Re: [meteorite-list] Kossuth IVA iron meteorite (USA, Iowa, 1975)

2015-02-04 Thread Anne Black via Meteorite-list

I have a very nice slice of Kossuth. 160.8g


Anne M. Black
www.IMPACTIKA.com
impact...@aol.com


-Original Message-
From: cbo via Meteorite-list meteorite-list@meteoritecentral.com
To: meteorite-list meteorite-list@meteoritecentral.com
Sent: Wed, Feb 4, 2015 11:58 am
Subject: [meteorite-list] Kossuth IVA iron meteorite (USA, Iowa, 1975)


Dear Listers!

Iam looking for the Kossuth IVA (USA, Iowa) iron
meteorite.

If you have anybody for sale piece please contact me.

MetBull link of Kossuth IVA iron meteorite:
http://www.lpi.usra.edu/meteor/metbull.php?code=12350


Best Regards!
Zsolt Kereszty
Hungary
IMCA#6251
Meteoritical Society

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[meteorite-list] Meteorite Picture of the Day

2015-02-04 Thread Paul Swartz via Meteorite-list
Today's Meteorite Picture of the Day: NWA 6112 TS

Contributed by: Peter Marmet

http://www.tucsonmeteorites.com/mpodmain.asp?DD=02/04/2015
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[meteorite-list] Calgary, Alberta, Canada Meteor Apprx. 1925 MST 03FEB2015 w/ video

2015-02-04 Thread drtanuki via Meteorite-list
List,


Calgary, Alberta, Canada Meteor Apprx. 1925 MST 03FEB2015 w/ video

http://lunarmeteoritehunters.blogspot.jp/2015/02/calgary-albert-canada-meteor-03feb2015.html

Dirk Ross...Tokyo
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Re: [meteorite-list] Ron Hartman Collection items coming to Tucson

2015-02-04 Thread Raremeteorites via Meteorite-list
Thank you for clarifying this and the well-thought out response.  I will 
make one correction.  There are no such thing as Nevada BLM agents.  They 
are federally employed so have no state boundaries and are free to roam 
about like the rest of the Department of Interior across state lines.


Adam

.


- Original Message - 
From: Robert Verish bolidecha...@yahoo.com
To: meteorite-list@meteoritecentral.com; Raremeteorites 
raremeteori...@centurylink.net

Sent: Tuesday, February 03, 2015 2:13 PM
Subject: Re: [meteorite-list] Ron Hartman Collection items coming to Tucson


Recently returned from a mineralogy symposium and every speaker commented 
on the problem with the BLM and Forest Service obstructing their field 
research.

But that is off-topic.
What is on-topic, and where more discussion needs to be done, is how these 
agencies are increasingly holding back meteorite researchers from 
conducting field work, by requiring more and more paperwork and permits. 
The next fall on public lands will find researchers unable to get to the 
strewn-field in a timely manner, because they will be mired in 
regulations.  The primary concern of these .gov agencies seems to be in 
generating more and more paperwork. My first hand experience with the 
Nevada BLM is that they have little interest in meteorite-recovery and 
even less about meteorite-hunters removing a scant few pounds from the 
surface of the ground.  They seem to have little interest in science, let 
alone hobbyists and their meteorites. So, it is no surprise that they have 
little concern about private property rights.

Good luck in your battles protecting your rights.
Bob V.

-- 
 On Feb 3, 2015, at 1:20 AM, Robert Verish via

 Meteorite-list meteorite-list@meteoritecentral.com
 wrote:

 I'm forwarding a
 message from the curator for the Ron Hartman Collection,
 that he will be in Tucson later this week and will be
making
 available some specimens from that collection.
 Here is a short list of some of the specimens
 being offered for trade or sale:

 ID# 35) Clover Springs Mesosiderite 6.6255 g. V. Good
Corner slice. (SMB)
 ID# 37) Bensour, Morocco Ordinary Chondrite, LL6 5.69 g.
Individual. Fell
2-11-2002
 ID# 49) Cleo Springs Ordinary Chondrite, H4 53.9 g. Good
Slice
 ID# 55) Songyuan [label has printed:
 Fuyu, (proposed name)] Jilin, China Ordinary Chondrite,
H5 13.75 g.
Part-slice. Fell 8-15-1993 (ex. mhmeteorites)
 ID# 56) Hebron Stone H6 Brecciated 17.19 g. Good Part
slice. Thayer Co.
Nebraska
 ID# 70) Silver Dry Lake Ordinary Chondrite, L4 S2 W2 1.272
g. Good endcut,
nice fusion crust. [On HOLD]
 ID# 79) Dar al Gani DaG 749 Carbonaceous Chondrite CO3
12.622 g. V. Good -
Rectangular slice.
 ID#380) Sahara SAH 99433 OC Stone 56.86 g. V. Good thick
complete slice.
 ID#875) Pallasovka Pallasite 11.0 g. V. Good quarter-circle
slice.

 The curators contact information will not be known until
after he arrives
in Tucson. In the meanwhile,
 if you are interested in making an offer or trade, you can
reply to me and
I will relay your messages.

 Bob Verish
 __







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Re: [meteorite-list] Ron Hartman Collection items coming to Tucson

2015-02-04 Thread Robert Verish via Meteorite-list
Recently returned from a mineralogy symposium and every speaker commented on 
the problem with the BLM and Forest Service obstructing their field research.  
But that is off-topic.  
What is on-topic, and where more discussion needs to be done, is how these 
agencies are increasingly holding back meteorite researchers from conducting 
field work, by requiring more and more paperwork and permits.  The next fall on 
public lands will find researchers unable to get to the strewn-field in a 
timely manner, because they will be mired in regulations.  The primary concern 
of these .gov agencies seems to be in generating more and more paperwork. My 
first hand experience with the Nevada BLM is that they have little interest in 
meteorite-recovery and even less about meteorite-hunters removing a scant few 
pounds from the surface of the ground.  They seem to have little interest in 
science, let alone hobbyists and their meteorites. So, it is no surprise that 
they have little concern about private property rights.  
Good luck in your battles protecting your rights. 
Bob V. 

-- 
  On Feb 3, 2015, at 1:20 AM, Robert Verish via
  Meteorite-list meteorite-list@meteoritecentral.com
  wrote:
 
  I'm forwarding a
  message from the curator for the Ron Hartman Collection,
  that he will be in Tucson later this week and will be
 making
  available some specimens from that collection.
  Here is a short list of some of the specimens
  being offered for trade or sale:
 
  ID# 35) Clover Springs Mesosiderite 6.6255 g. V. Good
 Corner slice. (SMB)
  ID# 37) Bensour, Morocco Ordinary Chondrite, LL6 5.69 g.
 Individual. Fell 
 2-11-2002
  ID# 49) Cleo Springs Ordinary Chondrite, H4 53.9 g. Good
 Slice
  ID# 55) Songyuan [label has printed:
  Fuyu, (proposed name)] Jilin, China Ordinary Chondrite,
 H5 13.75 g. 
 Part-slice. Fell 8-15-1993 (ex. mhmeteorites)
  ID# 56) Hebron Stone H6 Brecciated 17.19 g. Good Part
 slice. Thayer Co. 
 Nebraska
  ID# 70) Silver Dry Lake Ordinary Chondrite, L4 S2 W2 1.272
 g. Good endcut, 
 nice fusion crust. [On HOLD]
  ID# 79) Dar al Gani DaG 749 Carbonaceous Chondrite CO3
 12.622 g. V. Good - 
 Rectangular slice.
  ID#380) Sahara SAH 99433 OC Stone 56.86 g. V. Good thick
 complete slice.
  ID#875) Pallasovka Pallasite 11.0 g. V. Good quarter-circle
 slice.
 
  The curators contact information will not be known until
 after he arrives 
 in Tucson. In the meanwhile,
  if you are interested in making an offer or trade, you can
 reply to me and 
 I will relay your messages.
 
  Bob Verish
  __
 
 
 
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[meteorite-list] Kossuth IVA iron meteorite (USA, Iowa, 1975)

2015-02-04 Thread cbo via Meteorite-list
Dear Listers!

Iam looking for the Kossuth IVA (USA, Iowa) iron 
meteorite.

If you have anybody for sale piece please contact me.

MetBull link of Kossuth IVA iron meteorite:
http://www.lpi.usra.edu/meteor/metbull.php?code=12350


Best Regards!
Zsolt Kereszty
Hungary
IMCA#6251
Meteoritical Society

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[meteorite-list] UNM scientist studies the authenticity of meteorites

2015-02-04 Thread Shawn Alan via Meteorite-list
Hello Listers

Enjoy :)

Shawn Alan
IMCA 1633 
ebay store http://www.ebay.com/sch/imca1633ny/m.html
Website http://meteoritefalls.com 


UNM scientist studies the authenticity of meteorites

In 2011, Carl Agee received a rock in the mail from a meteorite
collector in Morocco. At the time, nobody knew what it was or where it
had come from. Even for Agee, director of UNM’s Institute for
Meteoritics, the rock’s origin remained a mystery for quite some time.

“This collector sent it to me because no one knew what it was, and it
took me months of laboratory analyses to figure it out,” Agee said.

At the Department of Earth and Planetary Sciences, he tested the
rock’s chemical composition, isotopic composition, and mineralogy to
determine its makeup.

“From all of those different lines of evidence, the picture that
emerged was that it was a meteorite from Mars,” he said.

Now, Agee is being funded by NASA to study the meteorite, known as NWA
7034, or “Black Beauty” for its dark color.

There are several reasons why NASA is interested in Black Beauty. Tests
showed that it contains 10 to 30 times more water than any previously
studied Martian sample. Agee and his team also found that the meteorite
is composed of a variety of minerals, ranging from 4.4 to 2.1 billion
years old.

“There are different fragments of the Martian crust all together in
the same meteorite in addition to the water, so there’s a record of
the surface processes on Mars for about two billion years,” Agee said.

Black Beauty is also notable, Agee said, because it is very similar to
the rock samples that are currently being collected by the two rovers on
Mars, which use a robotic remote sensing technique to identify the
rocks’ composition.

“Black Beauty finally forms the first tangible meteorite link to the
rocks that NASA’s rovers are sampling in outcrops on Mars,” Agee
wrote in the Universities Space Research Association’s report for the
Eighth International Conference on Mars. He notes that the meteorite
provides insight into volcanic activity on the planet, which is one of
his research specialties.

While Agee is best known for his work in meteoritics, he was originally
trained as a geologist, which is how he began researching volcanoes. He
said he became interested in planetary geology while working on his
doctoral degree at Columbia University.

“If you’re trained in geology, planets are like whole new worlds to
map out and understand,” Agee said.

After finishing at Columbia, he taught at Harvard for eight years before
moving to Houston to work at NASA’s Johnson Space Center. He said he
came to UNM because he enjoys the intellectual atmosphere of a
university.

“I have contracts for NASA that I work on, so I’m still involved
with them,” Agee said. “In addition to Black Beauty, they have also
funded me for years to study the processes of planetary volcanism.”

He uses the department’s high-pressure laboratory to simulate the
conditions of planetary interiors to study the behavior of magma, he
said.

Source: http://www.dailylobo.com/article/2015/02/2-4-agee-profile
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[meteorite-list] Met Bulletin Update - NWA, Lunar and Achondrites,

2015-02-04 Thread Galactic Stone Ironworks via Meteorite-list
Hi Bulletin Watchers,

There are 9 new approvals from the NWA DCA.  There is one lunar,
several achondrites of various types, and one OC.

Link : 
http://www.lpi.usra.edu/meteor/metbull.php?sea=%2Asfor=namesants=falls=valids=stype=containslrec=50map=gebrowse=country=Allsrt=namecateg=Allmblist=Allrect=phot=snew=1pnt=Normal%20tabledr=page=0

Best regards and Happy Huntings,

MikeG

-- 
-
Web - http://www.galactic-stone.com
Facebook - http://www.facebook.com/galacticstone
Twitter - http://twitter.com/galacticstone
Pinterest - http://pinterest.com/galacticstone
-
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[meteorite-list] Rosetta Swoops In For A Close Comet Encounter

2015-02-04 Thread Ron Baalke via Meteorite-list


http://www.esa.int/Our_Activities/Space_Science/Rosetta/Rosetta_swoops_in_for_a_close_encounter

Rosetta Swoops In For A Close Encounter
European Space Agency
4 February 2015

ESA's Rosetta probe is preparing to make a close encounter with its comet 
on 14 February, passing just 6 km from the surface.

Yesterday was Rosetta's last day at 26 km from Comet 67P/Churyumov-Gerasimenko, 
marking the end of the current orbiting period and the start of a new 
phase for the rest of this year.

Today, Rosetta is moving into a new path ahead of a very close encounter 
next week. First, it will move out to a distance of roughly 140 km from 
the comet by 7 February, before swooping in for the close encounter at 
12:41 GMT (13:41 CET) on 14 February. The closest pass occurs over the 
comet's larger lobe, above the Imhotep region.

The upcoming close flyby will allow unique scientific observations, providing 
us with high-resolution measurements of the surface over a range of wavelengths 
and giving us the opportunity to sample – taste or sniff – the very innermost 
parts of the comet’s atmosphere,” says Matt Taylor, ESA’s Rosetta project 
scientist.

The flyby will take Rosetta over the most active regions of the comet, 
helping scientists to understand the connection between the source of 
the observed activity and the atmosphere, or coma.

In particular, they will be looking for zones where the outflowing gas 
and dust accelerates from the surface and how these constituents evolve 
at larger distances from the comet.

The comet's surface is already known to be very dark, reflecting just 
6% of the light that falls on it. During the close flyby, Rosetta will 
pass over the comet with the Sun directly behind, allowing shadow-free 
images to be collected. By studying the reflectivity of the nucleus as 
it varies with the angle of the sunlight falling on it, scientists hope 
to gain a more detailed insight into the dust grains on the surface.

After this close flyby, a new phase will begin, when Rosetta will execute 
sets of flybys past the comet at a range of distances, between about 15 
km and 100 km, says Sylvain Lodiot, ESA's spacecraft operations manager.

It was always planned to change from bound orbits to flyby trajectories 
at this point in the mission, based on predictions of increasing cometary 
activity. The range of flyby distances also balances the various needs 
of Rosetta's 11 instruments in order to optimise the mission's scientific 
return.

During some of the close flybys, Rosetta will encounter the comet almost 
in step with the rotation, allowing the instruments to monitor a single 
point on the surface as it passes by.

Meanwhile, the more distant flybys will provide the broader context of 
a wide-angle view of the nucleus and its growing coma.

We're in the main science phase of the mission now, so throughout the 
year we'll be continuing with high-resolution mapping of the comet, says 
Matt.

We'll sample the gas, dust and plasma from a range of distances as the 
comet's activity increases and then subsides again later in the year.

Perihelion, closest approach to the Sun, occurs on 13 August when the 
comet and Rosetta will be 186 million kilometres from the Sun, between 
the orbits of Earth and Mars.

In the month before perihelion, as activity is reaching a peak, the team 
are planning to study one of the comet's jets in greater detail than ever.

We hope to target one of these regions for a fly-through, to really get 
a taste of the outflow of the comet, adds Matt.

After perihelion and once the comet's activity begins to subside, the 
mission team will determine if and when to return to a bound orbit around 
the comet, and how long Rosetta might be able to operate beyond the end 
of 2015.

Follow the Rosetta blog and the @ESA_Rosetta and @esaoperations twitter 
accounts for further details on the upcoming spacecraft operations.

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[meteorite-list] New Horizons Returns New Images of Pluto En Route to Historic Encounter

2015-02-04 Thread Ron Baalke via Meteorite-list


February 4, 2015
 
NASA Spacecraft Returns New Images of Pluto En Route to Historic Encounter

NASA's New Horizons spacecraft returned its first new images of Pluto on 
Wednesday, as the probe closes in on the dwarf planet. Although still just a 
dot along with its largest moon, Charon, the images come on the 109th 
birthday of Clyde Tombaugh, who discovered the distant icy world in 1930.

My dad would be thrilled with New Horizons, said Clyde Tombaugh's 
daughter Annette Tombaugh, of Las Cruces, New Mexico. To actually see the 
planet that he had discovered, and find out more about it -- to get to see 
the moons of Pluto-- he would have been astounded. I'm sure it would have 
meant so much to him if he were still alive today.

New Horizons was more than 126 million miles (nearly 203 million kilometers) 
away from Pluto when it began taking images. The new images, taken with New 
Horizons' telescopic Long-Range Reconnaissance Imager (LORRI) on Jan. 25 
and Jan. 27, are the first acquired during the spacecraft's 2015 approach 
to the Pluto system, which culminates with a close flyby of Pluto and its 
moons on July 14.

This is our birthday tribute to Professor Tombaugh and the Tombaugh 
family, in honor of his discovery and life achievements -- which truly became 
a harbinger of 21st century planetary astronomy, said Alan Stern, New 
Horizons principal investigator at the Southwest Research Institute (SwRI) in 
Boulder, Colorado. These images of Pluto, clearly brighter and closer than 
those New Horizons took last July from twice as far away, represent our first 
steps at turning the pinpoint of light Clyde saw in the telescopes at Lowell 
Observatory 85 years ago, into a planet before the eyes of the world this 
summer.

Over the next few months, LORRI will take hundreds of pictures of Pluto, 
against a starry backdrop, to refine the team's estimates of New 
Horizons' distance to Pluto. As in these first images, the Pluto system 
will resemble little more than bright dots in the camera's view until late 
spring. However, mission navigators can still use such images to design 
course-correcting engine maneuvers to direct the spacecraft for a more 
precise approach. The first such maneuver based on these optical navigation 
images, or OpNavs, is scheduled for March 10.

Pluto is finally becoming more than just a pinpoint of light, said Hal 
Weaver, New Horizons project scientist at the Johns Hopkins University 
Applied Physics Laboratory in Laurel, Maryland. LORRI has now resolved 
Pluto, and the dwarf planet will continue to grow larger and larger in the 
images as New Horizons spacecraft hurtles toward its targets. The new LORRI 
images also demonstrate that the camera's performance is unchanged since it 
was launched more than nine years ago.

Closing in on Pluto at about 31,000 mph, New Horizons already has covered 
more than 3 billion miles since it launched on Jan. 19, 2006. Its journey has 
taken it past each planet's orbit, from Mars to Neptune, in record time, 
and it is now in the first stage of an encounter with Pluto that includes 
long-distance imaging as well as dust, energetic particle and solar wind 
measurements to characterize the space environment near Pluto.

The U.S. has led the exploration of the planets and continues to do so 
with New Horizons, said Curt Niebur, New Horizons program scientist at 
NASA Headquarters in Washington. This mission will obtain images to map 
Pluto and its moons better than has ever been achieved by any previous 
planetary mission.

APL manages the New Horizons mission for NASA's Science Mission Directorate 
in Washington. Alan Stern, of SwRI, is the principal investigator and leads 
the mission. SwRI leads the science team, payload operations and encounter 
science planning. New Horizons is part of the New Frontiers Program, managed 
by NASA's Marshall Space Flight Center in Huntsville, Alabama. APL designed, 
built and operates the spacecraft.

To view the Pluto image online and see the mission timeline for upcoming 
images, visit:

http://www.nasa.gov/newhorizons 

and

http://pluto.jhuapl.edu 

-end-

Dwayne Brown
Headquarters, Washington
202-358-1726
dwayne.c.br...@nasa.gov 

Michael Buckley
Johns Hopkins University Applied Physics Laboratory, Laurel, Md.
240-228-7536
michael.buck...@jhuapl.edu 

Maria Stothoff
Southwest Research Institute, San Antonio
210-522-3305
maria.stoth...@swri.org 

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[meteorite-list] AD: New Rumuruti

2015-02-04 Thread Aras Jonikas via Meteorite-list
Dear List:

For those of you unable to make it to Tucson (like me...), I have several new 
stones to offer in the very near future. I loaded the first of the bunch to my 
site today. NWA 8720 is an R4 Rumuruti priced at a VERY reasonable $20/g.  Only 
several slices and an endcut(with beautiful crust) available. I will be loading 
one crooked slice on ebay tomorrow.

www.AJmetcltr.com/NWA8720

Thanks for peeking, and stay tuned for several more soon!

Aras
IMCA# 2117
www.AJmetcltr.com
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[meteorite-list] MRO HiRISE Images: February 4, 2015

2015-02-04 Thread Ron Baalke via Meteorite-list


MARS RECONNAISSANCE ORBITER HIRISE IMAGES
February 4, 2015

o Tangential Craters within Ptolemaeus Crater   
  http://hirise.lpl.arizona.edu/ESP_020065_1335

  This image shows two small craters, just touching on their 
  rims, in the much larger Ptolmaeus Crater.

o Curiosity Rover at Pahrump Hills  
  http://hirise.lpl.arizona.edu/ESP_039280_1755

  The region contains sedimentary rocks that scientists believe 
  formed in the presence of water.

o Yardangs in Arsinoes Chaos
  http://hirise.lpl.arizona.edu/ESP_039563_1730

  Yardangs are portions of rock that have been sand blasted into 
  long, skinny ridges by bouncing sand particles blowing in the wind.

o Icy Wonderland
  http://hirise.lpl.arizona.edu/ESP_039633_0950

  The weak boundaries of the polygonal structure of the surface have 
  been eroded by spring sublimation of carbon dioxide as energy from 
  the Sun turns ice to gas. 

All of the HiRISE images are archived here:

http://hirise.lpl.arizona.edu/

Information about the Mars Reconnaissance Orbiter is 
online at http://www.nasa.gov/mro. The mission is 
managed by NASA's Jet Propulsion Laboratory, a division 
of the California Institute of Technology, for the NASA 
Science Mission Directorate, Washington, D.C. Lockheed 
Martin Space Systems, of Denver, is the prime contractor 
and built the spacecraft. HiRISE is operated by the 
University of Arizona. Ball Aerospace and Technologies 
Corp., of Boulder, Colo., built the HiRISE instrument.

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[meteorite-list] Meteorite Picture of the Day

2015-02-04 Thread Paul Swartz via Meteorite-list
Today's Meteorite Picture of the Day: NWA 1951

Contributed by: Peter Marmet

http://www.tucsonmeteorites.com/mpodmain.asp?DD=02/05/2015
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