The age of the Jenolan Caves, Australia
by Emil Silvestru
The Jenolan Caves system is multi-phased with overlapping meteoric and hydrothermal
speleogenesis. Dating of this system was elusive until recently when illite from
clays assumed to be of paleokarstic origin was dated as being of Carboniferous age,
implying that the Jenolan Caves are at least of that age. However, there are serious
problems both with the karstological and dating approaches that led to this age
determination. Some sediments appear to be older than the paleokarst that hosts
them. The geomorphology, particularly the direction of the surface drainage, is
difficult to explain unless pre-existing conduits of hydrothermal origin are admitted,
which could have formed during the final stages of the Genesis Flood. The evolutionary
interpretation of the paleokarst and the sediments in it is riddled with difficulties
and leaves many basic questions unanswered. As for the dating, besides the well-known
problems with the K–Ar radiometric dating method, the particular geological
and karstological setting of the Jenolan Caves provides various sources of excess
40Ar which would yield exaggerated ages.
Location and setting
Figure 1. Outcrops of the Jenolan Caves Limestone in the Jenolan
River area. (After Osbourne4). The ‘Jenolan Caves’ are contained
mainly to the large limestone outcrop at the bottom of the diagram where road access
is provided.
The Jenolan Caves are located 175 km west of Sydney and are a major tourist attraction.
The local Aborigines knew the caves as Binoomea (Dark Places) and probably considered
them a dangerous place. In 1838 James Whalan discovered the caves as he was searching
for missing cattle, possibly stolen by the cattle thief and escaped convict James
McKeown. In fact, one of the less visited caves in the area is called McKeown’s
Hole. The initial name for the caves was Fish River Caves: the present name was
adopted in 1884 after the government of New South Wales took over the management
of the system in 1866. The name is derived from the Aboriginal for ‘high place’,
referring to the heights above the caves.1
There are nine show caves and the sum of all known passages in the caves is 22,503
m.2
The caves even provided the name for the limestones in which they are located: the
Jenolan Caves Limestone (JCL) believed to be of Late Silurian age. The JCL outcrops
as a narrow band (250 m wide) over a strike length of 5 km in the caves area, continuing
north as a series of isolated outcrops for a further 4 km, attaining a maximum thickness
of 265 m at the Caves House (figure 1).3
The dip is generally steep and quite variable, the layers being nearly vertical
in many places.
To the west, the limestone is faulted against Ordovician andesite and laminated
siliceous mudstone, whilst to the east the limestone is overlain by silicic volcaniclastics.
To the north, east and south of the caves Carboniferous granitic plutons intrude
the sedimentary sequence.3
The scientific literature about the caves is limited and leaves many significant
karstological questions unanswered.
The caves
The Jenolan Caves proper consist of interconnected passages and rooms of various
shapes and sizes, north and south of the ‘centrepiece’ of the location,
the Grand Archway. The caves on each side of this major landmark are distinctly
different: south of the Grand Archway the caves comprise a series of large dome-shaped
chambers, termed cupolas, formed by the dissolution of the limestone and interconnected
by north-south trending passages. Recent diving explorations in the Mammoth Cave,
one of the Jenolan Caves, have revealed even larger, flooded cupolas—up to
100 m high—below the water table (Daniel Cove, official cave guide, personal
communication, January 2004). There is also a large breakdown (formed by the breaking
down of the ceiling and walls) chamber, the Exhibition Chamber.3 Cupolas
are not characteristic north of the Grand Archway, where multi-level, north-south
trending passages are the norm. The northern caves contain significant amounts of
coarse alluvial sediment which does not display evidence of high velocity flow.3
One major characteristic of the caves is that they repeatedly intersect what are
believed to be paleokarstic deposits: these are deposits found in the caves that
predate the cave formation.3,4
Osborne4 has proposed karsting episodes during the Late Carboniferous,
Early Permian, Permian, Late Cretaceous, Tertiary and the Cainozoic (table 1).
Recently, the same author followed up by identifying clays inside the caves that
have been dated to the Carboniferous.3
The Jenolan Caves conundrum
Table 1. Osbourne’s4 framework chronology for
the Jenolan Caves. The number against the process indicates the number of times
it has taken place.
Existing literature acknowledges that, unlike the vast majority of documented cases,
some sections of the Jenolan Caves and caves in other karst areas in Eastern Australia
have developed along alleged paleokarst deposits which would have acted as guiding
features. Some authors like Ford5
believe that such situations are due to a different type of speleogenesis (cave
formation), namely per ascensum hydrothermal speleogenesis. Hydrothermal
solutions are driven by thermal convection through the limestone and in places have
followed pre-existing paleokarst filling. Consequently Osborne4 suggested
that at least two of his proposed paleokarsting episodes, the Early Permian and
the Late Cretaceous, were in fact hydrothermal.
There are not many cases in the karstological literature in which so many speleogenetic
phases, allegedly covering over 300 million years, have unfolded in such a small
lithostratigraphic unit. As a matter of fact, it may well be that this is the longest
overlapping speleogenesis anywhere in the world!
Osborne4 and Osborne et al.3 have pointed out that
the Jenolan Caves have a special characteristic: parallel surface and underground
drainages. The semi-dry channels of the Jenolan River and Camp Creek are closely
followed, almost bend-by-bend, by the present underground drainages. This also appears
to be the case for the paleochannels above the present rivers and previous, now
dry or sediment-filled, caves.
These unusual characteristics are part of a broader characteristic of the Jenolan
Caves and their surroundings which seems to be ignored in the literature I consulted.
The surface drainage of the Jenolan River and Camp Creek is longitudinal to the
structure in which the JCL represents a limestone bar that is, a narrow,
long limestone outcrop surrounded by non-karstic formations. In countless field
examples, such bars are cut more or less perpendicularly by the hydrographic network,
oftentimes through some of the most spectacular gorges.6 Such cases are even more characteristic when the
limestone bars were covered by other sediments in which the valleys were encased.
The Jenolan Caves area presents enough evidence to suggest that the limestone was
at some point covered by Permian conglomerates and sandstones and that valleys were
cut in those formations.
Longitudinal drainages represent a marked exception and even when they occur, the
valleys are cut along the boundary between the limestones and the adjacent rocks.
The Jenolan River and Camp Creek, however, are mostly confined within the narrow,
less than 300 m wide, limestone bar. Such a setting is most unusual and is an intrinsic
characteristic of the limestone, implying that conduits existed within the limestone
at the time it was first exposed to karsting. In other words, the limestones were
already karstified without any connection with the surface! Only one type of karsting
can achieve this: hydrothermal, per ascensum karsting.
Hydrothermal karsting
In the karstological literature ‘hydrothermal’ refers to ‘warm
water’ as against hot mineral rich magmatic emanations. There is evidence
that the same solutions can change their characteristics, dissolving rather than
depositing minerals.7 I
have referred to this type of karsting as ‘endogenous karsting’.8 Osborne3 does not
define the Jenolan Caves as hydrothermal karsting (HTK) but his attribution of pyrite
in the paleokarst fills to hydrothermal activity seems to suggest endogenous karsting
rather than thermal water activity. HTK seems to always involve two stages: 1) the
excavation of the karstic voids and 2) their total or partial filling with hydrothermal
deposits.
I have dealt extensively with HTK,9–11 especially in the context
of paleokarsts, pointing out that paleokarst features surviving over extended periods
of time in active karst areas represents a huge problem. Yet the scientific literature
I consulted seems to completely ignore that and proposes repeated, overlapping hydrothermal
and normal, meteoric karsting and speleogenesis over 300 million years, with each
phase leaving its own signature and karst network. This involves marine transgressions
which have invaded and filled the caves with layered crinoidal limestone.3,4
Yet crinoids would have not lived inside submerged caves. The notion of limestone
accumulation inside a submerged cave stretches the imagination especially in this
case where the authors have specifically emphasized the lack of calcite in the cave
samples.12 The only kind
of calcite found in these sediments is in the form of clasts coming from the host
limestone.
Figure 2. Recently cemented coarse gravel from the Thanksgiving
Cave (Vancouver Island, Canada) found in an area frequently flooded by the subterranean
stream. Note the cement-coated cobble in the centre.
I have seen recent calcite-cemented alluvia in Imperial Cave in the area where the
lower fossil cave connects to the active cave. Cemented alluvia is a common feature
in most active caves (figure 2) and I have even found it on the bottom of a flowing
subterranean stream in the cave Huda lui Papară in Romania. But such cementing
will never occur in salt water, during the submerged phase of the JCL.
In normal spelean conditions soluted calcite from the host limestone will always
end up in the cave sediments, even more so after an alleged 8 phases of karstification
covering 300 million years!
Osborne’s description of the paleokarst deposits3,4 suggests that
they are a clearly separated entity within the host limestone. As the assembly of
the JCL was submitted to HTK one would expect that all these entities—if they
predated the HTK—would have been seriously affected and not preserved untouched.
Such karsting develops by massive fronts of hydrothermal fluids ascending through
the host rock and all existing discontinuities, paleokarst being a major discontinuity.
Only meteoric speleogenesis, with passages acting as drains of infiltrated water,
would cut through paleokarstic deposits and leave the rest unaffected.
The paleofills and the associated problems
The way Osborne et al.3 present the geological and karstological
setting of JCL and the paleofills raises a series of problems if compared to other
more or less similar documented locations.
a) An overly long period of continuous karsting
Osborne et al.3 have recently dated ten primary cave paleofills
from the Jenolan Caves, as well as six surface samples, using the K–Ar method
on illite, and in one case dating cave clay, using the fission track method on zircon
grains. The ages yielded cover the interval from the Devonian (Emsian) to Middle
Jurassic (Bathonian) with the majority of cave samples falling within the Carboniferous-Permian,
from the Tournaisian to the late Ufimian, roughly 100 million years. This implies
that the JCL has been submitted to karsting for all of that time. Using the existing
measured karst denudation rate (KDR) in New South Wales, namely 24 mm ka-1 in the Coleman Plains,12 at least 2.4
km of limestone would have to be removed during this period. Though not clearly
specified in the texts, it appears that even the earliest alleged paleokarst features
are similar to the most recent ones, which are controlled by the nearly vertical
bedding planes. This seems to imply that the tilting of the JCL occurred in the
earlier stages of the Variscan Orogeny, hence the 2.4 km of limestone would not
have been removed from a more or less horizontal structure but from a nearly vertical
one.
Adding the other postulated karsting phases and assuming a similar KDR, the total
height of that limestone bar would have been at least double. For the sake of a
simpler argument, let us assume that for all the rest of the Carboniferous—nearly
100 Ma—the JCL was covered by other sediments which are now completely missing.
This would be very difficult to prove and even more difficult to admit in a karstological
context. Shaw and Flood (1993), quoted by Osborne et al.,3 believe
that up to 5 km of rock was removed from the Lachlan Fold Belt, of which the JCL
is part, during the Late Carboniferous! That means that the assumed removal of limestone
was not due to karsting but to some other, more energetic erosional episode.
Assuming the Late Carboniferous lasted for a maximum of 33 Ma, the erosional rate
would have been 150 mm ka-1, much higher than any measured KDR. Obviously,
if the period was shorter, the erosion rate would have been even more intense. Under
such circumstances karsting processes would have been extremely intense and would
have left much more visible landmarks than the ones found in the field. Also, the
issue of longitudinal drainage as mentioned above becomes even more problematic
since now we have to account for the preservation of a preferential drain in a very
narrow band of rock for 360 Ma whilst the regional erosion has eroded away all other
formations. A series of perpendicular gorges cutting the limestone bar would be
a much more appropriate interpretation.
b) An unreasonably deep burial
Based on the assumptions above, one can infer that the portions of the JCL that
are exposed today would have been buried at the time of the Late Carboniferous to
at least 5 km depth at which low grade metamorphic features should be present. I
find it very difficult to believe that karsting, even as HTK, could have occurred
at that depth without voids being constantly compressed leaving no room for infills.
It therefore seems very unlikely that the ages determined for the clays could fit
any known karsting scenario.
Timing discrepancies
Osborne et al.3 make no reference in their text to the discrepancy
between the timing of karsting/speleogenetic phases as shown in table 1 and the
span of the alleged ages the radiometric dating has yielded. Thus it is assumed
that the first meteoric karsting phase occurred in the Late Carboniferous, yet the
oldest karst filling is dated to the Early Carboniferous (Tournaisian) and is hydrothermal!
So when and how did those infilled karst voids form? Invoking a Devonian karsting
episode does not really work in the general context of their paper because one of
the cave samples was dated as Devonian. This represents a different type of clay
filling in a joint-like feature, unlike the true karstic samples dated as Carboniferous.
Their paper provides no answers, merely listing them as topics for further research.
The K–Ar dating method: more problems
This method is based on the decay of 40K, with a half life 1.39 x 109
years13,14 to 40Ar. The problems with using 40K–40Ar have been frequently described. Austin has dealt in detail
with the excess of 40Ar in dacite in a lava dome on Mount St Helens
formed in 1986 and which yielded a K–Ar age of 0.35 ± 0.05 Ma.15 The reason for this is
inherited argon from the magma itself which was incorporated in the phenocrysts
while they were formed. In the Jenolan Cave situation the mineral dated was illite,
a phyllosilicate with three layers very similar in structure to muscovite.
As mentioned before, Osborne4 proposes at least two hydrothermal speleogenetic
phases. The dated illite is believed to come from in situ alteration so
that the radiometric dates represent the age of the hydrothermal alteration rather
than the age of the altered mineral. Under such circumstances, no sample should
be dated earlier than the Late Cretaceous, the age of the last alleged hydrothermal
phase.
Recent research16 has
also revealed another source of Ar in pure authigenic, recent to present-day smectite
from Pacific sediments:
‘ … excess 40Ar, which represents radiogenic 40Ar released from nearby altered silicates, might be temporarily adsorbed at the
surface of the rock pore spaces and is therefore available for incorporation in
nucleating and growing particles’.
In other words radiogenic Ar produced in adjacent rocks can easily contaminate secondary
illite; the higher the 40Ar contents, the older the sample is supposed
to be. It is interesting to notice that Osborne et al.3 make
no reference to possible sources of 40Ar contamination. Yet one sample
dated to 167.12 ± 3.60 Ma, which corresponds to the Middle Jurassic (Bathonian),
is described as ‘weathered andesite’ from ‘Mesozoic dykes’:
however, these dykes are not shown on their map. This could well be a possible source
of excess Ar within the JCL itself.
In addition to this, this paper presents many other magmatic formations in the areas
adjacent to the Jenolan Caves: Early Devonian volcanics, Carboniferous granite and
Carboniferous basic intrusions.
It is very difficult to believe that with so many close sources of contamination,
all the 40Ar in the dated samples comes from the decay of 40K in these same samples! Therefore it is perfectly reasonable to question the Carboniferous
age of the cave sediment samples.
A simpler scenario
A simpler solution to all of these problems can be proposed: there weren’t
eight speleogenetic/karsting phases during 300 Ma. The majority of Jenolan Caves
were formed by hydrothermal karsting in four stages11 from the final
moments of the Genesis Flood to the present.
In stage 1, while the limestone was still submerged, hydrothermal solutions (HTS)
produced during the paroxysmal stages of the Genesis Flood, were ascending through
the crust causing rapid diagenesis.11 Locally, as diagenesis depleted
the mineral contents, the same solutions became aggressive, dissolving the rocks
they helped create. Such situations have been recorded in the case of hydrothermal
metasomatic ore deposits.7 Though still en masse, the circulation
of these aggressive solutions was partly controlled by the textural and structural
features of the newly-formed JCL. The larger karstic halls and cupolas connected
by large conduits were formed by such solutions. As the solutions were more aggressive
at depth, the size of the karstic voids should increase with depth, which is exactly
what explorations at the Jenolan Caves have revealed. This runs counter to a meteoric
speleogenesis.
In stage 2, during the recessive stage of the Genesis Flood,17 the entire sedimentary sequence emerged from the
sea and was tilted, the JCL being still covered by massive non-karstic deposits.
The HTS activity changed, the convectional per ascensum movement being
gradually replaced by a gravitational per descensum flow. This flow was
controlled by the structural features of the limestone. Confined between non-karstic
deposits, in its search for an outlet, the drain became mostly longitudinal. The
lack of cupolas north of the Great Archway suggests that the drain was from the
north towards the south, along large passages with some of the cupolas becoming
temporary collectors. The large amounts of HTS and the increased pressure resulted
in a dramatic acceleration of the karsting processes, the cupolas and halls rapidly
growing in size. Many authigenic sediments, mainly clay minerals from the insoluble
fraction in the dissolved limestone, were generated during this time and they travelled
extensively through the system, being trapped and rapidly cemented in what we could
call ‘hydrodynamic traps’—lateral, calmer passages.
During stage 3, erosion brought the JCL to the surface. By this time most of the
HTS in the system were chemically dampened as the supply from inside the crust had
practically ceased. At some point the fluid-filled system was opened by erosion
and the fluids rapidly drained. The longitudinal north-south subterranean drain
was thus made available not only to infiltrating water from the surface but also
to surface streams which were pirated by this ready-made drainage system.
Surface erosion would have eventually reached some of these drains, causing ceiling
collapse and turning the passages into surface river channels. Thus the Jenolan
River and Camp Creek were formed, preserving segments of the old conduits and even
erosional ledges paralleling the remaining subterranean drains. This pre-existing
drain was already so deeply entrenched that it ran and still runs counter to the
normal hydrographic trends for a limestone bar geomorphic setting.
The upper chambers and conduits that were partially or completely drained were reached
by infiltrating water which was probably much more aggressive than it is today due
to the abundance of organic materials in the adjacent Flood-laid sediments. As a
result, speleothems started growing very quickly.
Stage 4 corresponds more or less to the present conditions; no HTS are present.
Meteoric speleogenesis reshaped the existing voids and surface erosion further dissected
the cave system of the Jenolan Caves, leading to the present complex setting. The
constant decrease in precipitation and consequently the reduced flow in the subterranean
drain have left many of the passages dry. The deep, below water table, cupolas had
their fluids gradually replaced by the infiltrating water, with many of these large
reservoirs acting today as annexes to the main drain.18
Conclusions
Though recently hailed as the world’s oldest (340 Ma) open cave system, the
Jenolan Caves system can be explained as the result of hydrothermal karsting during
the final stages of the Noahic Flood
Though recently hailed as the world’s oldest (340 Ma) open cave system,19 the Jenolan Caves system
can be explained as the result of hydrothermal karsting during the final stages
of the Noahic Flood, subsequently reshaped and disorganized by meteoric speleogenesis
and surface erosion.
The standard evolutionary interpretation of the complex cave system assumes no less
than eight speleogenetic phases including both meteoric and hydrothermal activity.
This leads to many problems, discrepancies and unanswered questions.
Clay sediments in alleged paleokarst dissected by the cave passages have been dated
by the K–Ar method as Carboniferous. However, the K–Ar method is notoriously
error-prone, contamination being the most important issue. The geological and karstological
situation in the area provided abundant sources of contamination which could have
easily led to an excess of 40Ar and consequently exaggerated ages. In
an attitude that has been consistent for many years now, radiometric dating prevails
over logic, geomorphology and karstology. It seems that the accelerated return of
neo-catastrophism in geology is being compensated by a desperate quest for antiquity
of landscapes, both surficial and subterranean, and Australia has long been a first
stage for this quest.
Related articles
Further reading
Recommended Resources
References
- Jenolan Caves, <en.wikipedia.org/wiki/Jenolan_Caves>,
19 December 2006. Return to text.
- Gulden, B., World’s longest caves, 25 October 2006,
<www.caverbob.com/wlong.htm>, 19 December 2006. Return to text.
- Osborne, R.A.L., Zwingmann, H., Pogson, R.E. and Colchester,
D.M., Carboniferous clay deposits from Jenolan Caves, New South Wales: implications
for timing of speleogenesis and regional geology. Australian J. of Earth Sci.
53: 377–405, 2006. Return to text.
- Osborne, R.A.L., The Origin of Jenolan Caves: Elements of
a New Synthesis and Framework Chronology. Proc. Linn. Soc. NSW, 121:1–27,
1999. Return to text.
- Ford, T.D., Some thoughts on hydrothermal caves. Cave
and Karst Science 22(3):107–118, 1995.
Return to text.
- Cocean, P. and Silvestru, E., The Role of Magmatism in the
Genesis of Isolated Massifs Karst Relief of the Trascau-Metaliferi Mountains. Travaux
de l’Institut de Spéléologie ‘Emil Racovitza’,
Bucuresti, XXVII:89–93, 1988. Return to text.
- Mârza, I. and Silvestru, E., First Mention of the Hydrothermal
Karst Phenomenon Associated to Neogene Metasomatic Suplhide Ore deposits from Rodna
Veche. Studia Universitatis ‘Babes-Bolyai’, Geologica-Geographica
Cluj-Napoca XXXIII:77–81, 1988. Return to
text.
- Silvestru, E., Propositions pour une classification litho-génétiquedes
formes karstiques et apparentées. Karstologia, La Rivoire, France.
Nr. 15:55–57, 1990. Return
to text.
- Silvestru, E., Paleokarst—a riddle inside confusion,
Journal of Creation 14(3):100–108, 2000.
Return to text.
- Silvestru, E., The riddle of paleokarst resolved, Journal
of Creation 15(3):105–114, 2001. Return
to text.
- Silvestru, E., A Hydrothermal Model of Rapid Post-Flood Karsting,
Proc .5th Internat. Conf. Creationism, Creation Science
Fellowship Inc., Pittsburgh, PA, pp. 233–241, 2003. Return
to text.
- Osborne et al., ref. 3, pp. 391–392.
Return to text.
- Jennings, J.N., The Blue Waterholes, Coleman Plains, NSW,
and the Problem of Karst Denudation Rate Determination, Trans.Cave.Res.Gp.G.B.
14:109–117, 1972. Return to text.
- Pilot, J., Les isotopes en géochimie (Méthodes
et applications), Doin, Editeurs, SA, Paris, p.15, 1974. Return
to text.
- Austin, S.A., Excess Argon within Mineral Concentrates from
the New Dacite Lava Dome at Mount St Helens Volcano, Journal of Creation
10(3):335–343, 1996. Return to text.
- Clauer, N., Towards an isotopic modeling of the illitization
process based on data of illite-type fundamental particles from mixed-layer illite-smectite,
Clay and Clay Minerals 54(1):116–127, 2006.
Return to text.
- Walker, T., A biblical geologic model, Proc.3rd
Internat.Conf.Creat., Creation Science Fellowship Inc., Pittsburgh, pp.
581–622, 1994. Return to text.
- Mangin, A., Contribution a l’étude hydrodinamique
des aquifères karstiques. Thèse Doct. Sci. Nat. in Annales de Spéléologie
29(3):283–332; 29(4):495–601;
30(1):21–124, 1975. Return to text.
- Jenolan Caves 340 million years old, 26 July 2006, <news.ninemsn.com.au/article.aspx?id=117074>,
19 December 2006. Return to text.
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