PLEASE NOTE:
* 
Date sent:        Wed, 22 Oct
1997 09:39:55 -0400 (EDT) 
From:            
Benny J Peiser <B.J.PEISER@livjm.ac.uk 
Subject:         
CAMBRIDGE-CONFERENCE DIGEST 
To:              
cambridge-conference@livjm.ac.uk 
Priority:         NORMAL 
CAMBRIDGE-CONFERENCE DIGEST, 22 October 1997
1) SCIENTISTS DISCOVER POSSIBLE IMPACT CRATER IN YEMEN
2) MISSIONS TO GATHER SOLAR WIND SAMPLES AND TOUR THREE COMETS
   SELECTED AS NEXT DISCOVERY PROGRAM FLIGHTS 
3) SEND YOUR NAME TO A COMET ON A STARDUST SPACECRAFT 
  
In view of the constantly increasing information, research and
the growing number of news stories about neo-catastrophism, mass 
extinctions, NEOs and related topics, I intend to reduce the
number 
of separate postings on the CC-network. In order to reduce the 
overall number of electronic mail send out on the CC-network, I
will 
try to compile a regular digest with a list of interesting 
information. This digest, I hope, will further help to stem the
flood 
of electronic information from which we are all suffering, one
way or 
another. 
Benny J Peiser 
========================================================================
1) SCIENTISTS DISCOVER POSSIBLE IMPACT CRATER IN YEMEN
from: Ron Baalke <BAALKE@kelvin.jpl.nasa.gov
PUBLIC INFORMATION OFFICE 
JET PROPULSION LABORATORY 
CALIFORNIA INSTITUTE OF TECHNOLOGY 
NATIONAL AERONAUTICS AND SPACE ADMINISTRATION 
PASADENA, CALIF. 91109. TELEPHONE (818) 354-5011 
http://www.jpl.nasa.gov 
Contact: Mary A. Hardin
FOR IMMEDIATE RELEASE 
OCTOBER 20, 1997 
SCIENTISTS DISCOVER POSSIBLE IMPACT CRATER IN YEMEN
    Scientists using a variety of spaceborne
remote-sensing images, 
combined with limited ground research, have discovered what they
think is a 
possible impact crater in a dry river bed in the Yemen Arab
Republic. 
    "On the remote-sensing images, the
proposed crater appears as a 
770-meter-diameter (2,525-foot) circular feature centered on a
small wadi or 
dry river channel. Although sharp on the remote- sensing images,
the feature 
is unremarkable in the field," said Dr. Ronald Blom, a
research geologist at 
NASA's Jet Propulsion Laboratory. "This is another example
of how 
remote-sensing tools help us see things we wouldn't normally be
able to 
detect, or might overlook, on the ground." 
    Blom and his colleague Dr. Robert Crippen,
also of JPL, are 
presenting their findings this week at the annual meeting of the
Geological 
Society of America, being held in Salt Lake City. The image is
available at 
http://www.jpl.nasa.gov/news
. 
    They used radar images from the Spaceborne
Imaging Radar C/X-Band 
Synthetic Aperture Radar (SIR-C/X-SAR) that flew twice on the
space shuttle 
in 1994, and enhanced visible and near- infrared images from the
Landsat 
Thematic Mapper satellite. 
    "A very brief field reconnaissance in
January 1997 indicates, but 
does not confirm, that the feature may well be an impact
crater," Blom 
explained. "The crater is in a wadi that is filled with
sediment and 
windblown sand. No direct evidence of an impact, such as
overturned rims, 
shatter cones, or meteoritic material, were observed. However,
large 
circular features are uncommon. Other potential explanations for
this 
circular feature include a sinkhole or volcanic crater. But there
was no 
field evidence of volcanic or sinkhole activity. Thus, neither
seems likely 
in this case." 
    SIR-C/X-SAR, a joint mission with NASA and
the German and Italian 
space agencies, is managed by JPL, a division of the California
Institute of 
Technology, for NASA's Office of Mission to Planet Earth,
Washington, DC. 
Blom's field work was sponsored by New Wave International and the
Kaplan 
Fund. 
=======================================================================
2) 
MISSIONS TO GATHER SOLAR WIND SAMPLES AND TOUR THREE COMETS 
   SELECTED AS NEXT DISCOVERY PROGRAM FLIGHTS 
  
from: David Morrison <dmorrison@mail.arc.nasa.gov
NEO News (10/21/97)
Dear friends and students of NEOs:
NASA has announced the selection of another NEO mission, to
provide 
multiple comet flybys.  The Discovery mission called Contour
is led 
by PI Joseph Veverka of Cornell University.  This is the
third NASA 
Discovery mission to study small bodies.  Currently the
first 
Discovery mission, Near Earth Asteroid Rendezvous (NEAR), is en
route 
to Eros, while under development is the mission Stardust to
return 
samples of the coma of comet Wild-2.  More details of this
Discovery 
selection are given in the NASA press release below, taken from
the 
NASA homepage at http://www.nasa.gov.
David Morrison
------------------------------------------------------ 
Headquarters, Washington,
DC                 
October 20, 1997 
(Phone:  202/358-1753) 
RELEASE: 97-240
MISSIONS TO GATHER SOLAR WIND SAMPLES AND TOUR THREE COMETS 
SELECTED AS NEXT DISCOVERY PROGRAM FLIGHTS 
      A mission to gather samples of
the wind flowing from the Sun 
and a mission to fly by three near-Earth comets have been
selected 
as the next flights in NASA's Discovery Program of lower-cost, 
highly focused scientific spacecraft. 
      The Genesis mission is designed
to collect samples of the 
charged particles in the solar wind and return them to Earth 
laboratories for detailed analysis.  It is led by Dr. Donald
Burnett from the California Institute of Technology, Pasadena,
CA, 
at a total cost to NASA of $216 million.  Due for launch in 
January 2001, it will return the samples of isotopes of oxygen, 
nitrogen, the noble gases, and other elements to an airborne 
capture in the Utah desert in August 2003.  Such data are
crucial 
for improving theories about the origin of the Sun and the 
planets, which formed from the same primordial dust cloud. 
      The Comet Nucleus Tour
(CONTOUR) will take images and 
comparative spectral maps of at least three comet nuclei and 
analyze the dust flowing from them.  CONTOUR is led by Dr.
Joseph 
Veverka of Cornell University, Ithaca, NY, at a total cost to
NASA 
of $154 million.  It is scheduled for launch in July 2002,
with 
its first comet flyby to occur in November 2003.  This flyby
of 
Comet Encke at a distance of about 60 miles (100 kilometers) will
be followed by similar encounters with Comet
Schwassmann-Wachmann- 
3 in June 2006 and Comet d'Arrest in August 2008. 
      "This was a very difficult
selection, given the first-class 
science proposed by all five teams," said Dr. Wesley
Huntress, 
Associate Administrator for Space Science at NASA Headquarters, 
Washington.  "We picked two based on our distribution
of resources 
and the excellent fit of the timetables for these missions with 
other robotic space science explorers.  Genesis will give us
a 
sample of the Sun as we are preparing to receive samples of a 
comet and asteroid from other missions.  Meanwhile, CONTOUR
will 
help us better understand the breadth of the 'family' of comets, 
which are believed to be quite individual in their
properties." 
      The selection of these missions
is the second step of a two- 
step process.  In the first step, NASA selected five
proposals in 
April 1997 for detailed four-month feasibility studies. 
Funded by 
NASA at $350,000 each, these studies focused on cost, management 
and technical plans, including small business involvement and 
educational outreach. 
      The selected proposals were
among 34 proposals originally 
submitted to NASA in December 1996, in response to a Discovery 
Announcement of Opportunity (AO) issued on September 20,
1996.  As 
stated in the AO, the initial cost estimates were allowed to grow
by a maximum of 20 percent between the April selection and the 
detailed final proposals. 
      The investigations proposed in
response to this announcement 
(AO-96-OSS-02) were required to address the goals and objectives 
of the Office of Space Science's Solar System Exploration theme
or 
the search for extrasolar planetary systems element of the 
Astronomical Search for Origins and Planetary Systems
theme.  A 
selected mission was required to be ready for launch no later
than 
September 30, 2002, within the Discovery Program's cost cap of 
$280 million total per mission, including development, launch and
operations. 
      CONTOUR and Genesis follow four
previously selected NASA 
Discovery missions.  The Near Earth Asteroid Rendezvous
(NEAR) 
spacecraft was launched in February 1996 and returned sharp
images 
of the asteroid Mathilde from a distant flyby in June of this 
year, on its way to orbit the asteroid Eros in early 1999. 
The 
Mars Pathfinder lander, carrying a small robotic rover named 
Sojourner, landed successfully on the surface of Mars on July 4, 
and since has returned hundreds of images and thousands of 
measurements of the Martian environment. 
      The Lunar Prospector orbiter
mission to map the Moon's 
composition and gravity field is scheduled for launch in January 
1998, and the Stardust mission is designed to gather dust from 
Comet Wild-2 in 2004 and return it to Earth, following a planned 
February 1999 launch. 
====================================================================
3) SEND YOUR NAME TO A COMET ABOARD THE STARDUST SPACECRAFT
from: Ron Baalke <BAALKE@kelvin.jpl.nasa.gov
Send Your Name on a Journey to a Comet aboard the Stardust Spacecraft
The Planetary Society helped NASA's Jet Propulsion Laboratory
put 
nearly 600,000 names on the Cassini spacecraft, and now the
Society 
is helping JPL put names on another historic spacecraft. When the
Stardust mission launches in February 1999, it will carry the
names 
of thousands of Planetary Society members and other space
exploration 
supporters. And, if you act before November 30, 1997, your name
can 
also be on this comet-exploring spacecraft. 
Working with the Stardust Project, the Planetary Society is 
collecting names to be placed on a microchip that will be mounted
on 
the Stardust return capsule. This capsule is part of a spacecraft
that will be rocketed into the tail of comet P/Wild-2, collect 
samples of the comet's tail, and then return to Earth in January 
2006. 
To join Stardust on its journey, send your name, address,
city, 
state, country, postal code, and age (optional) to: 
Stardust 
The Planetary Society 
65 North Catalina Avenue 
Pasadena, CA 91106-2301 
All entries must be received no later than Sunday, November
30, 1997. 
The Society will also be posting a form for members and others to
submit their names on [their] web site. 
We Are Stardust
Stardust will be not only the first United States mission
solely 
dedicated to a comet but also the first robotic return of
cometary 
dust and volatile samples. The culmination of more than a
decade's 
quest for a comet sample return, this mission will help us
understand 
more about the formation of our solar system, since comets are 
well-preserved relics of the preplanetary material that accreted 
in the outer fringes of the solar nebula. The scientific value of
having comet samples in hand cannot be overestimated. 
Scientists consider comet P/Wild-2 to be a "fresh"
comet. In 1974, it 
was deflected by Jupiter's gravitational action from an earlier
orbit 
much farther out in the solar system. Samples from Wild-2 thus
offer 
us an exciting glimpse of the best preserved fundamental building
blocks out of which our solar system formed. And sample
collection 
will make use of exciting new aerogel material, the lowest
density 
solid material on Earth. 
Fortuitously, a rare but opportune orbital design using an
Earth 
gravity assist allows Stardust to capture cometary dust intact --
and 
parent volatiles as well -- at the incredibly low relative speed
of 
6.1 kilometers (about 4 miles) per second. With the aid of
onboard 
optical navigation, the flyby can take place at an encounter
distance 
as close as 50 kilometers (31 miles) from the comet's nucleus, 
permitting the capture of the freshest samples from within the 
coma parent molecule zone.. This rare trajectory imposes a very
low 
post-launch fuel requirement and enables launch by a Delta 2
launch 
vehicle. 
As an exciting bonus, Stardust will also collect interstellar
dust, 
recently discovered by Ulysses and confirmed by the Galileo
mission. 
In addition, a particle impact mass spectrometer provided by 
Germany's DLR will obtain in-flight data on the compositon of
both 
cometary and interstellar dust, especially the very fine
particles. 
Increasing the yield of science data, Stardust's optical
navigation 
will take images of the comet's nucleus. The spacecraft's dust
shield 
will also provide coma dust spatial and temporal distribution,
and 
the X-band transponder may provide an estimate of comet Wild-2's 
mass. 
You can get more information on this mission to comet Wild-2
at the 
Stardust Project's web site: 
* 
Date sent:        Wed, 22 Oct
1997 08:55:31 -0400 (EDT) 
From:            
Benny J Peiser <B.J.PEISER@livjm.ac.uk 
Subject:         
Massive Comet Blasted into Earth 370 Million Years ago 
To:              
cambridge-conference@livjm.ac.uk 
Priority:         NORMAL 
from: Bob Kobres <bkobres@uga.cc.uga.edu
From CNN.COM:
Massive Comet Blasted into Earth 370 Million Years Ago, Scientists Say
AP 
20-OCT-97 
SALT LAKE CITY (AP) New evidence suggests a comet slammed into
Earth 370 million years ago, blasting a huge crater into the sea 
floor and triggering 1,000-foot waves that led to the extinction 
of many species, scientists said Monday. 
The crash may have been the first in a series of comet strikes
that forever changed life on Earth, including the extinction of 
dinosaurs millions of years later. 
Charles Sandberg, a geologist emeritus with the U.S.
Geological 
Survey, said Monday at a conference that the comet hit roughly 
130 miles northwest of Las Vegas in southern Nevada when the 
region was covered by ocean. 
The force of the blast, dubbed the "Alamo Impact,"
created a 
crater on the sea floor that was 30 to 50 miles in diameter, 
ripping apart a reef on what was then the continental shelf, 
Sandberg said at the annual meeting of the Geological Society of 
America. 
Waves 1,000 feet high spewed chunks of reef as large as a 
half-mile-wide over an area in southern Nevada that was 120 miles
in diameter, he said. 
Sandberg said he has roamed the area for several years and
found 
shattered blocks of the reef, turned into a kind of rock named 
Alamo breccia. He said he and two other geologists John Warme of 
the Colorado School of Mines and Jared Morrow of the University 
of Colorado found evidence in June of the mass destruction 
stretching some 60 miles farther than previously believed. 
The crash, named after a town in the area, happened 3 million 
years before one of the five greatest extinctions of life in 
Earth's history at the end of the Devonian Period, when most 
organisms lived in the ocean, the researchers said. 
The evidence includes: crystals of shocked quartz that are
sand 
grains shattered by the force of the impact; a rock layer rich in
iridium, which is an element rare on Earth but common in 
asteroids and comets; and sphere-shaped pieces of limestone-like 
material created when small pieces of reef were blasted skyward 
and melted, then fell to Earth, Sandberg said. 
The area is rich in fossils that are 370 million years old. 
Researchers in recent years also found a crater and similar 
breccia rocks in other countries, suggesting the Devonian 
extinction was caused by a series of comet strikes, Sandberg 
said. 
He said a comet that hit Jupiter in 1994 is evidence that 
collisions by comets or asteroids are more than just theory. 
On the possibility that a future comet could strike Earth, 
Sandberg said. "It's something that we all have to think
about." 
He added: "There were impacts throughout time and mass 
extinctions. ... And we can expect this again." 
Some scientists are skeptical that cosmic impacts caused mass 
extinctions, citing gradual die-offs of species as evidence that 
climate changes due to other factors were to blame. 
Paleontologist Kevin Padian of the University of California, 
Berkeley told The Salt Lake Tribune that the timing of the Nevada
impact and the Devonian extinction are "close enough that
you 
want to look at it further. ... It's reasonable." He was not
involved in the research. 
  
Bob Kobres
email= <bkobres@uga.cc.uga.edu 
url= http://abob.libs.uga.edu/bobk
phone= 706-542-0583