PLEASE NOTE:
*
CCNet 78/2001 - 13 June 2001
---------------------------
"Two centuries since the first asteroid, Ceres, was spotted,
space
rocks are becoming identified as forces that mould our planet,
wiping
out species or crowning them, in a brutal act of death and
creation."
--Agence France-Press, 9 June 2001
(1) ASTEROIDS CAST AS THE BRINGERS OF DEATH - AND LIFE
Andrew Yee <ayee@nova.astro.utoronto.ca>
(2) NEWLY-FOUND METEORITE MAY POINT TO WATER UNDER MARTIAN
SURFACE
Andrew Yee <ayee@nova.astro.utoronto.ca>
(3) CONES ON MARS
Andrew Yee <ayee@nova.astro.utoronto.ca>
(4) WIND BLOWS WEST ON TITAN
Andrew Yee <ayee@nova.astro.utoronto.ca>
(5) ASTEROIDS 2001
Andy Smith <astrosafe@yahoo.com>
(6) 10TH ANNIVERSARY OF THE ERUPTION FELT AROUND THE WORLD
Mark Hess <mhess@pop100.gsfc.nasa.gov>
(7) ARTHUR C CLARK STANDS BY HIS BELIEF IN LIFE ON MARS
Space.com, 7 June 2001
(8) 100KM CIRCULAR FEATURE OFF THE COAST OF VIETNAM
Peter Haines <Peter.Haines@utas.edu.au>
(9) WELCOME TO SLOAN AND SUBARU
Andy Smith <astrosafe@yahoo.com>
(10) IMPACTS & TSUNAMI
Worth Crouch <doagain@jps.net>
(11) MULTIPLE IMPACTS AT THE TR/J EXTINCTION BOUNDARY?
Hermann Burchard <burchar@mail.math.okstate.edu>
(12) 2300BC CATASTROPHE
Alasdair Beal <a.beal@btinternet.com
>
=============
(1) ASTEROIDS CAST AS THE BRINGERS OF DEATH - AND LIFE
From Andrew Yee <ayee@nova.astro.utoronto.ca>
From Agence France-Presse, 9 June 2001
http://asia.dailynews.yahoo.com/headlines/technology/afp/article.html?s=asia/headlines/010609/technology/afp/Asteroids_cast_as_the_bringers_of_death_--_and_life.html
Saturday, June 9, 2001, 12:27 AM EDT
Asteroids cast as the bringers of death -- and life
PARIS (AFP) -- Two centuries since the first asteroid, Ceres, was
spotted,
space rocks are becoming identified as forces that mould our
planet, wiping
out species or crowning them, in a brutal act of death and
creation.
It is popular knowledge that an asteroid or comet slammed into
modern-day
Mexico around 65 million years ago, leaving behind a gigantic
crater and
extinguishing much of the life on Earth, notably ending the long
reign of
the dinosaurs.
But it is now clear that this was not a one-off. Scientists have
evidence of
four other cataclysms that have occurred over the last quarter of
a billion
years, and conclude that space plays a key role as kingmaker of
the species.
A study published last month by University of Washington
paleontologist
Peter Ward suggests a mass extinction suddenly occurred 200
million years
ago, destroying the mammal-like reptiles that dominated the
planet and
handing the throne to T. rex and his ilk.
"Something suddenly killed off more than 50 percent of all
species on Earth,
and that led to the age of the dinosaurs," says Ward.
His team's research is based on a count of fossilised marine
plankton that
died en masse because of rapid climate change. Ward suggests
asteroid impact
was the likely cause but does not rule out other factors, such as
a surge of
volcanic activity.
In their hurtling track around the Sun, comets or big asteroids,
say 10
kilometers (six miles) across, can unleash enormously destructive
energy if
they smack into the Earth.
They can release a shockwave equal to thousands of Hiroshima
bombs and kick
up a dust cloud that is borne by winds around the planet,
filtering out the
sunlight and changing weather patterns.
In this "impact winter," plants shrivel and die from
lack of photosynthesis,
denying food to life farther up the food chain. The extinction
studied by
Ward occurred in less than 10,000 years, "the blink of an
eye, geologically
speaking."
Benny Peiser, a social anthropologist at Liverpool John Moores
University,
says the emerging importance of asteroids as changers of
planetary life
poses a challenge to evolutionists.
Man, he argues, rose not as a gradual process of selective
fitness and
genetic supremacy but simply because he was lucky.
"The reason that Homo sapiens have survived in spite of
these global
disasters has little to do with the traditional explanations
given by
neo-Darwinists," says Peiser.
"It is sobering to realise that we are alive due to cosmic
luck rather than
our genetic makeup. After all, the populations of hominids and
early modern
humans were extremely small. Had any of these impacts occurred in
the
proximity of these population groups, we might also have gone the
way of the
dodo."
For all their destruction, asteroids may also have provided the
seed for
life on Earth billions of years ago, according to some minds.
Under this "panspermia" theory, asteroids or a comet
delivered the chemical
building blocks for DNA when the planet was in its infancy.
Testing the idea, astrobiologist Louis Allamandola of NASA's Ames
Research
Center froze a mixture of ice, carbonated gas, carbon monoxide,
ammonia and
methanol at temperatures nearing absolute zero.
He then bombarded the chilly soup with ultraviolet rays, seeking
to
replicate the conditions in the dense interstellar clouds in
which the Solar
System was born.
Complex, diverse molecules were created. And when water was added
to the
mixture, some of the solids spontaneously formed pouch-like
membranes that
converted energy from ultraviolet light into visible light,
necessary to
create life.
Panspermia is still struggling to rise above the "giggle
threshold" -- the
point at which a new theory is no longer considered ludicrous and
is widely
accepted in mainstream thinking.
But the same used to apply to the threat of asteroid collision,
which was
considered outlandish three or four decades ago.
That risk, while mathematically minute, is now pushing the United
States,
Britain and other countries to step up monitoring of galactic
bruisers and
prompt thinking about how any threatening rock could be nudged
aside or
destroyed.
Mankind's ambivalence towards asteroids was spelt out last year
by a
government-appointed British panel, the Task Force on Potentially
Hazardous
Near Earth Objects, which urged closer international cooperation
to detect
large rocks.
"As a species, humans would not exist without them. On the
one hand we can
rejoice in them; on the other, we can fear for our future."
Copyright © 2001 Agence France-Presse. All rights reserved.
============
(2) NEWLY-FOUND METEORITE MAY POINT TO WATER UNDER MARTIAN
SURFACE
From Andrew Yee <ayee@nova.astro.utoronto.ca>
[ http://sg.news.yahoo.com/010612/1/vuiy.html
]
Tuesday June 12, 12:05 PM EDT
Newly-found meteorite may point to water under Martian surface
PARIS (AFP) -- A meteorite found in the western Sahara contains
water that
may have come from below the surface of Mars, French researchers
said
Tuesday.
The rock, weighing 104 grammes (three and a half ounces), was
discovered by
French meteorite hunters last December.
It is the fourth meteorite to be identified as a nakhlite, a
Martian
mineral, the National Institute for Sciences of the Universe
(INSU) said,
confirming a report in the daily Le Monde.
INSU scientists carried out research into the ratio of deuterium
and
hydrogen in the meteorite, a figure which varies according to
whether the
rock was exposed to water and indicates the origin of that water.
Analysis of the three other nakhlites showed that they had been
exposed to
water, but which was on the planet's surface.
However, the new meteorite, NWA 817, was different.
"We detected a very low deuterium/hydrogen ration, close to
a reading for
Earth," INSU Director Philippe Gillet told Le Monde.
"Our interpretation is that this points to a fluid that came
from the
planet's interior, not its surface."
Gillet did not rule out the possibility that the meteorite may
have been
contaminated by water molecules when it landed on Earth.
"However, if we are right, that means part of the water
contained in the
Martian mantle did not rise to the surface of the planet,"
he said.
Whether water, the stuff of life, exists or has existed on Mars
has excited
enormous debate since NASA's Mars Global Surveyor orbiter sent
back pictures
a year ago, showed Martian valleys and gullies that some US
analysts believe
were dug out by ice flows, floods or even oceans.
Where the water is now is another question, with speculation that
it has
entirely evaporated into space or may still linger just below the
surface.
Martian meteorites are believed to have been knocked off the
surface of the
planet by an asteroid collision millions of years ago. The chunks
wandered
in space until they were finally drawn into the Earth's gravity
and made
landfall, surviving a fiery plunge through the atmosphere.
NWA 817's finders were Bruno Fectay and Carine Bidaut, who have
discovered
more than 400 meteorites.
One of the finds, a Martian rock named NWA 480, was sold to the
National
Centre for Space Studies (CNES), where it is being put to use to
prepare for
planned missions to Mars.
Copyright © 2001 Agence France-Presse. All rights reserved.
===========
(3) CONES ON MARS
From Andrew Yee <ayee@nova.astro.utoronto.ca>
[ http://www.nature.com/nsu/010614/010614-3.html
]
Monday, 11 June 2001
Cones on Mars
By TOM CLARKE
Cones poking out from the surface of Mars could be evidence for
recent water
ice on the red planet -- this time just beneath some of the most
parched
regions of its rocky terrain [1].
High-resolution images of an area the size of Canada taken by the
Mars
Orbiter Camera reveal what appear to be rootless cones. These
geological
formations are found on Earth where molten lava has flowed over
waterlogged
ground.
The images show vast fields of the objects, which can measure
between 20 and
300 metres across at the base. But unlike ordinary martian
volcanoes, the
cones are not associated with rock fissures.
The location of the cones, in Mars' equatorial region, is
"rather
disturbing", says Peter Lanagan of the Lunar and Planetary
Laboratory at the
University of Arizona in Tucson who carried out the work. It
suggests water
was present "in an area of Mars where we don't expect to see
water", he
says. Most distribution models predict that water occurred only
around Mars'
poles.
Drawing geological analogies between Earth and Mars "can be
a dangerous
game", cautions John Mustard, who studies martian climate at
Brown
University in Providence, Rhode Island. But the shape and
location of the
cones make the analogy probable, he concedes, indicating that
there might
well have been water around the equator.
Rootless cones are so called because they are not produced by
lava erupting
through cracks in surface rock. On Earth, they form when hot lava
flows over
damp ground causing the water beneath to boil. The water flashes
to steam
very quickly fuelling an explosive release of lava upwards, which
builds a
cone.
The cones on Mars occur in an area that was flooded by lava
within the past
10 million years and where there are channels hinting at the
presence of
water before then. This suggests that water was present when the
lava flowed
across.
"Although 10 million years ago sounds like a long
time," says Lanagan, "for
people studying Mars that's recent." Water was thought to
have evaporated
from equatorial Mars hundreds of millions of years ago.
The big question, says Mustard, "is whether that reservoir
of water is still
there".
Martian researchers may not have to wait for too long for
confirmation.
NASA's Mars Odyessy mission en route to Mars is equipped with a
gamma-ray
spectroscope that will look for the signature of hydrogen atoms
in water
ice.
[1] Lanagan, P. D., McEwen, A. S., Keszthelyi, L. P., &
Thordarson, T.
Rootless cones on Mars indicating the presence
of shallow equatorial
ground ice in recent times. Geophysical
Research Letters 28, 2365-2367
(2001).
© Macmillan Magazines Ltd 2001 - NATURE NEWS SERVICE
===========
(4) WIND BLOWS WEST ON TITAN
From Andrew Yee <ayee@nova.astro.utoronto.ca>
[ http://www.nature.com/nsu/010614/010614-5.html
]
Tuesday 12 June 2001
Wind blows west on Titan
By CORIE LOK
Gale-force winds on Titan, Saturn's largest moon, blow from west
to east,
researchers have now discovered [1]. Knowing which way the winds
blow should
help international space agency scientists in their plans to land
a probe on
the icy moon in 2004.
Using the 3-metre-wide Infrared Telescope Facility on Mauna Kea,
Hawaii,
Theodor Kostiuk of the NASA Goddard Space Flight Center in
Greenbelt,
Maryland, and his colleagues found that the winds some 200
kilometres above
Titan's surface were blowing at tornado speeds of about 750
kilometres per
hour.
Not knowing the direction of the winds complicated plans by NASA
and the
European Space Agency (ESA) to explore Saturn, its rings and its
17 moons,
including Titan. Launched in 1997, ESA's 350-kilogram Huygens
probe will
parachute in from NASA's 2-tonne Cassini orbiter.
The probe will beam data about Titan's clouds, atmosphere and
surface to
Earth via the Cassini spacecraft orbiting above. Knowing the wind
direction
will help NASA and ESA to predict the probe's path as it descends
through
Titan's thick, smoggy atmosphere. They can then point Cassini's
antenna more
precisely towards the probe as it lands.
Huygens' batteries will last only 153 minutes, and so it is
important to
maximize the contact between the orbiter and probe to gain as
much
information as possible from Titan's surface.
But these measurements of Titan's stratospheric wind are at only
one height.
It "tells us nothing about what's going on below, where
Huygens will spend
most of its time", warns Michael Bird of the University of
Bonn in Germany,
leader of an experiment the probe will carry out to investigate
wind on
Titan's surface. "We have to be there to see which way the
wind is blowing,"
says Bird. "We're ready for surprises."
To measure Titan's wind, Kostiuk and his team used a technology
analogous to
that used by police to detect speeding drivers. A police officer
sends out a
signal of a specific frequency; this frequency changes as it
bounces back
from a moving car, and the change is dependent on the car's
speed.
The telescope and other equipment detected infrared light emitted
by gaseous
ethane in Titan's upper atmosphere. The speed and direction of
the moving
ethane molecules altered the frequency of the infrared light.
Thus, by
comparing the frequencies from the eastern and western edges of
Titan, the
researchers calculated which way, and how fast, the wind was
blowing.
Now they plan to confirm their results using a larger, 8-metre
telescope
that will cut down on the noise from space.
Titan, the second-largest moon in the Solar System, and about 40%
of the
size of Earth, interests astrophysicists because its conditions
probably
resemble those of Earth before the appearance of life.
Says Caitlin Griffith, a Titan researcher from Northern Arizona
University:
"To understand how Earth evolved, we need to investigate how
atmospheres
function in a variety of contexts: Titan provides us with such
insights."
[1] Kostiuk, T. et al. Direct measurement of winds on Titan.
Geophysical
Research Letters 28, 2361-2364 (2001).
© Macmillan Magazines Ltd 2001 - NATURE NEWS SERVICE
=============
(5) ASTEROIDS 2001
From Andy Smith <astrosafe@yahoo.com>
Hello Benny and CCNet,
The Palermo meeting, sponsored by SPACEGUARD, NEODyS et al, is
being
outlined on the TUMBLING STONE e-publication. Your can find it
on:
http://spaceguard.ias.rm.cnr.it/tumblingstone/main.htm
The meeting started yesterday and continues until the 16th. Lots
of good
presentations on asteroid optical and radio astronomy and they
are making a
real effort to communicate.
The ASTEROIDS 2001 (Palermo) meeting abstracts can be seen at:
http://www.astropa.unipa.it/Asteroids2001/Programme.html
ASTEROIDS 2001 (SCIENTIFIC PROGRAMME)
http://www.astropa.unipa.it/Asteroids2001/Programme.html
Monday, June 11
09.00 - 09.30 Opening ceremony
SESSION I HISTORY
Chairs: R. Binzel and V. Zappala'
09.30 - 09.55 G. Fodera' Serio (Invited) History of
the Palermo
Observatory and the discovery of Ceres
10.10 - 10.35 B. Marsden (Invited) The asteroid
discovery rate: historical
perspective and future outlook
10.50 - 11.15 Coffee Break
SESSION II GROUND-BASED OBSERVATIONS: TECHNIQUES AND REPORT
OF RESULTS
Chair: B. Marsden and I. Belskaya
11.15 - 11.25 M.E. Sansaturio, A. Milani On asteroid
identifications: the
algorithms and the computational procedure
11.30 - 11.40 L.K.Kristensen Follow-up ephemerides
and the accuracy of
preliminary orbits
11.45 - 11.55 D.F. Lupishko, V.G. Shevchenko, N.
Tungalag On the
displacement of asteroid photocenter due to the surface
scattering
12.00 - 12.10 J. Ticha, M. Tichy, M. Kocer The
recovery as an important
part of NEA astrometric follow-up
12.15 - 12.25 A. Boattini, G. D'Abramo NEO follow-up
coordination
activities of the spaceguard central node: results and general
recommendations
12.30 - 13.00 S.J. Ostro (Invited) Radar observations
of asteroids:
progress and perspectives
13.00 Lunch
15.00 - 15.10 M.C. Nolan, J.L. Margot, E.S. Howell, L.
Benner, S.J. Ostro,
et al. Near-earth asteroids observed using the post-upgrade
Arecibo
planetary radar
15.15 - 15.25 L.A.M. Benner, M.C. Nolan, J.L. Margot et
al Recent radar
observations of four near-earth asteroids
15.30 - 15.40 D.J. Scheeres Dynamical constraints on
asteroid binaries
15.45 - 15.55 J.L. Margot, M.C. Nolan, L.A.M. Benner, S.J.
Ostro, M.E.
Brown, E.S. Howell, R.F. Jurgens et al Discovery and
characterization of
three binary asteroids 2000 DP107, 2000 UG11, and 87 Sylvia
16.00 - 16.10 C. Magri, S.J. Ostro, L.A.M. Benner, B.R.
Beeney Radar
constraints on asteroid composition using 433 Eros as ground
truth
SESSION III SPACE-BASED OBSERVATIONS
Chairs: D. Lupishko and M.A. Barucci
16.15 - 16.40 A. Cheng (Invited) Eros: The NEAR
mission and results
16.55 - 17.20 Tea Break
17.20 - 17.30 D.W. Dunham, R.W. Farquhar, J.V McAdams et
al Implementation
of the first asteroid landing
17.35 - 17.45 B.E. Clark, P. Helfenstein, J.F. Bell III et
al Space
weathering on Eros: constraints from albedo and spectral
measurements of
Psyche crater
17.50 - 18.00 D.E. Smith, M.T. Zuber Comparison of
imaging and altimeter
shape models for 433 Eros
18.05 - 18.15 J. Trombka, L.R. Nittler, D.Starr et al
Elemental analysis
of 433 Eros; results from the near X-Ray/Gamma-ray
spectrometer
18.20 - 18.30 D. Hestroffer; P. Tanga; J. Berthier; A.
Cellino; M.
Lattanzi; M. Di Martino and V. Zappalą HST/FGS
interferometric observations
of asteroids
18.35 - 19.35 POSTER SESSION SESSIONS I, II and
III
Tuesday, June 12
09.00 - 09.25 C.R. Chapman (Invited) Impact and
cratering history of
asteroids
09.40 - 09.50 M.T. Zuber, D.E. Smith, A.F. Cheng., J.B.
Garvin and the NLR
science team Physical structure and dynamics of 433 Eros
from NEAR-
Shoemaker altimetry and gravity
09.55 - 10.05 R.Sullivan, P. Thomas, S. Murchie, M.
Robinson Asteroid
geology from Galileo and
NEAR data
10.10 - 10-20 I. Richter, K.H. Glassmeier, F.Kuhnke, G.
Musmann et al
Magnetometer observations during the Flyby of the DEEP SPACE 1
spacecraft of
the asteroid Braille
10.25 - 10.35 E. Dotto, M.A. Barucci, T. G. Mueller et
al ISO observations
of asteroids
10.40 - 10.50 S.D. Price, M.P. Egan Space-based
infrared characterization
of asteroids
10.55 - 11.20 Coffee Break
SESSION IV DYNAMICAL STRUCTURE AND ORIGIN
Chairs: A. Milani and W.B. Bottke
11.20 - 11.45 A. Morbidelli (Invited) Dynamical
structure of the asteroid
belt
12.00 - 12.10 J. Spitale, R. Greenberg
Finite-different calculations of
the general Yarkovsky effect
12.15 - 12.25 A. Shukolyukov, G.W. Lugmair Chronology
of asteroid
accretion and differentiation
12.30 - 12.40 V. Carruba, J. A. Burns, W. B. Bottke
Dynamical scattering
of asteroid families
12.45 - 12.55 W. Bottke, D. Vokrouhlicky, M. Broz, A.
Morbidelli
Yarkovsky-assisted escape of kilometer-sized asteroids from the
main belt
13.00 Lunch
15.00 - 15.10 W.R. Ward Early erosion of the asteroid
belt
15.15 - 15.25 O. Manuel Compositional variations in
asteroids: a record of
the early solar system
15.30 - 15.40 M. Nagasawa, S. Ida, H. Tanaka Orbital
excitation of
asteroids during depletion of a protoplanetary disk
15.45 - 15.55 D. Nesvorny, A. Morbidelli, D. Vokrouhlicky,
B. Bottke, M.
Broz The Flora family: a case of the dynamically dispersed
collisional
swarm ?
SESSION V COMPOSITION AND PHYSICAL STRUCTURE
Chairs: K. Muinonen and E.S. Howell
16.00 - 16.25 P.Pravec, A.W. Harris USA Asteroid
rotations
16.40 - 16.50 I.N. Belskaya, V.G. Shevchenko
Photometry and polarimetry of
main-belt asteroids: main features and correlations
16.55 - 17.20 Tea Break
17.20 - 17.30 K.S. Jarvis, A.L. Cochran, M.S. Kelley, F.
Villas More
Vesta, more Vestoids: New spectra and their significance for
parent body
composition
17.35 - 17.45 E.S. Howell, A.S. Rivkin, F. Vilas
Uneven distribution of
aqueously altered minerals on asteroids
17.50 - 18.15 S.J Bus (Invited) Spectroscopic and
taxonomic
characterization of asteroids
18.30 - 19.30 POSTER SESSION SESSIONS IV, V and
VI
Wednesday, June 13
09.00 - 09.10 R.P. Binzel Physical properties of
Near-Earth objects: an
overview
09.15 - 09.25 A.W.Harris, DLR Berlin The albedos and
taxonomy of small
asteroids
09.30 - 09.40 L.V. Moroz, A.V. Korochantsev, R. Waesch, G.
Arnold Surface
color variations of dark asteroids and other low albedo small
bodies due to
organic components
09.45 - 09.55 S. Sasaki, K. Nakamura, W. Hamabe, E.
Kurahashi, T. Hiroi A
successful simulation of space weathering: spectral darkening and
reddening
by production of nanophase iron particles
10.00 - 10.10 C.W. Hergenrother, R. J. Whiteley, P. Pravec,
S. M. Larson
Small monolithic fast-rotating asteroids
10.15 - 10.25 M.Yanagisawa Rotation rates of
non-spherical asteroids
10.30 - 10.40 K.A. Holsapple Shape limits for Rock
Pile asteroids
10.45 - 10.55 D.T. Britt, D.K. Yeomans, G.J. Consolmagno
S.J., K.R. Housen
Asteroids porosity and internal structure
11.00 - 11.25 Coffee Break
11.25 - 11.50 A. Ghosh, H.Y. McSween, Jr., R.E. Grimm,
L.Wilson, E.D. Young
(Invited) Importance of thermal models in understanding
asteroid evolution
12.05 - 12.15 P. Washabaugh, D.J. Scheeres Energy and
stress distributions
in ellipsoids
12.20 - 12.30 R.J.Whiteley, D.J. Tholen
Spectrophotometric observations of
small near-earth asteroids
12.35 - 12.45 K. Muinonen Interpreting asteroid
photometry and polarimetry
using a single multiple-scattering model
12.50 - 13.00 Yu. Shkuratov, A. Ovcharenko, K. Muinonen, J.
Piironen, R.
Nelson Laboratory studies for the opposition effect and
negative
polarization of simulated asteroid regoliths
13.05 Lunch
14.00 ca. Excursion
Thursday, June 14
SESSION VI ASTEROID FAMILIES AND COLLISIONAL PROCESSES
Chairs: B. Clark and A. Cellino
09.00 - 09.25 E. Asphaug, E. Ryan, M. Zuber (Invited)
Asteroid interiors
09.40 - 10.05 W.J. Merline (Invited) Asteroid
satellites
10.20 - 10.30 D.D. Durda, W. Bottke Jr., E. Asphaug et
al Numerical models
of the formation of asteroid satellites
10.35 - 10.45 A. Campo Bagatin, J.M. Petit Geometric
constraints on the
size distributions of asteroidal fragments
10.50 - 11.00 A. Cellino, V. Zappalą The
identification of the most likely
parent bodies of large NEAs
11.05 - 11.30 Coffee Break
11.30 - 11.40 P. Michel, W. Benz, P. Tanga, D.C.
Richardson New
simulations of collisions between asteroids in the gravity
regime:
comparison with the properties of some observed asteroid
families
11.45 - 11.55 K.R.Housen Impact cratering on porous
asteroids
12.00 - 12.25 V. Zappalą (Invited) New results in
asteroid families
12.40 - 12.50 M.S. Kelley Progress on genetic testing
and geologic mapping
of dynamical asteroid families: the FACES database
12.55 - 13.05 B.A. Ivanov, G. Neukum, W.K. Hartmann
The comparison of
size-frequency distributions of impact craters and asteroids, and
the
planetary cratering rate
13.10 Lunch
15.00 - 15.10 Z.M. Leinhardt, D.C. Richardson
Planetesimal evolution: a
mass ratio study of rubble pile collisions
15.15 - 15.25 D. O'Brien, R. Greeenberg The
collisional evolution of
really tiny asteroids: implications for their size-distribution
and
lifetimes
SESSION VII INTERRELATIONSHIPS WITH INNER SS OBJECTS: NEAR-EARTH
OBJECTS,
METEORITES, METEOR STREAMS
Chairs: A. Carusi and D. Steel
15.30 - 15.55 D.Morrison (Invited) Dealing with the
Asteroids impact
hazard
16.10 - 16.20 G. D'Abramo, A.W.Harris USA, A. Boattini,
S.C. Werner, A.W.
Harris DLR, G. B. Valsecchi Estimating the population of
near-earth
asteroids through the detection/re-detection method
16.25 - 16.35 A.W. Harris, USA The Spaceguard Survey:
How are we doing?
16.40 - 16.50 A. Rossi, D.J. Scheeres, F. Marzari
Evolution of NEOs
rotation rate due to repeated close encounters with the
earth
16.55 - 17.20 Tea Break
17.20 - 17.45 T. H. Burbine (Invited)
Asteroid-meteorite relationships
18.00 - 18.10 G.J.Flynn Physical properties of stone
meteorites:
implications for the properties of stone asteroids
18.15 - 18.25 D.I. Steel Groupings among near-earth
objects
18.30 - 19.30 POSTER SESSION SESSIONS VII, VIII and
IX
Friday, June 15
09.00 - 09.10 T. Mukai, M. Ishiguro, M. Fujino et al
Observations of
asteroidal dust clouds
09.15 - 09.25 S. Dermott, D. Durda, K. Grogan, T.
Kehoe Asteroidal dust
SESSION VIII INTERRELATIONSHIPS WITH OUTER SS OBJECTS:
TROJANS CENTAURS,
EDGEWORTH-KUIPER OBJECTS, COMETS
Chairs: D. Lazzaro and C.M. Lisse
09.30 - 09.55 P.Weissman, W. Bottke, M.Hicks, H.Levison
(Invited)
Evolution of comets into asteroids
10.10 - 10.20 Virtanen J., Muinonen K., Laakso T.,
Kaasalainen M., Bowell
E. Optimized orbital ranging for trans-Neptunian and
near-Earth objects
10.25 - 10.35 Y. Fernandez, D. Jewitt, S. Sheppard
Low albedo among
extinct comet candidates
10.40 - 10.50 H.U. Keller Are inactive comets
asteroids?
10.55 - 11.20 Coffee Break
11.20 - 11.45 M.A. Barucci (Invited) Trojans,
Centaurs and relations to
the Kuiper belt
12.00 - 12.10 C.M. Lisse The evolution of cometary
bodies into asteroids -
clues from observations of cometary dust
12.15 - 12.25 S. Mottola, M. Di Martino, A. Erikson
Rotation properties of
Jupiter Trojan asteroids
12.30 - 12.40 F. Marzari, H. Scholl On the
instability of Jupiter Trojans
12.45 Lunch
SESSION IX THE FUTURE OF ASTEROIDS
Chairs: M. Fulchignoni and C. Chapman
14.45 - 15.10 D.K. Yeomans, R.W. Farquhar, J. Kawaguchi,
C.T. Russel, G.H.
Schwehm, J. Veverka (Invited) Spacecraft exploration of
asteroids: past,
present and future
15.25 - 15.35 H.Yano, M. Abe, H.Yamakawa, M. Yoshikawa, A.
Fujiwara The
Family Mission: multiple Fly-bys and sample returns to main belt
asteroid
families
15.40 - 15.50 A. Fujiwara, T. Mukai, A. Abe, H. Yano, J.
Kawaguchi, K.
Uesugi Sample return and science by MUSES-C
15.55 - 16.05 L. Bussolino, A. Ferri, R. Somma, V.
Zappalą, A. Cellino, A.
Carusi, G. Valsecchi Studying a mission for physical
characterization of
NEOs
16.10 - 16.20 A.R. Hildebrand, K.A. Caroll, D.D. Balam, et
al The
near-earth space surveillance (NESS) mission: discovery, tracking
and
characterization of asteroids and comets with a
microsatellite
16.25 - 16.35 A. Milani, S. R. Chesley, P.W. Chodas, G.B.
Valsecchi
Asteroid close approaches and monitoring for possible
impacts
16.40 - 17.05 Tea Break
17.05 - 17.15 M.S.J. Belton, E. Asphaug, W. Huebner, D.
Yeomans Scientific
requirements for NEO impact mitigation
17.20 - 17.30 A. Carusi, G. Valsecchi, G. D' Abramo, A.
Boattini
Deflecting near-earth objects (NEOs) in route of collision with
the earth:
preliminary results of numerical simulations
17.35 - 17.45 G. Sommer A policy framework for the
NEO problem: advocates,
institutions and social benefit
17.50 - 18.30 R. Binzel, V. Zappala' Concluding
remarks and Discussion
Chair: E. Bowell
18.30 End
===========
(6) 10TH ANNIVERSARY OF THE ERUPTION FELT AROUND THE WORLD
From Mark Hess <mhess@pop100.gsfc.nasa.gov>
Cynthia
O'Carroll
Cynthia.M.OCarroll.1@gsfc.nasa.gov
June 12, 2001
Goddard Space Flight Center, Greenbelt, Md.
(Phone: 301/614-5563)
Release No. 01-62N / Note to Editors
10TH ANNIVERSARY OF THE ERUPTION FELT AROUND THE WORLD
The explosion of the Mt. Pinatubo volcano on June 15, 1991, was
the largest
volcanic eruption the world had seen in nearly a century. In
addition to the
widespread destruction that the volcano wrought on the Philippine
island of
Luzon, Mt. Pinatubo's impact was felt around the world. Global
average
temperatures cooled for more than a year after the eruption due
to the
massive injection of dust and gases into the upper atmosphere.
With the 1991 Mt. Pinatubo eruption, the global effects of
volcanoes on
climate were captured in detail for the first time by a suite of
Earth-observing satellites. The following scientists who were
involved in
many of these trailblazing studies are available for interviews:
... A Temporary Global Cooling. Global warming was halted - at
least
temporarily - by the aerosol cloud from the eruption, which
lowered global
average temperatures by 0.5 degrees Celsius (about 1 degree
Fahrenheit)
through 1992. NASA climate modelers precisely predicted this
volcano-induced
cooling - a powerful demonstration of the capability of these
computer
simulations. Contact: James Hansen, NASA Goddard Institute for
Space
Studies, New York, N.Y.; tel. 212-678-5500; e-mail jhansen@giss.nasa.gov
... A Global Pall of Dust and Aerosols. Pinatubo pumped so much
volcanic ash
and gas into the upper reaches of the atmosphere that the normal
levels of
stratospheric aerosols increased by more than 20 times, leading
to a
short-lived global cooling. Contact: Phil Russell, NASA Ames
Research
Center, Moffett Field, Calif. Public Affairs contact: John Bluck;
tel.
650-604-5026 or 9000; e-mail jbluck@mail.arc.nasa.gov
... Ozone Levels Drop Worldwide. The protective ozone layer in
the upper
atmosphere weakened for more than a year as the result of gases
injected
into the stratosphere by the eruption. NASA's TOMS instrument
tracked the
decline and eventual recovery from start to finish. Contact: Jay
Herman,
NASA Goddard Space Flight Center, Greenbelt, Md.; tel.
301-614-6039; e-mail
herman@tparty.gsfc.nasa.gov
... A Shift in the Weather and Winds. The eruption also caused
changes in
regional weather patterns. Climate models showed that Pinatubo
produced a
shift in wind patterns in the North Atlantic that lead to a
warmer-than-usual winter in Europe in 1991-92. Contacts: Gavin
Schmidt,
Columbia University and NASA Goddard Institute for Space Studies,
New York,
N.Y.; tel. 212-678-5627; e-mail gschmidt@giss.nasa.gov.
Drew Shindell, NASA
Goddard Institute for Space Studies, New York, N.Y.; tel.
212-678-5561;
e-mail dshindell@giss.nasa.gov
... Mudflows: A Continuing Hazard. The millions of tons of ash
and rock that
blanketed the flanks of Mt. Pinatubo created dangerous rivers of
mud during
the annual rainy season. Scientists are keeping an eye on this
shifting
natural hazard with airborne and space sensors. Contact: Peter
Mouginis-Mark, University of Hawaii, Honolulu; tel. 808-956-3147;
e-mail
pmm@pgd.hawaii.edu
... A New View of the Swirling Atmosphere. The Mt. Pinatubo
eruption was a
unique natural experiment that unveiled movements in the
atmosphere that
scientists had never seen before. As satellites tracked volcanic
aerosols
moving around the globe, researchers saw movements through the
troposphere
into the stratosphere for the first time. Contact: Chip Trepte,
NASA Langley
Research Center, Hampton, Va.; tel. 757-864-5836; e-mail
c.r.trepte@larc.nasa.gov
Visualizations of Mt. Pinatubo and several of these global
climate effects
will be broadcast on NASA TV on Wednesday, June 13 at 12 noon,
3:00 p.m. and
6:00 p.m. EDT. NASA TV is broadcast on the GE2 satellite which is
located on
Transponder 9C, at 85 degrees West longitude, frequency 3880.0
MHz, audio
6.8 MHz.
===========
(7) ARTHUR C CLARK STANDS BY HIS BELIEF IN LIFE ON MARS
from Space.com, 7 June 2001
http://space.com/peopleinterviews/clarke_mars_010601.html
By Leonard David
Senior Space Writer
WASHINGTON -- Noted space visionary and writer, Sir Arthur C.
Clarke,
believes that new images of Mars clearly show the red planet
dotted with
patches of vegetation, including trees. Such a find may help
spark a far
grander space program more aligned with the adventure and
exploration
portrayed in the epic film, 2001: A Space Odyssey - the
collaborative work
of both Clarke and director Stanley Kubrick.
Clarke spoke last night, June 6, via phone from his home in Sri
Lanka as key
speaker in the Wernher von Braun Memorial Lecture series held
here at the
Smithsonian's National Air and Space Museum.
Pouring over images on his home computer taken by the
now-orbiting Mars
Global Surveyor (MGS), Clarke said that there are signs of
vegetation
evident in the photos.
"I'm quite serious when I say have a really good look at
these new Mars
images," Clarke said. "Something is actually moving and
changing with the
seasons that suggests, at least, vegetation," he said.
Clarke repeated several times that he was serious about his
observations,
pointing out that he sees something akin to Banyan trees in some
MGS photos.
Science met its match
Joining Clarke in last night's lecture was a panel of space
authorities,
Apollo 17 moonwalker, Eugene Cernan, science fiction writer, Ben
Bova, and
space historian Fred Ordway.
Cernan said that he has concluded there's little difference
between science
fiction and science fact. He said that the only difference is
time, a
dimension we know so little about.
"Standing on the surface of the Moon in sunlight, you are
surrounded by the
blackest black that you can allow your mind to conceive. Not
darkness, but
blackness," Cernan said. That view affords a person a
face-to-face look at
the endlessness of time and the endlessness of space, with Earth
moving
through that blackness. What you see is infinity, he said.
"I have looked and focused as far as I can focus on
infinity. I can tell you
that it literally does exist," Cernan said.
Awestruck by the vista from his trek to the Moon, now over a
quarter of a
century ago, Cernan said that he came to a point "where
science did not have
an explanation" for what he saw. "It was just too
beautiful to have happened
by accident. Science met its match," he said.
The other things
Cernan decried the fact that the country's space exploration
agenda today
rings hollow compared to the past.
"What's it going to take to get people to dream again, to
realize they can
once again do the impossible?" Cernan asked. "John F.
Kennedy said that we
plan to go the Moon 'and do those other things'...we haven't done
the other
things yet," he said.
Ben Bova said that NASA's program is driven by politics. If
there's no
political push and no political will, then "I think it's
going to have to
come from the private sector," he said.
How to reactivate America's space program to do bold things
"is the $64
trillion question," Clarke responded by phone. Space tourism
may act as a
trigger, he said, as could some major discovery, such as new
findings on
Mars.
Ordway said that 2001: A Space Odyssey, and the vision it
portrays, came at
a time "when space was on everybody's agenda," he said.
Old and new worlds
"I think there's a real possibility there may be a
propulsion breakthrough,"
Clarke said. "The rocket is going to play the same role in
space as the
balloon did in aviation. It will be superseded by something much
better," he
said.
Cernan said he remains optimistic about the future of space
exploration.
In the future, people will not only be living on Mars, "they
are going to be
coming back to see where their forefathers grew up," Cernan
said. "I think
someday they will be talking about the Old World and the New
World, and
we're going to co-exist together. That's science fiction today,
but give us
time," he said.
Clarke said however, that such a scenario has one problem.
"I'm afraid the great, great grandchildren won't be very
happy back here on
Earth at three times normal gravity," Clarke said.
Copyright 2001, Space.com
============================
* LETTERS TO THE MODERATOR *
============================
(8) 100KM CIRCULAR FEATURE OFF THE COAST OF VIETNAM
From Peter Haines <Peter.Haines@utas.edu.au>
Dear Benny,
In CCNet 77/2001 Michael Paine wrote:
Here is an extract from a web page about tektites that Hermann
Burchard brought to my attention. Does anyone have more
information about
the 'circular feature' mentioned below?
The circular feature in question is clearly the 'Qui Nhon Slope
Anomaly'
described by Schnetzler et al. in 1988: Schnetzler, C.C., Walter,
L.S.,
Marsh, J.G. 1988. Source of the Australasian tektite strewn field
- A
possible off-shore impact site. Geophysical Research Letters 15,
357-360.
An abbreviated version of the abstract can be found here:
http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=1988GeoRL..15..357S&db_key=AST&high=3ab06a1e8c14329
To my knowledge no follow-up work has been done to further
investigate the
anomaly, it's age or origin.
Regards, Peter Haines
University of Tasmania
*****************************************************
* Dr Peter Haines
* Lecturer in Sedimentology
* School of Earth Sciences, University of Tasmania
* GPO Box 252-79 Hobart, Tasmania 7001,
AUSTRALIA
* email: Peter.Haines@utas.edu.au
* phone: +61 3 6226 7157 fax:
+61 3 6223 2547
***********************************
===========
(9) WELCOME TO SLOAN AND SUBARU
From Andy Smith <astrosafe@yahoo.com>
Hello Benny and CCNet,
It was great to see the reports from the Sloan Digital Sky Survey
(SDSS) and
the Subaru Telescope (8 June CCNet report). We need their help to
find the
Near-Earth Objects (NEO), before the next one of them finds us.
Since most of the NEO are smaller than magnitude 21, they (and
the other
super-telescopes) are the only ones who can easiely find most of
them.
It was especially interesting to learn that the SDSS can
determine good
orbits, during the 5 minutes of asteroid visibility. This is
extremely
valuable data to us, and we want to request that both the SDSS
and the
Subaru submit NEO reports to the Minor Planet Center, on new
discoveries, if
at all possible and if they are not presently doing so.
If this is not possible, perhaps a way can be found to have their
discoveries followed-up by some other facility(s), which could
make a report
to MPC and share the discovery credit.
The most important thing, from the planetary protection
standpoint, is to
identify these potential killers, at every opportunity. The
present World
data base (MPC) contains only a tiny fraction of the serious
threat
population (about 1%) and without the help of these large
telescopes, it
will take about 300 nail-biting years to find the rest.
A look at the asteroid size distribution, provided in the SDSS
article,
suggests that the magnitude of the NEO threat is not changed
significantly,
by the new SDSS main-belt findings. We are still facing more than
100,000
menacing NEO that are larger than the Tunguska and Arizona
super
rock-bombs.... each equal to 20 megatons(TNT) or so of
destructive impact
energy.
We welcome the super-telescopes (SDSS, Subaru, CFH and others) to
the NEO
hunt and we emplore them to help us identify the undiscovered
NEO.
Cheers,
Andy Smith
International Planetary Protection
Alliance(IPPA)planpro2002@yahoo.com
==========
(10) IMPACTS & TSUNAMI
From Worth Crouch <doagain@jps.net>
Dear Dr. Peiser:
I was pleased to read the May 31, 2001 extract taken from Edward
A. Bryant's
new book TSUNAMI: THE UNDERRATED HAZARD. For many years I have
been a
proponent of the historical and anthropological evidence
indicating a
maritime seafaring people from America, that built megalithic
type tombs and
structures, discovered and inhabited parts of coastal Europe
about 7000
years ago. However, a question has remained in my mind even
though evidence
gathered by Dr. William Fitzheau of the Smithsonian Institute in
1980, and
Erich Brinch Petersen of the Danish National Museum indicate
American
Maritime Archaic people probably migrated to Europe at least 7200
years ago.
I have always questioned how the Maritime Archaic, or Red Paint
People as
they were called by the American anthropologist Dr. Moorhead,
were able to
get a foothold in a Europe composed of folks with a different
complexion,
culture, and competing for similar resources. I know the Norsemen
or Vikings
tried to colonize America for at least 200 years without success
and were
eventually stopped by Native Americans. Moreover, Norse
technology in AD 800
-1000 was superior to the Native American's as well as the
earlier Maritime
Archaic technology. Until now I have wondered how the Red Paints
could
colonize even a few sights on the European coast successfully
considering
the Maritime Archaic in Europe, like the Vikings in America, must
have been
terribly outnumbered. Evidence from excavations in Nuilliak Cove
Labrador,
Vedbaek Norway, Port au Cvhoix Newfoundland, Teviec Brittany,
L'Anse Amour
Newfoundland, and Muge Portugal all indicate the communities were
probably
populated by Red Paint People. The oldest Maritime Archaic sight
in Europe
is Teviec prospering about 7200 years ago, off the coast of
Brittany in
France, and the artifacts, method of burial, artistic designs,
and evidence
of shamanistic rituals of the Maritime Archaic in Europe are
amazingly
similar to the other Red Paint sights in America.
The purpose of this correspondence is not to argue the merits of
the Red
Paint People's claim to Europe, but instead to use information
from Edward
A. Bryant's new book and answer my previously unanswered
question. He
writes, "One of the more disturbing accounts has been
compiled from these
legends by Edith and Alexander Tollmann of the University of
Vienna, who
believe that a comet circling the sun fragmented into seven large
bodies
that crashed into the world's oceans 8,200 ± 200 years ago. This
age is
based on radiocarbon dates from Vietnam, Australia and Europe.
The impacts
generated an atmospheric fireball that globally affected society.
This was
followed by a nuclear winter characterised by global cooling.
More
significantly, enormous tsunami swept across coastal plains and,
if the
legends are to be believed, overwashed the centre of continents.
The latter
phenomenon, if true, most likely was associated with the splash
from the
impacts rather than with conventional tsunami run-up. Massive
floods then
occurred across continents. The event may well have an element of
truth.
Figure 8.9 plots the location of the seven impact sites derived
from
geological evidence and legends. Two of these sites, in the
Tasman and North
Seas, have been identified as having mega-tsunami events around
this time.
The North Sea impact centre corresponds with the location of the
Storegga
slides described in Chapter 6. Here, the main tsunami took place
7,950 ±190
years ago."
If the before mentioned information in Bryant's book is correct
it would
explain why the Red Paints did not face a formidable European
population
opposing their coastal colonization. In fact the coastal European
population
would have been washed away by the results of a comet's North Sea
impacting
tsunami 700 years before the Red Paints discovered Europe. Also
if the
actions of New Zealand Aboriginal Coastal tribes surviving a
comet's
resulting tsunami in AD 1178, can be superimposed on those
Europeans
surviving the resulting North Sea tsunami around 7950 years ago
the
Europeans would probably have avoided the coast as did the New
Zealand
Aboriginals for hundreds of years. Thus, allowing the Red Paints
to colonize
without much opposition, and build their fragile coastal
communities along
with their sturdy megaliths, the origons of which subsequently
frustrate
future generations of historians.
Sincerely,
Worth F. Crouch
(Talako)
Society of Choctaw Astrobiologists
===========
(11) MULTIPLE IMPACTS AT THE TR/J EXTINCTION BOUNDARY?
From Hermann Burchard <burchar@mail.math.okstate.edu>
Dear Benny,
below are three abstracts from the pages of NATURE constituting
an
interesting discussion among two groups of authors (Spray et al.
vs. Kent)
on a Tr/J (late Triassic)-related theory of multiple cosmogenic
impacts -- a
single comet breaking up immediately prior to impact and making
five
well-known craters.
If it happened then, it may have happened at other times as well,
such as
P/Tr. This lends new credence to some of my
"wild" speculations (see note
on CCNet of April 27 and Errata May 2).
These articles are a bit older, so it is quite possible that
references to
or abstracts of this material below have been posted by the
moderator on
CCNet on an earlier occasion.
There is clearly some information missing in the second abstract
(Kent's,
although the text given is the full abstract as posted by
NATURE). However,
no harm is done as the missing parts (Kent's objections to Spray
et al.'s
proposed multiple impact theory) are readily apparent from
reading the third
abstract (Spray's reply to Kent). Also, I have deleted some
of the HTML.
Regards,
Hermann
_ _ _ _ _ _ _ _ _ _ _ _ _ _ _ _ _ _ _ _ _ _ _ _ _ _
_ _ _ _ _ _
12 March 1998
Letters to Nature
Nature 392, 171 - 173 (1998) © Macmillan Publishers Ltd.
Evidence for a late Triassic multiple impact event on Earth
JOHN G. SPRAY, SIMON P. KELLEY & DAVID B. ROWLEY
Evidence for the collision of fragmented comets or asteroids with
some of
the larger (jovian) planets and their moons is now well
established
following the dramatic impact of the disrupted comet
Shoemaker-Levy 9 with
Jupiter in 1994 (ref. 1). Collisions by fragmented objects result
in
multiple impacts that can lead to the formation of linear crater
chains, or
catenae, on planetary surfaces. Here we present evidence for a
multiple
impact event that occurred on Earth. Five terrestrial impact
structures have
been found to possess comparable ages (214 Myr), coincident with
the Norian
stage of the Triassic period. These craters are Rochechouart
(France),
Manicouagan and Saint Martin (Canada), Obolon' (Ukraine) and Red
Wing (USA).
When these impact structures are plotted on a tectonic
reconstruction of the
North American and Eurasian plates for 214 Myr before present,
the three
largest structures (Rochechouart, Manicouagan and Saint
Martin) are
co-latitudinal at 22.8° (within 1.2°, [glyph.gif] 110 km), and
span 43.5° of
palaeolongitude. These structures may thus represent the remains
of a crater
chain at least 4,462 km long. The Obolon' and Red Wing craters,
on the other
hand, lie on great circles of identical declination with
Rochechouart and
Saint Martin, respectively. We therefore suggest that the five
impact
structures were formed at the same time (within hours) during a
multiple
impact event caused by a fragmented comet or asteroid colliding
with Earth.
_ _ _ _ _ _ _ _ _ _ _ _ _ _ _ _ _ _ _ _ _ _ _ _ _ _
_ _ _ _ _ _
10 September 1998
Scientific Correspondence
Nature 395, 126 (1998) © Macmillan Publishers Ltd.
Impacts on Earth in the Late Triassic
DENNIS V. KENT
Sprayet al. postulate that five widely dispersed terrestrial
impact
structures with very similar geological age estimates (about 214
million
years ago, in the Late Triassic epoch) are evidence of a multiple
impact
event. Most notably, the three largest impact structures, Saint
Martin in
western Canada (40 km diameter), Manicouagan in eastern Canada
(100 km
diameter), and Rochechouart in France (25 km diameter), plot at
virtually
the same palaeolatitude in a continental reconstruction. Spray et
al.
suggest that this apparent crater chain was produced within hours
as a
series of coaxial projectiles collided in rapid succession with
the rotating
planet Earth, and drew analogies to the recent collision sequence
of
fragmented comet Shoemaker-Levy 9 with Jupiter.
_ _ _ _ _ _ _ _ _ _ _ _ _ _ _ _ _ _ _ _ _ _ _ _ _ _ _ _ _ _
_ _
10 September 1998
Scientific Correspondence
Nature 395, 126 (1998) © Macmillan Publishers Ltd.
Reply: Impacts on Earth in the Late Triassic
JOHN G. SPRAY
Spray replies --Kent raises an interesting point regarding the
proposed late
Triassic multiple-impact event. It might appear contradictory
that the
Manicouagan (100 km diameter) and Rochechouart (25 km diameter)
impact
structures possess normal and reversed geomagnetic reversals,
respectively,
if they were formed within hours of each other, as we suggested.
However,
palaeomagnetic fields are acquired when magnetic mineral phases
pass through
their Curie points (the temperatures at which iron minerals
assume magnetic
order and remain with their magnetic moments parallel to the
Earth's
magnetic field at that time). Critically, this does not
necessarily coincide
with the time of formation of the host rocks.
==============
(12) 2300BC CATASTROPHE
From Alasdair Beal <a.beal@btinternet.com
>
Dear Benny,
2300BC Catastrophe - new papers by Moe Mandelkehr
Those interested in evidence that the Earth suffered a major
catastrophe
around 2300BC may be interested to know that Moe Mandelkehr, who
first put
forward the theory in a series of articles in SIS Chronology
& Catastrophism
Review in the 1980s (C&CR V 1983 pp. 77-95, C&CR IX
1987, pp. 34-44 and
C&CR X 1988, pp. 11-22), has continued his researches and a
new series of
paper by him is being published in SIS Chronology &
Catastrophism Review.
'The Causal Source for the climatic Changes in 2300BC' and 'The
Causal
Source for the Geological Transients at 2300BC' appeared in
C&CR 1999:1 (pp.
3-16) and C&CR 2001:1 features Moe Mandelkehr's latest paper
'Geomagnetic
Effects of an Earthwide Event in 2300BC' (pp. 4-10).
More details of these plus subscription details can be obtained
at
http://www.knowledge.co.uk/sis/
Yours sincerely,
Alasdair Beal
Editor SIS Chronology & Catastrophism Review
-------------------------------------------------------------------
THE CAMBRIDGE-CONFERENCE NETWORK (CCNet)
--------------------------------------------------------------------
The CCNet is a scholarly electronic network. To
subscribe/unsubscribe,
please contact the moderator Benny J Peiser <b.j.peiser@livjm.ac.uk>.
Information circulated on this network is for scholarly and
educational use
only. The attached information may not be copied or reproduced
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any other purposes without prior permission of the copyright
holders. The
fully indexed archive of the CCNet, from February 1997 on, can be
found at
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DISCLAIMER: The opinions, beliefs and viewpoints expressed in the
articles
and texts and in other CCNet contributions do not
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opinions, beliefs and viewpoints of the moderator of this
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*
CCNet ESSAY: ESTIMATED FLUX OF ROCKS BEARING VIABLE LIFEFORMS
EXCHNAGED
BETWEEN EARTH
http://abob.libs.uga.edu/bobk/ccc/ce061201.html
by Michael Paine, The Planetary Society Australian Volunteers
<mpaine@tpgi.com.au>
Introduction
A possible mechanism for transfer of life between planets is via
rocks
ejected by major asteroid or comet impacts. The term
"transpermia" was
coined by Oliver Morton to describe the transfer of lifeforms by
this method
and to distinguish it from the more general concept of
panspermia. Davies
(1998a-c) discusses several possibilities for transpermia
including
hypothetical Mars-life reaching Earth; Earth-life reaching Mars,
the Earth's
Moon and moons of the outer solar system and interstellar
transfers via
meteoroids. Melosh (1994) outlines the mechanisms by which such
transfers
can take place. Mileikowsky and others (2000) build on Melosh's
work and
provide estimates of transfer rates between Mars and Earth over
the past 500
million years.
[continued @ http://abob.libs.uga.edu/bobk/ccc/ce061201.html ]