Re: [meteorite-list] Park Forest strewnfield map

2004-03-16 Thread joseph_town
Hi again,

Please excuse the PK typo. I meant Park Forest strewnfield. I must have had LP mud on 
my mind.

Sincerely,
Bill Kieskowski


> Hi all,
> 
> I understand that since last March a number of people have been working on a 
> definitive map of the PK srewnfield. Can anyone direct me to a source?
> 
> Thanks,
> Bill Kieskowski
> 
> 
> __
> Meteorite-list mailing list
> [EMAIL PROTECTED]
> http://www.pairlist.net/mailman/listinfo/meteorite-list

__
Meteorite-list mailing list
[EMAIL PROTECTED]
http://www.pairlist.net/mailman/listinfo/meteorite-list


[meteorite-list] Norwegian Meteorites

2004-03-16 Thread Fred Olsen
Does anyone know what the rules governing the exportation of meteorites from
Norway?
Thanks,  Fred Olsen, Denver


__
Meteorite-list mailing list
[EMAIL PROTECTED]
http://www.pairlist.net/mailman/listinfo/meteorite-list


[meteorite-list] Planet definition

2004-03-16 Thread Matson, Robert
Hi Rosemary and List,

> I have always considered if it had an orbit around a star it was
> called a planet.

While your definition is succinct, it fails in four cases:
asteroids, comets, dust and man-made satellites.  (I won't muddy
things further with multiple-star systems).  All of these objects
orbit our star, so you see size has to be part of the definition.

If it weren't for all the other plutinos that have been discovered,
I would be happy to call Pluto a planet.  Likewise, if Ceres were
the only asteroid, I would promote it to planetary status.  Instead,
Ceres and Pluto are simply the largest examples of their respective
types.

By choosing the requirement that a planet have a greater mass than
the sum of all other bodies in a similar orbit, you avoid ambiguity
over the minor planets, and in particular the Trojan asteroids of
Mars and Jupiter).  The definition correctly handles all the planetary
satellites as well, without the necessity of addressing the bodies
they orbit.

The only problem case I can imagine is if two nearly equally sized
bodies were orbiting the sun in nearly the same orbit.  But for
the most part I think this is a non-problem, since two moderately-
sized planetoids cannot ordinarily coexist in a similar orbit,
unless they are orbiting each other (double-planet).  Not sure
what happens if you put another earth 60 degrees ahead of or behind
earth in the same orbit (Lagrange points).  There's probably a
mass limit on the second earth, beyond which L4 and L5 are no
longer stable.  --Rob



__
Meteorite-list mailing list
[EMAIL PROTECTED]
http://www.pairlist.net/mailman/listinfo/meteorite-list


Re: [meteorite-list] Pluto - Part 2 of 2

2004-03-16 Thread Rosemary Hackney



Sharky. Whatever floats your boat.
 
Rosie

  - Original Message - 
  From: 
  [EMAIL PROTECTED] 
  
  To: [EMAIL PROTECTED] ; [EMAIL PROTECTED] 
  
  Sent: Tuesday, March 16, 2004 8:20 
  PM
  Subject: Re: [meteorite-list] Pluto - 
  Part 2 of 2
  
  
  
   [EMAIL PROTECTED] 
  writes:
  if it had an orbit around a star it was called aplanet. If it 
orbited  anything else, like a planet, I would consider it 
amoon.
  But by that definition (as opposed to a size/mass-based definition), 
  wouldn't a comet also be considered a planet?
   
  GregoryJ. 
  Gregory Wilson2118 Wilshire Blvd. #918Santa Monica, CA 
  90403


[meteorite-list] Pluto a Planet: A POem

2004-03-16 Thread Francis Graham
 I am really asking for it, but here goes:

PLUTO TO EARTH

"Have you heard the news from Earth?"
Asked the Plutonians (For all it's worth
Although they were used to the cryogenic
A little heat was loved; and made them phrenetic
Increasing their thoughts; yea, near perihelion
Their best of sages could count to a billion.)
"The scoundrels on that blue dot near the Sun
Count eight planets now, and we're not one!"
Another Plutonian retorted, "It must be the glare,
Of the Sun that maddens them. It's not fair!
To pronounce this judgement is mere sophistry
When I doubt they even know our geography."
"And what of our atmosphere, whose pressure is felt,
Is that like an asteroid of the Kuiper Belt?"
"And our moon," said another,"Who's tidally locked;
If we're not a planet, why’s not Mercury defrocked?"
"In lieu of this," cried another, "Let the planets
begin
With Jupiter; and those rocks further in
Are the Sun's satellites; to be pedantic
The Earth's a double moon--how's that for semantic!?"
Yet one more Plutonian, of a psychological bent
Said, "Consider where Earth's spacecraft were sent.
To all orbs but ours. But in their spacefaring nations
The rulers defunded  planetary explorations.
So like Aesop's fable, 'The Grapes and the Fox'
What man cannot conquer, he demotes and mocks!"
And so the wise subzero Plutonians agreed
Their lower status was from a cold human need
To conquer all; failing that, what is left
Is from what is worthy to conquer cleft.
No doubt if Pluto had an American probe
Visiting; each Congressional ear lobe
Would be told the expensive spacecraft hurled
To a major planet,  not some trivial world.
Said  one more Plutonian, twice as cynical,
"Thus even planetology has gotten political."

Francis
















__
Do you Yahoo!?
Yahoo! Mail - More reliable, more storage, less spam
http://mail.yahoo.com

__
Meteorite-list mailing list
[EMAIL PROTECTED]
http://www.pairlist.net/mailman/listinfo/meteorite-list


[meteorite-list] Worden Micromount On Ebay

2004-03-16 Thread RYAN PAWELSKI
Good Evening List,

I just finished listing an auction on Ebay for a very nice 1.4g part-slice of the 
Worden (MI) garage/ car smasher. Please take a look if you want a piece of this 
awesome meteorite for your collection. 

http://cgi.ebay.com/ws/eBayISAPI.dll?ViewItem&item=2232831654&category=3239&sspagename=STRK%3AMESSE%3AIT&rd=1

Thank you and G'nite!

-Ryan



__
Meteorite-list mailing list
[EMAIL PROTECTED]
http://www.pairlist.net/mailman/listinfo/meteorite-list


Re: [meteorite-list] Pluto - Part 2 of 2

2004-03-16 Thread Sharkkb8




 [EMAIL PROTECTED] writes:
if it had an orbit around a star it was called aplanet. If it orbited  anything else, like a planet, I would consider it amoon.
But by that definition (as opposed to a size/mass-based definition), wouldn't a comet also be considered a planet?
 
GregoryJ. Gregory Wilson2118 Wilshire Blvd. #918Santa Monica, CA 90403


Re: [meteorite-list] Pluto - Part 2 of 2

2004-03-16 Thread Rosemary Hackney
I have always considered if it had an orbit around a star it was called a
planet. If it orbited  anything else, like a planet, I would consider it a
moon. Not that I am an expert.. but it seems to be it would depend on the
body it orbited.

Satellite of a star = planet
Satellite of planet or other body = moon

Even the asteroid belt is considered the remnants of a planet either that
did not form or exploded.

My 2 cents worth.

Rosie
- Original Message - 
From: <[EMAIL PROTECTED]>
To: <[EMAIL PROTECTED]>
Sent: Tuesday, March 16, 2004 10:43 AM
Subject: [meteorite-list] Pluto - Part 2 of 2


> Sky & Telescope, March 1990, pp. 295-296:
> A Far Out Planet, George Lovi, excerpt:
>
> Finally, a rather interesting astronomical issue has surfaced as to
whether
> Pluto should legitimately be included in the roster of nine major planets.
Its
> decidedly small size (some 2,280 km across) makes it considerably smaller
> than any other planet, even smaller than several planetary satellites
(including
> our own Moon). It also has a most unplanetary, asteroid-like orbit.
>
> For sometime people have suggested that Pluto is an escaped satellite of
> Neptune, one resembling Triton. Others have proposed that Pluto might be
> some sort of condensed clumping of icy cometary nuclei, or the material
that
> makes up these bodies.
>
> It's really too bad that we cannot look forward anytime soon to a probe
answering
> some of our questions about this "neither fish nor fowl" planet - or
whatever it happens
> to be.
>
>
> CRUIKSHANK D.P. (1999) Pluto and Charon edited by S. Alan
> Stern and David Tholen (MAPS 34-4, 1999, 682, excerpt):
>
> While this book is at least a wonderful compilation of our best
understanding of Pluto and
> Charon, it also represents a window on the other small bodies of the outer
solar system,
> notably Triton, a few other outer planet satellites, and the newly
revealed population of icy
> bodies constituting the Kuiper Disk.
>
> Many Kuiper Disk objects share Pluto's orbital resonance with Neptune;
vastly more lie
> beyond Pluto and form a distribution that may extend to 200 AU or more.
Indeed, Pluto
> and Charon appear to be only the largest known representatives of this
new-found
> component of the solar system. Although the exploration of the Kuiper Disk
is in its
> infancy, this book about the properties of Pluto and Charon in its broader
context helps
> to establish the importance of primitive icy bodies and is a kind of
guidebook toward the
> understanding of their physical properties.
>
> This excellent book is a credit to the Arizona series, to its editors, and
to the chapter authors.
> I recommended it to investigators in the field, advanced students, and
science libraries without
> reservation. (D.P. Cruikshank)
>
>
>
> __
> Meteorite-list mailing list
> [EMAIL PROTECTED]
> http://www.pairlist.net/mailman/listinfo/meteorite-list
>


__
Meteorite-list mailing list
[EMAIL PROTECTED]
http://www.pairlist.net/mailman/listinfo/meteorite-list


[meteorite-list] AD - A few meteorites for sale

2004-03-16 Thread Rob Wesel
Hello all -

I just got done taking a few pictures for some eBay auctions and thought I
would make them available to the list first.

Some nice unclassified chondrites $0.35 per gram
http://makeashorterlink.com/?X4AE25EB7

and some complete LL3 slices $4.00 per gram
http://makeashorterlink.com/?O2CE12EB7

Give the links a moment to find the site, Yahoo loves to make URL's that are
two full lines across.
Feel free to browse the other photos, including the riker mount frames,
ready to download and snazz up your micros.

Payment can be made via PayPal  to:
[EMAIL PROTECTED]

or mail to:

Robert Wesel
2941 N.E. 1st Court
Hillsboro, Oregon 97124
USA

Rob Wesel
--
We are the music makers...
and we are the dreamers of the dreams.
Willy Wonka, 1971




__
Meteorite-list mailing list
[EMAIL PROTECTED]
http://www.pairlist.net/mailman/listinfo/meteorite-list


[meteorite-list] Park Forest Impacts

2004-03-16 Thread Comcast Mail



I just talked to a guy who hunts PF with me and we 
both agree that all the ground impacts that were found by us were on an angle 
from the north to the south.
The biggest one found was 1.2 Kilo and the angle of 
impact was consistent with the others.
Does anyone have any knowlege of other ground 
impact finds? and if they also impacted the soil on an angle , coming in from 
the north.
 
This is consistent with the winslow street impact 
also. It hit the street and sprayed the houses on the south side of the 
street
 
Thanks
Bob Evans


Re: [meteorite-list] Interesting asteroid names

2004-03-16 Thread Ron Baalke
> 
> Ron & all,
> 
> I would have to add Sudbury to the list.

Done!

7610 Sudbury

Ron B.

__
Meteorite-list mailing list
[EMAIL PROTECTED]
http://www.pairlist.net/mailman/listinfo/meteorite-list


Re: [meteorite-list] Interesting asteroid names

2004-03-16 Thread Roman Jirasek
Ron & all,

I would have to add Sudbury to the list.

This event, involving a gigantic nine kilometer diameter rock traveling at
30 kilometers
per second, slamming into the earth with an impact force equivalent to the
detonation
of several billion tons of TNT!

Be ready, if that sized impactor ever hits again, we may be doomed!
I'm sure we all hope someone is watching our collective human asses.

Roman



- Original Message -
From: "Ron Baalke" <[EMAIL PROTECTED]>
To: "Meteorite Mailing List" <[EMAIL PROTECTED]>
Sent: Tuesday, March 16, 2004 3:57 PM
Subject: [meteorite-list] Interesting asteroid names


> Here are some interesting asteroid names:
>
> 1691 Oort
> 1776 Kuiper
> 2224 Tucson
> 2404 Antarctica
> 2421 Nininger
> 2606 Odessa
> 3581 Alvarez
> 3693 Barringer
> 5071 Shoemaker
> 5471 Tunguska
> 10799 Yucatan
> 18725 Atacama
>
> __
> Meteorite-list mailing list
> [EMAIL PROTECTED]
> http://www.pairlist.net/mailman/listinfo/meteorite-list
>



__
Meteorite-list mailing list
[EMAIL PROTECTED]
http://www.pairlist.net/mailman/listinfo/meteorite-list


[meteorite-list] New LL3.7 meteorite

2004-03-16 Thread Michael Farmer



http://www.meteoriteguy.com/nwa3126.htm
Hi everyone, I have just listed a beautiful new 
meteorite. I have had it in UCLA for the last two years, I just got the 
classification data, so it is now up for sale. 
This is a very nice but weathered LL3.7, lots of 
multi-colored chondrules. Check it out even if not buying just to see a very 
nice new meteorite. 
Mike Farmer
I only have small pieces as it was fractured and 
would not cut well.


Re: [meteorite-list] Mesosiderite types

2004-03-16 Thread Devin Schrader
Rob,

A full description is in:
Reviews in Mineralogy Volume 36
Planetary Materials, J.J. Papike, editor
Publisher: Mineralogical Society of America, 1998

"The mesosiderites are divided into three petrologic groups based on the
orthopyroxene content (Hewins 1984, 1988: see Fig. 53). Compositional class
A mesosiderite silicates are relatively basaltic in composition, containing
more plagioclase and clinopyroxene. The compositional class B mesosiderite
silicates contain a greater proportion of orthopyroxene, and are therefore
more ultramafic. A unique mesosiderite from Antarctica, RKPA79015, contains
almost exclusively orthopyroxene as its silicate phase (Prinz et al. 1982a),
and is the sole member of compositional class C (Hewins
1988)." ect(pg 4-143)

This is from 1998, and at least one more C type has come out of Morocco so
the definition of class C might be better refined, ect.

Devin Schrader



- Original Message -
From: "Rob Wesel" <[EMAIL PROTECTED]>
To: "Meteorite List" <[EMAIL PROTECTED]>
Sent: Tuesday, March 16, 2004 3:40 PM
Subject: [meteorite-list] Mesosiderite types


> Hello all-
> Can anyone out there point me in the right direction as to the differences
> between type A, B, and C mesosiderites...and what those differences mean?
> Thanks in advance,
>
> Rob Wesel
> --
> We are the music makers...
> and we are the dreamers of the dreams.
> Willy Wonka, 1971
>
>
>
>
> __
> Meteorite-list mailing list
> [EMAIL PROTECTED]
> http://www.pairlist.net/mailman/listinfo/meteorite-list


__
Meteorite-list mailing list
[EMAIL PROTECTED]
http://www.pairlist.net/mailman/listinfo/meteorite-list


[meteorite-list] Park Forest strewnfield map

2004-03-16 Thread joseph_town
Hi all,

I understand that since last March a number of people have been working on a 
definitive map of the PK srewnfield. Can anyone direct me to a source?

Thanks,
Bill Kieskowski


__
Meteorite-list mailing list
[EMAIL PROTECTED]
http://www.pairlist.net/mailman/listinfo/meteorite-list


[meteorite-list] Mesosiderite types

2004-03-16 Thread Rob Wesel
Hello all-
Can anyone out there point me in the right direction as to the differences
between type A, B, and C mesosiderites...and what those differences mean?
Thanks in advance,

Rob Wesel
--
We are the music makers...
and we are the dreamers of the dreams.
Willy Wonka, 1971




__
Meteorite-list mailing list
[EMAIL PROTECTED]
http://www.pairlist.net/mailman/listinfo/meteorite-list


Re: [meteorite-list] Interesting asteroid names

2004-03-16 Thread Pekka Savolainen
As a finn I have to add Rosettas first planned target, 46P/Wirtanen, 
which is
named after Carl A. Wirtanen, whos parents was from Finland;

http://www.eso.org/outreach/press-rel/pr-1999/phot-27-99.html


the final target is 67P/Churyumov-Gerasimenko, but a good try anyway...;-

http://www.universetoday.com/am/publish/rosetta_asteroid_targets_decided.html?1132004

best,

pekka s



Ron Baalke wrote:

Here are some interesting asteroid names:

1691 Oort
1776 Kuiper
2224 Tucson
2404 Antarctica
2421 Nininger
2606 Odessa
3581 Alvarez
3693 Barringer
5071 Shoemaker
5471 Tunguska
10799 Yucatan
18725 Atacama
__
Meteorite-list mailing list
[EMAIL PROTECTED]
http://www.pairlist.net/mailman/listinfo/meteorite-list
 

--



Pekka Savolainen
Jokiharjuntie 4
FIN-71330 Rasala
FINLAND
+ 358 400 818 912

Group Home Page: http://www.smartgroups.com/groups/eurocoin
Group Email Address: [EMAIL PROTECTED]


__
Meteorite-list mailing list
[EMAIL PROTECTED]
http://www.pairlist.net/mailman/listinfo/meteorite-list


[meteorite-list] Color Image of Bonneville Crater

2004-03-16 Thread Ron Baalke

Take a look at this full-resolution color image of Bonneville crater:

http://marsrovers.jpl.nasa.gov/gallery/press/spirit/20040315a.html

Download the highest-resolution image (26.4 MB).  You can see
the heat shield rather clearly on the far rim of the crater.
Also, look closely at the rocks in the foreground close to the
rover. I could swear, it looks like some of the rocks have 
fusion crust.

Ron Baalke

__
Meteorite-list mailing list
[EMAIL PROTECTED]
http://www.pairlist.net/mailman/listinfo/meteorite-list


[meteorite-list] Interesting asteroid names

2004-03-16 Thread Ron Baalke
Here are some interesting asteroid names:

1691 Oort
1776 Kuiper
2224 Tucson
2404 Antarctica
2421 Nininger
2606 Odessa
3581 Alvarez
3693 Barringer
5071 Shoemaker
5471 Tunguska
10799 Yucatan
18725 Atacama

__
Meteorite-list mailing list
[EMAIL PROTECTED]
http://www.pairlist.net/mailman/listinfo/meteorite-list


[meteorite-list] Most Distant Object In Solar System Discovered

2004-03-16 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

Jane Platt  (818) 354-0880
Jet Propulsion Laboratory, Pasadena, Calif.

Donald Savage/Dwayne Brown  (202) 358-1547/1726
NASA Headquarters, Washington 

NEWS RELEASE:  2004-085 March 15, 2004

Most Distant Object In Solar System Discovered

NASA-funded researchers have discovered the most distant object
orbiting Earth's Sun. The object is a mysterious planet-like body
three times farther from Earth than Pluto.

"The Sun appears so small from that distance that you could completely
block it out with the head of a pin," said Dr. Mike Brown, California
Institute of Technology, Pasadena, Calif., associate professor of
planetary astronomy and leader of the research team. The object,
called "Sedna" for the Inuit goddess of the ocean, is 13 billion
kilometers (8 billion miles) away, in the farthest reaches of the
solar system.

This is likely the first detection of the long-hypothesized "Oort
cloud," a faraway repository of small icy bodies that supplies the
comets that streak by Earth. Other notable features of Sedna include
its size and reddish color. After Mars, it is the second reddest
object in the solar system. It is estimated Sedna is approximately
three-fourths the size of Pluto. Sedna is likely the largest object
found in the solar system since Pluto was discovered in 1930. 

Brown, along with Drs. Chad Trujillo of the Gemini Observatory,
Hawaii, and David Rabinowitz of Yale University, New Haven, Conn.,
found the planet-like object, or planetoid, on Nov. 14, 2003. The
researchers used the 48-inch Samuel Oschin Telescope at Caltech's
Palomar Observatory near San Diego. Within days, telescopes in Chile,
Spain, Arizona and Hawaii observed the object. NASA's new Spitzer
Space Telescope also looked for it.

Sedna is extremely far from the Sun, in the coldest know region of our
solar system, where temperatures never rise above minus 240 degrees
Celsius (minus 400 degrees Fahrenheit). The planetoid is usually even
colder, because it approaches the Sun only briefly during its
10,500-year solar orbit. At its most distant, Sedna is 130 billion
kilometers (84 billion miles) from the Sun, which is 900 times Earth's
solar distance.

Scientists used the fact that even the Spitzer telescope was unable to
detect the heat of the extremely distant, cold object to determine it
must be less than 1,700 kilometers (about 1,000 miles) in diameter,
which is smaller than Pluto. By combining available data, Brown
estimated Sedna's size at about halfway between Pluto and Quaoar, the
planetoid discovered by the same team in 2002.

The elliptical orbit of Sedna is unlike anything previously seen by
astronomers. However, it resembles that of objects predicted to lie in
the hypothetical Oort cloud. The cloud is thought to explain the
existence of certain comets. It is believed to surround the Sun and
extend outward halfway to the star closest to the Sun. But Sedna is 10
times closer than the predicted distance of the Oort cloud. Brown said
this "inner Oort cloud" may have been formed by gravity from a rogue
star near the Sun in the solar system's early days.

"The star would have been close enough to be brighter than the full
moon, and it would have been visible in the daytime sky for 20,000
years," Brown explained. Worse, it would have dislodged comets farther
out in the Oort cloud, leading to an intense comet shower that could
have wiped out some or all forms of life that existed on Earth at the
time.

Rabinowitz said there is indirect evidence that Sedna may have a moon.
The researchers hope to check this possibility with NASA's Hubble
Space Telescope. Trujillo has begun to examine the object's surface
with one of the world's largest optical/infrared telescopes, the
8-meter (26-foot) Frederick C. Gillett Gemini Telescope on Mauna Kea,
Hawaii. "We still don't understand what is on the surface of this
body. It is nothing like what we would have predicted or what we can
explain," he said.

Sedna will become closer and brighter over the next 72 years, before
it begins its 10,500-year trip to the far reaches of the solar system.
"The last time Sedna was this close to the Sun, Earth was just coming
out of the last ice age. The next time it comes back, the world might
again be a completely different place," Brown said.

NASA's Jet Propulsion Laboratory, Pasadena, Calif, manages the Spitzer
Space Telescope. For more information about the research and images on
the Internet, visit

http://www.spitzer.caltech.edu/Media/releases/ssc2004-05/

For information about NASA on the Internet, visit 

http://www.nasa.gov

-end-



__
Meteorite-list mailing list
[EMAIL PROTECTED]
http://www.pairlist.net/mailman/listinfo/meteorite-list


RE: [meteorite-list] New Solar system planet discovered

2004-03-16 Thread kenoneill

Hi 

Some Sedna info at :

http://news.bbc.co.uk/2/hi/science/nature/3511678.stm

and 

http://www.nasa.gov/vision/universe/solarsystem/planet_like_body.html


Regards

Ken O'Neill



-Original Message-
From: [EMAIL PROTECTED]
[mailto:[EMAIL PROTECTED] Behalf Of Rafael B.
Torres
Sent: 15 March 2004 17:53
To: [EMAIL PROTECTED]; [EMAIL PROTECTED]
Subject: RE: [meteorite-list] New Solar system planet discovered



Hello List can anyone send more informtion about this new planet found?

_
Help STOP SPAM with the new MSN 8 and get 2 months FREE*  
http://join.msn.com/?page=features/junkmail


__
Meteorite-list mailing list
[EMAIL PROTECTED]
http://www.pairlist.net/mailman/listinfo/meteorite-list


__
Meteorite-list mailing list
[EMAIL PROTECTED]
http://www.pairlist.net/mailman/listinfo/meteorite-list


[meteorite-list] Amgala versus Zag versus DJERMAIA

2004-03-16 Thread Michel Franco
Dear list

I have identified a new individual of the historic fall Djermaia, 25 feb
1961, Chad. Only 2 meteorites are known from this country. And only one
Fall, Djermaia.

It is a H xenolitic Gas rich chondrite, in pristine state of conservation.
regmaglypts, fusion crust of course and flow lines .

The new individual is 2947 g see: www.caillou-noir.com/Djermaia.html

I have sliced off a end cut 95 g and showed it at MNHN in Paris where is
stored the type Specimen of this fall. Michèle Bourot Denise has examined
carfully my end cut and the Djermaia specimen: she is formal about the new
individual I have ( for sale ) it is a new Djermaia Fall stone. She asked me
to make a declaration with her comments at the Nom Com, what I did today.

The Djermaia Fall  declared TKW is 1 kg but Bob Haag has a 3.7 kg stone of
Djermaia according his catalog.

I have left a 2835 g individual for sale. With TKW estimated below 8 kg and
prices according what I ready on the list: I may expect offers above $ 7 per
gram.

If anyone is tented, I will consider them, I am entitled to sell this
meteorite by its owner, Michel Husson.

Best regards.

Michel FRANCO


- Original Message - 
From: "Adam Hupe" <[EMAIL PROTECTED]>
To: <[EMAIL PROTECTED]>
Sent: Sunday, March 14, 2004 10:11 AM
Subject: Re: [meteorite-list] Amgala versus Zag


> Hello All,
>
> At first glance Amgala is somewhat similar looking to Zag.  I do not
believe
> it is going to classify as a regolith breccia but rather a polymict
breccia.
> Unlike Zag, no type 3 areas have been identified.  Two laboratories are
> currently studying Amgala and neither one has observed water bearing
> minerals although some interesting clasts have been found which we will
> report on later.  Another party suggested halite because ~10% of the most
> recently collected broken stones show some oxidation and this would help
to
> explain this.  This was mentioned to a scientists who felt there maybe
some
> water bearing halite but none was found thus far.
>
> As far as the price dropping into the $5.00 to $7.00 a gram range it is
very
> doubtful because there is less than 12 kilograms TKW, fully which half has
> already been sold to collectors for between $7.50 a gram for fragments and
> $12.00 a gram for fully crusted specimens.  Add the fact the seventh and
> final trip to the area by our Moroccan partners only produced five stones
> making it less than cost effective to return to the region.  The last trip
> did not produce enough material to cover the rental rig or diesel costs.
> All indications are that this is a very small fall with precious little
more
> material coming out.  After all, nomads avoid this area and soldiers have
> been methodically searching it for four months now.  Only the soldiers
know
> which areas are safe and which are not and they are done searching because
> of the lack of new finds associated with this fall.
>
> We incurred communication, transportation, purchase material, sample
> material, supplies, shipping and lab fee costs making this a very
expensive
> undertaking.  The fact that 26% of the recovered stones which we paid the
> high field price for turned out to be a black chondrite not related to
this
> fall increased our acquisition costs by nearly the same percentage.  Add
all
> of this together and it was a costly ordeal chasing this one down.
>
> We will update as lab results come in which promise to be interesting.
>
> All the best,
>
> Adam
>
>
> - Original Message -
> From: <[EMAIL PROTECTED]>
> To: <[EMAIL PROTECTED]>
> Sent: Saturday, March 13, 2004 6:23 PM
> Subject: [meteorite-list] Amgala versus Zag
>
>
> > Hello All,
> >
> > Yesterday I received a small individual of Amgala from the Hupes that
was
> probably an individual broken in half. While most of the piece has a
> beautiful black crust, the broken face was quite oxidized, so I decided to
> cut that end off today to see the inside. As stated by Mike and Adam,
Amgala
> is a nice breccia with lots of metal. To me it looks a lot like a fresh
> piece of Zag with it's lightened H6 areas in contrast with the darker
veined
> H4 +/- areas. The darker areas have that same blueish grey look to it as
Zag
> does with lighter chunks and chondrules mixed in. Is Amgala a water
bearing
> meteorite too? The metal I've seen in Zag is more homogeneous, while the
> piece of Amgala I have has more patches of metal in it, especially in the
> lighter H6 like parts.  Amgala's crust is little better than the nicer
> pieces of Zag I have.
> >
> > The amazing thing to me is that they fell in the exact same region of
> Africa... and look very similar...IMHO.
> >
> > All in all Amgala is very nice, but I can see this meteorite eventually
> falling into the $5 to $7 range like most other falls these days...except
> Park Forest that is. The present pricing of $8 to 12/g seems too high to
> me...but then again I bought a piece for $10/g while it is still new to us
> all. :)
> >
> > Reporting in on Amgala,

Re: [meteorite-list] OT: Pluto planet/planetoid

2004-03-16 Thread almitt
Hi Robert, Bernd, Tom and all,

Regardless of efforts trying to redefine Pluto's status, it was a Planet by definition
for 60 some years. I have little doubt that it is a KB object. I know that Clyde
Tombaugh felt it should remain in a planetary status, grand fathered in. I think it
would be respectful to keep it that way but name new found objects as KB's from here
on out. Sort of a contradiction but how a lot of people feel.

Clyde mentioned to me one time (and it is in his book I think) that because of world
war II a percentage of the sky was not surveyed like they had hoped to and even though
those areas of sky were away from the planetary plane there could certainly be lurking
an undiscovered planet.

Initially when the size of Pluto was measured it was thought to be smaller than 4,000
miles or about 6,300 km across. Perhaps Pluto's moon Charon played a part in this.
When Charon was discovered some different models were applied and a smaller diameter
computed. I believe the measurements of Pluto were done at the Hale Telescope (Mt.
Polarmar Observatory) by Gerald Kuiper ironically.

--AL Mitterling




__
Meteorite-list mailing list
[EMAIL PROTECTED]
http://www.pairlist.net/mailman/listinfo/meteorite-list


Re: AW: [meteorite-list] Amgala, Tsarev and Zag

2004-03-16 Thread j . divelbiss
Joern,

Thanx for the clarification on regolith versus the basic breccia types. 

As far as chondrites go...is a genomict breccia with a regolith history like Zag more 
or less unusual when compared to a polymict breccia for chondrites, as in the supposed 
case for Amgala? I ask this since you did point out that achondrites are the ones that 
usually have the polymict breccias, and not chondrites. 

Does this make NWA 1955 (H/L 3-4) a polymict breccia also? Or does its classification 
as being unequilibrated chondrite make it different than a breccia per say?

John

> Tsarev noble gas data data:
> 
> he_3  he_4ne_20   ne_21   ne_22   ar_36   ar_38   ar_40
> 1,58  121 0,540,540,600,420,11575
> 2,07  108 0,780,820,880,830,201635
> all values: x 10E-8 cc STP/g
> 
> Reference: Herzog G. F., Vogt S., Albrecht A., Xue S., Fink D., Klein J., 
> Middleton R., Weber H. W. and Schultz L. (1997) Complex exposure histories for 
> meteorites with "short" exposure ages. Meteoritics 32, 413-422.
> 
> According to this, Tsarev isn't a regolith breccia.
> 
> BTW: A regolith breccia can be either polymict (different source types of 
> clasts, e.g., H3 + L6), xenolithic (some minor exotic (non-host type) clasts, 
> e.g. CM clasts in L6 host), genomict (same material type but different 
> petrologic grades, e.g. H3 + H5), or monomict (e.g. light H3 + dark H3 
> (irradiated) lithologies). Usually, regolith breccias are monomict or genomict 
> breccias. Achondrites are often polymict breccias (e.g. howardites, eucrites, 
> diogenits, ureilites, lunaites).
> 
> Regards,
> Joern
> 
> ___
> Joern Koblitz
> MetBase Editor
> The MetBase Library of Meteoritics and Planetary Sciences
> Benquestrasse 27
> D-28209 Bremen, Germany
> phone: +49 421 24 100 24
> fax: +49 421 24 100 99
> email: [EMAIL PROTECTED]
> ___
> 
> 
> 
> > -Ursprüngliche Nachricht-
> > Von: [EMAIL PROTECTED] [mailto:[EMAIL PROTECTED]
> > Gesendet: Montag, 15. März 2004 21:20
> > An: [EMAIL PROTECTED]
> > Betreff: [meteorite-list] Amgala, Tsarev and Zag
> > 
> > 
> > Adam wrote:
> > 
> > > I do not believe it is going to classify as a
> > > regolith breccia but rather a polymict breccia.
> > 
> > Adam also wrote:
> > 
> > > I thought one distinction made for a regolith breccia is that
> > > there are signs of crystal damage caused by the solar wind
> > 
> > Martin A. chirped:
> > 
> > > Tsarev which is brecciated but not polymict
> > > is also altered by solar winds, isn't it?
> > 
> > Hello Adam, Martin, and List,
> > 
> > There are 3 types of inert and/or noble gases in some meteorites:
> > 
> > (1) those produced by cosmic ray bombardment (cosmogenic);
> > (2) those resulting from radioactive decay of elements (radiogenic)
> > in the meteorite;
> > (3) those present originally (= trapped or primordial gases).
> > 
> > No. (3) is what we are interested in to find out if Amgala, Tsarev
> > and Zag have or have not been altered by solar wind particles.
> > 
> > These gases are 4^He, 20^Ne, 36^Ar, 84^Kr, 132^Xe.
> > 
> > There are two different sources for these inert/noble gases:
> > 
> > (a) solar-type gas
> > (b) planetary-type gas
> > 
> > To find out "what is what" and "which is which", meteoriticists
> > consider the relative amounts and, above all, ratios of a number
> > of isotopes.
> > 
> > J.T. Wasson proposed the following arbitrary
> > definition of a solar gas-rich meteorite:
> > 
> > - The 20^Ne/22^Ne ratio should be greater than 2.5
> > - Ne isotopic data should plot above the dashed line
> >   you find on p. 102 and on p. 111 of Wasson's and
> >   Sears' books (see: Reference)
> > - The 4^He content should exceed 2 x 10^-5 cm^3 g^-1
> > - The 20^Ne / 36^Ar ratio should be greater than 0.3
> > 
> > Unfortunately, I don't have any of these isotope data handy for
> > Tsarev :-( What I do have are some 3^He and 21^Ne data from
> > the MPI Mainz but they are of little help at the moment).
> > 
> > There is an abstract paper by Honda et al. but they only discuss
> > cosmogenic nuclides (see: Reference) - again of little help.
> > 
> > Anyway, Tsarev is a special case and as such mentioned in a
> > research article by S.K. Vogt et al. The authors group Tsarev
> > with a number of other H and L chondrites that underwent a
> > complex "two-stage exposure history":
> > 
> > t1 = 8 million years, radius ca. 200 cm
> > t2 = ca. 0.3 million years, radius ca. 140 cm
> > 
> > 
> > Best wishes,
> > 
> > Bernd
> > 
> > 
> > References:
> > 
> > VOGT S.K. et al. (1993) On the Bur Ghelulai H5 chondrite and other
> > meteorites with complex exposure histories (Meteoritics 28, 
> > 1993, 71-85).
> > 
> > HONDA M. et al. (1992) Cosmogenic nuclides in the
> > Tsarev chondrite (Meteoritics 27-3, 1992, 234-235).
> > 
> > WASSON J.T. (1974) Meteorites Classification 

[meteorite-list] OT: Pluto planet/planetoid

2004-03-16 Thread Matson, Robert



My 2 cents on the 
Pluto planet/planetoid debate:
 
There is one 
commonality shared by Mercury, Venus, Earth, Mars, 
Jupiter,
Saturn, Uranus and Neptune 
-- and NO other known solar system bodies.
They 
each represent more than 50% of the 
total mass of all other bodies
in a 
similar 
orbit.  Note that Ceres 
would not be part of this group -- it 
is
not 
more 
massive than the sum of all 
other asteroids in a similar 
orbit.
Pluto, 
likewise, would not meet this 
requirement -- like Ceres, it is 
the
largest body in its 
type of orbit, but the sum of the masses of all 
other
bodies 
in similar orbits exceeds that of 
Pluto.
 
The nice thing about this 
definition is that it is simple and 
unambiguous.
 
--Rob
 


[meteorite-list] Ebay auctions ending tonight.

2004-03-16 Thread Michael Farmer



http://members.ebay.com/ws2/eBayISAPI.dll?ViewUserPage&userid=meteoritehunters
http://members.ebay.com/ws2/eBayISAPI.dll?ViewUserPage&userid=meteorite-hunter
 
I have alot of meteorite auctions ending tonight. 
Some nice pieces up for grabs. 
Mike Farmer


[meteorite-list] NP, 11-1936 University of Texas collecting Texas meteorites

2004-03-16 Thread MARK BOSTICK
 Paper: Monessen Daily Independent City: Monessen, Pennsylvania Date: Wednesday, November 18, 1936 Page: 5   Records in Texas Show Fall of 38 Meteorites Austin, Texas. - Stars have fallen on Alabama, but meteorites are known to have fallen 38 times on Texas. Dr. H. B. Stenzel, supervisor of the division of geology of the museum, being established by the University of Texas, is gathering samples of the meteorite falls for permanent display. Twelve already are in possession of the university. Three more have been left for display purposes. The largest, lent for centennial display, weighs more than 200 pounds. It was found in 1850 in an Indian reservation on the upper Brazos river. A depression near Odessa, Texas is believed by scientists to have been caused by the largest meteor to strike within the state.       Please visit, www.MeteoriteArticles.com, a free on-line archive of meteor and meteorite articles.


AW: [meteorite-list] Amgala, Tsarev and Zag

2004-03-16 Thread Jörn Koblitz
Tsarev noble gas data data:

he_3he_4ne_20   ne_21   ne_22   ar_36   ar_38   ar_40
1,58121 0,540,540,600,420,11575
2,07108 0,780,820,880,830,201635
all values: x 10E-8 cc STP/g

Reference: Herzog G. F., Vogt S., Albrecht A., Xue S., Fink D., Klein J., Middleton 
R., Weber H. W. and Schultz L. (1997) Complex exposure histories for meteorites with 
"short" exposure ages. Meteoritics 32, 413-422.

According to this, Tsarev isn't a regolith breccia.

BTW: A regolith breccia can be either polymict (different source types of clasts, 
e.g., H3 + L6), xenolithic (some minor exotic (non-host type) clasts, e.g. CM clasts 
in L6 host), genomict (same material type but different petrologic grades, e.g. H3 + 
H5), or monomict (e.g. light H3 + dark H3 (irradiated) lithologies). Usually, regolith 
breccias are monomict or genomict breccias. Achondrites are often polymict breccias 
(e.g. howardites, eucrites, diogenits, ureilites, lunaites).

Regards,
Joern

___
Joern Koblitz
MetBase Editor
The MetBase Library of Meteoritics and Planetary Sciences
Benquestrasse 27
D-28209 Bremen, Germany
phone: +49 421 24 100 24
fax: +49 421 24 100 99
email: [EMAIL PROTECTED]
___



> -Ursprüngliche Nachricht-
> Von: [EMAIL PROTECTED] [mailto:[EMAIL PROTECTED]
> Gesendet: Montag, 15. März 2004 21:20
> An: [EMAIL PROTECTED]
> Betreff: [meteorite-list] Amgala, Tsarev and Zag
> 
> 
> Adam wrote:
> 
> > I do not believe it is going to classify as a
> > regolith breccia but rather a polymict breccia.
> 
> Adam also wrote:
> 
> > I thought one distinction made for a regolith breccia is that
> > there are signs of crystal damage caused by the solar wind
> 
> Martin A. chirped:
> 
> > Tsarev which is brecciated but not polymict
> > is also altered by solar winds, isn't it?
> 
> Hello Adam, Martin, and List,
> 
> There are 3 types of inert and/or noble gases in some meteorites:
> 
> (1) those produced by cosmic ray bombardment (cosmogenic);
> (2) those resulting from radioactive decay of elements (radiogenic)
> in the meteorite;
> (3) those present originally (= trapped or primordial gases).
> 
> No. (3) is what we are interested in to find out if Amgala, Tsarev
> and Zag have or have not been altered by solar wind particles.
> 
> These gases are 4^He, 20^Ne, 36^Ar, 84^Kr, 132^Xe.
> 
> There are two different sources for these inert/noble gases:
> 
> (a) solar-type gas
> (b) planetary-type gas
> 
> To find out "what is what" and "which is which", meteoriticists
> consider the relative amounts and, above all, ratios of a number
> of isotopes.
> 
> J.T. Wasson proposed the following arbitrary
> definition of a solar gas-rich meteorite:
> 
> - The 20^Ne/22^Ne ratio should be greater than 2.5
> - Ne isotopic data should plot above the dashed line
>   you find on p. 102 and on p. 111 of Wasson's and
>   Sears' books (see: Reference)
> - The 4^He content should exceed 2 x 10^-5 cm^3 g^-1
> - The 20^Ne / 36^Ar ratio should be greater than 0.3
> 
> Unfortunately, I don't have any of these isotope data handy for
> Tsarev :-( What I do have are some 3^He and 21^Ne data from
> the MPI Mainz but they are of little help at the moment).
> 
> There is an abstract paper by Honda et al. but they only discuss
> cosmogenic nuclides (see: Reference) - again of little help.
> 
> Anyway, Tsarev is a special case and as such mentioned in a
> research article by S.K. Vogt et al. The authors group Tsarev
> with a number of other H and L chondrites that underwent a
> complex "two-stage exposure history":
> 
> t1 = 8 million years, radius ca. 200 cm
> t2 = ca. 0.3 million years, radius ca. 140 cm
> 
> 
> Best wishes,
> 
> Bernd
> 
> 
> References:
> 
> VOGT S.K. et al. (1993) On the Bur Ghelulai H5 chondrite and other
> meteorites with complex exposure histories (Meteoritics 28, 
> 1993, 71-85).
> 
> HONDA M. et al. (1992) Cosmogenic nuclides in the
> Tsarev chondrite (Meteoritics 27-3, 1992, 234-235).
> 
> WASSON J.T. (1974) Meteorites Classification and Properties
> (Springer-Verlag, Berlin, Heidelberg, New York, pp. 97-109).
> 
> SEARS D.W. (1978) The Nature and Origin of
> Meteorites (Adam Hilger Ltd. Bristol, pp. 110-115).
> 
> McSWEEN H.Y. (1999) Meteorites and Their Parent Planets
> (Cambridge University Press, Glossary, pp. 41-44, 111-112, 244-248).
> 
> 
> __
> Meteorite-list mailing list
> [EMAIL PROTECTED]
> http://www.pairlist.net/mailman/listinfo/meteorite-list
> 

__
Meteorite-list mailing list
[EMAIL PROTECTED]
http://www.pairlist.net/mailman/listinfo/meteorite-list


[meteorite-list] Bring the Paragould Meteorite home

2004-03-16 Thread John Sinclair
http://www.paragoulddailypress.com/articles/2004/03/15/news/news01.txt

Residents attempting to bring the 'Paragould Meteorite' home

PARAGOULD -- If the efforts of the community are successful, Paragould could
once again be home to the phenomenal 800-pound "Paragould Meteorite."

Larry Hancock, a lifelong resident of Paragould, recently became interested
in bringing the cosmic artifact back to northeast Arkansas.

The meteorite, which crashed a few miles southwest of Finch at 4:08 a.m. on
Feb. 17, 1930, is the third largest meteorite ever discovered.

W.H. Hodges, a farmer, discovered the meteorite in a hole that measured
8-feet deep.

After its discovery, meteorite collector Harvey Nininger purchased the
meteorite before selling it for profit to the Field Museum of Natural
History in Chicago.

Today, the meteorite resides at the University of Arkansas in Fayetteville,
where it is being kept on loan from the Field Museum.

Hancock stated he has contacted both UA faculty member Dr. Derek Sears --who
has been instrumental in the displaying of the meteorite at UA-- and
Meenakshi Wadhwa, Field Museum meteorite curator, about the possibility of
bringing the Paragould Meteorite home for public display.

However, the current dilemma resides in the fact that, according to Hancock,
UA officials have not been in violation of the loan requirements, and
therefore, will remain in possession of the meteorite until the Field Museum
determines them to be unsuitable keepers of the relic.

According to Hancock, Sears has not been willing to relinquish possession of
the meteorite, which is being used for scientific purposes at UA.

"If God would've wanted that thing in Fayetteville, he would've landed it
there," Hancock said.

With support from the public, Hancock believes that the Paragould Meteorite
could be brought back to northeast Arkansas.

Paragould Mayor Mike Gaskill stated that he supports the effort, but also
added that Paragould needs a place to house the meteorite during its
displaying in northeast Arkansas.

"The problem is, we don't have anywhere to put it," Gaskill said.

Main Street Paragould Director Sherry Cunningham expressed much of the same
sentiment.

"I believe that this is where it belongs," Cunningham said. "But my question
is 'where do you store it?'"

According to Cunningham, the Greene County Historical Preservation Society
is currently looking into the possibility of finding a home for a Greene
County/Paragould Museum.

Cunningham also added that such an attraction would be a great opportunity
for Greene County and the state, as the Crowley's Ridge Scenic Byway --
Arkansas' only national scenic byway -- passes through downtown Paragould.

"I think we're well overdue for a museum here," Cunningham said. "I think we
need something to show off here in Greene County."

Bettye Busby, president of the Greene County Historical Preservation
Society, stated that the organization would be extremely interested in
displaying the meteorite once the goal of finding a home for a county museum
has been accomplished.

"I think this is where it should be," Busby said, "especially if we do
succeed in getting a museum."

"If it turns out that there are more people interested in it, I would like
to see it come to Paragould," Hancock said. "There's only one 'Paragould
Meteorite,' really. This is a historical thing for us, and it would be a
historical justice for the meteorite to return to Paragould."

At 7 p.m. on April 8, a public meeting will be hosted by the Greene County
Historical Preservation Society at First Presbyterian Church.

According to Busby, this initial meeting will determine the amount of
interest the community has in housing a museum.

"We'd have to have the support of the community to begin, or there'd be no
reason to pursue it," Busby said.

"It's going to be an uphill battle," Hancock said. "Without the support of
the people, it probably will not happen."

According to Hancock, after the meeting on April 8, the next step will
entail gathering support and sending a packet to the Field Museum to request
that the meteorite be sent to Paragould.

"The key," Hancock said, "is getting support."


__
Meteorite-list mailing list
[EMAIL PROTECTED]
http://www.pairlist.net/mailman/listinfo/meteorite-list


[meteorite-list] Pluto - Part 2 of 2

2004-03-16 Thread bernd . pauli
Sky & Telescope, March 1990, pp. 295-296:
A Far Out Planet, George Lovi, excerpt:

Finally, a rather interesting astronomical issue has surfaced as to whether
Pluto should legitimately be included in the roster of nine major planets. Its
decidedly small size (some 2,280 km across) makes it considerably smaller
than any other planet, even smaller than several planetary satellites (including
our own Moon). It also has a most unplanetary, asteroid-like orbit.

For sometime people have suggested that Pluto is an escaped satellite of
Neptune, one resembling Triton. Others have proposed that Pluto might be
some sort of condensed clumping of icy cometary nuclei, or the material that
makes up these bodies.

It's really too bad that we cannot look forward anytime soon to a probe answering
some of our questions about this "neither fish nor fowl" planet - or whatever it 
happens
to be.


CRUIKSHANK D.P. (1999) Pluto and Charon edited by S. Alan
Stern and David Tholen (MAPS 34-4, 1999, 682, excerpt):

While this book is at least a wonderful compilation of our best understanding of Pluto 
and
Charon, it also represents a window on the other small bodies of the outer solar 
system,
notably Triton, a few other outer planet satellites, and the newly revealed population 
of icy
bodies constituting the Kuiper Disk.

Many Kuiper Disk objects share Pluto's orbital resonance with Neptune; vastly more lie
beyond Pluto and form a distribution that may extend to 200 AU or more. Indeed, Pluto
and Charon appear to be only the largest known representatives of this new-found
component of the solar system. Although the exploration of the Kuiper Disk is in its
infancy, this book about the properties of Pluto and Charon in its broader context 
helps
to establish the importance of primitive icy bodies and is a kind of guidebook toward 
the
understanding of their physical properties.

This excellent book is a credit to the Arizona series, to its editors, and to the 
chapter authors.
I recommended it to investigators in the field, advanced students, and science 
libraries without
reservation. (D.P. Cruikshank)



__
Meteorite-list mailing list
[EMAIL PROTECTED]
http://www.pairlist.net/mailman/listinfo/meteorite-list


[meteorite-list] Pluto - Part 1 of 2

2004-03-16 Thread bernd . pauli
Hi Tom, AL, and List,

> I have a book that I recommend her to read or do research from, it is 
> called "Out Of The Darkness" The Planet Pluto by Tombaugh and Moore

The articles Ron posted on Sedna also contain several interesting
passages with regard to Pluto's present status as a planet or a KB
(Kuiper Belt) object, for example:

"Is it a planet? The new discovery will reignite the debate about what constitutes
a planet. One group of astronomers believe that Pluto is not a true planet but merely 
one of the largest of a vast number of minor objects in the outer Solar System. The
alternative standpoint is that Pluto is a planet and those who believe that will have 
to
classify Sedna as the 10th planet."

or:

"Is Sedna a planet? NO, at least not by our definition. Astronomers have been
unable to agree on a precise definition of planet, but we have a suggestion for
a definition below. By our definition, Sedna is not a planet. Nor is Pluto ..."


Here is a review of the book AL mentions:

Sky & Telescope, March 1981, pp. 244-245

Out of the darkness: The planet Pluto

C.W. Tombaugh and Patrick Moore Stackpole
Books, Harrisburg, Pa., 1980, 221 pages - $14.95.

The year 1980, being the 50th anniversary of Pluto's discovery, saw at least three
books devoted to this intriguing little planet. Fortunately, the best has been saved
for last. This modest volume captures the drama of the planet's detection as only
its discoverer could; much of it reads more like a novel than a scientific account of
a series of events. There is relatively little science (see the other books if you want
much of that). Rather, here unfolds the story of the events leading up to the search,
the personalities involved, the project itself, and what happened after the excitement
died down. The second author's contribution is basically to supply background material
and to summarize present knowledge of Pluto.

Since there is not very much known about this small world, this book is almost 
exclusively
a history of its discovery - as all books on this subject more or less are. There are 
16
chapters, 11 being by Clyde Tombaugh. An early autobiographical sketch by Tombaugh
leads to four chapters by Patrick Moore that discuss the discovery of Uranus, the 
asteroids,
and the prediction and identification of Neptune (which sets the stage for the Pluto 
story).
These chapters are quite brief yet cover all the important people and events.

Tombaugh follows with nine more extensive chapters covering the early searches, the
acquisition of the 13-inch astrograph at Lowell Observatory, the photographic program,
the discovery itself, subsequent developments, our knowledge of Pluto since 1930, and
the discovery of its satellite in 1978. Details of the latter event are also 
elaborated by the
discoverer, James W. Christy, in a very nice foreword.

Next is a too short chapter by Moore on Pluto as we now know it, followed by the final 
one
by Tombaugh discussing the possibilities that there might still be something else out 
there,
for which claims have already been made. This reviewer suspects that Tombaugh might be
a bit pessimistic here, but it is probably the caution of experience. 

There are also four appendixes, a helpful glossary, and a rather brief index. The 
first appendix
describes the 50th anniversary celebration in Las Cruces, New Mexico, on February 18, 
1980,
a spectacular affair primarily honoring Tombaugh. It also included a scientific 
symposium
devoted to our present understanding of Pluto, and it is unfortunate that this book 
has no real
discussion of the results.

Other appendixes contain pertinent numerical data and important dates in the Pluto 
story. Finally,
there is a mildly interesting but somewhat irrelevant descriptive scale model of the 
solar system.
The book follows a generally narrative style with relatively few technical details. 
There are no
equations, a few numbers where needed, a variety of good photographs, and a few 
diagrams
of which some, unfortunately, are virtually incomprehensible.

This volume provides generally fascinating reading for anyone with even a mild 
interest in
astronomy, and especially for those interested in planetary astronomy or the history 
of science.
It could even be recommended as supplemental background reading for a general astronomy
course, as a good example of how seemingly dull routine work can be made quite 
interesting.
I would certainly recommend this work to anyone who is interested enough to read the 
book
reviews in Sky And Telescope. ROBERT S. HARRINGTON (U.S. Naval Observatory)

To: [EMAIL PROTECTED]
[EMAIL PROTECTED]
Cc: [EMAIL PROTECTED]


__
Meteorite-list mailing list
[EMAIL PROTECTED]
http://www.pairlist.net/mailman/listinfo/meteorite-list


[meteorite-list] OT, Book Recommendation, Pluto

2004-03-16 Thread MexicoDoug
Asunto: Re: [meteorite-list] OT, Book Recommendation, Pluto 
Fecha:  03/16/2004 8:10:37 AM Mexico Standard Time  
De: MexicoDoug  
Para:   [EMAIL PROTECTED]  



Tom,

Well it sound like you are looking for resources although the title says ... book.  The best bet might actually be a combination of dictionary and internet.

Whether it is pro or con, she will need to start in the dictionary - a trusty reference book.  The term planet is not an astronomical nor technical term.  It has its roots in concept of "wanderers" against the "fixed" stars of the ancient ones.  So the negative that your daughter would like to support could be argued by saying the planets are only the wanderers believed to be recognized by the ancient ones, I don't think that will even include Uranus, definitely not the gas giant Neptune, nor the moon sized Pluto, so there are only six planets.  While one might claim Neptune had been theoretically visible on a clear ancient night to the naked eye to a person with telescopic vision, that would be impossible with Pluto.

If she chooses the technical route, she can search on the internet for orbital eccentricity and inclination of orbit in the solar plane and compare the planets.  (Note planets go through the Zodiac, although the Zodiac actually changes, check the constellation Pluto was in last year).  Then she can search it for formation of the inner and outer planets and why is Pluto not a gas giant if the other outer "planets" are.  Addressing of course whether we have a double standard for the outer and inner planets regarding gas giants and rocks.

Then she can also ignore or the fact that the dictionary sometimes defines asteroids as minor planets.  The wander, have fixed orbits ... and as we know have even differentiated cores in some cases.  That is a two edged axe so maybe she can consider it, as although minor planet has the word planet in it, we are not really taught by our expert kindergarten and primary school teachers that Ceres for example is a planet.

Probably it is a much more persuasive argument that Ceres is a planet.

Hope she has fun.

Saludos
Doug Dawn
Mexico

En un mensaje con fecha 03/16/2004 12:24:05 AM Mexico Standard Time, [EMAIL PROTECTED] escribe:

Asunto: [meteorite-list] OT, Book Recommendation, Pluto 
Fecha: 03/16/2004 12:24:05 AM Mexico Standard Time
De: [EMAIL PROTECTED]
Para: [EMAIL PROTECTED]
Enviado por Internet 



Hello List,
I was wondering if I could get your help.  My daughter is doing
persuasive-research essay.  Her topic of choice is:  Pluto should not be
considered a planet.  Does anybody know of any resources that could help her
justify her argument?
Thanks, Tom
peregrineflier <><
Proudest member of the YMCA # OU812



Re: [meteorite-list] OT, Book Recommendation, Pluto

2004-03-16 Thread almitt
Hi Tom and all,

I have a book that I recommend her to read or do research from, it is called "Out Of
The Darkness" The Planet Pluto by Tombaugh and Moore. Stackpole Books, Harrisonburg,
Pa. Lutterworth Press copyright is 1980. Book has a dark cover with white title and a
artist rendering of Pluto and Charon on the cover. My copy is signed by the author.
Best.

--AL Mitterling


__
Meteorite-list mailing list
[EMAIL PROTECTED]
http://www.pairlist.net/mailman/listinfo/meteorite-list


RE: [meteorite-list] OT: bacteria & ferromanganese nodules

2004-03-16 Thread moni waiblinger-seabridge
Hi List,

be sure when you click on the URL to scroll down. At first it only comes up 
that it needs the latest version of the simplified Chinese language support 
package installed and I almost thought it didn't work. Well, at least on my 
computer.
Otherwise you will find the article and images quite interesting.
Thanks!

Sternengruss, Moni


From: Robert Verish <[EMAIL PROTECTED]>
To: Meteorite-list Meteoritecentral <[EMAIL PROTECTED]>
Subject: [meteorite-list] OT:  bacteria & ferromanganese nodules
Date: Mon, 15 Mar 2004 23:37:20 -0800 (PST)
http://www.scienceinchina.com/yk/yd/0002/yd0187.pdf

On Page 188 in:  SCIENCE IN CHINA (Series D) Vol. 43

Moreover, a combined theory called biology-chemistry
mechanism has been put forward.
Therefore, to find microbe bodies acting as
constructors of the ferromanganese nodules is the key
work to prove the microbe origin theory. For the
reasons above, a high-precision fluoroscope study was
systematically conducted on the ferromanganese nodules
collected from the East Pacific Ocean in 1997, as well
as EPMA research. The result of the study is that a
lot of microbe bodies were discovered in these
ferromanganese nodules and microbic fluorescent
microstructures can be seen in them. The work shows
that the living activities of microbes are closely
related to the origin of the ferromanganese nodules.
1 Samples and study methods --
1.1 Samples -
The studied ferromanganese nodules were collected from
the East Pacific deep sea floor by a scientific
investigation ship of the State Oceanic Administration
in late 1997. Two types of samples were selected from
two sites. No. 161 is an irregular cauliflorate
ferromanganese nodule with a rough surface and a
growing root, collected from the muddy sediments at
the depth of 4,862 m,
11 45.3 N, 139 31.86 W.
The other, No.23562, is a potato-shaped one with a
relatively smooth surface, collected at the
depth of 5,107 m,
10 07.50 N, 154 07.50 W.
1.2 Sample treating -
Since the nodules have high porosity and a high water
content, before slicing, the samples must be
consolidated by a special reagent to fill in the pore
space. According to the analytic requirements of the
fluorescence microscope and EPMA, the glue 502 was
selected as the reagent because it is less fluorescing
and high temperature-resistant. After being
onsolidated the samples are sliced along both the
perpendicular and parallel directions of growing.

Bob V.
__
Do you Yahoo!?
Yahoo! Mail - More reliable, more storage, less spam
http://mail.yahoo.com
__
Meteorite-list mailing list
[EMAIL PROTECTED]
http://www.pairlist.net/mailman/listinfo/meteorite-list
_
Find things fast with the new MSN Toolbar – includes FREE pop-up blocking! 
http://clk.atdmt.com/AVE/go/onm00200414ave/direct/01/

__
Meteorite-list mailing list
[EMAIL PROTECTED]
http://www.pairlist.net/mailman/listinfo/meteorite-list