Dear Bernhad,
Yes, but where's the dirt?
What? No dirt? You mean oh METEORITES
That's interesting.
Michael
on 9/5/04 12:00 PM, Bernhard Rems at [EMAIL PROTECTED] wrote:
With all the politics going on here now (and internal politics as well),
I thought you
What's that around your neck Bernhard?
Has anyone been to the Soutpan crater near Pretoria in South Africa?
When I was a student pilot we used to fly over it, it was a strange
feeling as the ground dropped away. I lived 50km away and never visited!
Now I'm way too far away.
Hello Cj,
According to the CD-Rom made by Pierre-Marie Pele about NWAs, the TKW of NWA
237 (LL6) is 61g.
I do not know about SAU 119.
All the best,
Frederic Beroud
www.meteoriteshow.com
IMCA #2491
- Original Message -
From: Peanut .. [EMAIL PROTECTED]
To: [EMAIL PROTECTED]
Sent: Sunday,
Bernhard Rems wrote:
Hmm...
I never saw that Michael made accusations against Mauro Daniel. I can
remember that he accused a certain Matteo - but this Matteo was banned
from the list, if I remember correctly (or he said he would leave
forever, don't quite remember), so I really don't understand
Frederic Beroud wrote:
According to the CD-Rom made by Pierre-Marie
Pele about NWAs, the TKW of NWA 237 is 61g.
Also does anyone have information on SAU 119?
SaU 119, H4; S2; W4
Find Jan 20, 2002
21° 00.2' N / 57° 18.9' E
TKW 472 grams / 1 stone
Classification: S. Afanasiev
Analysis: A.
Also in Met.Bull. 88 (MAPS 39-8, 2004, August, pp. A199-A213):
Report
Oral histories in meteoritics and planetary science XIII :
F r e d L. W h i p p l e
Author: U.B. Marvin
__
Meteorite-list mailing list
[EMAIL PROTECTED]
METEORITE NAME: NWA 2225
COUNTRY/STATE: Morocco/Algeria
CLASS:Ureilite
DATE OF FALL/FIND: 2003
TKW:40 gram
SPECIMEN WEIGHT:1,99 gram
SPECIMEN DESCRIPTION: Part slice
Remarks: Very fine specimen
Picture on request
To whom it concerns - I just got this mail :
Hi Bernd, Hope things are well with you over there. Can you
tell me how I go about unsubscribing from the meteorite list?
Can't find my original email and I've had enough of all the
ranting; life's too short.
.. and this mail does not come from
Greetings
I've got a meteorite question. Having seen enough Raman data to be
convinced that the diamonds in urelites are formed by shock
compression, I'm wondering - does anyone have an opinion on what sort
of meteorite they started out as? They had to have been carbonaceous
meteorites of
I wonder why this kind of crazy fight happens from time to time on the
meteorite list, as if some people miss it when topics are only related to
meteorites, without any conflict to take part... I've been a member for
almost two years now, and still manage to bear those periods of crazyness,
Hopefully Bernd they will come back again like other very respected, highly
esteemed, intelligent, long-time member(s) of this list have!
All the best,
Greg
Greg Redfern
JPL NASA Solar System Ambassador
http://www.jpl.nasa.gov/ambassador/index.html
International Meteorite Collectors Association
Hello,
I am not a scientist and therefore not able to analyse Raman data futher
than seing which type of mineral was hit by the laser beam. But I have also
heard that some scientits suggest that some diamonds in Ureilites could be
presolar, and therefore not necessarily formed by shock... Also, I
Here Here!! Jerry Flaherty
- Original Message -
From: meteoriteshow [EMAIL PROTECTED]
To: [EMAIL PROTECTED]; [EMAIL PROTECTED]
Sent: Monday, September 06, 2004 1:53 PM
Subject: Re: [meteorite-list] Ain't it a s * h * a * m * e ? ? ?
I wonder why this kind of crazy fight happens from
Hi list,
please have a look at the Cabin Creek and an few other meteorite
pictures I took
at the Vienna Museum of Natural History in February 2004.
http://www.marmet-meteorites.com/
... just to help you find back to the topic of this wonderful list:
Meteorites!!!
Peter Marmet
They had to have been carbonaceous meteorites of some sort to begin
with, but the articles I've seen don't seem to offer a clear picture
of what they were like before they were shocked. CM, perhaps?
Hello Marc, Frédéric, and List,
Here is what I've harvested during the last few minutes:
Hello All and whoever wants to leave,
I just wanted to say that the real shame here is that somebody here is
letting this get to them. This is going to happen in ANY forum or mailing
list. this person shouldn't punish or deny themselves the other information
and conversation that is put out on
Hi Bernd and all,
I cannot help but be continually amazed that
people choose to leave the list rather than learn to
use their DELETE button. I just don't get it. When
one of these ridiculous rant exchanges occur, there
are TWO dead giveaways:
1) the SENDER posting to the list at that
Thanks for your response Bernd!
As far as CI are concerned, yes they have no chondrule and I did not think
of them before writing my e-mail. But then the oxygen-isotope study is
getting us confused... CV?...
As far as I know, there was no evidence of presolar diamonds existence. Am I
right or
In a message dated 9/6/2004 11:42:01 AM Mountain Standard Time,
[EMAIL PROTECTED] writes:
To whom it concerns - I just got this mail :
Hi Bernd, Hope things are well with you over there. Can you
tell me how I go about unsubscribing from the meteorite list?
Can't find my original email and
Bernd and List,
Aside from the origin of ureilites, it appears that traces of chondrules are
found in polymict ureilites and are probably from impactors - like the
chondrules sometimes found in howardites. See Mr. Weir's page on DaG 319.
I might be lucky enough to have a thin section of DaG
Hi
Here is the last sales ad from me.
I have 3 specimens to sell as one deal.
-A 9,9 gram whole Juancheng individual 99 % crusted.
-A nice10,6 gram Zag, full slice, very brechiated, very blueish aperance.
-And finaly a very nice NWA 788 , whole individual, 9,96 gram
Anyone who will PayPal me
Hi All,
I have two very nice partial individuals of Pasamonte, both with crust and Nininger
numbers. However one is highly attracted to a magnet, while the other is not.
Before jumping to all kinds of speculation, I would like to ask a favor of this List
that really uses the power of a
Bernd and List,
Hi John and List,
Aside from the origin of ureilites, it appears that traces of chondrules
are found in polymict ureilites and are probably from impactors - like
the chondrules sometimes found in howardites. See Mr. Weir's page
on DaG 319.
I might be lucky enough to have
In addition to Peter´s own pics here is a link to a photo
of the famous Hraschina meteorite, from the museum´s website:
http://www.nhm-wien.ac.at/NHM/Mineral/pic/11HRASCH.htm
I have been there only a few weeks ago and will return in
February next year. What a museum, and what a display - just
Hi Martin list,
I used one of the rare earth magnets (about 1 oz - identical to
the one taped very near the end of my meteorite cane). These magnets
are so powerful you will get a blood blister if any flesh is between the
surfaces when you put one within 4 to 6 inches of iron. VERY
Hello Martin and all,
Nice experiment. I have two specimens for your database:
1. 100% crusted individual; oriented, 7 grams, Nininger #197.hh
2. a cut, crusted fragment, 6.32 grams
Neither one has the slightest attraction to a strong rare earth magnet
(circular 1 dia., 1/4 thick)
By the way,
Lars, I've tried to send this privately but it bounced so I'll take the
three for $55 [EMAIL PROTECTED] if they're not already spoken for. Jerry
- Original Message -
From: Solvænget [EMAIL PROTECTED]
To: Meteorite List [EMAIL PROTECTED]
Sent: Monday, September 06, 2004 3:55 PM
Subject:
Hi List,
I am trying to locate a small etched slice of meteorite which would show
the finest octahedrite widmanstatten lines .2 mm.
If someone has an answer, please email me.
Thanks
Jerry A. Baird
__
Meteorite-list mailing list
[EMAIL PROTECTED]
Hola Martin,
Your question about Pasamonte is a very interesting one for me, because last night I
was pondering the same thing for some terrestrial rocks found while meteorite hunting
Sunday. I got a total of about 40 hematite nodules shaped from nice kidney-rose
balls to a crinoidal
29 matches
Mail list logo
