The
rockon
which
these noteshave been
writtenoccurs as a basaltic flow in a small promontory,
on
the farside
from
Hobart, ofSandy
Bay.The
geological age of basaltic flowsand
tuffs is givenby
Mr. R.M.
Johnston (SystematicAccount
of theGeology
of Tasmania, p. 249 et seq.) as being
younger
than thetertiary leaf-beds,
and from
the occurrence of this rockand
its associates, sections ofwhich
can clearly be seenon
the
Brown's
River Road, thereseems
to beno
reason for doubting that the age ascribed is approximately correct.The
average thickness of the flow ison
the exposedsection about nine feet,and
the extent of the sheet, as far as itcan be traced, is not great. {Ihid.^ p. 281.)
This paper has
been
written rather to givean
account ofthe peculiar Petrographical character of this rock than to
attempt a description of its geological occurrence,
and
further, such
an
attemptwould
only be a trespasson
ground
already wellworked.
In the title the
name
"Fayalite Basalt" hasbeen
usedas descriptive of this rock. This
term
may
beopen
tosome
criticismwhen
we
consider the definitions givenby
the leading authorities of the
term
" Basalt."For
example,
Rosenbusch
defines basalt as a rock consistingessentially of olivine, augite,
and
plagioclase,and
regardssuch rocks as the tertiary
and
recent equivalentsof olivine,diabase,
and
melaphyre. This rock willanswer
the requirements as to geological age, but not those relating tomineralogical constituents, for in
some
seven sectionsexamined
not a trace of augitewas
discovered. Olivineexists as the redvariety Fayalite (FeO, SiOg),
and
plagio-clase felspar, probably as labradorite. This peculiarmineralogical composition involves almost a total absence
of magnesia,
and
this absence is confirmedby
chemicalanalysis, the result of
which
is given below.From
a78
"FAYALITE
BASALT."
to be justifiable.
The
terms "Dolerite," "Anamesite,"and
" Basalt " are here ap})lied respectively to the coarselytt^xtured,finely textured, but still visible to the
naked
ej'e,and
the very finely textured or microscopic varieties.This rock, then,
would
preferably be classed as a basalt asregards texture,
though
the fayalites are just visible to thenaked
eye. Briefly, therefore, this rock is a basalt inwhich
fayalite has replaced augiteand
olivine. Macros-copically, the rock is of a dark,compact
appearance;
fracture, conchoidal.
The
fayalite crystals are just visibleas small dark red spots,
which
stand out clearlyunder
anordinary
hand
lens.The
specific gravity obtainedby
weighing
in airand
water, oftwo
specimens is 2*81.According
toYon
Lasaulx the specific gravity of basalt variesfrom
2-80 to 3-00.The
following is a chemical analysis of an averagespecimen
of fragments takenfrom
the upper, middle,and
lower zones of the flow, care being taken to avoidweathered
fragments :—
SiO, ... 47-21
AI2O3 ... ... ... ... ... 16-06
Fe^Og 11-87
FeO ... ... ... ... ... 4-43
CaO ... ... ... ... ... 7-34
MgO
-12K^O
... ... 2-40Na-^O ... ... ... ... ... 7-51
Ignition Loss ... ... ... ... 2-55
Total... ... ... 99-49
From
the nature of the case, that ison
account of thegradual
merging
of different varieties of rocks, it isdifficultto state definitely a typical average analysis of Basalt, but
most
analysesshow
MgO
in considerable quantity, say,from two
or three tosevenor eight percent., andin severalanalyses of this rock only traces of
MgO
w^ere obtained.This
would
point to the olivinemineral being true Fayalite,thatis,
FeO,
SiOj.Not
havingmaterial for Specific Gravity solutions,we
were
unable to separateany
of the fayalite crystalsand
confirm this point, but trust, atsome
futuretime, to investigate thismatter,
and
bring the resultsof ourinvestigations before the Society.
•
The
following is a brief account of the microscopiccharacters displayed in thin section
by
this rock :—
The
most
striking mineralunder
the microscope is Fayalite,which
appears in crystalsand
grains of abeautifuldinal
and
cross sections.Here
and
there occur patches ofFayalite exhibiting
no
discernable crystalline outline. Inlength the crystals vary
from
()-5m.m.
downwards.
The
inclusions visible
under
a highpower
(one-sixth inch)appear to be apatite
and
needles of felspar,and
perhapsglass, though,
on
account of theirminute
dimensions, it isdifficult to obtain
good
extinctionsunder
crossed nicols.Under
crossed nicols the Fayalites exhibit the ordinaryinterference colours
and
thenormal
extinction ofrhombic
crystals. Pleochroism is not noticeable.
We
have noticed neither augite norolivine inany
of thesections examined,
and most
probably these are entirelyabsent in this rock. Apatite
was
mentioned
above asoccurring in the Fayalites. It isalso
found
hereand
therein the base as long needles of a faint violet-brown tint,
and
exhibiting pleochroismfrom
a very faint brotvn tintto a deeper violet-brown (E
>
0).On
treating a section with hydi-ochloric acid the apatites slowly dissolved out,leaving the glass slip visible underneath.
The
Fayaliteswere
also attacked,though
less rapidly.The
base consists of a ground-work
of glass, penetratedwith needles
and
fine laths of felsparrunning
in alldirections, the
whole
being thickly dusted with grainsof magnetite.
The
felspars exhibit extinction angles,varying
from
40° to 48°, which, according to Michel Levy's table for microlites, indicates a basic felspar,pro-bably labradorite or anorthite.
The
percentage of lime(7•34°/q
CaO)
in the analysis,and
also that of the alkalies,some
9°Q, point to the felspar being labradorite (in
which
the proportion of alkalies to lime is approximately one to
three)
mixed
with a little andesine orsome more
acidfelspar. This supposition is based
on
the assumption that the base is of thesame
composition as the microlitesof felspar,
—
asomewhat
doubtful hypothesis.This rock appears to
have
followed thenormal
order of consolidation,—
the apatiteand
magnetite consolidating first, then the Fayaliteand
felspars. It is difficult todetermine exactly the relation of the Faj^alite to the
felspar microlite, for, included in the Fayalite crystals,
appear thin rods,
which
insome
cases are glass, but inothers are doubtful,
on
account of the difficulty ofobtain-ing
good
extinctionsunder
crossed nicols. All the80 "
FAYALTTE
BASALT."
consolidated quickly,
and under
little pressure. Sectionswere
takenfrom
both the topand
])ottom of the flowto determine if there
was
any
difference in thesetwo
regions, but the results
were
disappointing,and
itwould
clearly require a flow of
much
greater thickness to giveany
distinct points of difference in crystallisationdue
topressure. This rock appears to stand the influence of the
weather
and
sea,and
little sign of decompositionwas
noticed in
any
of the sections,though
hereand
there, insome
of themore
weathered
sections, traces ofsome
chloritic mineralwere
seen. If occurring in larger flows itwould
no doubt
make
agood
stone for such purposes asthe foundations of buildings, road-metal, &c.
Appended
aretwo
water-colour drawings of Sections—
No. 1.
Low
power
(x 50)showing
(a) fayalite crystals ;(b) apatite crystal.
The
relative proportions of Fayaliteand
base are hereshown.
No. 2.
Shows
a fayalite crystalunder
a higherpower
(
X
300).The
small rod-like inclusions are hereshown
;also the character of the felspar microlite
and
magnetitegrains in the base.