastic materials,
still hot, caused these materials to
lapidify after a
final outgassing in situ and
to cool slowly. On the other hand,
the sedimentary materials that were
thrown up towards
the end of the eruption or thrown a
greater distance from the crater
were already cooled as they fell
and did not
undergo diagenesis.
The same
eruption, thus, could have produced
stratified yellow tuff and, at a
greater distance, an accumulation of
incoherent grey
tuff. Furthermore, note that the
gradual and subtle change, as one
moves upward, from stratified
yellow tuff to
semicoherent grey tuff was produced
by the same eruptive activity.
We don’t know the
mechanical and physical
characteristics of this kind of tuff
[trans. note. i.e. stratified yellow
tuff].
That is due in
part (1) to the fact that it is not
widely used as construction material
(given the limited extent of
outcroppings, the
difficulty in mining them, and their
heterogeneous nature, all factors
that discourage practical or
commercial use)
and (2) to the fact that this tuff
is often commonly confused with
common yellow tuff. It is even quite
probable that
stratified yellow tuff is more
common than we think, especially
within the hills that urban Naples
rests on; thus,
it is likely that some of the
ancient volcanic complexes of Naples
are made up of stratified yellow
tuff and not
chaotic yellow
tuff. That might be of extreme
importance from a technical point of
view and should be duly kept in mind
as plans are made
for new underground lines of
communication and new structures
that affect the subsoil.
CHAOTIC YELLOW TUFF
This is also
called, simply, “yellow Neapolitan
tuff” as if to say that this is the
true, typical, Neapolitan rock; it
is the
kind most used in
construction of all types and the
one that lends a particular
character to architecture of the
region.
Yellow tuff,
which has a chemical composition
analogous to that of an
alkalitrachyte, is due to the
autocementation of
various kinds of
volcanic detritus (primarily ash,
lapideous lapilli, pumices,
scoriae,etc.) that erupted from
various active
craters during the ancient eruptive
cycle of the Campi Flegrei. The
volcanoes known to have produced
yellow chaotic...
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image
14 - Cavity at via #18,
tunnel of the
Carmigmamo aqueduct enlarged for use as an air raid shelter |
image 15 - Cavity beneath #59 via Montesanto ![]() |
image 16 - Cavity beneath largo Vasto a Chiaia |
image 17 |
image 18 |
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|
There was only a slight difference —a higher degree of freshness [retention of color] in the pumice embedded in the green variety. After a few hours of treatment in a solution of hydrogen peroxide, green tuff became indistinguishable from yellow tuff. Later tests on greenish tuff showed that the difference between these two varieties is a matter of degree of oxidation. That explains why we never see outcroppings of green tuff except at freshly dug sites. Guadagno thinks that the masses of green tuff are the relics of an original green tuff, almost totally oxidized and transformed into yellow tuff. Salvatore says, however, that the greenish areas might be the product of “intimate, secondary reactions” that happened in the tuff after it was formed. In any event, we can exclude that the type of greenish tuff found as “inclusions” in yellow tuff is the same as the grey-green tuff found in various deep wells at the base of yellow tuff (such as those described by F. Ippolito in the port zone of Naples, or by Guadagno at the well in the square of Santa Maria la Fede or, yet again, by D’Erasmo in some of his works). That tuff is to be attributed to the formation of grey Campanian tuff, the product of volcanic activity that occurred before the activity of yellow tuff. We can’t even group this type of green tuff in with the green tuff of Epomeo in Ischia, which we often find in redisgorged blocks in with the yellow tuff of Campi Flegrei. As a matter of fact, the tuff from Epomeo has a stable green color, not oxidizable, given it by the presence of minute tags of a mineral in the glauconite group.
During the construction of the Vomero tunnel of the Circumflegrean railway, a large (longer than one meter) fragment of fossilized wood was found in this kind of oxidizable greenish tuff. The fragment was 250 meters to the east of Torre San Domenico; it was at a depth of 20 meters and 80 meters above sea-level. Carbon dating put the age of the fragment at about 10,000 years. This dating shows the antiquity of the Flegrean eruptive phase that produced yellow Neapolitan tuff; it fits perfectly with the chronology of Flegrean-Somma-Vesuvian volcanism reconstructed by Rittman. Even from a petrographic point of view, there were practically no differences between the kind of greenish tuff found in the areas of S. Stefano and Vallone Riccardi in the Vomero hill, and the corresponding kind of yellow tuff and the physical and mechanical characteristics of the greenish tuff were notably better. The green tuff from Vallone Riccardo showed a resistance to crushing that varied from 116 to 166 Kg/cm253 while green tuff from S. Stefano actually reached 230 Kg/cm2, the highest reading ever recorded for all types of Neapolitan volcanic tuff. It should be noted that the surrounding yellow tuff also showed elevated readings, but noticeably lower than the green tuff embedded in it.
We have spent some time discussing this greenish tuff (which is practically the same as yellow chaotic tuff) because it forces us to dwell on the proper interpretation of stratigraphic samples done in the past in urban Naples. Such samples showed the presence of grey-greenish tuff at a depth where we might have logically expected yellow tuff; in effect, we can’t exclude the possibility, in some cases, that it is all the same yellow tuff formation.
This underscores, all the more, the need to study wells, excavations and core-samples with caution in order to avoid false interpretations that can lead to noteworthy consequences both from a scientific point of view and a practical one. Yellow tuff is present in banks that range widely from zone to zone in the city: up to more than 180 meters in the area of ex-Piazza Leopardi in Fuorigrotta; up to about 110 meters in some areas of the Vomero hill; around 60 meters at and around Piazza Vittoria; around 90 meters in the area of Piazza Plebiscito; around 50 meters in the area of Santa Marria della fede; and 30-35 meters in the eastern part of the urban conglomerate. These data are sporadic and scattered because there are really only a few stratigraphic core samples across the entire range of the formations of chaotic yellow tuff. It is certain, however, that the yellow tuff in the urban area is not formed as a single bank but, rather, of superimposed, mostly horizontal layers or strata of lapideous chaotic tuff (each one of which representing a single eruption), separated by levels of more or less coherent pyroclastic materials (representing the beginning or the end of an eruption of yellow tuff) interlaid with banks of piperno, accumulations of volcanic brecce, and expansions of lava. Furthermore, it is certain that towards the eastern edge of the urban conglomerate the yellow tuff formation thins out until it disappears altogether. In its place we then find loose pyroclastic materials, either Flegrean or Somma-Vesuvian, as well as alluvial deposits transported from various sources.
The yellow tuff formation must have undergone many powerful tectonic dislocations, (primarily a lowering) caused by a series of collapses of the roof of the volcanic basin following the emptying of the basin of enormous amounts of magma in the form of hot clouds. That is why yellow tuff then split into various clumps affected by frequent fracturing grouped along tectonic lines of movement below. Furthermore, in the mass of yellow tuff there are many other regularly occurring and characteristic fractures and lithoclasts due to the contraction of the diagenetized (by autometamorphism) cinaretic mass after cooling. Finally, before being mantled and partially buried by later eruptions (by mostly loose cinerites and pozzolana) the yellow tuff formation was exposed for a long period of time to violent erosive atmospheric activity. (This occurred in the relatively peaceful period between the ancient and recent eruptive cycles of the Campi Flegrei.)
All this produced an extremely complex morphology buried in yellow tuff, one that is often different from the one we see today. In this mass of tuff —dislocated, faulted, fractured and eroded— abundant other loose pyroclastic materials have superimposed themselves, partially filling in the furrows, leveling and softening the once jagged and irregular morphology. Added to the leveling effect of the recent Campi Flegrean eruptive cycle, we now have to deal with manmade effects, which have often filled in valleys and leveled bumps and irregularities. This has made it all the more difficult to reconstruct the original course and pace of the tufaceous subsoil. That can only be done by patiently selecting, collecting and studying all of the current and future data that pertain to the urban subsoil. That work has already started and is the subject of the next chapter in this report. The work is just beginning and is a long way from reaching conclusions.
For many centuries, people preferred to mine chaotic yellow tuff for construction not from embankments or open-air quarries but from underground sites. This was probably because they wanted to build the structure from material mined right on the spot rather than transport it from farther away. There were two different methods for extracting the stone: one was to dig a vertical well through the loose pyroclastic material above the stone. Once into the stone, they gradually started to expand the cavity out into a bell-like shape. A second way (possible only under some conditions) was to dig a horizontal or slightly downward angled shaft into the tuff, then cut out large chambers off the shaft, and extract the stone by way a series of deepening excavated layers, or rarely, a series of excavations which lowered the overhead ceiling in a series of steps as the tuff strata encountered loose pockets of subsoil. This topic is amply covered in another chapter of this report by R. Di Stefano, who has reconstructed the distribution, development and evolution of underground excavations in the Neapolitan subsoil over the centuries.
At this point, we simply note their presence of these cavities and the presence of any number of other items such as cisterns to hold rainwater and, then, water run in from the aqueduct. These excavations and cavities can, in some cases, have a direct or indirect influence on the stability of the buildings above them. They can also (1) put serious obstacles in the path of important underground work on the urban infrastructure (such as, for example, building an underground train line) and (2) also sometimes be used to the advantage of such public works. We have direct knowledge of many cases. As far as the first one goes, we cite the case of the first station of the Flegrean railway line at Montesanto; completion of the station was held up for years by the difficulties encountered in trying to expand one of the two existing tunnels; the tunnels are hard up against, or even partially run through, a deep and vast cavity that is in ruins and supported by a series of monumental buttresses, arches and columns. As an example of the second type of situation, we cite the case of the main SIP telephone center on the hill at Mt. Echia, where a number of vast cavities were found, some of which went down to the level of the Galleria [tunnel] Vittoria of Chaitamone, that is, about 40 meters deep. These cavities were used to create a large underground storage facility. These two examples, on either extreme, show the great importance of knowing about the Neapolitan subsoil in any plan of urban expansion; they demonstrate the need for organized investigations in order to map our subsoil, a great part of which remains unknown even today.
In this chapter we shall not deal with the effect that this extensive underground network of cavities might have on the stability of structures both on the surface as well as underground. That is handled in the chapter dedicated to such problems as cave-ins, collapses, etc. brief mention of some of the chemical properties of the rock, information that has only come to light in recent years. Detailed studies by R. Serslae have shown that...Yellow Neapolitan
tuff, contrary to what we used to think until just a few years ago, is “hydraulically reactive” (that is, it reacts with calcium hydroxide in water to form products with cement-like properties) even more so than pozzolana, the material used to make hydraulic mortar. It is evident...(cont.)
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(cont.) that, at least in the area of Naples, this new information is largely of scientific interest; that is, as long as we still have high quality pozzolana, there is no advantage to using yellow tuff, which would first have to be finely ground.LOOSE PYROCLASTIC MATERIALS
To complete the examination of Neapolitan yellow tuff, we now make Finally, some current investigations at the laboratory of Health Engineering of C.N.E.N. (Comitato Nazionale per l’Energia Nucleare) [National Committee for Nuclear Energy] have found that yellow Neapolitan tuff has excellent exchange properties as regards two longlived radionuclides, Cs 137 and St 90; the yellow tuff has exchangeproperties clearly superior to those of other natural exchangers (montmorillonite and vermiculite), such as to render yellow tuff competitive with the best inorganic exchangers for the treatment ofwater contaminated by refuse.
As noted earlier, loose pyroclastic materials are quite difficult to classify. This is due to the great variability in types as well as to the different conditions of genesis and the many external factors that later intervened to modify their original characteristics. For those reasons, we have chosen to distinguish between undisturbed and disturbed material. [trans. note: “disturbed” in this context means moved from its original position.] In our view, the action of disturbing [or moving] the materials either by external dynamic events or by man, is almost always what causes their mechanical and physical characteristics to change. With that, we now rapidly review these materials, limitingUNDISTURBED MATERIALS
ourselves to their genesis and petrography and at how those factors anfthe structure of the materials influence the physical and mechanical characteristics.
The materials have been divided, in part, along the lines of their genesis and, in part, their granulometrics. The basic types are: volcanic breccia; scoria; pumices; lapilli; ash and pozzolana.
volcanic breccia — are made up of a coarse accumulation of lava fragments (and other rock) produced by the explosion of an obstructed conduit or torn by the explosion from the walls of the conduit; they may also be material that has collapsed from the sides of the mouth of the crater into the conduit and then been ejected. In general, breccia are a mixture of fine materials and represent sporadic episodes of volcanic activity. The classic case is that of the “breccia museo” (so-called because of the great variety of rocky material it contains) on top of the piperno and in part of the Soccavo piperno eruption at the base of the Camaldoli hill. In volcanic breccia we sometimes see the phenomenon of pneumatolysis, a determining factor in certain kinds of diagenesis, but, generally, the breccia are present in a loose, incoherent state. We find masses of volcanic breccia in some underground cavities in the urban area (for example, in some tunnels of the new aqueduct). Pinning down their exact location would be be very useful in reconstructing the stratigraphy of the subsoil of Naples.
scoria — can be divided, depending on their genesis, into “ejected scoria” and “lava socriae”. Ejected scoria are lava shreds thrown from the mouth of the volcano during the eruptive phase, in fact, now named for that activity of scoria ejection. These breccia are only moderately frothy, but in their entire mass are made up of a glasslike substance containing sporadic intratelluric crystallization. Sometimes the shreds settle when they are still liquid or doughy and are thus flattened at contact with ground, often fusing themselves to one another, producing a so-called “fused[or welded] scoria formation.” Piperno is a special case of welded scoria. Lava scoria, on the other hand, are made up of a substantially compact lava nodule the outside of which has a foamy or frothy crust, rough and irregular, on which you find flakes of pneumatolitic minerals.
Lava scoria form the upper and lower parts of a lava flow where the material takes on a frothy look due to the escape of gasses and then a glassy appearance because of the rapid cooling. Among the most common and important lava scoria is the so-called “ferrugine” [ferrous, metallic] variety, which is of Vesuvian origin. It is widely used in Naples for the production of light, cement-like mixtures that are highly resistant. Ferrugine owes its properties as a construction material to its make-up and structure, combining the mechanical resistance of lava with high adhesion and low weight.
From the foregoing, it is clear that there is a substantial difference between lava scoria (i.e. essentially ferrugine) and ejected scoria. In the latter, we have lava shreds dragged into the air by erupting gasses and cooled in flight into a black mass of frothy glass (with an occasional lava nucleus). Lava scoria, on the other hand, is substantially microcrystalline with little glass on the surface. Ejected scoria are more frequently the product of Flegrean rather, than Somma-Vesuvian volcanism, while Flegrean lava scoria practically don’t exist at all. That is not chance; it is a direct result of the chemical composition of the two magma types. The size of the scoria, whether ejected or lava, vary a great deal, from a few cubic decimeters [trans. note: for example, 4 cubic decimeters = 244 cubic inches] and larger all the way down to sand.
pumices — are shreds of lava of various sizes, from the size of a pea to that of a human head. They are very frothy and glass-like, extremely porous and light, and are ejected from explosive volcanic activity, almost always during the initial phases. Alomng with pumices, even larger amounts of ash are thrown up, but during their flight through the air, they are sorted on the basis of their weight (and, thus, size) and settle in strata that are granulometrically quite distinct. If, however, the pace of explosions accelerates, that sorting process no longer occurs and the pumices then settle together with ash from earlier explosions, producing a mixed mass of pumices and ash.
Pumices are generally formed from very viscous magmas. The very porous rhyolitic pumices (for example, those found on the island of Lipari) are typical and plentiful; trachytic pumices (such as in the Campi Flegeri) are less finely porous, but still relatively plentiful. Pumices are less frequent in Vesuvian magmas unless, after a long period of blockage in the conduit, there conditions that allow them to form (i.e., a chemical-gravitative differentiation in the magma and a build-up of gasses in the upper part of the conduit), which is what happened in 79 AD in the initial eruption of Vesuvius, which destroyed Pompeii under a blanket of pumice and ash. On that occasion, the bank of pumice reached a width of 2.5 meters at some points, but that is a unique case in the 2,000 year-old history of Vesuvius. [trans. note on “initial eruption”: By definition, “Vesuvius” starts with that eruption. Obviously, the earlier volcano named Somma has a longer history of activity.] Since that eruption, pumices have been a negligible part of the products of the volcano. Pumices are widely used in cement-mortar mixtures to make blocks, hollow bricks, etc., which due to the low weight per volume, high moisture resistance, and fair mechanical characteristics lend themselves very well to the construction of non-load-bearing structures.
Among the pumice banks from the recent Flegrean eruption and well known to old-time Neapolitan miners is the one called “sette palmi” [trans. note: seven palms, one palm being a unit of measure based on the hand-span] because it was about two meters thick. Until a few years ago (and possibly still today) pumices were extracted from a series of unreinforced underground shafts dug down and then branching off into the subsoil of Naples. This practice is now forbidden because it led to potentially dangerous conditions and was the cause of at least some cave-ins.
In that respect, we might cite, among other examples, the case of the recent, huge cave-in on via E. Cortese in the Vomero section of town; that cave-in brought to light an old shaft dug in a pumice bank just a short distance from sewer lines. The shaft evidently promoted further erosion from a leak that had originated at the sewage line; once that erosion started and expanded, it produced a vast underground cavity, tens of meters deep and causing the collapse of a large stretch of road-bed (fortunately with no victims).
lapilli — The term lapillo (the singular) [little stone] has a strictly granulometric meaning; it indicates loose pyroclastic materials roughly the size of fine gravel or pebbles. We thus have to define the genesis and nature of lapilli (lapideous, scoria or pumice) in order to define their physical and mechanical characteristics. In the terrain we studied, lapilli, (except in the case of pumices) are found in banks a few decimeters in width at the most, and they alternate with other loose pyroclastic materials. If we finder thicker banks of lava lapilli or scoria that are granulometrically uniform, they are certainly disturbed materials from an alluvial or marine environment. Naturally, lapilli may also be found frequently in mixed accumulations of loose pyroclastic materials and all other products of explosive activity.
ash and pozzolana — Volcanic ash is a collection of extremely tiny shreds of glassy and frothy lava. It has a small bubbly texture and is mixed with other vitreous and non vitreous detritus, among which are fragments of intratelluric crystals and rock ripped from the walls of the conduit by erupting magma and gasses. In the area of Naples, volcanic
ash is more or less rich in pumices, lapideous lapilli and scoria from both Campi Flegrei and Somma-Vesuvius. The ash is called, generically, pozzolana, independently of its main use [trans. note: pozzolana comes from the word pozzo— a well], that of furnishing, together with calcium hydrate, water-resistant mortar; thus, in local terminology, ash and pozzolana are synonyms.
A local distinction is made only between Flegrean pozzolana (called,simply, “pozzolana”) and that which comes from Vesuvius (called pozzolana di fuoco [fiery pozzolana]). There is a substantial difference between the two types of pozzolana. The Flegrean variety is glassyand frothy with only a secondary amount of crystalline fragments
(especially Sanidine); fiery pozzolana, on the other hand, is characterized by a prevalence of crystalline fragments (mostly leucite) with little glassy substance. Furthermore, Flegrean pozzolanas have not been disturbed (at least those that are actually used as pozzolana), while Vesuvian pozzolana has been frequently disturbed and moved by rainwater. Accurate terminology would require that “pozzolana” be reserved for those cineritic materials with hydraulic reactivity, thus reacting with calcium hydroxide in water. That reaction is, in fact, termed a“pozzolanic” property.
It has now been ascertained that only some cineritic material of Flegrean origin displays pozzolanic properties, which derives from its essentially vitreous state, from the chemical composition and from the fine frothy texture. Ash of Vesuvian origin, on the other hand, has pozzolanic properties only rarely, and that is not so much due to the chemical composition as it is to the scarcity of materials in a vitreous state. Experience from Parravano and Caglioti, thirty years ago, showed that melting Vesuvian ash (inactive) (tempering it such that ittakes on a glassy, spongy state) and then pulverizing it produces pozzolana that reacts very well with calcium hydroxide.
As far as the granulometry of these materials is concerned, we should bear in mind that during an explosive eruption material ejected from the mouth of a volcano is very mixed as to form, size and density; it is only at a greater distance from the crater that the size and density of settled material can be classified. Generally speaking, the sorting process happens only with the heaviest and most voluminous products, the reason why volcanic ash is almost always a mixture of abundant small pumices and frequent lapideous lapilli and scoria. The texture and form of the single elements in this terrain depends strictly on the chemistry and conditions of the magma at the time of eruption as well as on the type of eruption; that is what determines the physical and mechanical properties.
This is especially true as regards porosity. The material can be very porous but still have particular characteristics due to the fact that only some of the pores are accessible, while some, depending on the nature of the frothy, bubbly texture, are very thin and isolated.
The angle of internal friction is higher than in other loose sedimentary materials that were granulometrically the same. That depends on the markedly jagged form of the single elements. The tiny granules are so jagged that it leads one to think, in some cases, (particularly between 5mm and 0.05 mm—which includes most pozzolanas and pumices) that there must be an increase in the critical angle of repose as the granules get smaller. That is theopposite of what happens in loose sedimentary materials, where the critical angle of repose increases as the granules get bigger.
Finally we consider cohesion, a factor that seems to be of little importance in geotechnical laboratory tests, but which, in real life, should not be overlooked. Cohesion depends not so much on water content or degree of compaction as it does on the conditions when the material was formed. Cohesion increases if the materials settled hot and rich in volatiles (which would then cause partial diagenesis through autometamorphism). That is particularly true in those uniform and powerful pozzolana formations that settled rapidly after veryviolent closely-spaced explosive eruptions. We don’t notice this cohesion so much in laboratory tests because it is destroyed during core-sampling or during the preparation of the samples; we do notice the cohesion, however, on site. We have also noticed that the same materials, if they have been disturbed atmospherically, do not display the same cohesion even if they are more densely packed.
We said at the outset that classification of disturbed pyroclastic materials has to be based on granulometery. It is, however, still important to determine the genesis of these materials; that gives useful information as to the physical and mechanical characteristics of the materials as well as to their position in the surrounding terrain. In fact, if loose pyroclastic materials are disturbed, the mass of material can be modified not only in granulometric assortment and
petrographic composition of the entire mass, but the individual components, themselves, can undergo change. These changes will be a function of the length and intensity of the disturbance, and the mechanical and physical characteristics of the disturbed materials can wind up being notably different from the characteristics of the original,
undisturbed materials.
It is, thus, useful to know the nature of the disturbance that the materials are subject to. As a typical case in point, we look at littoral marine deposits, where we find a gravitative and mechanical selection of the finest and lightest materials and the destruction of the most fragile elements. This causes an enrichment of the heaviest and most resistant elements (lava pebbles, lapideous lapilli or scoria, crystalline fragments. etc.) which always appear smooth or, at least, softened and rounded off.
Pinning down precisely where the disturbance and, above all, later sedimentation took place is also important in reconstructing the characteristics of how the materials are positioned. Thus, for example, we know that the stratification in alluvial deposits is lenticular and variable, both vertically and laterally, for which reason we can extrapolate data from perforations only within certain limits. On the other hand, deposits in a lake or marsh might still have a certain variation vertically but, generally, will be uniform horizontally (or at least the variations will more subtle and gradual), making extrapolations that much easier. Furthermore, especially in marshes, we can predict frequent layers of humus and even peat, which have notoriously bad mechanical characteristics. Investigations in this type of terrain have to go to a greater depth than elsewhere, possibly limiting the number of core perforations.
Recognizing and distinguishing among different types of disturbed pyroclastic materials in the terrain of Naples and environs is not always easy since it entails painstaking investigations using the very latest techniques of sedimentary petrography. Also, various types of deposits are often found alternating with one another depending on the changed conditions at the sites where they are found; that is, marine or littoral deposits may come after alluvial and marsh deposits, and vice versa. For those reasons, on the 10,000:1 scale geo-technical map of the urban area that follows in the next chapter, the disturbed materials are not indicated individually; they are all represented by a single symbol.
It goes without saying that disturbed materials also include the products of erosion, the atmosphere acting on rock, whether lavas or cement-like pyroclastic materials or the artificial accumulations produced by man. These last materials, at least in the urban area, represent a fair percentage of the disturbed materials, at least down to the first few meters below the surface. Of secondary importance are those disturbed material that are not of volcanic origin; they appear sporadically, mixed in with volcanic materials and come from sedimentation around the entire Campania basin.
While this chapter was going to press, there appeared in Vol. XVI, 1966-67 of the Atti dell’Accademia pontaniana a note by A. Scherilloand E. Franco entitled “Introduzione alla carta stratigrafica del suolo di Napoli” [Introduction to the Stratigraphy of the Soil of Naples]. The authors say that this is an introduction to a more complete work to appear shortly. They have shown a very simplified statigraphy, using the classical subdivision into the three periods proposed by De Lorenzo. That version has piperno at the base of the stratigraphic column together with grey tuff and stratified yellow tuff; then, in the second period, they have yellow Neapolitan tuff and, finally, in the third period, loose products, primarily pumices and pozzolanas.
There are some substantial differences between that stratigraphy and our own (which is the one reconstructed by Rittmann and his collaborators in 1949). Theirs considers piperno as coming before all eruptions of yellow tuff and excludes the presence of yellow tuff craters in the urban area. Yellow tuff is said to have come from an eruptive center at quite a distance from the urban center; there might be some craters in the urban area that result from eruptions after those that produced yellow tuff. The most likely candidate for that would be the so-called Chiaia volcano.
As far as the stratigraphic position of piperno is concerned, the presence of re-disgorged blocks of yellow tuff in the breccia museo, not to mention the appearance of various piperno borders interlaced in the yellow tuff (for example, the piperno at via Palizzi) should be enough to prove that there are banks of yellow tuff below the piperno. As for yellow tuff volcanoes, it seems to us that at least the Chiaia volcano should be considered one of those, and we, too, think that there are still stratified yellow tuff volcanoes in the urban area that have not been discovered.
In any event, we await the appearance of the more detailed study announced by the authors, so that we may better compare their ideas to our own. We shall be quite content over the ideas that we share, since that means we have all taken another step towards understanding the subsoil of Naples.