Re: [meteorite-list] From the strewnfield of the newest meteorite fall..........

2004-05-28 Thread Mikestockj


Hi Rob
You are correct about the Montrose fireball. It fragmented very high above the city of Montrose. I have included the text from Chris Peterson's website www.cloudbait.com below. He explains it much better than I could.
The fireball began about 25 miles southeast of Montrose at a height of 75 miles, and descended steeply towards the town (47° from the vertical), exploding at a height of 48 miles directly over the southeast corner. This event was captured by the allsky camera at Montrose High School (the orange dot labeled "MHS" is seen very close to the end of the meteor path). From the view of this camera (video, 87K ), the meteor is seen to start high in the sky and rise nearly overhead before exploding, with the final material disappearing behind the camera.
This fireball exploded unusually high. Normally, meteoroids are much closer to the ground before the stress of deceleration in the denser atmosphere causes them to break up. The high altitude suggests that the parent body was particularly fragile, possibly cometary debris or a carbonaceous chondrite. This reduces the possibility that material survived to reach the ground. Nevertheless, after a close examination of the decay following the terminal explosion, I think there remains a good possibility that meteorites were formed. Although the path makes it appear that debris would fall over Montrose, the altitude of the breakup combined with high altitude winds that evening make it likely any strewn field produced would actually lie about 12 miles to the northeast, between Montrose and Crawford.
My guess is that due to the high winds aloft it flew over Denver 3-4 hours later then again in 24 hours, then againwell you get the "drift". I figure if Mike Farmer and Blaine Reed could not find anything chances are not good that anything will be found.
Mike
Mike Jensen IMCA 4264Bill Jensen IMCA 2359Jensen Meteorites16730 E Ada PLAurora, CO 80017-3137303-337-4361Web Site: Jensen Meteorites New Book: Meteorites from A to Z 
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[meteorite-list] Cassini-Huygens Mission Status Report - May 28, 2004

2004-05-28 Thread Ron Baalke


MEDIA RELATIONS 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

Carolina Martinez (818) 354-9382
Jet Propulsion Laboratory, Pasadena, Calif.

Donald Savage (202) 358-1727  

NASA Headquarters, Washington

News Release: 2004-134   May 28, 2004

Cassini-Huygens Mission Status Report

The Cassini spacecraft successfully performed a critical six-minute
trajectory correction maneuver May 27 to put it on course with its
first encounter, Saturn's outermost moon Phoebe, set for June 11.  The
spacecraft is operating normally and is in excellent health.

The maneuver is very critical for getting us into Saturn orbit
because it is the first checkout of the bipropellant pressurization
system after nearly five years of dormancy, said Todd Barber,
propulsion engineer for Cassini at NASA's Jet Propulsion Laboratory,
Pasadena, Calif.  It sets the stage for Saturn orbit insertion on
June 30.

During the course of its trip, Cassini has traveled 3.4 billion
kilometers (2.1 billion miles). We couldn't have asked for a smoother
ride, said Robert T. Mitchell, program manager for the
Cassini-Huygens mission at JPL. All the instruments are performing
well, and for almost seven years we have traveled without any major
hitches. The excitement is building as we are getting ready to put
Cassini in orbit around the ringed planet. The orbiter has relied on
three radioisotope thermoelectric generators to power all the
electrical components, including the 12 science instruments. The
European-built Huygens probe on board Cassini carries six instruments.

If the road to Saturn were a highway, the Cassini orbiter would have
passed the sign along the road that says 'Saturnian County line,'
said Jeremy Jones, chief navigator for the Cassini-Huygens mission at
JPL. The next exits are Phoebe, 9 million kilometers (5.4 million
miles) ahead, Saturn 19 million kilometers (12 million miles) ahead.

Phoebe is an oddly shaped moon with a dark surface. It orbits in the
opposite direction from the motion of most other bodies in the solar
system. The backwards-revolution leads scientists to believe that it
is an object captured from distant Kuiper Belt, making it an
interesting target. The Phoebe flyby may offer the first glimpse of
what the frigid bodies at the edge of the solar system look like,
said Dr. Bonnie Buratti, scientist on the Cassini-Huygens mission at
JPL. These bodies, which include Pluto and its satellite Charon, are
believed to be remnant objects left over from the formation of the
planets 4.5 billion years ago.

After the Phoebe flyby, Cassini will be on course for Saturn. On
arrival date June 30 (July 1 Universal Time), Cassini will become the
first orbiter around Saturn. The two Voyager and Pioneer spacecraft
flew by the planet and saw it from a distance two or three days at a
time. With Cassini, we will be in the city limits for four years,
said Dr. Dennis Matson, project scientist for Cassini at JPL. The
difference is like driving by the Grand Canyon versus stopping,
getting off and enjoying the sights for a while.

On arrival, Cassini will begin a 96-minute burn designed to put the
spacecraft into Saturn's orbit. As part of getting the spacecraft into
orbit, Cassini will twice cross between known gaps in the rings. As a
precautionary measure, the spacecraft will use its antenna as a shield
to protect it from tiny particle hits.

A prime target for Cassini and the piggyback Huygens probe built by
the European Space Agency is the smoggy moon Titan. In the 350 years
since the discovery of Titan we have come to see it as a world with
surprising similarities to our own, yet located almost 1.5 billion
kilometers (900 million miles) from the Sun, said Dr. Jonathan
Lunine, Huygens interdisciplinary scientist and professor of planetary
science and physics at the University of Arizona, Tucson. With a
thick, nitrogen-rich atmosphere and possible hydrocarbon seas, Titan
may harbor organic compounds important in the chain of chemistry that
led to life on Earth.

Six months after reaching Saturn, Cassini will release the wok-shaped
Huygens probe towards Titan on Dec. 24, 2004 (Dec. 25 Universal Time).
The event will be by far the most distant descent of a robotic probe
on another object in the solar system. On Jan. 14, 2005 (Jan. 15
Universal Time), Huygens will enter Titan's atmosphere, deploy its
parachute, and begin its scientific observations of Titan.

The Cassini-Huygens mission is a cooperative project of NASA, the
European Space Agency, and the Italian Space Agency. The Jet
Propulsion Laboratory, a division of the California Institute of
Technology in Pasadena, manages the Cassini-Huygens mission for NASA's
office of Space Science, Washington, D.C. JPL designed, developed and
assembled the Cassini orbiter.

For the latest images and more 

[meteorite-list] polyeuc. vs. howardite

2004-05-28 Thread harlan trammell
so...am i to understand that they are both basically vesta dirt-clods  cemented together somehow, but actual howardite just has more diogenite sand mixed in?
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[meteorite-list] Walter Branch made the Phoenix newspaper

2004-05-28 Thread star-bits
http://www.azcentral.com/arizonarepublic/local/articles/0528clay28.html

Enjoy the article Walter.

--
Eric Olson
ELKK Meteorites
http://www.star-bits.com
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[meteorite-list] test

2004-05-28 Thread Robert Woolard
test




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[meteorite-list] SAU oo1

2004-05-28 Thread Solvænget



Hi list

I was sitting looking at my SAU 001 and I 
thought it is one of the most beautifull meteorites I have ever 
seen.

Have you ever seen the Huble deepfield images 
?
They look just the same as a slice of SAU 
001.

Yes one can get religious by looking at 
such
a slice :-)

If anyone have a $100 full slice (or so) of 
SAU 001 I am very interested... let me know.

Please let me in on your thoughts 
.
Lars Pedersen
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[meteorite-list] Mars Odyssey THEMIS Images - May 24-28, 2004

2004-05-28 Thread Ron Baalke

MARS ODYSSEY THEMIS IMAGES
May 24-28, 2004

o Acidalia Planitia Crater (Released 24 May 2004)
  http://themis.la.asu.edu/zoom-20040524a.html

o Rampart Crater Ejecta (Released 25 May 2004)
  http://themis.la.asu.edu/zoom-20040525a.html

o Acidalia Planitia Crater (Released 26 May 2004)
  http://themis.la.asu.edu/zoom-20040526a.html

o Moreux Crater (Released 27 May 2004)
  http://themis.la.asu.edu/zoom-20040527a.html

o South Polar Cap (Released 28 May 2004)
  http://themis.la.asu.edu/zoom-20040528a.html


All of the THEMIS images are archived here:

http://themis.la.asu.edu/latest.html

NASA's Jet Propulsion Laboratory manages the 2001 Mars Odyssey mission 
for NASA's Office of Space Science, Washington, D.C. The Thermal Emission 
Imaging System (THEMIS) was developed by Arizona State University,
Tempe, in collaboration with Raytheon Santa Barbara Remote Sensing. 
The THEMIS investigation is led by Dr. Philip Christensen at Arizona State 
University. Lockheed Martin Astronautics, Denver, is the prime contractor 
for the Odyssey project, and developed and built the orbiter. Mission 
operations are conducted jointly from Lockheed Martin and from JPL, a 
division of the California Institute of Technology in Pasadena. 


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[meteorite-list] Numbered meteorites

2004-05-28 Thread Jeff Grossman
Some of you may enjoy looking at a web page I decided to put 
together.  It's not done yet, but will be soon.

http://meteoriticalsociety.org/bulletin/areas/regions.html
jeff
Dr. Jeffrey N. Grossman
Chair, Meteorite Nomenclature Committee (Meteoritical Society)
US Geological Survey
954 National Center
Reston, VA 20192, USA
Phone: (703) 648-6184   fax:   (703) 648-6383
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Re: [meteorite-list] Numbered meteorites

2004-05-28 Thread bernd . pauli
 Some of you may enjoy looking at a web page I decided
 to put together.  It's not done yet, but will be soon.

 http://meteoriticalsociety.org/bulletin/areas/regions.html

Kudos from Germany, Jeff! This will certainly be a useful tool
and a excellent source of reference - especially the JPEGs
showing the strewn field maps in full color like Sayh al Uhaimir,
Dhofar, etc.

Bravo, excellent!

Bernd

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[meteorite-list] Mars Exploration Rover Update - May 27, 2004

2004-05-28 Thread Ron Baalke

http://marsrovers.jpl.nasa.gov/mission/status.html

SPIRIT UPDATE: Taking Time to Trench - sol 134-135, 
May 27, 2004

Spirit roved an impressive 109.5 meters (359.3 feet) 
on sol 134. Two hours of the drive were guided by the
autonomous navigation system. After the long traverse, 
Spirit completed an hour of post-drive science
observations with the panoramic and navigation cameras 
and mini thermal emission spectrometer. The rover
finished the sol healthy and ready for another day on 
Mars.

After so much driving on sol 134, Spirit got a break 
and spent sol 135 doing in-situ science investigations 
of its surroundings. It began the sol observing nearby 
soil with the alpha particle X-ray spectrometer and
Moessbauer spectrometer. It then used the microscopic 
imager to see the soil up close. After stowing the
instrument deployment device, Spirit used its wheels 
to dig a trench and then imaged the trench with the
cameras on the mast.

Spirit's odometer now reads 2,585.52 meters (1.6 miles). 
The rover still has 680 meters (0.42 miles) to go
before reaching the base of the Columbia Hills, but 
will likely get there before sol 160.

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[meteorite-list] SAU 001 - L4/5 - S2; W1

2004-05-28 Thread bernd . pauli
 Hi list, I was sitting looking at my SAU 001 and I thought
 it is one of the most beautiful meteorites I have ever seen.
 Have you ever seen the Hubble deepfield images? They
 look just the same as a slice of SAU 001. Please let me
 in on your thoughts ... Lars Pedersen

Hello Lars and List,

I absolutely concur. When I got my slice from Michael Blood on
13 Jun 2001, I wrote to him: Thank God, the SaU 001 was a
real sleeper 'cause it almost knocked my two socks off!!!

The description which I wrote that night for my personal collection
database will confirm your feelings and thoughts about SaU 001:

A thin fully-crusted slice with lots of perfect chondrules of various
sizes and colors, and abundant small to medium-sized FeNi specks. The FeNi
which surrounds several armored chondrules consists of a minute spray
of nickel-iron. One light-colored chondrule measuring 2 mm across, sports
a 0.5 mm round FeNi bleb sitting within. The pointed end displays some
shock darkened areas where chondrules are less abundant.

 Have you ever seen the Hubble deep field images?

There are some outstanding ones in the July issue of Sky  Telescope
(pp. 30-31, pp. 42- 49) ... and, yes, they do remind me of the gorgeous,
colorful matrix and chondrules of my 16.5-gram SAU 001 slice.

I also wrote to Capt'n Blood:

Well, this L4/5 is a real 'Sleeping Beauty'. It does look much
more like an L3 than an L4/5 and reminds me of Cole Creek.

I was so intrigued that I also got a thin section from Michael in August 2001,
and, to top it off, I acquired a 340-gram, completely fusion-crusted individual
at a local rock and gem show that same month. It has numerous shallow
regmaglypts, and is, together with my 194-gram Gao individual from Michael
Cottingham, and my 160-gram Allende individual one of the most beautiful
pieces that I own.

Best regards,

Bernd

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Re: [meteorite-list] Numbered meteorites

2004-05-28 Thread Michael Farmer
Jeff, I noticed the meteorite that is placed out in the ocean in the Oman
map. I saw this a year back when plotting the points and thought it was a
simple error. Can you find which meteorite that is and see who found it and
why it plots in the ocean?
Great job, wonderful work.
Mike Farmer
- Original Message - 
From: Jeff Grossman [EMAIL PROTECTED]
To: [EMAIL PROTECTED]
Sent: Friday, May 28, 2004 1:03 PM
Subject: [meteorite-list] Numbered meteorites


 Some of you may enjoy looking at a web page I decided to put
 together.  It's not done yet, but will be soon.

 http://meteoriticalsociety.org/bulletin/areas/regions.html

 jeff

 Dr. Jeffrey N. Grossman
 Chair, Meteorite Nomenclature Committee (Meteoritical Society)
 US Geological Survey
 954 National Center
 Reston, VA 20192, USA
 Phone: (703) 648-6184   fax:   (703) 648-6383


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[meteorite-list] Deception Point by Dan Brown

2004-05-28 Thread Matson, Robert
Hi All,

Don't remember anyone here mentioning Dan Brown's novel,
_Deception Point_ (the same Dan Brown who wrote _Angels  Demons_
and _The Da Vinci Code_).  Meteorites figure prominently in this
story, so I thought list members would enjoy reading it.  I think
Dan has a little bit of confusion over what a chondrule is, but
aside from that he spins a good yarn.  --Rob
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[meteorite-list] AW: Numbered meteorites

2004-05-28 Thread Christian Anger

Great job, Jeff !

Thanks a lot for making that available.

all the best from Austria,

Christian


IMCA #2673
www.austromet.com
 
Christian Anger
Korngasse 6
2405 Bad Deutsch-Altenburg
AUSTRIA
 
email: [EMAIL PROTECTED]
-Ursprüngliche Nachricht-
Von: [EMAIL PROTECTED]
[mailto:[EMAIL PROTECTED] Im Auftrag von Jeff
Grossman
Gesendet: Freitag, 28. Mai 2004 22:03
An: [EMAIL PROTECTED]
Betreff: [meteorite-list] Numbered meteorites

Some of you may enjoy looking at a web page I decided to put 
together.  It's not done yet, but will be soon.

http://meteoriticalsociety.org/bulletin/areas/regions.html

jeff

Dr. Jeffrey N. Grossman
Chair, Meteorite Nomenclature Committee (Meteoritical Society)
US Geological Survey
954 National Center
Reston, VA 20192, USA
Phone: (703) 648-6184   fax:   (703) 648-6383


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