Re: [meteorite-list] Randall on ebay! Want those aerial shots?!!

2007-10-08 Thread ensoramanda


Yes Sterling...I also found this...!!  At first I thought someone else 
was having a joke...but apparently not!


http://cgi.ebay.com/Ultra-high-res-photos-of-the-Carancas-meteorite-crater_W0QQitemZ300159255522QQihZ020QQcategoryZ3239QQssPageNameZWDVWQQrdZ1QQcmdZViewItem

Sterling K. Webb wrote:


Hi,

   A search of the user name on eBay US
site turns up this less than detailed listing:
http://cgi.ebay.com/ws/eBayISAPI.dll?ViewItemcategory=3810item=300158570494


Sterling K. Webb
--
- Original Message - 
From: ensoramanda [EMAIL PROTECTED]

To: Meteorite-list@meteoritecentral.com
Sent: Sunday, October 07, 2007 9:14 PM
Subject: [meteorite-list] Randall joke on ebay!



Ok...who is the one with the sense of humour after the carancas fragment
on ebay...bidding here :-)
Made me laugh anyway.

http://offer.ebay.co.uk/ws/eBayISAPI.dll?ViewBidsitem=180167268481
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Re: [meteorite-list] Thin Sections of Carancas Meteorite Chondritic or not

2007-10-08 Thread ensoramanda

Hi Elton,

I thought these looked like shock veins...still having trouble knowing 
the difference between shock veins and slickenslides in this one?


http://i117.photobucket.com/albums/o43/LaburnumStudio/DSCN6902.jpg

Graham

Mr EMan wrote:


As to what Rob has raised--I did see several
chondrules in the photos. This looks much like the
friable L;s we have seen and contains slickensides
which would tend to make it a monomyct breccia. 
However these large metal blebs are intriguing and

might make this an anomalous stone.  I didn't see any
thing in the photos which appeared to be a true shock
vein, only the slicken sides.  However for there to be
large blebs/clasts of iron and or olivine in the stone
it must have had a very shocked history with possibly
injected components of an iron or pallasite.  If so,
this might explain the initial declaration that this
was a chondritic pallasite.

Elton


--- Rob Matson [EMAIL PROTECTED] wrote:
 


Based only on the images of the exteriors, I would
consider the specimens very unlikely to be
   


chondritic. But there~are~ some chondrite-like
features in the thin sections (though I wouldn't call
them unambiguously chondrules). The rims are
indistinct,
there are no shock veins visible, and the interference
colors don't seem quite right. I'll forward the images
to a few experts to get their opinions, but if this
 


is a chondrite, it would seem to be a metamorphised,
highly brecciated one. 
--Rob
   


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[meteorite-list] Randall joke on ebay!

2007-10-08 Thread David Kitt Deyarmin

It looks like he's shilling his auction
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[meteorite-list] AD - Ebay Auctions ending soon

2007-10-08 Thread M come Meteorite Meteorites
at some hours some my auctions ended. Take a look to the
rappresentation of the Holbrook fall in the Domenica del
Corriere newspaper in perfect conditions, rare to find.

http://members.ebay.com/ws/eBayISAPI.dll?ViewUserPageuserid=mcomemeteorite


Matteo

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[meteorite-list] Rocks From Space Picture of the Day - October 8, 2007

2007-10-08 Thread SPACEROCKSINC
http://www.spacerocksinc.com/October_8_2007.html   




** See what's new at http://www.aol.com
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[meteorite-list] Publications of the Carancas event

2007-10-08 Thread K. Ohtsuka
Hello list members,

I have just reached the Carancas' publication list site in Peru:

http://fcpn.umsa.bo/fcpn/app?service=page/Planetarium_PublicationList

where some articles have already been introduced by some list members,
but the rest ones are not introduced yet and seem indeed interesting,
although
I cannot understand Spanish at all.

Does anyone translate and introduce their summary?

Best wishes,

Katsu OHTSUKA
Tokyo, JAPAN

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Re: [meteorite-list] Publications of the Carancas event

2007-10-08 Thread K. Ohtsuka
Sorry the link is by Mayor de San Andres Universitys Web site (UMSA)
in Bolivia.

Katsu
 
- Original Message - 
From: K. Ohtsuka [EMAIL PROTECTED]
To: meteorite-list@meteoritecentral.com
Sent: Monday, October 08, 2007 11:37 PM
Subject: Publications of the Carancas event 


 Hello list members,
 
 I have just reached the Carancas' publication list site in Peru:
 
 http://fcpn.umsa.bo/fcpn/app?service=page/Planetarium_PublicationList
 
 where some articles have already been introduced by some list members,
 but the rest ones are not introduced yet and seem indeed interesting,
 although
 I cannot understand Spanish at all.
 
 Does anyone translate and introduce their summary?
 
 Best wishes,
 
 Katsu OHTSUKA
 Tokyo, JAPAN
 
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Re: [meteorite-list] Randall joke on ebay!

2007-10-08 Thread Stefan Brandes

That´s even better ::))

http://offer.ebay.co.uk/ws/eBayISAPI.dll?ViewBidsitem=180167029071

Stefan



Ok...who is the one with the sense of humour after the carancas fragment 
on ebay...bidding here :-)

Made me laugh anyway.

http://offer.ebay.co.uk/ws/eBayISAPI.dll?ViewBidsitem=180167268481
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[meteorite-list] Sale - Nevada meteorite- Starvation Flat , Arizona- Franconia

2007-10-08 Thread wahlperry

Hi,

I have a couple of meteorites for sale. Nevada meteorite Starvation 
Flat L-5 recently listed in the meteorite bulletin.Total mass 1250 
grams . This is one of the larger pieces that I have. Most of the other 
pieces have been spoken for. This is the first time it has been offered 
for sale. 3.00 per gram for a 158 gram piece.


I have two Franconia meteorites that were pictures in Meteorite 
Magazine August 2004 issue. I am asking $2.00 per gram. It would be 
hard to find specimens like these anymore. These are some of the nicest 
ones from the area. I have a 507 and a 617 gram. I will include in situ 
pictures. These meteorites can be viewed on my web page under Arizona 
meteorites.


Email me off list for pictures.
Sonny

www.nevadameteorites.com

Email and AIM finally together. You've gotta check out free AOL Mail! - 
http://mail.aol.com

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Re: [meteorite-list] Randall joke on ebay!

2007-10-08 Thread Michael Farmer
I guess Randall's 4 kilos is not enough, he needs to
buy this piece as well.
I am selling and shipping pieces today, anyone who
wants one, no need to risk your money in Bolivia, you
can have it sent out this afternoon.
Mike
--- Stefan Brandes [EMAIL PROTECTED] wrote:

 That´s even better ::))
 

http://offer.ebay.co.uk/ws/eBayISAPI.dll?ViewBidsitem=180167029071
 
 Stefan
 
 
  Ok...who is the one with the sense of humour after
 the carancas fragment 
  on ebay...bidding here :-)
  Made me laugh anyway.
 
 

http://offer.ebay.co.uk/ws/eBayISAPI.dll?ViewBidsitem=180167268481
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[meteorite-list] New Arizona meteorite on E bay Ad/ Sacramento Wash 02

2007-10-08 Thread Mike Miller
Hi everyone I think I had this formatted wrong so I am sending it
again. I apologize if it comes across twice. Thanks
  Hello everyone sorry to bother you with another E bay a Ad But I do
have something that some of you might be interested in. It is the
first piece of Sacramento Wash 02 ever offered for sale. It is a 41.4
gram fragment, it is the actual piece that ASU cut and classified as
an H4 S1 W1. It fits on to the only other piece I have like a puzzle.
The only other piece known was donated to ASU. So if I cut this
meteorite any other material will be in the form of slices.

I also have a couple of pieces of the Warm Springs meteorite on there.

Thanks to Maria Haas here is a link to my E bay offerings.
http://search.ebay.com/_W0QQsassZflattoprocks
Thanks


-- 
Mike Miller 230 Greenway Dr. Kingman Az 86401
www.meteoritefinder.com
 928-753-6825
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[meteorite-list] AD - my hand made extraordinary scale cube ending on ebay in 4 hours

2007-10-08 Thread Mirko Graul
Hello List,

i have produced a scale cube from Seymchan meteorite
material.
The time for producing this cube was more than 7
hours.
A realy extraordinary cube for your collection.
This cube ending in 4 hours on ebay .

http://cgi.ebay.com/Meteorite-extraordinary-scale-cube-SEYMCHAN-etched_W0QQitemZ300156192929QQihZ020QQcategoryZ3239QQssPageNameZWDVWQQrdZ1QQcmdZViewItem

Thank you for interest

Mirko Graul
IMCA#2113

www.meteorite-mirko.de


   
Yahoo! Clever: Stellen Sie Fragen und finden Sie Antworten. Teilen Sie Ihr 
Wissen. www.yahoo.de/clever

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[meteorite-list] Questions about Uruacu - Shiny Black Inclusions / Images / Etching

2007-10-08 Thread David Kitt Deyarmin
I am processing some Uruacu and some of the pieces have huge shiny black 
inclusions that almost have a mirror like reflective surface.


Does anyone know what these are, you can see a lot of them in this 354 gram 
slice:



http://i131.photobucket.com/albums/p298/BobaDebt/Uruacu/354grSlice1.jpg







Does anyone have any tips on photographing this material.  It doesn't have a 
lot of contrast but the etch looks 1000% better then what this image shows:


http://i131.photobucket.com/albums/p298/BobaDebt/Uruacu/354grSlice2.jpg

I have tried shooting it from various angles, with and with out flash, 
inside, outside, nothing seems to really capture the look of the etch








Speaking of the etch, does anyone have any ideas on how to get more 
contrast, I have tried a variety of Nitric Acid and Ferric Chloride 
Solutions and I have even tried various combination of both.


If anyone can offer any help it would be greatly appreciated.

Thanks 


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Re: [meteorite-list] Randall joke on ebay!

2007-10-08 Thread Alexander Seidel
British humo(u)r striking again (...after that certain Proud T)??  

Alex
Berlin/Germany


 Original-Nachricht 
 Datum: Mon, 8 Oct 2007 17:47:09 +0200
 Von: Stefan Brandes [EMAIL PROTECTED]
 An: Meteorite-list@meteoritecentral.com
 Betreff: Re: [meteorite-list] Randall joke on ebay!

 That´s even better ::))
 
 http://offer.ebay.co.uk/ws/eBayISAPI.dll?ViewBidsitem=180167029071
 
 Stefan
 
 
  Ok...who is the one with the sense of humour after the carancas fragment
  on ebay...bidding here :-)
  Made me laugh anyway.
 
  http://offer.ebay.co.uk/ws/eBayISAPI.dll?ViewBidsitem=180167268481
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[meteorite-list] NEW Angrite - NWA 4801 - AD

2007-10-08 Thread Greg Hupe

Dear List Members,

Another week, another rare and exciting meteorite offering. I would like to 
introduce NWA 4801, what I feel may be the most beautiful angrite yet 
discovered (along with NWA 4590 Tamassint). I have loaded all that I have 
except for a few small fragments on eBay under my seller name, NaturesVault. 
Click here to see all that I currently have to offer, just scroll through 
the pages to see the NWA 4801 Angrite specimens: 
http://search.ebay.com/_W0QQsassZnaturesvault


Here are a couple quick links to show the beauty and importance of NWA 4801:

Photograph of slice displaying matrix and large white anorthite clasts:
http://www.lunarrock.com/nwa4801/nwa4801slice.jpg

Optical thin section image of a 1.5 cm wide slice in partially 
cross-polarized light showing clinopyroxene and olivine (colors), anorthite 
(white to gray) and spinels (black):

http://www.lunarrock.com/nwa4801/nwa4801ts.jpg

Link to the abstract on NWA 4801 for the Workshop on Chronology of 
Meteorites and the Early Solar System in November 2007:

http://www.lpi.usra.edu/meetings/metchron2007/pdf/4050.pdf

Link to abstract reporting ages of NWA 4801, NWA 4590 Tamassint and NWA 
2999:

http://www.lpi.usra.edu/meetings/metchron2007/pdf/4061.pdf

I hope you enjoy the photos and if you are interested, Good Luck getting 
that special specimen for your collection!


See all that I have currently have on eBay here: 
http://search.ebay.com/_W0QQsassZnaturesvault too many to list in this email 
but you will certainly see something you like!


This Wednesday I have a number of other eBay auctions ending, many still at 
just 99 cents. There are also several specialties with Buy it Now so if you 
are interested in anything from planetary, ordinary to extraordinary, or 1-2 
kilo lots, you will find it available by me, seller NaturesVault.


Best regards and Thank You for bidding and/or looking,
Greg



Greg Hupe
The Hupe Collection
NaturesVault (eBay)
[EMAIL PROTECTED]
www.LunarRock.com
IMCA 3163




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[meteorite-list] SALE - Uruacu and Toluca Slices / End Cuts For Sale

2007-10-08 Thread David Kitt Deyarmin

Uruacu and Toluca Slices / End Cuts For Sale

I etched a few pieces of Uruacu and Toluca today and wanted to post them 
here before I listed them on ebay.


I am in the process of taking pictures and updating my web site but that 
will take a few days


You can see some of what I have for sale on my web site at:

http://home.ec.rr.com/bobadebt/Rocks/FS.htm

If you check back be sure to refresh your browser to get the newest images



For now here is a list of everything I have, if you would like pictures of 
info email me off list at bobadebt at ec.rr.com


Thanks


URUACU - 75 CENTS TO $1 PER GRAM

These pieces look a lot better then the images, I have a difficult time 
capturing the etch with digital images.



354 Gram Slice $300

506 Gram End Cut  $506

268 Gram End Cut  $268

83 Gram End Cut $83

66 Gram Slice  $49



TOLUCA - 75 CENTS PER GRAM

623 Gram End Cut  $468

168 Gram End Cut  $126

76 Gram End Cut  $57

69 Gram End Cut  $52

54 Gram End Cut  $40

94 Gram Slice $70

72 Gram Slice $54

28 Gram Slice $21 


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[meteorite-list] Mars Exploration Rover Update - October 8, 2007

2007-10-08 Thread Ron Baalke

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

SPIRIT UPDATE: Rover Experiences Data Backlog - sol 1329-1336, 
October 08, 2007:

Spirit is in good health and on the move toward an appealing field of
boulders at the southwest corner of Home Plate. Preliminary data from
the miniature thermal emission spectrometer indicates these boulders may
be compositionally related to Comanche-class rocks first encountered
on Husband Hill.

Flash memory limited the rover's activities as the volume of memory in
use edged up to more than 70 percent of capacity. After completing work
on a 360-degree panorama from site 3, Spirit had more than 711
megabits of unsent data in flash memory, 453 of which were data from the
panoramic camera. Spirit now has enough power to transmit data to Earth
during overnight Odyssey passes and took advantage of two of those
opportunities this week.

Sol-by-sol summary

In addition to starting and ending each day by measuring atmospheric
dust levels (known as a tau measurement) and surveying the sky and
ground with the miniature thermal emission spectrometer, Spirit
completed the following activities:

Sol 1329 (Sept. 29, 2007): Spirit restarted the Moessbauer spectrometer
and collected data for 22 hours from a target known as Texas Chili.
The rover acquired a 3-by-2-frame mosaic of images of site 3 with the
panoramic camera.

Sol 1330: Spirit acquired a microscopic image mosaic of Texas Chili and
a bore sight of the microscopic imager with the panoramic camera to
check the accuracy of its alignment. The rover then stowed the robotic
arm, surveyed the external calibration target, and acquired a 5-point
survey of the sky and ground with the miniature thermal emission
spectrometer. During the afternoon overpass of the Odyssey orbiter,
Spirit acquired data from a target known as Harmony Point2 with the
miniature thermal emission spectrometer.

Sol 1331: Spirit acquired a 5-by-1 image mosaic of site 3 with the
panoramic camera and completed acquisition of the 360-degree panorama of
the rover's surroundings as viewed from site 3. Spirit also acquired a
6-by-1 mosaic of images with the navigation camera and took thumbnail
images of the sky with the panoramic camera. During the afternoon
Odyssey overpass, the rover surveyed a target known as Ohridiski2 with
the miniature thermal emission spectrometer.

Sol 1332: Spirit acquired a 5-by-1 image mosaic of site 3 and a 4-by-1,
pre-drive image mosaic with the panoramic camera. The rover bumped
backward 50 centimeters (20 inches) and acquired full-color images of
the work volume studied by instruments on the robotic arm using all 13
filters of the panoramic camera. Spirit drove 10.1 meters (33.1 feet)
toward a target area known as site 3a, pausing to take mid-drive
images with the navigation camera. The rover acquired a 5-by-1,
post-drive image mosaic with the navigation camera and a 4-by-1 image
mosaic with the panoramic camera.

Sol 1333: Martian winds cleared away some dust from the solar panels,
resulting in a 1-percent increase in solar power, or about 10
watt-hours. Total solar output for the day was 361 watt-hours (100
watt-hours is the amount of energy needed to light a 100-watt light bulb
for 1 hour). Spirit surveyed the horizon with the panoramic camera and
completed a full-color, systematic ground survey using all 13 filters of
the panoramic camera.

Sol 1334: Spirit completed a survey of rock clasts using the panoramic
camera and then continued to drive toward site 3a. After the drive, the
rover acquired images with the hazard avoidance cameras and a 4-by-1
image mosaic with the navigation camera. Spirit transmitted data to
Odyssey during the overnight pass of the orbiter.

Sol 1335: Spirit completed a 5-point survey and then a 7-point survey of
the sky and ground using the miniature thermal emission spectrometer.

Sol 1336 (Oct. 6, 2007): Spirit monitored dust on the panoramic camera
mast assembly and acquired images with the navigation camera in support
of observations with the miniature thermal emission spectrometer. The
rover then completed a 7-point survey of the sky and ground as well as a
systematic foreground survey with the miniature thermal emission
spectrometer. Spirit transmitted data to the Odyssey orbiter during its
overnight pass. The rover was slated to conduct a 5-point survey of the
sky and ground the next morning with the miniature thermal emission
spectrometer.

Odometry:

As of sol 1333 (Oct. 3, 2007), Spirit's total odometry was 7,244.32
meters (4.5 miles).

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[meteorite-list] Cassini is on the Trail of a Runaway Mystery (Iapetus)

2007-10-08 Thread Ron Baalke

http://www.jpl.nasa.gov/news/news.cfm?release=2007-113

Cassini is on the Trail of a Runaway Mystery
Jet Propulsion Laboratory
October 08, 2007

NASA scientists are on the trail of Iapetus' mysterious dark side, which
seems to be home to a bizarre runaway process that is transporting
vaporized water ice from the dark areas to the white areas of the
Saturnian moon.

This thermal segregation model may explain many details of the moon's
strange and dramatically two-toned appearance, which have been revealed
exquisitely in images collected during a recent close flyby of Iapetus
by NASA's Cassini spacecraft.

Infrared observations from the flyby confirm that the dark material is
warm enough (approximately minus 230 degrees Fahrenheit or 127 Kelvin)
for very slow release of water vapor from water ice, and this process is
probably a major factor in determining the distinct brightness boundaries.

The side of Iapetus that faces forward in its orbit around Saturn is
being darkened by some mysterious process, said John Spencer, Cassini
scientist with the composite infrared spectrometer team from the
Southwest Research Institute, Boulder, Colo.

Using multiple instruments on Cassini, scientists are piecing together a
complex story to explain the bright and dark faces of Iapetus. But yet
to be fully understood is where the dark material is coming from. Is it
native or from outside the moon? It has long been hypothesized that this
material did not originate from within Iapetus, but instead was derived
from other moons orbiting at a much greater distance from Saturn in a
direction opposite to Iapetus.

Scientists are now converging on the notion that the darkening process
in fact began in this manner, and that thermal effects subsequently
enhanced the contrast to what we see today.

It's interesting to ponder that a more than 30-year-old idea might
still help explain the brightness difference on Iapetus, said Tilmann
Denk, Cassini imaging scientist at the Free University in Berlin,
Germany. Dusty material spiraling in from outer moons hits Iapetus
head-on, and causes the forward-facing side of Iapetus to look different
than the rest of the moon.

Once the leading side is even slightly dark, thermal segregation can
proceed rapidly. A dark surface will absorb more sunlight and warm up,
explains Spencer, so the water ice on the surface evaporates. The water
vapor then condenses on the nearest cold spot, which could be Iapetus's
poles, and possibly bright, icy areas at lower latitudes on the side of
the moon facing in the opposite direction of its orbit. So the dark
stuff loses its surface ice and gets darker, and the bright stuff
accumulates ice and gets brighter, in a runaway process.

Scientists say the result is that there are virtually no shades of gray
on Iapetus. There is only white and very dark.

Ultraviolet data also show a non-ice component in the bright, white
regions of Iapetus. Spectroscopic analysis will reveal whether the
composition of the material on the dark hemisphere is the same as the
dark material that is present within the bright terrain.

The ultraviolet data tell us a lot about where the water ice is and
where the non-water ice stuff is. At first glance, the two populations
do not appear to be present in the pattern we expected, which is very
interesting, said Amanda Hendrix, Cassini scientist on the ultraviolet
imaging spectrograph team at NASA's Jet Propulsion Laboratory, Pasadena,
Calif.

Because of the presence of very small craters that excavate the bright
ice beneath, scientists also believe that the dark material is thin, a
result consistent with previous Cassini radar results. But some local
areas may be thicker. The dark material seems to lie on top of the
bright region, consistent with the idea that it is a residual left
behind by the sublimated water ice.

Some other mysteries are coming together. There are more data on the
signature mountain ridge that gives Iapetus its walnut appearance. In
some places it appears subdued. One big question that remains is why it
does not go all the way around.

Was it partially destroyed after it formed, or did it never extend all
the way around the moon? Scientists have ruled out that it is a youthful
feature because it is pitted with craters, indicating it is old. And the
ridge looks too solid and competent to be the result of an equatorial
ring around the moon collapsing onto its surface. The ring theory cannot
explain features that look like tectonic structures in the new high
resolution images.

Over the next few months, scientists hope to learn more about Iapetus'
mysteries.

New Iapetus images, temperature maps and other visuals on Iapetus are
available at: http://saturn.jpl.nasa.gov and http://www.nasa.gov/cassini .

The Cassini-Huygens mission is a cooperative project of NASA, the
European Space Agency and the Italian Space Agency. JPL, a division of
the California Institute of Technology in Pasadena, manages the Cassini
mission for NASA's 

Re: [meteorite-list] Publications of the Carancas event

2007-10-08 Thread Sterling K. Webb
Hi, Katsu, List, and Petrological Fans Everywhere,

Here is a first rough cleaned-up machine translation
of one of the documents on the University of San Andres
website, the most recent petrographic analysis. Please,
any absurdities and holes in the road are likely mine.

A smart machine, the translator; it identified several
usages as Costa Rican. I wonder if oine of the authors
was from Costa Rica. If so, my respect for translating
machines just went up...

Here it is, from
http://fcpn.umsa.bo/fcpn/app?service=external/PublicationDownloadsp=232

ANALYSIS

by

Ing. Hugo Alarcón,
Docente titular de Yacimientos Minerales Metálicos
Ing. Elena Gorinova,
Docente Titular de Mineralogía.


The polished section of a fragment of
the meteorite to been observed by means
of light polarized in the microscope of
reflection, deciding the following minerals
or metals:

MINERAL COMPONENTS AND APPROXIMATE PERCENTAGES
TEANITE (Alloy of Fe with Ni)25-30 %
Mackiwanita-vallerita ((Fe, Ni, Cr) 9S8*   8-10%
Un-identified phase1 %
Rock 50 -- 60 %
* This phase can be named also as TROILITE AND/OR
cosmic periodotite, depending on its chemical
elements and nature with relation to their origin.

GENERAL DESCRIPTION OF THE SAMPLE
The sample is constituted basically by a rock
counterfoil, which includes fragments of teanite,
troilite, of millimeter dimensions, primarily and
minor dimensions to 0.5 mm secondarily, existing
also as particles spread in the rock with dimensions
much changed in the range from 50 to 200 microns and
minors to 20 microns. (Photograph 1)


TEANITE
It appears in anhedral particles with a metallic sheen
of soft color, generally it presents inclusions of
silicates and less of troilita. The Teanite seems
to be partially replaced by the rock and this way
the glazing presents irregular forms. (Photograph 2)


TROILITE
The troilite corresponds to another phase of mineral in the
sample, it is of pink color and strongly anisotrópic, very
similar to periodotite, the library [literally, bibliography] characterizes
this one mineral as Mackiwanita-Vallerita, a isomorphic series
of sulfides of iron with Iron, Nickel, Chromium and Cobalt
but it can be named Troilite when it has a cosmic origin or
also cosmic perriodite. The TroIlite happens as inclusions in
rock and also as inclusions in the Teanite. (Photograph 3).


UN-IDENTIFIED PHASE
A un-identified third phase happens as inclusions in the
Teanite, the phase is of light gray color, isótropic and
it might possibly be loadstone (?). (Photograph 4)


ROCK
The rock is characterized by presenting glazing of the silicates,
and it grazes very thin, the rock has been characterized as a
Peridotite in the petrographic analysis.


CONCLUSIONS
The studies so far of petrography as mineragraphy in the sample
might indicate the sample corresponds to a METEORITE OF THE TYPE
CONDRITE.

The sample is characterized by the predominance of the lithic
phase over the metallic phase (a pallasitic condrite or siderolite)
with a hetereogenous cummulative texture and the following
mineralogical  composition:

Orthopiroxene   70 - 73 %
Olivine  5 - 6 %
Condrules 2 - 3 %
Fitosilicato (mafic mica?)   0.5 %
Metallic Minerals8-10 %
Oxides and hydroxides of Fe  3 - 4 %
Glass 5 - 7 %

The orthopiroxene is probably represented by the variety bronsite,
is in the anhedral form, sometimes of fibrous aspect. It shows
perfect exfoliation, numerous breaks and texture of printfingers.
The sizes are heterogeneous, changing between thin particles of 450
micrometers of length. (Photographs 5,6).


The olivine with anhedral  forms is subrounded, sporadically stuffed
into the intergranular spaces of the orthopiroxenes and generally it
happens as heaps in the rock. Sizes of olivines are homogeneous between
70 and 100 micrometers of diameter. They are observed some light
features of alteration, probably interacting in the interstices
[literally, probably talking each other of idingstita.] (Photographs 7 and 
8)


In the very limited quantity there happens the fitosilicato (mafic mica)
of a scaly aspect, the thinnest, whose exact identification needs study
under the microprobe. The presence of chondrules is clear with forms
that are ferrule-like [esferulìticas ?], refilled by one thinnest substance
of the scaly aspect, fibrously distributed in radial form.
(Photographs 9 and 10).

The metallic phase happens as inclusions and diseminations in the rock.
The glass occurrence is observed, formed by impact in the meteorite.

IDENTIFICATION OF THE SAMPLE:
METEORITE -- CONDRITE OF THE TYPE
(SIDEROLITE) WITH THE LITHIC PHASE
PREDOMINANT, REPRESENTED BY
PERIDOTITE ( THE VARIETY:
ORTHOPIROXENITE OLIVINE).


Re: [meteorite-list] Publications of the Carancas event ADDITIONAL

2007-10-08 Thread Sterling K. Webb
Hi,

I downloaded all the publications on the site (URL below) and
started translating then, but...

One is the earlier analysis which I already translated and posted
a week ago. The two PowerPoint presentations are general
presentations of craters (very nicely done, BTW -- muy bueno!)
but don't mention Carancas. One is a press-release style .pdf
that describes the event and spends a lot of time explaining
what a meteorite is, that they come from the asteroids, that there
are craters elsewhere on the planet, that the world is not ending,
the usual...

There are a few more .pdf are press releases. The only document
with any specifics is their physical estimates of the impact and
such, all taken from playing with the LPI online Impact Calculator;
I recognize the language! Like I haven't already done that 300 times
this last week (and you too).

And if you're keeping score, the Bolivians (unlike the Peruvians)
got the Universal Time of the event right.


Sterling K. Webb

- Original Message - 
From: K. Ohtsuka [EMAIL PROTECTED]
To: meteorite-list@meteoritecentral.com
Sent: Monday, October 08, 2007 9:37 AM
Subject: [meteorite-list] Publications of the Carancas event


Hello list members,

I have just reached the Carancas' publication list site in Peru:

http://fcpn.umsa.bo/fcpn/app?service=page/Planetarium_PublicationList

where some articles have already been introduced by some list members,
but the rest ones are not introduced yet and seem indeed interesting,
although
I cannot understand Spanish at all.

Does anyone translate and introduce their summary?

Best wishes,

Katsu OHTSUKA
Tokyo, JAPAN

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[meteorite-list] new fall south mali.

2007-10-08 Thread habibi abdelaziz
hello list
concerning the new fall south mali , or where ever it
falls, we are still collecting information, for the
date of fall and looking if there is any witnesses,
it's realy not easy to get comunication on border's
with nomades you need to send a bird to get the
information.or to wait.outside that now it's ramadan
and the speed is very slow.
this apart, this new fall is very very fresh and it's
a fantastic meteorite looking like the best fall i
have seen lately , it's 90/100 a type 3.that is
probaly an h chondrite, showing some beauty's inside.
we will be ready with photo soon.
and be ready to get a wonderfull meteorite.
all the best
aziz



  
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Re: [meteorite-list] Slickensides vs Shock Veins Revisited

2007-10-08 Thread Mr EMan
Hello Graham, Bernd, list

While there is no technical definition of a shock
vein so far as I know, it is in wide use and I hold
it to be a version of a healed fracture; healed by
the 1) injection or accumulation of adjacent wall melt
where the filling material has an origin in high
pressure, high temperature phase change or 2) formed
by shock front passage: compression melting followed
by decompression solidification.  In the later case,
material goes from crystalline solid to non
crystalline liquid to non crystalline solid aka
glass within a nano to micro to a second of time. 
Feldspars form masklynite glass but since fledspar in
meteorites are usually limited to small blebs it isn't
a major shock vein component.  

Other silicates such as olivine go through a phase
change and melt only to recrystallize into the mineral
ringwoodite.  In this case the high pressure squeezes
all the extra space out of the crystal matrix on an
atomic level by repacking them but maintaining
molecular bonds  There are other minerals that are
formed by other pyroxenes resulting in similar phase
shifts (majorite, akimotoite, NaAlSi3O8--a felspar,
hollandite and jadeite). Oxides such as chromite also
morph. there presence of these minerals provide
information about the shock history of the parent.

Fractures occur when there is a physical rupture of
adjacent material. It may be unhealed-- meaning a
void filled only by liberated gases or it may be
healed by any one of a several processes. If that
process is shock melting, it is a high pressure, high
temperature event where a rapid cycling of solid-melt-
solid, expands to cement the adjacent sides and
strengthening the fracture. As such, meteorites almost
never fragment along shock veins but across them, from
personal observation. 

When vewing under a hand lens or microscope,
Ringwoodite has a dark almost black yet translucent
appearance, with a slight purple hue. Maskylenite is
transparent and clear.

A fracture can be a slickenside filled with smectite:
a low temperature,low to mid pressure, mechanical
weathering mixture produced as adjacent surfaces mill
and grind each other down. Separation of surfaces
along these is more common as they are natural lines
of weakness.  

Slickensides are striated and the striations generally
orientated in the same direction; shock veins are
smooth and may be branched. Slickensides are opaque
and look like dark shale, graphite, or fusion crust in
color and texture.

I believe that formation of slickensides and shock
veins at the same location in the same event are
mutually exclusive.

So as to your question. I believe that all the veins
seen in this photo represent mid to low pressure, low
temperature fractures of which slickensides are a
subset.  Without examination under a microscope, one
would not be able to positively determine if any shock
veins are present.  Given the clear presence of
slickensides and the appearance of the matrix of this
meteorite to others which have an easily crumbled
consistency (i.e. friable), the occurrence of shock
veins is unlikely--Furthermore, it is extremely remote
that any of these features are from terrestrial
impact.

This meteorite over all appears to have had a really
brutal cosmic history.
EPILOGUE:
That said there is a report that slickensides in
meteorites might be better interpreted as shock
fractures as opposed to analogues of terrestrial
slickensides.
http://adsabs.harvard.edu/abs/1966Metic...3...31D

Elton
For more reading:
http://adsabs.harvard.edu/abs/2004AGUFMMR11A0925X
http://www.nsls.bnl.gov/newsroom/science/2004/06-Chen.htm
http://www3.sympatico.ca/jeff.rowell/Shock.htm
http://www.meteorites.com.au/features/sahara99898.html
http://adsabs.harvard.edu/abs/1966Metic...3...31D
http://books.google.com/books?id=ZnUPIAAJpg=PA182lpg=PA182dq=slickensides+in+meteoritessource=webots=YfWcqNTll-sig=kIPuKfITF2U4paiP_RBNB36db9g

--- ensoramanda [EMAIL PROTECTED] wrote:

 Hi Elton,
 
 I thought these looked like shock veins...still
 having trouble knowing 
 the difference between shock veins and slickenslides
 in this one?

http://i117.photobucket.com/albums/o43/LaburnumStudio/DSCN6902.jpg
 
 Graham
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[meteorite-list] photographing irons

2007-10-08 Thread Laurence Garvie
Regarding photographing irons - I have had good success scanning them  
on a flatbed scanner.  I typically use 1200 dpi and color. Note, this  
can produce a large file. I'll try and send a link to an image tomorrow.


Laurence
CMS
ASU


Message: 5
Date: Mon, 8 Oct 2007 15:38:56 -0400
From: David  Kitt Deyarmin [EMAIL PROTECTED]
Subject: [meteorite-list] Questions about Uruacu - Shiny Black
Inclusions /Images / Etching
To: meteorite-list@meteoritecentral.com
Message-ID: [EMAIL PROTECTED]
Content-Type: text/plain; format=flowed; charset=iso-8859-1;
reply-type=original

I am processing some Uruacu and some of the pieces have huge shiny  
black

inclusions that almost have a mirror like reflective surface.

Does anyone know what these are, you can see a lot of them in this  
354 gram

slice:


http://i131.photobucket.com/albums/p298/BobaDebt/Uruacu/ 
354grSlice1.jpg








Does anyone have any tips on photographing this material.  It  
doesn't have a
lot of contrast but the etch looks 1000% better then what this  
image shows:


http://i131.photobucket.com/albums/p298/BobaDebt/Uruacu/ 
354grSlice2.jpg


I have tried shooting it from various angles, with and with out flash,
inside, outside, nothing seems to really capture the look of the etch







Speaking of the etch, does anyone have any ideas on how to get more
contrast, I have tried a variety of Nitric Acid and Ferric Chloride
Solutions and I have even tried various combination of both.

If anyone can offer any help it would be greatly appreciated.

Thanks



--



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Re: [meteorite-list] photographing irons

2007-10-08 Thread M come Meteorite Meteorites
some my examples

http://www.imagehosting.com/show.php/1233977_WabarMin.jpg.html
http://img166.imageshack.us/img166/8708/udeistation4mingh3.jpg

Matteo

- Original Message -
Da : Laurence Garvie [EMAIL PROTECTED]
A : meteorite-list@meteoritecentral.com
Oggetto : [meteorite-list] photographing irons
Data : Mon, 8 Oct 2007 22:26:47 -0700

 Regarding photographing irons - I have had good success
 scanning them   on a flatbed scanner.  I typically use
 1200 dpi and color. Note, this   can produce a large file.
 I'll try and send a link to an image tomorrow.
 
 Laurence
 CMS
 ASU
 
  Message: 5
  Date: Mon, 8 Oct 2007 15:38:56 -0400
  From: David  Kitt Deyarmin [EMAIL PROTECTED]
  Subject: [meteorite-list] Questions about Uruacu - Shiny
  Black Inclusions /Images / Etching
  To: meteorite-list@meteoritecentral.com
  Message-ID: [EMAIL PROTECTED]
  Content-Type: text/plain; format=flowed;
  charset=iso-8859-1; reply-type=original
 
  I am processing some Uruacu and some of the pieces have
  huge shiny   black
  inclusions that almost have a mirror like reflective
 surface. 
  Does anyone know what these are, you can see a lot of
  them in this   354 gram
  slice:
 
 
  http://i131.photobucket.com/albums/p298/BobaDebt/Uruacu/
  354grSlice1.jpg
 
 
 
 
 --
 -- 
 
 
  Does anyone have any tips on photographing this
  material.  It   doesn't have a
  lot of contrast but the etch looks 1000% better then
  what this   image shows:
 
  http://i131.photobucket.com/albums/p298/BobaDebt/Uruacu/
  354grSlice2.jpg
 
  I have tried shooting it from various angles, with and
  with out flash, inside, outside, nothing seems to really
 capture the look of the etch 
 
 
 
 --
 -- 
 
 
  Speaking of the etch, does anyone have any ideas on how
  to get more contrast, I have tried a variety of Nitric
  Acid and Ferric Chloride Solutions and I have even tried
 various combination of both. 
  If anyone can offer any help it would be greatly
 appreciated. 
  Thanks
 
 
 
  --
 
 
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