[meteorite-list] Meteorite Picture of the Day

2013-04-08 Thread valparint
Today's Meteorite Picture of the Day: Berduc

Contributed by: Paul Swartz

http://www.tucsonmeteorites.com/mpod.asp
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Re: [meteorite-list] Chelyabinsk purchase

2013-04-08 Thread M come Meteorite
 On ebay you find many many others for low prices with good crust percentage or 
complete...for me time the snow melts and many many other fragments arrive, and 
the price go down even more

Matteo
 
M come Meteorite Meteoriti
i...@mcomemeteorite.it
http://www.mcomemeteorite.it
http://www.mcomemeteorite.eu
Mindat Gallery
http://www.mindat.org/gallery-5018.html
ChinellatoPhoto Servizi Fotografici
http://www.chinellatophoto.com


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Re: [meteorite-list] AD-Chelyabinsk meteorite now 10% off

2013-04-08 Thread M come Meteorite
 exaggerated prices, on ebay I have buy many similar material for many many 
under this price, type a at 3 gr. piece with 90% crust for 57$
 
Matteo 
 
M come Meteorite Meteoriti
i...@mcomemeteorite.it
http://www.mcomemeteorite.it
http://www.mcomemeteorite.eu
Mindat Gallery
http://www.mindat.org/gallery-5018.html
ChinellatoPhoto Servizi Fotografici
http://www.chinellatophoto.com



Da: meteorite-list-boun...@meteoritecentral.com
A: meteorite-list@meteoritecentral.com
Cc: 
Data: Sat, 6 Apr 2013 19:28:07 -0700 (PDT)
Oggetto: [meteorite-list] AD-Chelyabinsk meteorite now 10% off


 Dear List.
 If you are still searching for a specimen of the Chelyabinsk meteorite here 
 is a link to his site. http://finlandspectrolite.blogspot.jp/
 
 Andrei Barakshan (Finland Spectrolite and Meteorites), has just discounted 
 all by 10% price listed minus 10%. 
 He is a reliable seller and material normally arrives in 7-10 days.
 Best Regards, Dirk Ross...Tokyo
 
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[meteorite-list] Ad: NWA7034

2013-04-08 Thread Ahmad Bouragaa
Dear list,
I want tooffer the last pieces avialable for sole of Black beauty:
82g; 2,6g; 1,9g; 0,5g; 0,4g and 0,3g, enjoy the pictures via this
link:
http://www.flickr.com/photos/36221954@N07/
who's interested contact me off the list
best regards
Ahmad
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[meteorite-list] Comet C/2013 A1 May Postpone India's Mars Mission

2013-04-08 Thread Ron Baalke

http://www.dnaindia.com/scitech/1819996/report-dna-exclusive-comet-mars-isro-s-rs450cr-dream-mission
  

Comet Mars Isro's Rs450cr dream mission
Nirad Mudur
DNA India
April 8, 2013

India's Mars mission is suffering from birth pangs. A comet heading
towards the planet could derail Indian Space Research Organisation's
(Isro) project, worth Rs450 crore, scheduled to take off in
October-November this year.

Scientists are now exploring the possibility of postponing the launch to
allow the comet to pass by Mars before the spacecraft lands.

The comet - C/2013 A1 - is approaching the red planet at a speed of 2
lakh km/hour and has a probability of 1 in 8,000 to strike Mars.

As per current trajectory projections, calculated by US' National
Aeronautics and Space Administration (Nasa), the comet will be closest
to Mars at a distance of 3 lakh km. But the planet will be engulfed in
the tail of the comet - extending to millions of kilometres - which will
be on Mars' sunward side.

The tail of a comet points away from the sun due to radiation effects.

The comet poses a problem because no one knows its precise properties,
and therefore, the effects it'll leave behind. It was discovered only on
January 3 this year by Rob McNaught at the Siding Spring Observatory in
Australia. And our mission will reach the planet just a month before the
comet's arrival.

Isro scientists admit that India'™s Mars mission will be affected by the
comet.

One of the main objectives of the mission is to detect methane in the
Martian atmosphere with a methane sensor for Mars (MSN). The sensor will
be one of the five payloads on board the unmanned spacecraft, which is
expected to orbit the planet at an altitude of 500km after covering a
journey 5.46 crore km through space in nine months.

A senior scientist working on the Mars mission explains how the comet
could scuttle the project.  Most comets have methane, and there is a good 
chance that our MSN payload may confuse the methane it detects from the 
comet as that of Mars and transmit wrong data. Such data will mislead us. 
Even Nasa is wary.

Prof Tushar Prabhu, dean of Bangalore-based Indian Institute of
Astrophysics (IIA), agrees that the comet's tail, which is packed with
methane, will play the spolier. He hopes that Isro will take a guarded
decision on the mission.

M Annadurai, Mars mission project director, is non-committal on whether
the launch date would be pushed ahead, saying it all boils down to the
comet's trajectory. It's too early to say anything right nowbut we
are in touch with Nasa scientists on this.

Although he neither denies nor confirms the rescheduling, he gave enough
hints that the current date - November 27 - of the launch could be changed.

Isro had zeroed in on three launch windows for the mission - November
2013-January 2014, January-April 2016; and April-May 2018.

Isro scientists are not sure if the launch date could be postponed
within the current launch window (November 2013-January2014) or if
they'd have to wait till 2016 or 2018.

But Prof UR Rao, one of India's staunchest supporters for exploring and
colonising Mars and who is also chairman of the governing council of
Isro's Ahmedabad-based Physical Research Laboratory (PRL), suggests that
we have to take some risks.

There is still time [to change plans], says IIA's Prof Prabhu. I hope
Isro scientists take the right decision on time. It will be a difficult
decision.

The presence of methane on Mars is indicative of two things - signs of
life or possibilities of chemical reactions, just like on Earth.

Methane was faintly detected on Mars a few years ago. But its presence
could not confirmed as the Nasa rover then could detect only a larger
volume of the gas at a go - about several parts per billion.

Prof JN Goswami, director of PRL, says India's MSN payload can detect
even faint amounts - 10 parts per billion.

The comet has taken even Nasa by surprise. It, too, will send out a
craft - MAVEN (Mars Atmosphere and Volatile Evolution) - to study Mars'
upper atmosphere in November this year.

The launch was planned much ahead of C/2013 A1's discovery and its close
Mars fly-by. It will reach the planet around the same time as India's
spacecraft.

Isro Mars probe, the victim

Scheduled to be launched on November 27, 2013

Will carry five payloads, including those to detect methane and hydrogen

Will take nine months to reach Mars, which is 54.6 million kilometres away

The problem

Mars will be within the comet's tail from October 19, 2014, but no one
knows for how long

This would confuse the spacecraft-borne detectors about the source of
the gases they are trying to detect

The entire Rs450-crore mission could be affected because the comet's
properties could be confused with those of Mars by the spacecraft's sensors
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[meteorite-list] Remaining Martian Atmosphere Still Dynamic (MSL)

2013-04-08 Thread Ron Baalke

Remaining Martian Atmosphere Still Dynamic
Jet Propulsion Laboratory
April 8, 2013

* This image shows the first holes into rock drilled by NASA's Mars
  rover Curiosity #1
* This illustration shows the instruments and subsystems of the
  Sample Analysis at Mars (SAM) suite on the Curiosity Rover of
  NASA's Mars Science Laboratory Project #2
* the Sample Analysis at Mars (SAM) suite of instruments on NASA's
  Curiosity Mars rover #3
* This image shows the ratio of the argon isotope argon-36 to the
  heavier argon isotope argon-38, in various measurements. #4
* This pair of images taken a few minutes apart show how laser
  firing by NASA's Mars rover Curiosity removes dust from the
  surface of a rock. #5
* The Chemistry and Camera (ChemCam) instrument on NASA's Curiosity
  Mars rover #6
* The Chemistry and Camera (ChemCam) instrument on NASA's Curiosity
  Mars rover analyzes Martian rocks, soils and dust at scales of
  less than 0.04 inch (1 millimeter) #7
* This graph shows about one-fourth of a Martian year's pattern
  atmospheric pressure at the surface of Mars, as measured by the
  Rover Environmental Monitoring Station on NASA's Curiosity rover #8
* This pair of graphs shows about one-fourth of a Martian year's
  record of temperatures (in degrees Celsius) measured by the Rover
  Environmental Monitoring Station (REMS) on NASA's Curiosity rover
  #9
* NASA's Curiosity Mars rover has detected dozens of whirlwinds, or
  vortex events #10
* This graphic tracks the maximum relative humidity and the
  temperature at which that maximum occurred each Martian day for
  about one-fourth of a Martian year, as measured by NASA's
  Curiosity Mars rover #11
* This diagram and the one at PIA16917 illustrate how the Dynamic
  Albedo of Neutrons (DAN) instrument on NASA's Curiosity Mars rover
  detects hydrogen in the ground beneath the rover #12
* This diagram and the one at PIA16916 illustrate how the Dynamic
  Albedo of Neutrons (DAN) instrument on NASA's Curiosity Mars rover
  detects hydrogen in the ground beneath the rover #13

VIENNA -- Mars has lost much of its original atmosphere, but what's left
remains quite active, recent findings from NASA's Mars rover Curiosity
indicate. Rover team members reported diverse findings today at the
European Geosciences Union 2013 General Assembly, in Vienna.

Evidence has strengthened this month that Mars lost much of its original
atmosphere by a process of gas escaping from the top of the atmosphere.

Curiosity's Sample Analysis at Mars (SAM) instrument analyzed an
atmosphere sample last week using a process that concentrates selected
gases. The results provided the most precise measurements ever made of
isotopes of argon in the Martian atmosphere. Isotopes are variants of
the same element with different atomic weights. We found arguably the
clearest and most robust signature of atmospheric loss on Mars, said
Sushil Atreya, a SAM co-investigator at the University of Michigan, Ann
Arbor.

SAM found that the Martian atmosphere has about four times as much of a
lighter stable isotope (argon-36) compared to a heavier one (argon-38).
This removes previous uncertainty about the ratio in the Martian
atmosphere from 1976 measurements from NASA's Viking project and from
small volumes of argon extracted from Martian meteorites. The ratio is
much lower than the solar system's original ratio, as estimated from
argon-isotope measurements of the sun and Jupiter. This points to a
process at Mars that favored preferential loss of the lighter isotope
over the heavier one.

Curiosity measures several variables in today's Martian atmosphere with
the Rover Environmental Monitoring Station (REMS), provided by Spain.
While daily air temperature has climbed steadily since the measurements
began eight months ago and is not strongly tied to the rover's location,
humidity has differed significantly at different places along the
rover's route. These are the first systematic measurements of humidity
on Mars.

Trails of dust devils have not been seen inside Gale Crater, but REMS
sensors detected many whirlwind patterns during the first hundred
Martian days of the mission, though not as many as detected in the same
length of time by earlier missions. A whirlwind is a very quick event
that happens in a few seconds and should be verified by a combination of
pressure, temperature and wind oscillations and, in some cases, a
decrease is ultraviolet radiation, said REMS Principal Investigator
Javier Gómez-Elvira of the Centro de Astrobiología, Madrid.

Dust distributed by the wind has been examined by Curiosity's
laser-firing Chemistry and Camera (ChemCam) instrument. Initial laser
pulses on each target hit dust. The laser's energy removes the dust to
expose underlying material, but those initial pulses also provide
information about the dust.

We knew that Mars 

[meteorite-list] Shaking ExoMars

2013-04-08 Thread Ron Baalke

http://www.esa.int/Our_Activities/Space_Science/Shaking_ExoMars  
  
Shaking ExoMars
European Space Agency
8 April 2013

The structural model of the Entry, Descent and Landing
Demonstrator Module, or EDM, of ESA's 2016 ExoMars mission has
been subjected to a series of intense shaker tests to simulate the
rigours of launching into space.

EDM will be launched to Mars together with the Trace Gas Orbiter
and will test key landing technologies in preparation for the 2018
ExoMars rover mission and subsequent missions to Mars.

The orbiter will search for evidence of methane and other
atmospheric gases that could be signatures of active biological or
geological processes. It will also act as a relay for EDM and the
ExoMars rover, which will search the planet's surface and drill to
depths of 2 m, looking for signs of life, past and present.

Before being launched to the Red Planet, each component of the
mission must undergo thorough testing to certify it for the
journey from Earth to the surface of Mars, and for the harsh space
environment.

EDM arrived at ESTEC, ESA's technical centre in Noordwijk, the
Netherlands, in mid-February, on a lorry from the Turin facility
of Thales Alenia Space in Italy.

After unpacking in one of ESTEC's cleanrooms, it was subjected to
a leak-test, to verify the bio-seal between its main structural
elements, the aeroshell, front shield and back cover.

The bio-seal prevents contamination of the inside of EDM from
Earth-borne organisms during ground transportation and testing.

After that, EDM has undergone a series of vibration tests on the
ESTEC Test Centre Multishaker and QUAD shaker. These intense tests
qualify the spacecraft design by ensuring that it will be able to
withstand the vibrations it will experience when it lifts off on a
Proton rocket in 2016.

During the tests, EDM was mounted on a table where it was shaken
up and down or from side to side for several minutes over a
frequency range of 5 Hz to 2 kHz.

Afterwards, another leak demonstrated that the bio-seal had not
been degraded by the vibration tests.

The EDM structural model has now returned to the Turin factory,
where it will undergo further structural testing. This will
include tests to simulate entering the martian atmosphere and
deploying the module's parachutes.

At Mars, EDM will hit the atmosphere at 21 000 km/h, decelerating
to just 15 km/h in less than 8 minutes.

The ExoMars missions in 2016 and 2018 are being performed by ESA
in partnership with Russia's Roscosmos space agency.

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[meteorite-list] AD: NWA-numbered meteorite that fell in 2009

2013-04-08 Thread Rob Lenssen
Dear List,

I have a very special meteorite for sale:
A 91g stone of NWA 7449: An NWA-numbered meteorite, that fell only as recent
as 2009.

NWA 7449 (L6 S2 W0 ) was found mid-2009, and consists of two stones with a
total known mass of only 405g.
Gamma-spectroscopy has shown that NWA 7449 fell in February or March 2009,
only months before it's find.

Meteoritical Bulletin Database entry for NWA 7449:
http://www.lpi.usra.edu/meteor/metbull.php?code=56103

General information about NWA 7449, its discovery, and the classification
process can be found here:
http://alturl.com/awwyb


For sale is the 91g stone (also mentioned in the MetBul database writeup):
http://alturl.com/kc6z5


If you are interested, please contact me off-list.

Thanks,
Rob Lenssen
IMCA #1681
www.AsteroidChippings.com

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[meteorite-list] AD _ Awesome Auctions Ending In A Few Hours!

2013-04-08 Thread Adam Hupe
Dear List Members,

I have several Awesome auctions ending this evening and some more tomorrow 
night.  Be sure to check out the very odd Sikhote Alin.  It looks like there is 
pink pebble imbedded in it?  Pretty bizarre! 


Link to all auctions:
http://shop.ebay.com/raremeteorites!/m.html


LEGENDARY Northwest Africa 5000 Lunar Meteorite .274g 
http://r.ebay.com/F7iGmH 

NWA 5406 
Very Nice Lunar Moon Meteorite .200g - AWESOME!!! 
http://r.ebay.com/2VOiAC
 
LEGENDARY Northwest Africa 5000 Lunar Meteorite .276g 
http://r.ebay.com/UMhRco 


Bizarre Stone Clast!
Excellent Example Sculptural Sikhote Alin Meteorite 
3.60g NICE - MUST 
SEE!! http://r.ebay.com/PDF47N 

Link to all auctions:
http://shop.ebay.com/raremeteorites!/m.html

Thank you for looking and if you are bidding, good luck,

Adam
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[meteorite-list] House-AD: In Honor of Vesta - Dreampiece (only AHOW-an) and Dreambits

2013-04-08 Thread Martin Altmann
Dear collectors,

the Meteorite House crew is of the opinion, that in all that
Chelyabinsk-hustle it would be unfair to neglect one of our all favorite
luminary;
Goddess Vesta - now where the Dawn spaceprobe said farewell to her (what a
picture!):
http://www.nasa.gov/images/content/685735main_pia15678-43_full.jpg

Dawn, which had made a pass to her in such an unbeseeming manner,
that the wrinkles of the Lady became visible, her pockmarks and the layers
of powder she applied to cover them - and that we got the final missing
evidence, that some of the rocks in our drawers and cabinets are truly of
Vesta's belongings.

Therefore we compiled a little piece, wherein specimens for really everyone
can be found, from the budget collector, who nevertheless doesn't want cut
back in quality
to the toppest notch, who has severe problems to find still something
substantially new for his/her collection.
Four movements we have to play,
but we try to keep it short this time, for not taxing your attention span 
(which is getting shorter and shorter in the FB-ages).

1st) NWA 6475 
Cuuutest pearls and real gems, crusted and fresh individuals of a polymict
eucrite. (All love them. And don't worry, also the highrollers amassing
stones of museums sizes - quite all of them have a feeble for such
miniatures!
And will set 6475 with caution between their Mini-Camel Dongas and
Bilangas).

Btw. also internally NWA 6475 has all, a fine polymict EUC needs, even
larger carbonaceous inclusions, here an example:
http://www.meteoritenhaus.de/img/NWA_6475_end_1_59_g_01.JPG

It's our second lot, the first one went so quickly, that nothing was left to
advertize here, sorry. Same price.

Fresh Individuals (the numbers painted on them are Buhl-numbers from the
Meteorite Recon Coll.):

A)  1.24g   $40
A little bit broken, but in the crack by chance you find a large
eucrite-nest.
http://www.meteoritenhaus.de/img/NWA_6475_1_24_g_01.JPG
http://www.meteoritenhaus.de/img/NWA_6475_1_24_g_02.JPG
http://www.meteoritenhaus.de/img/NWA_6475_1_24_g_03.JPG
http://www.meteoritenhaus.de/img/NWA_6475_1_24_g_04.JPG

B)  1.77g   $57
http://www.meteoritenhaus.de/img/NWA_6475_1_77_g_01.JPG
http://www.meteoritenhaus.de/img/NWA_6475_1_77_g_02.JPG
http://www.meteoritenhaus.de/img/NWA_6475_1_77_g_03.JPG
http://www.meteoritenhaus.de/img/NWA_6475_1_77_g_04.JPG

C)  1.83g   $59
http://www.meteoritenhaus.de/img/NWA_6475_1_83_g_01.JPG
http://www.meteoritenhaus.de/img/NWA_6475_1_83_g_02.JPG
http://www.meteoritenhaus.de/img/NWA_6475_1_83_g_03.JPG
http://www.meteoritenhaus.de/img/NWA_6475_1_83_g_04.JPG

D)  1.94g   $63
http://www.meteoritenhaus.de/img/NWA_6475_1_94_g_01.JPG
http://www.meteoritenhaus.de/img/NWA_6475_1_94_g_02.JPG
http://www.meteoritenhaus.de/img/NWA_6475_1_94_g_03.JPG

E)  3.31g   $107
http://www.meteoritenhaus.de/img/NWA_6475_3_31_g_01.JPG
http://www.meteoritenhaus.de/img/NWA_6475_3_31_g_02.JPG
http://www.meteoritenhaus.de/img/NWA_6475_3_31_g_03.JPG
http://www.meteoritenhaus.de/img/NWA_6475_3_31_g_04.JPG


2nd) Exclusive reference specimens for numbers fetishists.

There we'd have to offer as specialty three different eucrites of newer and
newest NWA-entries. Exclusive they are inasmuch as these numbers are not
available else than through these few references pieces, while the rest of
the masses remained in the private collection of the purchasers + at the
classifying institutes.
Hence stuff and in sizes, which would most probably disproportionally highly
paid,
if thrown into ebay. 
However, they are pretty fresh!

F) NWA 6730

Bulletin entry:
http://www.lpi.usra.edu/meteor/metbull.php?code=54599

A monomict one (monomict eucrites are rarer than polymict ones).
Well fresh, note the fusion crust on the edge.
Displays two lithologies, one is leopardialic Millbillillie-style, the other
coarser (to the left, down).

Two grinded slices in a box:
1.97g + 1.21g = 3.18g   $59

http://www.meteoritenhaus.de/img/NWA6730_3_18_g_01.JPG
http://www.meteoritenhaus.de/img/NWA6730_3_18_g_02.JPG
http://www.meteoritenhaus.de/img/NWA6730_3_18_g_03.JPG


G) NWA 7705
A polymict eucrite and a true beauty.
Nice extra - the finder is given in the Bulletin:
http://www.lpi.usra.edu/meteor/metbull.php?code=57152

Elegant - we like especially the faint whitish cumuli clouds of the matrix,
giving the view depth and the little black clasts and fragments like a flock
of birds playing high in the air.
It's only weakly shocked.

It's even an idea fresher than the first one, as one can detect by means of
the fusion crust.

Two grinded reference slices
3.81g + 1.43g = 5.24g $124

http://www.meteoritenhaus.de/img/NWA7705_5_24_g_01.JPG
http://www.meteoritenhaus.de/img/NWA7705_5_24_g_02.JPG
http://www.meteoritenhaus.de/img/NWA7705_5_24_g_03.JPG


H) NWA 7706

http://www.lpi.usra.edu/meteor/metbull.php?code=57153

Remarkably stronger shocked is that new polymict eucrite.
Had a typical high-gloss-crust,
but unfortunately and despite its 

[meteorite-list] TN GA KY OH AL NC Meteors 08APR2013

2013-04-08 Thread drtanuki
Dear List,
Map is updated and posted.
MBIQ Detects TN GA KY OH AL NC Meteors 08APR2013
http://lunarmeteoritehunters.blogspot.jp/2013/04/mbiq-detects-tn-ga-ky-meteor-08apr2013.html
Dirk Ross...Tokyo
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[meteorite-list] Scientific Articles Accepted (Personal Checks, Too)

2013-04-08 Thread Paul H.
Scientific Articles Accepted (Personal Checks, Too)
by Gina Kolata, New york times, April 7, 2013,
http://www.nytimes.com/2013/04/08/health/for-scientists-an-exploding-world-of-pseudo-academia.html?pagewanted=print
 
or 
http://www.nytimes.com/2013/04/08/health/for-scientists-an-exploding-world-of-pseudo-academia.html

Yours,

Paul H.
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