Problem 16:
Multiple cosmic dust and Be-10 events are problematic for the
supernova theory. Five of the eight Greenland polar ice dust
samples I studied had been filtered from the ice by glaciologist
Lonnie Thompson (1977) as part
of his microparticle study and three I filtered myself from Camp
Century polar ices. In his study, Thompson had found tin-bearing
particles in 3 out of the 11 Camp Century, Greenland ice core
samples he analyzed. My study confirmed the high Sn level he
had previously observed in the 50,500 year b2k sample and also
reported high concentrations in two other samples from his collection,
(dating 38.65 and 78.5 kyrs b2k) which had levels too low for
him to detect with his electron microprobe technique. Low levels
of Sn, but again far above crustal abundance, were present in
one other sample (49.5 kyrs b2k) that I had filtered from Camp
Century ice. I also found high concentrations of iridium, nickel,
and in some cases high levels of tin, in three Antarctic polar
ice core samples, including a 31,500 year old dust band which
I have listed in Table I along with the Greenland ET dust samples
I processed as well as two samples (dating 17 and 125 kyrs b2k)
for which Thompson had reported high levels of Sn in his 1977
study. I include these two in the list as well on the assumption
that the Sn is an indicator for cosmic dust of anomalous composition.
All together these comprise 9 cosmic dust horizons additional
to the event found at the YD boundary.
This evidence of multiple past cosmic dust incursion
events raises a serious problem for the Firestone-West supernova-comet-explosion
theory. For example, six of the dust events listed in Table I
take place prior to the time of their proposed 41,000 years b2k
supernova explosion date, which leaves these earlier events unaccounted
for. Furthermore we should also add to the list of possible ET
events the beryllium-10 concentration peaks present in the Vostok
ice core record which date around 57, 64, 76, 97, 106, 117, and
133 kyrs b2k. So in all there may be at least 16 cosmic dust/cosmic
ray volley events that have occurred in the last 140,000 years.
As I pointed out in 1983, comet and asteroid impacts
occur far too infrequently to explain such multiple cosmic dust
incursion episodes (LaViolette,
1983a). Impacts by comets having a diameter of several kilometers,
the size being suggested for the YDB event, occur about once
every 30 million years unless triggered to enter by some other
galactic event, and nearby energetic supernova, as mentioned
earlier, occur less frequently than once in a million years.
The superwave theory, though, offers an appropriate explanation
for them since galactic explosions are a recurrent phenomenon.
The cores of spiral galaxies are estimated to spend approximately
15% - 20% of their time in an active cosmic ray radiating mode.
A spectral analysis study conducted by Liritzis and Grigori (1998) indicates recurrence intervals
of 5 k, 12 k, 19 k, 25 k, and 40 k years in the Vostok Be-10
record. A study conducted by Omerbashich (2006)
indicates a period as short as 3600 years may also be present.
So if these Be-10 peaks reflect times of past superwave arrivals,
it is clear that they arrive frequently enough to explain the
observed cosmic dust events.
Interestingly, one of the samples in which I found
high levels of iridium correlates with the tail end of the 40
kyrs b2k cosmic ray event and another falls at the time of the
76 kyrs b2k event. The 40 kyrs b2k correspondence may be seen
in figure 7 which compares the iridium deposition rates in these
polar ice samples to the Be-10 data of Beer, et al. Furthermore,
one should not overlook the fact that the cosmic dust influx
that occurred at the time of the megafaunal extinction also coincided
with a Be-10 cosmic ray peak, as I note below. So one can make
a good case for a connection between cosmic ray volley events
and cosmic dust incursions.
(click to enlarge)
Figure 7. Upper profiles, oxygen isotope ratio
and Be-10 concentration. Lower profile, iridium deposition
rate (data from LaViolette, 1985b,
2005a).
Problem 17:
Past cosmic dust deposition events last too long to be accounted
for by comet impacts. Another difficulty to ascribing
a comet impact origin to these past ET dust peaks is that in
some cases more than one iridium peak is found, suggesting that
the ET material influx lasted several hundred years. For example,
analysis of YDB sediments taken from Blackwater Draw, New Mexico
and Lake Hind, Manitoba show two iridium peaks, one falling close
to the AL/YD boundary and a second occurring about 200 years
later; see figure 8. The peaks are separated by 4 cm of sediment
at Blackwater and 17 cm of sediment at Lake Hind. The finding
that the upper Ir peak at the Lake Hind site has a sediment date
several hundred years younger than the peak below it gives reason
to believe that the peaks are not contemporaneous. This evidence
contradicts the claim made by Firestone et al. (2007c) that iridium
was found only at the YD boundary and neither below or above
it. If the extinction were due to a cometary explosion or impact,
only one peak should have been formed, most of the dust being
expected to settle out within a few years. Multiple peaks would
require multiple impact events with the consequent problem that
it is highly improbable that impacts would recur with such frequency.
Multiple peaks, however, do not pose a problem for the superwave
interpretation since a superwave would have pushed cosmic dust
into the solar system over a period lasting hundreds of years.
(click to enlarge)
Figure 8. Iridium concentration in sediments
from Lake Hind, Manitoba (top), and Blackwater Draw, New Mexico
(bottom); after Firestone, et al.
(2007c).
.
Additional evidence
that cosmic dust was being deposited over an extended period
of time is seen in the case of the 50.5 kyrs b2k tin dust event
registered in Greenland ice. The dust in this sample was filtered
from a 35 centimeter long ice core sample which represents an
ice accumulation time span of at least 360 years. Thompson, who
initially analyzed this sample, divided the ice core section
into 17 consecutive samples each representing about two centimeters
of core depth (~21 years) and used a Coulter counter to count
the number of particles in each sample that were greater than
0.6 microns in diameter. He found that while the particle count
varied from one increment to the next this variation for the
most part did not exceed 100% of the mean number count; see figure
9. Only one sample had a count about three times the mean value,
but this sample represented only about 15% of the particle count
for all 17 samples totaled together. This indicates that
this tin-rich dust, which was later found to be mostly of extraterrestrial
origin, was entering the Earth's atmosphere at a relatively constant
but variable rate during this 360 year period. This negates the
possibility that the dust originated from a cometary explosion
or cometary impact event. For, if it had originated in this fashion,
it should have remained airborne for no more than a few years
before settling and hence should have formed a single dust band
within a single increment of the 35 cm long section. It is reasonable
to infer that the other ice core depths containing high Sn concentrations
(discovered both in Thompson's study as well as in my own) also
involved a relatively continual dust particle influx over periods
of hundreds of years. In other words, what is evident from analysis
of the 50.5 kyr b2k event may be typical of other tin influx
events as well. So cometary impact explanations for those events
seem unlikely.
(click
to enlarge)
Figure 9. Particle count versus depth in Camp
Century, Greenland ice core sample at a depth of 1230.5 meters
dating from 50,500 years b2k. (after Thompson, 1977, p. 128)
Another important point is that microspheres were
relatively absent in the 50.5 kyr b2k dust sample. The tin-bearing
dust particles are irregular in shape and have a flat, plate-like
appearance. To maintain this shape during entry through the Earth's
atmosphere without melting into microspheres indicates that they
must have been entering at a low velocity and experienced essentially
no heating or atmospheric ablation. So while microspheres discovered
at the 12.9 kyr b2k boundary, as well as those found embedded
in PaleoIndian artifacts, might point toward the occurrence of
one or more comet explosions or impacts at that time, some other
kind of mechanism must be put forth to explain the earlier dust
events. They require a theory that explains how large quantities
of dust manage to enter the solar system in particulate form.
The superwave theory is one such theory.
Some microtektites and cosmic microspheres could have
a noncometary impact origin. Although
Firestone and West make a good case for a comet explosion origin
for the high concentration of microtektites and microspheres
observed at the YD boundary, we might venture that melted particles
of this sort discovered at the YD boundary may not all have originated
from a comet explosion/impact. Although spherules can be
produced during atmospheric heating and ablation of impacting
bodies such as meteors, comets, or asteroids, and also in the
fireball of an exploding comet, as happened in 1908 at Tunguska,
in reality, they are most commonly produced in space, not on
Earth. They can be produced when interplanetary dust particles
pass within Mercury's orbit and are melted by exposure to the
Sun's radiation. Chondrules (microspheres) found in meteorites
are also believed to be a component of cometary ice and would
be released along with the more friable cosmic dust particles
when cometary ice material is vaporized. Such vaporization may
occur either when the comet is sufficiently heated by the Sun
during its entry into the inner solar system, or in the case
of a superwave event, when a comet passes through a high intensity
region of Galactic cosmic ray radiation, as would exist in the
heliopause sheath and surrounding shock front region during a
superwave encounter. Evidence that cosmic spherules more commonly
enter our atmosphere already in spherical form, as opposed to
originating from the explosions or impacts of comets or asteroids,
is discussed in my dissertation (LaViolette,
1983a, ch. 8); download chapter
8 excerpt.
Also during this terminal Pleistocene period, when
the zodiacal cloud is theorized to have contained high concentrations
of cosmic dust, the Earth during this time would have accumulated
a dense shroud of electrically charged dust particles forming
a kind of meteoric veil (LaViolette,
1983a). Particles trapped in this veil, as well as dust particles
present in the dust conjested interplanetary environment would
have melted during exposure to the intense radiation of a major
solar coronal mass ejection (CME). We know that solar flare activity
was exceedingly high during the extinction event, as indicated
from the rapid rise in C-14 at this boundary (figure
1) and from studies of solar flare tracks in lunar rocks.
So it would have been quite possible that spherules were being
produced by very intense CMEs. If the Earth's magnetopause had
been impacted by a very large CME, temperatures in the Earth's
storm-time radiation belts could have risen high enough to melt
into spherules many of the dust particles residing in its metoeric
veil. Furthermore the shock of the CME impact and the collapse
of the geomagnetic field would have caused this spherule-bearing
dust to become precipitously deposited on the Earth's surface,
thereby creating a concentrated layer of ET bearing debris. So
a solar coronal mass ejection event could mimic a comet impact.
In discussing the YD boundary, one must also be aware
that glacier waves, floods of glacial meltwater, issuing at that
time in many places would have caused catastrophic sedimentary
deposition at this boundary resulting in sediments being stratigraphically
graded with the heavier higher density fraction concentrated
at the bottom. Thus even though metallic dust particles and spherules
may have had a history of gradual deposition over hundreds of
years, during a meltwater flood the sediments would become stratified
giving the false impression that their cosmic material fraction
had been abruptly deposited.
Helium-3 evidence also supports the superwave theory. Along a similar line, the helium-3 findings that
the YDB group sites as evidence for their comet explosion theory
need not necessarily originate from an incoming comet, at least
not all the helium-3 reported at the YD boundary. For helium-3
is a common component of interplanetary dust particles. It becomes
implanted in the particles during their exposure in space to
the solar wind. So if there was an enhanced influx of cosmic
dust at that time, one would expect to see elevated levels of
helium-3 in soil sediments as well.
Additional cosmochemical evidence that the tin particles
are extraterrestrial. Further support
of the extraterrestrial origin of the polar ice tin rich particles
came in 1984. I had sent a piece of the tin-bearing polar ice
dust to a laboratory in Australia for isotopic analysis. The
sample had previously been stored in a safe place away from radiation
sources. Three of the ten isotopes of this tin were found to
contain isotopic anomalies, the abundance ratio for one of these,
Sn-115, deviating by over three standard deviations from the
terrestrial ratio. Hence these early results provided quite strong
confirmation that the Sn was in fact of ET origin. Additional
corroboration came in 1985 when the German cosmochemist Franz
Rietmeijer (1985) announced
finding tin oxide grains in interplanetary dust particles captured
from the Earth's stratosphere. Although the Sn abundance was
not anywhere near the abundance I had reported in one of my polar
ice samples, it was nevertheless six times higher than concentrations
typically found in carbonaceous chondrites.
Claims that the tin arose from contamination were
successfully rebutted. My discovery
of volatile elements being found in polar ice dust in combination
with high levels of ET indicators challenged accepted beliefs
in the field of cosmochemistry. Previous studies on chemical
composition of extraterrestrial material were derived primarily
from analyses of meteorites. Hence any report of compositions
different from standard meteorite abundances were looked upon
with skepticism. In 1972, Hemenway, et al. reported finding unusually
high concentrations of heavy metals in submicron sized dust particles
collected from the stratosphere. But other than this, no researcher
had previously reported the presence of high concentrations of
such volatiles in cosmic dust.
As a result, my findings encountered considerable
resistance from certain conservative scientists in the cosmochemistry
community. For example, in 1988, the French geochemist Claude
Boutron published a paper in the journal Monthly Notices
questioning the validity of my polar ice cosmic dust measurements
(Boutron, 1988). He claimed
that my samples must have been contaminated since I had reported
that tin was present in many of them at substantially enhanced
concentrations. I rebutted his paper that same year (LaViolette,
1988) giving detailed reasons why sample contamination was
unlikely and arguing in support of an ET origin for the particles.
So I am quite pleased to learn that high concentrations of tin
have been discovered in YD boundary sediments alloyed with ET
markers. For this gives even more reason to believe that I have
been right in maintaining an ET origin for the tin found in polar
ice.
|