Re: [meteorite-list] Habital Planet Discovery Announcement

2010-09-30 Thread Matthias Bärmann


See you there at the Bar, Guido. Icecubes not necessary, and heavy enough to 
rest for a while. Waiting for very strange meteorites to come in.


Best, Matthias


- Original Message - 
From: countde...@earthlink.net

To: meteorite-list@meteoritecentral.com
Sent: Thursday, September 30, 2010 1:37 AM
Subject: [meteorite-list] Habital Planet Discovery Announcement



Hello List,

Maybe...just maybe...

http://news.yahoo.com/s/afp/20100929/sc_afp/usastronomyplanet_20100929210707

Best to all,

Count Deiro
IMCA 3536

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[meteorite-list] Tr : Tr : AW: nwa 5400 pairing to nwa 5363

2010-09-30 Thread habibi abdelaziz
hi all,

albert wrote today to me.
he said,
'

I did write to Norbert. He has the data now. .



thanks albert for your effort and your help ;
and thanks norbert for helping this issue to move on to  the good way.
do we have this  data now
all the best

aziz habibi


 - Message transféré  De : Norbert Classen riffr...@timewarp.de À : 
habibi abdelaziz azizhab...@yahoo.com; meteorite list 
meteorite-list@meteoritecentral.com Envoyé le : Mer 29 septembre 2010, 23h 
11min 20s Objet : AW: [meteorite-list] nwa 5400 pairing to nwa 5363 Dear Aziz 
 
All, You wrote:  he said too that he has given all the data that confirm  
the 
pairing including the isotope to norbert classen in  end june where they talk 
abaout this and as i asked him  to do so. Maybe there's a slight 
misunderstanding here. I actually emailed with Dr. Jambon in June, and we also 
intended to meet at the Ste. Marie Show at the end of June where Dr. Jambon 
wanted to show me all the data (including the O-isotope data). However, 
unfortunatelly we missed each other at the show, and so the meeting didn't 
take 
place. Don't get me wrong, I have no reason to doubt Dr. Jambon's word on this 
- 
I just wanted to get the facts straight. Maybe you misunderstood Dr. Jambon? 
But 
up to this day I haven't seen the O-isotope data for NWA 5363. All I have seen 
is a writeup on NWA 5363 which didn't include the O-isotope data. Again, that 
doesn't mean much, and I'm also looking forward to the official publication of 
NWA 5363. This will hopefully answer all the questions. We all need to 
remember 
that meteorite classification (including the voting process on new meteorites 
at 
the NomCom of the Meteoritical Society) takes time. So we as collectors 
should, 
IMHO, be patient, and wait with conclusions until the scientific work has been 
done and published. All the best, Norbert -Ursprüngliche Nachricht- hi 
all and i m happy that this issue is becoming a very polit and civilised 
discussion; well 3 months that i do not want to get caught inside this 
discussion any more, but well this is becoming repeated to a point that we 
forget what the debat is about, for nwa 5363; i get a talk on albert jambon 
mobile , i asked him that many dealers or collectors still think that nwa 5400 
is not paired to nwa 5363 and he answered me this. he said that he have 
submited 
to the nomcom all the information, and he coudln't have said that they are 
paired if he haven't done isotope so clearly he  indicate that he has done 
isotope and have submited them to the nomcom dr wisberg or so , its on the 
phone. and  he said he is surprised why the nomcom didn't pubilsh them yet, he 
said too that he has given all the data that confirm the pairing including the 
isotope to norbert classen in end june where they talk abaout this and as i 
asked him to do so. so i ask here do we have any guy from the nomcom here , 
please end this torture and tell us if you have this data or not,and why you 
didn't publish them. thanks aziz habibi 
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--
Albert JAMBON

UPMC Univ  Paris 06
(UMR 7193) Institut des Sciences de la Terre Paris
Laboratoire Magie  46-0 4eme étage, Case 110

4 place jussieu 75252 Paris Cedex O5 France
Tel: 33 (0) 144 27 51 35
FAX: 33 (0) 144 27 39 11

Vient de paraître : Géochimie : géodynamique et cycles
http://www.dunod.com/auteur-dunod-9782100516124-76933-albert-jambon.html

Parcours de Planétologie d'Ile de France
http://www.aerov.jussieu.fr/themes/APACHE/PlanetoIDF/index.html

Site du master SDUEE
http://www.master.sduee.upmc.fr


  
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Re: [meteorite-list] Habital Planet Discovery Announcement

2010-09-30 Thread Martin Altmann
Yep,

Any emerging life forms on the new planet would have a wide range of stable
climates to choose from and to evolve around, depending on their longitude,
Vogt said.

If it has a bound rotation, one side always facing the sun
and if it has a dense atmosphere, and if it has water - then I would expect
it to have a catastrophic climate.

(And we'd need moore gravity for not being blown away by the
tempests...)

Martin

-Ursprüngliche Nachricht-
Von: meteorite-list-boun...@meteoritecentral.com
[mailto:meteorite-list-boun...@meteoritecentral.com] Im Auftrag von Sterling
K. Webb
Gesendet: Donnerstag, 30. September 2010 04:28
An: countde...@earthlink.net; meteorite-list@meteoritecentral.com
Betreff: Re: [meteorite-list] Habital Planet Discovery Announcement

Hi, Count, List,

Also reported here:
http://www.space.com/scienceastronomy/earth-like-exoplanet-possibly-habitabl
e-100929.html

The finder is excessively enthusiastic about the chances
of life. There are problems with a three-earth-mass. It
will not be like a Big Earth. It's more complicated than
that.  (The Yahoo article has the mass wrong, BTW.)

   If you start with the same recipe mix of ingredients
as the Earth and just made a bigger batch of planet, is
it just the same as the Earth, only more so? Nope,
more of the same is definitely not the same.

   If the Earth were bigger, the volume of water would
increase faster than the increase in surface area, so the
oceans would be deeper. Because of the deeper
oceans and the greater gravity, the pressures at the
bottoms of those oceans would be much higher.

   Continents and their mountains would be much
lower, because the temperatures in the crust would
increase faster with depth, until the fluid point would
be reached in the crust instead of the mantle like it is
on our Earth. Mountains can only pile up until the
pressures under them are about 3000 to 3500
atmospheres, and that zone would be reached at
shallower and shallower depths on a bigger and
bigger Earth.

   Since the solid crust of a larger Earth would be
much thinner, heat transfer to the surface much faster,
vulcanism much livelier, plate tectonics much zippier.

   This Earth has a diameter 1.40 times that of our Earth:
11,200 miles across. It would have twice the surface area,
2.75 times the volume, and 3 times the mass (compressibility
squishes). It's surface gravity would be 51% greater. If the planet
is four Earth masses, its diameter would be 1.58 times the
Earth's without accounting for compressibility and about
1.50 to 1.53 Earth radii squished. Its surface gravity would
be 73% greater than the Earth's, in that case.

But I'll continue to calculate based on three E-masses...

   Because it would have 3 times the water but only two
times the surface, the average ocean depth would be about
4500 meters! The pressure at the depths of these oceans
would be about 9000 atmospheres. The highest mountains
possible would be about 4000 meters (calculating from the
median diameter), so if you were the greatest mountain
climber on this Super Earth, standing on the top of Super
Earth's highest mountain, you would still have 500 meters
of water above you!

   On our Earth, the crust is about 30 kilometers thick, but
the lithosphere (rocks that stay stiff and not slushy and
slippy) is about 75 kilometers, so the Earth's lithosphere
contains all the crust and the top part of the mantle.

   The crust of the Super Earth would be about 60 km thick, but
the lithosphere would only be about 40 kilometers thick. This
means that it would be very difficult to sink pieces of crust
(subduction) and equally difficult to bring deep basalt magmas
to the surface.

   On the other hand, the Super Earth's silicate crust would be
recylced very rapidly with lots of local vulcanism and lots of
hotspots and have a very similar composition everywhere. The
only weathering that would be possible would be chemical,
because all the volitiles are released into the oceans rather
than the atmosphere.

  So a bigger Earth is not just a bigger Earth. Knowing that
somebody will ask how much bigger a bigger Earth has to be
before there's no land at all, just oceans, the answer is:
somewhere between 2-1/2 and 3 Earth masses is the point
where the median ocean depths equal the height of the
highest possible mountain.

   Whoops! No continents. This Super Earth is a WaterWorld!
Possibly very few islands. That's serious. It means No Surfing,
because there's no land for the waves to break on. It's almost
certain that it would have more water than our Earth, because
the star is metall-poor (see below).

 A red dwarf is a main sequence star: once a dwarf, always a
dwarf. It's just a low-mass star with a longer lifetime (25 billion
years?) than our Sun (10 billion years?). At a third of a solar
mass, it's got a respectable little heliosphere and all the
usual solar (or stellar) apparatus, just less extensive than a
G0 dwarf star like us. But it doesn't have as big 

[meteorite-list] Specific Gravity Question

2010-09-30 Thread David Gunning

Hi All,

I'm a confessed specific gravity advocate for all things mineralogical,
including meteorites.  It seems to me that there is very little useful
specific gravity information on the web concerning meteorites, with the
singular exception of Randy L. Korotev', excellent website at Washington
University in St. Louis;  an informative website listing various specific
gravity values for various meteorite types and classifications.

It occurs to me that many people may not be taking specific gravity
measurements of their meteorite specimens because of some sort of biased
but unfounded fear of specimen contamination. Is this true?

One of the benefits of measuring specific gravity is in being able to
spot density anomalies in meteorites.  For example, you procure a small
meteorite specimen of a meteorite has been classified as an L ordinary
stoney chondrite, with a range of specific gravity values, as found on
Professor Korotev' s.g. list, of between 2.50 and 3.96 (with an average
s.g. of 3.35).  When you, yourself,  measure the specific gravity of your
L chondrite, and it's s.g. value comes in at 4.06, what does that mean?

Would such a s.g. reading #1: be possible?  And #2: be meaningful?

Are meteorite specific gravity values exclusively constrained to the
range of values that the scientists peg them at?

And, if not, if actual specific gravity measurements cam occur outside
the conventionally accepted range of values of the experts, should
anyone give a hoot one way or another?

Best wishes,

Dave Gunning













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Re: [meteorite-list] Specific Gravity Question

2010-09-30 Thread Peter Scherff
Hi,

Here is the way around contamination
http://www.psrd.hawaii.edu/Aug99/densityMeasure.html. Guy Consolmagno has
published data for hundreds of meteorites.

Peter

-Original Message-
From: meteorite-list-boun...@meteoritecentral.com
[mailto:meteorite-list-boun...@meteoritecentral.com] On Behalf Of David
Gunning
Sent: Thursday, September 30, 2010 6:46 AM
To: meteorite-list@meteoritecentral.com
Cc: davidgunn...@fairpoint.net
Subject: [meteorite-list] Specific Gravity Question


Hi All,

I'm a confessed specific gravity advocate for all things mineralogical,
including meteorites.  It seems to me that there is very little useful
specific gravity information on the web concerning meteorites, with the
singular exception of Randy L. Korotev', excellent website at Washington
University in St. Louis;  an informative website listing various specific
gravity values for various meteorite types and classifications.

It occurs to me that many people may not be taking specific gravity
measurements of their meteorite specimens because of some sort of biased
but unfounded fear of specimen contamination. Is this true?

One of the benefits of measuring specific gravity is in being able to
spot density anomalies in meteorites.  For example, you procure a small
meteorite specimen of a meteorite has been classified as an L ordinary
stoney chondrite, with a range of specific gravity values, as found on
Professor Korotev' s.g. list, of between 2.50 and 3.96 (with an average
s.g. of 3.35).  When you, yourself,  measure the specific gravity of your
L chondrite, and it's s.g. value comes in at 4.06, what does that mean?

Would such a s.g. reading #1: be possible?  And #2: be meaningful?

Are meteorite specific gravity values exclusively constrained to the
range of values that the scientists peg them at?

And, if not, if actual specific gravity measurements cam occur outside
the conventionally accepted range of values of the experts, should
anyone give a hoot one way or another?

Best wishes,

Dave Gunning













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[meteorite-list] [Fwd: RE: Specific Gravity Question]

2010-09-30 Thread David Gunning
--- Original Message 
Subject: RE: [meteorite-list] Specific Gravity Question
From:David Gunning davidgunn...@fairpoint.net
Date:Thu, September 30, 2010 7:55 am
To:  Peter Scherff petersche...@rcn.com
-

Howdy,

Thanks for the e-burp.

There was no link, however, to the published data for hundreds of
meteorites, mentioned in your e-burp.  Why allude to information that
cannot be referenced and verified?

While it's interesting to read of your specific gravity bead method,
there are other less convoluted ways or dealing with the fear of
potential contamination in meteorites and mineral samples, in general.

What particularly interests me is exploring ways and utilizing lower tech
methods that bring the ordinary collector into the the loop.

Your suggested method would seem to exclude that possibility.



 Hi,

   Here is the way around contamination
 http://www.psrd.hawaii.edu/Aug99/densityMeasure.html. Guy Consolmagno has
 published data for hundreds of meteorites.

 Peter

 -Original Message-
 From: meteorite-list-boun...@meteoritecentral.com
 [mailto:meteorite-list-boun...@meteoritecentral.com] On Behalf Of David
 Gunning
 Sent: Thursday, September 30, 2010 6:46 AM
 To: meteorite-list@meteoritecentral.com
 Cc: davidgunn...@fairpoint.net
 Subject: [meteorite-list] Specific Gravity Question


 Hi All,

 I'm a confessed specific gravity advocate for all things mineralogical,
 including meteorites.  It seems to me that there is very little useful
 specific gravity information on the web concerning meteorites, with the
 singular exception of Randy L. Korotev', excellent website at Washington
 University in St. Louis;  an informative website listing various specific
 gravity values for various meteorite types and classifications.

 It occurs to me that many people may not be taking specific gravity
 measurements of their meteorite specimens because of some sort of biased
 but unfounded fear of specimen contamination. Is this true?

 One of the benefits of measuring specific gravity is in being able to
 spot density anomalies in meteorites.  For example, you procure a small
 meteorite specimen of a meteorite has been classified as an L ordinary
 stoney chondrite, with a range of specific gravity values, as found on
 Professor Korotev' s.g. list, of between 2.50 and 3.96 (with an average
 s.g. of 3.35).  When you, yourself,  measure the specific gravity of your
 L chondrite, and it's s.g. value comes in at 4.06, what does that mean?

 Would such a s.g. reading #1: be possible?  And #2: be meaningful?

 Are meteorite specific gravity values exclusively constrained to the
 range of values that the scientists peg them at?

 And, if not, if actual specific gravity measurements cam occur outside
 the conventionally accepted range of values of the experts, should
 anyone give a hoot one way or another?

 Best wishes,

 Dave Gunning













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 http://www.meteoritecentral.com/mailing-list-archives.html
 Meteorite-list mailing list
 Meteorite-list@meteoritecentral.com
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Re: [meteorite-list] [Fwd: RE: Specific Gravity Question]

2010-09-30 Thread peterscherff
Hi Dave, 

Father Guy's results are published in Meteoritics. I am at work now and can't 
look up the issue/s. 

Thanks, 

Peter 
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Re: [meteorite-list] [Fwd: RE: Specific Gravity Question]

2010-09-30 Thread Sterling K. Webb

Hi, Dave,

You should try actually reading the references that
people give to help you with your question. If you
had, you would have found the citation to the published
data in about 30 seconds, just like I did:

Consolmagno, G. J. and D. T. Britt, 1998, The Density
and Porosity of Meteorites from the Vatican Collection,
Meteoritics and Planetary Science, vol. 33, p. 1231-1241.

Getting unpaid internet access to a scholarly journal is
another matter, though.


Sterling K. Webb
--
- Original Message - 
From: David Gunning davidgunn...@fairpoint.net

To: meteorite-list@meteoritecentral.com
Cc: davidgunn...@fairpoint.net
Sent: Thursday, September 30, 2010 7:08 AM
Subject: [meteorite-list] [Fwd: RE: Specific Gravity Question]


--- Original 
Message 

Subject: RE: [meteorite-list] Specific Gravity Question
From:David Gunning davidgunn...@fairpoint.net
Date:Thu, September 30, 2010 7:55 am
To:  Peter Scherff petersche...@rcn.com
-

Howdy,

Thanks for the e-burp.

There was no link, however, to the published data for hundreds of
meteorites, mentioned in your e-burp.  Why allude to information that
cannot be referenced and verified?

While it's interesting to read of your specific gravity bead method,
there are other less convoluted ways or dealing with the fear of
potential contamination in meteorites and mineral samples, in general.

What particularly interests me is exploring ways and utilizing lower 
tech

methods that bring the ordinary collector into the the loop.

Your suggested method would seem to exclude that possibility.




Hi,

Here is the way around contamination
http://www.psrd.hawaii.edu/Aug99/densityMeasure.html. Guy Consolmagno 
has

published data for hundreds of meteorites.

Peter

-Original Message-
From: meteorite-list-boun...@meteoritecentral.com
[mailto:meteorite-list-boun...@meteoritecentral.com] On Behalf Of 
David

Gunning
Sent: Thursday, September 30, 2010 6:46 AM
To: meteorite-list@meteoritecentral.com
Cc: davidgunn...@fairpoint.net
Subject: [meteorite-list] Specific Gravity Question


Hi All,

I'm a confessed specific gravity advocate for all things 
mineralogical,
including meteorites.  It seems to me that there is very little 
useful
specific gravity information on the web concerning meteorites, with 
the
singular exception of Randy L. Korotev', excellent website at 
Washington
University in St. Louis;  an informative website listing various 
specific

gravity values for various meteorite types and classifications.

It occurs to me that many people may not be taking specific gravity
measurements of their meteorite specimens because of some sort of 
biased

but unfounded fear of specimen contamination. Is this true?

One of the benefits of measuring specific gravity is in being able to
spot density anomalies in meteorites.  For example, you procure a 
small
meteorite specimen of a meteorite has been classified as an L 
ordinary
stoney chondrite, with a range of specific gravity values, as found 
on
Professor Korotev' s.g. list, of between 2.50 and 3.96 (with an 
average
s.g. of 3.35).  When you, yourself,  measure the specific gravity of 
your
L chondrite, and it's s.g. value comes in at 4.06, what does that 
mean?


Would such a s.g. reading #1: be possible?  And #2: be meaningful?

Are meteorite specific gravity values exclusively constrained to the
range of values that the scientists peg them at?

And, if not, if actual specific gravity measurements cam occur 
outside

the conventionally accepted range of values of the experts, should
anyone give a hoot one way or another?

Best wishes,

Dave Gunning













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[meteorite-list] Rocks from Space Picture of the Day - September 30, 2010

2010-09-30 Thread Michael Johnson
http://www.rocksfromspace.org/September_30_2010.html
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[meteorite-list] NASA's EPOXI Mission Sets Up for Comet Hartley 2 Flyby

2010-09-30 Thread Ron Baalke

http://www.jpl.nasa.gov/news/news.cfm?release=2010-317  

NASA's EPOXI Mission Sets Up for Comet Flyby
Jet Propulsion Laboratory
September 29, 2010

PASADENA, Calif. - Earlier today, navigators and mission controllers for
NASA's EPOXI mission watched their computer screens as 23.6 million
kilometers (14.7 million miles) away, their spacecraft successfully
performed its 20th trajectory correction maneuver. The maneuver refined
the spacecraft's orbit, setting the stage for its flyby of comet Hartley
2 on Nov. 4. Time of closest approach to the comet was expected to be
about 10: 02 a.m. EDT (7:02 a.m. PDT).

Today's trajectory correction maneuver began at 2 p.m. EDT (11 a.m. PDT)
today, when the spacecraft fired its engines for 60 seconds, changing
the spacecraft's velocity by 1.53 meters per second (3.4 mph).

We are about 23 million miles and 36 days away from our comet, said
EPOXI project manager Tim Larson of NASA's Jet Propulsion Laboratory in
Pasadena, Calif. I can't wait to see what Hartley 2 looks like.

On Nov. 4, the spacecraft will fly past the comet at a distance of about
700 kilometers (435 miles). It will be only the fifth time in history
that a spacecraft has been close enough to image a comet's nucleus, and
the first time in history that two comets have been imaged with the same
instruments and same spatial resolution.

We are imaging the comet every day, and Hartley 2 is proving to be a
worthy target for exploration, said Mike A'Hearn, EPOXI principal
investigator from the University of Maryland, College Park.

EPOXI is an extended mission that utilizes the already in flight Deep
Impact spacecraft to explore distinct celestial targets of opportunity.
The name EPOXI itself is a combination of the names for the two extended
mission components: the extrasolar planet observations, called
Extrasolar Planet Observations and Characterization (EPOCh), and the
flyby of comet Hartley 2, called the Deep Impact Extended Investigation
(DIXI). The spacecraft will continue to be referred to as Deep Impact.

NASA's Jet Propulsion Laboratory, Pasadena, Calif., manages the EPOXI
mission for NASA's Science Mission Directorate, Washington. The
University of Maryland, College Park, is home to the mission's principal
investigator, Michael A'Hearn. Drake Deming of NASA's Goddard Space
Flight Center, Greenbelt, Md., is the science lead for the mission's
extrasolar planet observations. The spacecraft was built for NASA by
Ball Aerospace  Technologies Corp., Boulder, Colo.

For more information about EPOXI visit http://epoxi.umd.edu/.

DC Agle 818-393-9011
Jet Propulsion Laboratory, Pasadena, Calif.
a...@jpl.nasa.gov

2010-317

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[meteorite-list] '100 percent' chance for life on newly found planet?

2010-09-30 Thread Thunder Stone

Wow - 100% chance of life; how do they figure that?

Still want that ticket - only 20 light-years away.

Could stay a whole year - 37 days.  So that would be about 9 days for each 
season - WOW!

Greg S.


http://news.blogs.cnn.com/2010/09/30/100-percent-chance-for-life-on-newly-found-planet/?hpt=C2


'100 percent' chance for life on newly found planet?



Gliese 581g may be the new Earth.

A team of astronomers from the University of California and the Carnegie 
Institute of Washington say they've found a planet like ours, 20 light years 
(120 trillion miles) from Earth, where the basic conditions for life are good.

The chances for life on this planet are 100 percent, Steven Vogt, a UC 
professor of astronomy and astrophysics says. I have almost no doubt about it.

The planet is three times the size of Earth, but the gravity is similar.

Dr. Elizabeth Cunningham, planetarium astronomer at the Royal Observatory in 
Greenwich, says the discovery is a huge deal.

It could have liquid water on the surface, she said. That's the first step 
to find life.

The Gliese 581 system's orbit compared to our own solar system. The planet 
labeled G is the one scientists believe could very likely support life.

There are hundreds of known extrasolar planets that have been discovered in the 
Milky Way, but this is the first that could support life.

Earthlings won't be traveling to Gliese 581g any time soon unfortunately. 
Scientists say a spaceship traveling close to the speed of light would take 20 
years to make this journey.

But if we did - we'd find some other things familiar. The atmosphere and 
gravity are similar to Earth, and if you're from the polar regions, you'd 
definitely feel right at home. Scientists say the highest average temperature 
is about -12 degrees Celcius (10 Fahrenheit), but they point out that the 
planet doesn't have a night and day - one side continually faces the star and 
the other side faces the darkness of space. This means one side is blazing hot 
and the other freezing cold.

Gliese orbits a red dwarf star called Gliese 581. Cunningham says it's a 
Goldilocks planet.

It's not too hot, it's not too cold, it's just right for water to form, 
Cunningham said.

The area is called the Goldilocks zone.

Other planets near Gliese 581g have been discovered, but they are not habitable 
and are mainly comprised of gas. Gliese 581g, however, is a rocky planet.

It was discovered using the Keck telescope in Hawaii which has been observing 
the star Gliese 581 for 11 years.

Keck's long-term observations of the wobble of nearby stars enabled the 
detection of this multi-planetary system, said Mario R. Perez, Keck program 
scientist at NASA headquarters in Washington.

Astronomers are excited this new planet was discovered so fast and relatively 
close by.

I'm surprised we found one so fast, Cunningham said. The implication is 
either we were very lucky or these planets could be relatively common.

Gliese 581g is in the constellation of Libra. While Earth takes 365 days to 
orbit our star, the sun, Gliese 581g orbits its star in 37 days.
  
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[meteorite-list] MRO HiRISE Images - September 29, 2010

2010-09-30 Thread Ron Baalke


MARS RECONNAISSANCE ORBITER HIRISE IMAGES
September 29, 2010

o Linear Dunes and Sand Sheets in Herschel Crater
  http://hirise.lpl.arizona.edu/ESP_016916_1655

o Layered Bedrock in Oyama Crater near Mawrth Valles
  http://hirise.lpl.arizona.edu/ESP_018820_2035

o Very Fine Layers in Juventae Chasma
  http://hirise.lpl.arizona.edu/PSP_002590_1765

o Kaiser Crater Dune Field
  http://hirise.lpl.arizona.edu/PSP_003141_1330

o Pedestal Crater in the Medusa Fossae Formation
  http://hirise.lpl.arizona.edu/PSP_003253_1880

o Ares Vallis Cataract
  http://hirise.lpl.arizona.edu/PSP_003538_1885

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] New Paper About Younger Dryas Impact Hypothesis

2010-09-30 Thread Paul H.
Dear Friends,

A new paper about the Younger Dryas Impact Hypothesis
has been published. Associated with it are a number of
comments, both pro and con, about it. The paper is:

Holliday, V. T., and D. J. Meltzer, 2010, The 12.9-ka ET 
Impact Hypothesis and North American Paleoindians.
Current Anthropology. vol. 51, pp. 575–607 (Oct. 2010)
0011-3204/2010/5105-0002
http://www.journals.uchicago.edu/doi/abs/10.1086/656015
http://www.journals.uchicago.edu/doi/pdf/10.1086/656015

The Current Anthropology press release about the above 
paper can be found at:

http://www.journals.uchicago.edu/doi/story/10.1086/pr.2010.09.29.3011

Comments about this paper is “No Evidence For Clovis 
Comet Catastrophe, Archaeologists Say” by Alton 
Parrish at:

http://beforeitsnews.com/story/195/688/No_Evidence_For_Clovis_Comet_Catastrophe,_Archaeologists_Say.html

Yours,

Paul H.
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Re: [meteorite-list] '100 percent' chance for life on newly found planet?

2010-09-30 Thread Marc Fries
I have 100% certainty that someone just bought themselves 15 minutes of fame, 
and that's about it.

Interesting planet - from what I understand it is tidally locked with its star 
so that one side is always facing its sun.  The light from the star is reddish. 
 So picture that - you'd basically live somewhere on a ring around the 
permanently-lit side of the planet to avoid the hottest parts directly under 
the sun and the coldest parts on the permanently dark side, with the red sun 
always hanging in place.  I wonder if there would be seasons at all.  No 
seasons means no major weather changes, and anything that lived there probably 
wouldn't be driven to migrate.  And any critters that MIGHT live there would 
probably be adapted to see better in the red light than we can.  Fascinating.  
No doubt we'll have more info in hand about this planet in the coming years.

Cheers,
Marc Fries



On Sep 30, 2010, at 11:04 AM, Thunder Stone wrote:

 
 Wow - 100% chance of life; how do they figure that?
 
 Still want that ticket - only 20 light-years away.
 
 Could stay a whole year - 37 days.  So that would be about 9 days for each 
 season - WOW!
 
 Greg S.
 
 
 http://news.blogs.cnn.com/2010/09/30/100-percent-chance-for-life-on-newly-found-planet/?hpt=C2
 
 
 '100 percent' chance for life on newly found planet?
 
 
 
 Gliese 581g may be the new Earth.
 
 A team of astronomers from the University of California and the Carnegie 
 Institute of Washington say they've found a planet like ours, 20 light years 
 (120 trillion miles) from Earth, where the basic conditions for life are good.
 
 The chances for life on this planet are 100 percent, Steven Vogt, a UC 
 professor of astronomy and astrophysics says. I have almost no doubt about 
 it.
 
 The planet is three times the size of Earth, but the gravity is similar.
 
 Dr. Elizabeth Cunningham, planetarium astronomer at the Royal Observatory in 
 Greenwich, says the discovery is a huge deal.
 
 It could have liquid water on the surface, she said. That's the first step 
 to find life.
 
 The Gliese 581 system's orbit compared to our own solar system. The planet 
 labeled G is the one scientists believe could very likely support life.
 
 There are hundreds of known extrasolar planets that have been discovered in 
 the Milky Way, but this is the first that could support life.
 
 Earthlings won't be traveling to Gliese 581g any time soon unfortunately. 
 Scientists say a spaceship traveling close to the speed of light would take 
 20 years to make this journey.
 
 But if we did - we'd find some other things familiar. The atmosphere and 
 gravity are similar to Earth, and if you're from the polar regions, you'd 
 definitely feel right at home. Scientists say the highest average temperature 
 is about -12 degrees Celcius (10 Fahrenheit), but they point out that the 
 planet doesn't have a night and day - one side continually faces the star and 
 the other side faces the darkness of space. This means one side is blazing 
 hot and the other freezing cold.
 
 Gliese orbits a red dwarf star called Gliese 581. Cunningham says it's a 
 Goldilocks planet.
 
 It's not too hot, it's not too cold, it's just right for water to form, 
 Cunningham said.
 
 The area is called the Goldilocks zone.
 
 Other planets near Gliese 581g have been discovered, but they are not 
 habitable and are mainly comprised of gas. Gliese 581g, however, is a rocky 
 planet.
 
 It was discovered using the Keck telescope in Hawaii which has been observing 
 the star Gliese 581 for 11 years.
 
 Keck's long-term observations of the wobble of nearby stars enabled the 
 detection of this multi-planetary system, said Mario R. Perez, Keck program 
 scientist at NASA headquarters in Washington.
 
 Astronomers are excited this new planet was discovered so fast and relatively 
 close by.
 
 I'm surprised we found one so fast, Cunningham said. The implication is 
 either we were very lucky or these planets could be relatively common.
 
 Gliese 581g is in the constellation of Libra. While Earth takes 365 days to 
 orbit our star, the sun, Gliese 581g orbits its star in 37 days.
 
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 Meteorite-list@meteoritecentral.com
 http://six.pairlist.net/mailman/listinfo/meteorite-list

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Re: [meteorite-list] [Fwd: RE: Specific Gravity Question]

2010-09-30 Thread Sterling K. Webb

One of the papers on density and porosity can be downloaded here:
http://homepage.mac.com/brother_guy/.Public/Asteroid%20Densities.pdf
directly from Brother Guy's webpages

More references:
CONSOLMAGNO G.J. et al. (1977) Composition and evolution of the eucrite
parent body: evidence from rare earth elements (GCA 41, 1271-1282).
BRITT D.T., CONSOLMAGNO G.J. (1996) Estimating porosities from bulk
densities (abs. Meteoritics 31, 1996, A022).
CONSOLMAGNO G.J. et al. (1996) Density and porosity measurements of the
Vatican meteorite collection (abs. Meteoritics 31, 1996, A031).
CONSOLMAGNO G.J. et al. (1997) Model porosities of chondrites and the
nature of asteroidal material (MAPS32, Suppl., A031-A032).
CONSOLMAGNO G.J. et al. (1998) Metamorphism, shock, and porosity: Why
are there meteorites? (Meteoritics 33-4, 1998, A034).
CONSOLMAGNO G.J. et al. (1998) The porosities of ordinary chondrites:
Models and interpretation (MAPS 33-6, 1998, 1221).
CONSOLMAGNO G.J. et al. (1998) The density and porosity of meteorites
from the Vatican collection (MAPS 33-6, 1998, 1231-1241).

Another paper on asteroid densities:
http://adsabs.harvard.edu/full/1999M%26PS...34..479W

Densities of Martian meteorites:
http://gsa.confex.com/gsa/2002AM/finalprogram/abstract_40458.htm

A short summary paper:
http://www.lpi.usra.edu/meetings/metsoc2001/pdf/5171.pdf



Sterling K. Webb
-
- Original Message - 
From: David Gunning davidgunn...@fairpoint.net

To: meteorite-list@meteoritecentral.com
Cc: davidgunn...@fairpoint.net
Sent: Thursday, September 30, 2010 7:08 AM
Subject: [meteorite-list] [Fwd: RE: Specific Gravity Question]


--- Original 
Message 

Subject: RE: [meteorite-list] Specific Gravity Question
From:David Gunning davidgunn...@fairpoint.net
Date:Thu, September 30, 2010 7:55 am
To:  Peter Scherff petersche...@rcn.com
-

Howdy,

Thanks for the e-burp.

There was no link, however, to the published data for hundreds of
meteorites, mentioned in your e-burp.  Why allude to information that
cannot be referenced and verified?

While it's interesting to read of your specific gravity bead method,
there are other less convoluted ways or dealing with the fear of
potential contamination in meteorites and mineral samples, in general.

What particularly interests me is exploring ways and utilizing lower 
tech

methods that bring the ordinary collector into the the loop.

Your suggested method would seem to exclude that possibility.




Hi,

Here is the way around contamination
http://www.psrd.hawaii.edu/Aug99/densityMeasure.html. Guy Consolmagno 
has

published data for hundreds of meteorites.

Peter

-Original Message-
From: meteorite-list-boun...@meteoritecentral.com
[mailto:meteorite-list-boun...@meteoritecentral.com] On Behalf Of 
David

Gunning
Sent: Thursday, September 30, 2010 6:46 AM
To: meteorite-list@meteoritecentral.com
Cc: davidgunn...@fairpoint.net
Subject: [meteorite-list] Specific Gravity Question


Hi All,

I'm a confessed specific gravity advocate for all things 
mineralogical,
including meteorites.  It seems to me that there is very little 
useful
specific gravity information on the web concerning meteorites, with 
the
singular exception of Randy L. Korotev', excellent website at 
Washington
University in St. Louis;  an informative website listing various 
specific

gravity values for various meteorite types and classifications.

It occurs to me that many people may not be taking specific gravity
measurements of their meteorite specimens because of some sort of 
biased

but unfounded fear of specimen contamination. Is this true?

One of the benefits of measuring specific gravity is in being able to
spot density anomalies in meteorites.  For example, you procure a 
small
meteorite specimen of a meteorite has been classified as an L 
ordinary
stoney chondrite, with a range of specific gravity values, as found 
on
Professor Korotev' s.g. list, of between 2.50 and 3.96 (with an 
average
s.g. of 3.35).  When you, yourself,  measure the specific gravity of 
your
L chondrite, and it's s.g. value comes in at 4.06, what does that 
mean?


Would such a s.g. reading #1: be possible?  And #2: be meaningful?

Are meteorite specific gravity values exclusively constrained to the
range of values that the scientists peg them at?

And, if not, if actual specific gravity measurements cam occur 
outside

the conventionally accepted range of values of the experts, should
anyone give a hoot one way or another?

Best wishes,

Dave Gunning













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Re: [meteorite-list] [RE: Specific Gravity Question]

2010-09-30 Thread Richard Kowalski
--- On Thu, 9/30/10, Sterling K. Webb sterling_k_w...@sbcglobal.net wrote:

 
 Getting unpaid internet access to a scholarly journal is
 another matter, though.

I find that many, if not most scientists are more than happy to send seriously 
interested parties electronic versions of any and all published papers if 
requested.

I have no doubt Guy would be happy to send his paper to anyone that is 
interested in his work.


--
Richard Kowalski
Full Moon Photography
IMCA #1081





  
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Re: [meteorite-list] Habital Planet Discovery Announcement

2010-09-30 Thread Darren Garrison
On Wed, 29 Sep 2010 21:27:42 -0500, you wrote:

   Because it would have 3 times the water but only two
times the surface, the average ocean depth would be about
4500 meters! The pressure at the depths of these oceans
would be about 9000 atmospheres. The highest mountains
possible would be about 4000 meters (calculating from the
median diameter), so if you were the greatest mountain
climber on this Super Earth, standing on the top of Super
Earth's highest mountain, you would still have 500 meters
of water above you!

Which has serious implications to the types of life that would be
possible/likely.  On Earth, the elements needed by the primary producers in the
ocean (phytoplankton) are mostly supplied from erosion of the land-- either
supplied through run-off into the ocean or through wind-blown sand and dust.  No
land means no elements delivered to the top layers of the ocean means that the
phytoplankton equivalent would be limited to only the equilibrium-state elements
dissolved into the sea water which means orders of magnitude lower biomass
production as compared to a world with continents and erosion.  Think of
agricultural nitrate and phosphate run-offs causing algal blooms.  Think of
experiments seeding the ocean surface with iron leading to as much as 85x
increase in growth of diatoms.  Very low production of phytoplankton means very
low production of zooplankton, means very small production of the critters that
eat the plankton, means very low production of the critters that eat the
critters that eat the plankton...

The most likely ecosystems on a waterworld would be hydrothermal vent
communities with primary producers being chemoautotrophs, the way they are on
the abyssal plains of Earth.  You could imagine life-forms that would bulk up
on building blocks down at the hydrothermal vents and then migrate to the
surface waters, but _why would they_?  It would be a stretch to imagine
selective pressures that would lead to that. 

If you are currently packing for a trip to Gliese 581g, you better make room for
Alvin.

http://en.wikipedia.org/wiki/Eutrophication

http://www.palomar.edu/oceanography/iron.htm

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[meteorite-list] Ad: October Natural History Auction - Heritage Auction Galleries

2010-09-30 Thread Yinan Wang
Hello Everyone!

Heritage Auction Galleries' Natural History Internet Auction is now
live and ready for bidding.

Although we do not many meteorites for this auction, the catalog is
still worth a look:
http://historical.ha.com/common/auction/catalog.php?SaleNo=810091type=yinan-meteorite

For our Internet Auction we gathered many pieces that have low or no
reserves. Auction ends with the live-online session October 17th.
Here are some highlights:

A 20.9 gram slice of Esquel, with a starting bid of only $150:
http://historical.ha.com/common/view_item.php?Sale_No=810091Lot_No=81045type=yinan-meteorite

A 439 gram etched end-piece of Sikhote-Alin:
http://historical.ha.com/common/view_item.php?Sale_No=810091Lot_No=81046

A very pretty 20.7 gram Moldavite, starting at $150:
http://historical.ha.com/common/view_item.php?Sale_No=810091Lot_No=81047

A very nicely etched Nantan slice, 437 grams:
http://historical.ha.com/common/view_item.php?Sale_No=810091Lot_No=81043

A very large 595 gram Muonionalusta slice:
http://historical.ha.com/common/view_item.php?Sale_No=810091Lot_No=81042

And a couple of other pieces here and there.
- Yinan Wang
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Re: [meteorite-list] [Fwd: RE: Specific Gravity Question]

2010-09-30 Thread David Gunning

Hi Sterling,

I've never declined to read any reference that's been offered for my
additional understanding, on any subject matter.  More to the point, you
might ought to climb down from your high horse, for a minute, and
actually read the actual intent of my question.

My question centered around the idea of an individual taking their own
specific gravity measurement of their own meteorites.

I take it from your response that you would defer to Brother Consolmagno
for any specific gravity measurements you might be curious about.  Just
because the good Brother is associated with the Vatican, I wonder, do you
treat his findings as gospel?  If so, good for you.

Now, I am sure the good Brother is very exacting in his methods and
measurements. I have no difficulty with that.  Good for him!

Most of his references, however, according to the links you provided,
have to do with measuring the the grain bulk density of asteroids. 
That's quite a headful and a rarefied arena I would not presume to know 
much about.  And has, for the most part, little, if any, practical
application with actually measuring the specific gravity of meteorites.

As may be, I think it's rather silly of you to compare measuring home
grown specific gravity values of meteorites with measuring the bulk grain
density of asteroids (or the bulk grain density of meteorites, for that
matter).

They are horses of different colors.

One valuable insight I was able to glean from the good Brother's writing
is when he suggests that his margin of error in his measurements is
something on the order of plus or minus .07 percent, if I understand
correctly.  That agrees with my own estimation of a possible range of
error for ordinary specific gravity measurements for meteorites.

My stated interest has to do with common meteorites (if such a term may
apply!) and how ordinary people might gain more insight into their own
ordinary meteorites (to the extent that any meteorite can be thought of
as being ordinary!) by utilizing traditionally proven time worn methods
of measuring the specific gravity of their own space rocks.

Is there something intrinsically wrong with wanting to do that?

Glad tidings!

Dave Gunning







 Hi, Dave,

 You should try actually reading the references that
 people give to help you with your question. If you
 had, you would have found the citation to the published
 data in about 30 seconds, just like I did:

 Consolmagno, G. J. and D. T. Britt, 1998, The Density
 and Porosity of Meteorites from the Vatican Collection,
  Meteoritics and Planetary Science, vol. 33, p. 1231-1241.

 Getting unpaid internet access to a scholarly journal is
 another matter, though.


 Sterling K. Webb
 --
 - Original Message -
 From: David Gunning davidgunn...@fairpoint.net
 To: meteorite-list@meteoritecentral.com
 Cc: davidgunn...@fairpoint.net
 Sent: Thursday, September 30, 2010 7:08 AM
 Subject: [meteorite-list] [Fwd: RE: Specific Gravity Question]


 --- Original
 Message 
 Subject: RE: [meteorite-list] Specific Gravity Question
 From:David Gunning davidgunn...@fairpoint.net
 Date:Thu, September 30, 2010 7:55 am
 To:  Peter Scherff petersche...@rcn.com
 -

 Howdy,

 Thanks for the e-burp.

 There was no link, however, to the published data for hundreds of
 meteorites, mentioned in your e-burp.  Why allude to information that
 cannot be referenced and verified?

 While it's interesting to read of your specific gravity bead method,
 there are other less convoluted ways or dealing with the fear of
 potential contamination in meteorites and mineral samples, in general.

 What particularly interests me is exploring ways and utilizing lower
 tech
 methods that bring the ordinary collector into the the loop.

 Your suggested method would seem to exclude that possibility.



 Hi,

 Here is the way around contamination
 http://www.psrd.hawaii.edu/Aug99/densityMeasure.html. Guy Consolmagno
 has
 published data for hundreds of meteorites.

 Peter

 -Original Message-
 From: meteorite-list-boun...@meteoritecentral.com
 [mailto:meteorite-list-boun...@meteoritecentral.com] On Behalf Of
 David
 Gunning
 Sent: Thursday, September 30, 2010 6:46 AM
 To: meteorite-list@meteoritecentral.com
 Cc: davidgunn...@fairpoint.net
 Subject: [meteorite-list] Specific Gravity Question


 Hi All,

 I'm a confessed specific gravity advocate for all things
 mineralogical,
 including meteorites.  It seems to me that there is very little
 useful
 specific gravity information on the web concerning meteorites, with
 the
 singular exception of Randy L. Korotev', excellent website at
 Washington
 University in St. Louis;  an informative website listing various
 specific
 gravity values for various meteorite types and classifications.

 It occurs to me that many people 

[meteorite-list] Amateur Meteoriticists?

2010-09-30 Thread Richard Kowalski
David's original question got me thinking a little bit about a conversation Guy 
 I had over dinner a few weeks ago, during his last visit to Tucson. Ill get 
to that in a moment.

My own question is this. Are there (m)any amateur meteoriticists out there? 
IOW, amateurs who contribute to the Science of Meteorites, just as many, many 
amateur astronomers are doing very real and valuable science, often 
collaborating with professionals in various areas of research to secure needed 
observations. Now of course very few amateurs can afford or have the skill set 
to have a microprobe in their basements, but I would imagine that there are 
some areas of research that amateurs can contribute to the science. I'm 
wondering how many amateurs are actively contributing and publishing papers?

Now to a more direct response to David. Over dinner Guy commented a bit about 
his work and how amateurs could perform density and specific gravity 
measurements of their own meteorites. I suggested contacting him, and other 
scientists for copies of their papers if you don't have access to pay sites. 
Guy is rather busy and a response may take a while, but I'm sure he'd be happy 
to correspond with anyone seriously interested in contributing to this effort 
and offer some direction on how to proceed.

I can't say he is looking for co-authors, but he may be able to direct 
interested amateurs to the researchers who would be interested. 

--
Richard Kowalski
Full Moon Photography
IMCA #1081


--- On Thu, 9/30/10, David Gunning davidgunn...@fairpoint.net wrote:

 From: David Gunning davidgunn...@fairpoint.net
 Subject: Re: [meteorite-list] [Fwd: RE:  Specific Gravity Question]
 To: Sterling K. Webb sterling_k_w...@sbcglobal.net
 Cc: meteorite-list@meteoritecentral.com
 Date: Thursday, September 30, 2010, 5:44 PM
 
 Hi Sterling,
 
 I've never declined to read any reference that's been
 offered for my
 additional understanding, on any subject matter.  More
 to the point, you
 might ought to climb down from your high horse, for a
 minute, and
 actually read the actual intent of my question.
 
 My question centered around the idea of an individual
 taking their own
 specific gravity measurement of their own meteorites.
 
 I take it from your response that you would defer to
 Brother Consolmagno
 for any specific gravity measurements you might be curious
 about.  Just
 because the good Brother is associated with the Vatican, I
 wonder, do you
 treat his findings as gospel?  If so, good for you.
 
 Now, I am sure the good Brother is very exacting in his
 methods and
 measurements. I have no difficulty with that.  Good
 for him!
 
 Most of his references, however, according to the links you
 provided,
 have to do with measuring the the grain bulk density of
 asteroids. 
 That's quite a headful and a rarefied arena I would not
 presume to know 
 much about.  And has, for the most part, little, if
 any, practical
 application with actually measuring the specific gravity of
 meteorites.
 
 As may be, I think it's rather silly of you to compare
 measuring home
 grown specific gravity values of meteorites with measuring
 the bulk grain
 density of asteroids (or the bulk grain density of
 meteorites, for that
 matter).
 
 They are horses of different colors.
 
 One valuable insight I was able to glean from the good
 Brother's writing
 is when he suggests that his margin of error in his
 measurements is
 something on the order of plus or minus .07 percent, if I
 understand
 correctly.  That agrees with my own estimation of a
 possible range of
 error for ordinary specific gravity measurements for
 meteorites.
 
 My stated interest has to do with common meteorites (if
 such a term may
 apply!) and how ordinary people might gain more insight
 into their own
 ordinary meteorites (to the extent that any meteorite can
 be thought of
 as being ordinary!) by utilizing traditionally proven
 time worn methods
 of measuring the specific gravity of their own space
 rocks.
 
 Is there something intrinsically wrong with wanting to do
 that?
 
 Glad tidings!
 
 Dave Gunning
 
 
 
 
 
 
 
  Hi, Dave,
 
  You should try actually reading the references that
  people give to help you with your question. If you
  had, you would have found the citation to the
 published
  data in about 30 seconds, just like I did:
 
  Consolmagno, G. J. and D. T. Britt, 1998, The Density
  and Porosity of Meteorites from the Vatican
 Collection,
   Meteoritics and Planetary Science, vol. 33, p.
 1231-1241.
 
  Getting unpaid internet access to a scholarly journal
 is
  another matter, though.
 
 
  Sterling K. Webb
 
 --
  - Original Message -
  From: David Gunning davidgunn...@fairpoint.net
  To: meteorite-list@meteoritecentral.com
  Cc: davidgunn...@fairpoint.net
  Sent: Thursday, September 30, 2010 7:08 AM
  Subject: [meteorite-list] [Fwd: RE: Specific Gravity
 Question]
 
 
  

Re: [meteorite-list] Meteorite Densities - Brother Guy

2010-09-30 Thread ted brattstrom
Aloha - 

This looks like a possible source of information - :-)   

Grain densities, Bulk Densities, and Porosity... 

Now to find a source of those tiny glass beads!

Cheers - ted


Stony Meteorite Porosities and Densities: A Review of the Data through 2001
D. T. BRITT1 and G. J. CONSOLMAGNO S.J

http://homepage.mac.com/brother_guy/.Public/Meteorite%20Densities.pdf




--- On Thu, 9/30/10, Richard Kowalski damoc...@yahoo.com wrote:

 From: Richard Kowalski damoc...@yahoo.com
 Subject: [meteorite-list] Amateur Meteoriticists?
 To: meteorite-list@meteoritecentral.com
 Date: Thursday, September 30, 2010, 3:05 PM
 David's original question got me


snip ..

 
 Now to a more direct response to David. Over dinner Guy
 commented a bit about his work and how amateurs could
 perform density and specific gravity measurements of their
 own meteorites. I suggested contacting him, and other
 scientists for copies of their papers if you don't have
 access to pay sites. 

...snip...
 
 I can't say he is looking for co-authors, but he may be
 able to direct interested amateurs to the researchers who
 would be interested. 
 
 --
 Richard Kowalski
 Full Moon Photography
 IMCA #1081
 


  

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Re: [meteorite-list] Meteorite Densities - Brother Guy

2010-09-30 Thread Richard Kowalski
--- On Thu, 9/30/10, ted brattstrom volcano...@yahoo.com wrote:

 
 
 Now to find a source of those tiny glass beads!

Seem to be pretty common at sand blasting suppliers.


--
Richard Kowalski
Full Moon Photography
IMCA #1081


  
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Re: [meteorite-list] Amateur Meteoriticists?

2010-09-30 Thread Martin Altmann
Hi Richard,

IOW, amateurs who contribute to the Science of Meteorites

Yes there are. Only a very few of these, who are doing the field work and
who brought and are bringing the largest part of the world meteorite
inventory to the labs, institutes and museums
do have an academic degree in geology.

And each amateur purchasing a meteorite contributes to science in helping
these people to continue their work.

Best!
Martin 




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Re: [meteorite-list] Twice Blessed Yankee Lobsterman

2010-09-30 Thread Bob Loeffler
Hi Dave,

I was only trying to tell you that those are not official meteorites, but if
you were well aware that the two Round Pond meteorites had not been
mentioned with official citations, I would think that you would be well
aware that they then cannot be considered meteorites (since they have not
been officially classified).

Regarding wasting our time and what your style is, I have not seen too many
postings from you, so I have no idea what your style is or whether you were
wasting our time.  From what you said in your e-mail, I assumed you were a
meteorite newbie, not just a newbie to this list.  Like I said above, I
was just trying to let you know that they aren't official (so you probably
won't find many details about them).

If you had told us that the Maine Geological Survey mentioned them on their
website, maybe that could've helped us research it, don't you think?  And
next time, you might want to say that you have already done some research
and therefore others who want to help you won't repeat what you have already
done.

Regards,

Bob



-Original Message-
From: meteorite-list-boun...@meteoritecentral.com
[mailto:meteorite-list-boun...@meteoritecentral.com] On Behalf Of David
Gunning
Sent: Wednesday, September 29, 2010 10:05 AM
To: Meteorite-list@meteoritecentral.com
Subject: [meteorite-list] Twice Blessed Yankee Lobsterman


Hi Rob  Elton,

Believe it or not, guys, I was well aware that the two Round Pond
meteorites had not been mentioned with official citations.  You think I
would want to waste peoples time without first getting the factual lay of
an issue?  That's not my style.

I first learned about the Round Pond meteorites on a web site hosted by
the Maine Geological Survey.  Unless I'm mistaken that information is
offered by the Maine Geological Survey without qualifiers.  Because of
the source, I took the information at face value, statistically
improbable or not.

There is another Maine meteorite report that references a 321 lb.
metallic stone having been found on the shore of Great Chebeague Island
in Casco Bay, in 1973.  As I lived on a neighboring island in Casco Bay
for five years and never heard of it PLUS the lack of mention by the
Maine Geological Survey in any of their public literature, I did not make
mention of that particular meteorite in my original query to the list.

I mean, how on earth could an islander hide a 321 lb. metallic stone
meteorite.   .   .without half the other islanders knowing about it?
Talk about your statistical improbabilities.  .  .  !

Now, if it turns-out that the story of the lobsterman meteorite finder
was either factually incorrect or a creative fabrication on the part of
the State of Maine and the Maine Geological Survey I would suggest to all
interested parties, from the Governor on down, that the citizens of
Maine, myself included, deserve better than to be fibbed to in such a
bald faced manner.

I'd like to know the Maine peat bog location you've referenced, Elton, if
it's not too much trouble.

Best wishes,

Dave Gunning






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[meteorite-list] Meteorites in Maine Web Page (Maine Geological Survey)

2010-09-30 Thread Paul H.
The web page that the Maine Geological Survey has on Maine 
meteorites is Meteorites in Maine: Is the sky falling??? at:
http://www.maine.gov/doc/nrimc/mgs/explore/minerals/sites/mar99.htm

This web page states:

Though many meteorites probably have landed in Maine, only 5 
have been found and authenticated and described in the scientific 
literature, and portions of each are preserved in museum collections.

Nowhere in this web page is there any mention of meteorites
being found by lobstermen as described in previous posts,
which started with:

http://six.pairlist.net/pipermail/meteorite-list/2010-September/069269.html

I am a little skeptical of such finds without seeing some documentation
because last year, a person call me and another geologist to tell us
that he had hauled up a 3-foot in diameter meteorite from the
bottom of the the Gulf of Mexico off of Terrebonne Island, Terrebonne 
Parish, Louisiana while fishing. Anyway he brought over to my 
office in the back of his minivan. It turned out to be a well rounded 
boulder of granite gneiss. I still wonder how a 3-foot in diameter 
nicely rounded boulder of granite gneiss ended up on the bottom 
of the Gulf of Mexico.

Best wishes,

Paul 

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Re: [meteorite-list] [Fwd: RE: Specific Gravity Question]

2010-09-30 Thread David Gunning

Aloha,

Thanks for the note.  Yeah, that Brother Guy fellow is a rare bird. I am
not so concerned with taking precise specific gravity value measurements
(I've been doing that for years) so much as wanting to get the word out
that there are ways of dealing with potential contamination issues, which
seems to be the big bugaboo for most folks. The actual process of taking
and achieving an exacting specific gravity measurement is so straight
forward a child could do it.

Appears to me that the willingness to measure specific gravity may be a
reasonably accurate bellwether of whether a person is really, really
interested in meteorites for what they are, and might be, as opposed to
being used as mere lucrative commodities to be bought and sold.

Such is life!

Dave Gunning



 Aloha -

 Just started looking through this:

 http://homepage.mac.com/brother_guy/.Public/Meteorite%20Densities.pdf

 and at the end, it has grain density And bulk density for a whole bunch
 of meteorites, and meteorite classes...  (yeah, it's got the porosity
 data too...)

 In that listing, it doesn't give the sub-class of H / L / LL, but that
 should be able to be looked up if you want to get finer information out
 of this data.

 Now, this doesn't address how to do it at home, other than replicating
 the process that they used (small glass beads - and all)

 Looked pretty interesting

 cheers = ted

 --- On Thu, 9/30/10, David Gunning davidgunn...@fairpoint.net wrote:

 From: David Gunning davidgunn...@fairpoint.net
 Subject: Re: [meteorite-list] [Fwd: RE:  Specific Gravity Question]
 To: Sterling K. Webb sterling_k_w...@sbcglobal.net
 Cc: meteorite-list@meteoritecentral.com
 Date: Thursday, September 30, 2010, 2:44 PM

 Hi Sterling,

 I've never declined to read any reference that's been
 offered for my
 additional understanding, on any subject matter.  More
 to the point, you
 might ought to climb down from your high horse, for a
 minute, and
 actually read the actual intent of my question.

 My question centered around the idea of an individual
 taking their own
 specific gravity measurement of their own meteorites.

 I take it from your response that you would defer to
 Brother Consolmagno
 for any specific gravity measurements you might be curious
 about.  Just
 because the good Brother is associated with the Vatican, I
 wonder, do you
 treat his findings as gospel?  If so, good for you.

 Now, I am sure the good Brother is very exacting in his
 methods and
 measurements. I have no difficulty with that.  Good
 for him!

 Most of his references, however, according to the links you
 provided,
 have to do with measuring the the grain bulk density of
 asteroids.
 That's quite a headful and a rarefied arena I would not
 presume to know
 much about.  And has, for the most part, little, if
 any, practical
 application with actually measuring the specific gravity of
 meteorites.

 As may be, I think it's rather silly of you to compare
 measuring home
 grown specific gravity values of meteorites with measuring
 the bulk grain
 density of asteroids (or the bulk grain density of
 meteorites, for that
 matter).

 They are horses of different colors.

 One valuable insight I was able to glean from the good
 Brother's writing
 is when he suggests that his margin of error in his
 measurements is
 something on the order of plus or minus .07 percent, if I
 understand
 correctly.  That agrees with my own estimation of a
 possible range of
 error for ordinary specific gravity measurements for
 meteorites.

 My stated interest has to do with common meteorites (if
 such a term may
 apply!) and how ordinary people might gain more insight
 into their own
 ordinary meteorites (to the extent that any meteorite can
 be thought of
 as being ordinary!) by utilizing traditionally proven
 time worn methods
 of measuring the specific gravity of their own space
 rocks.

 Is there something intrinsically wrong with wanting to do
 that?

 Glad tidings!

 Dave Gunning







  Hi, Dave,
 
  You should try actually reading the references that
  people give to help you with your question. If you
  had, you would have found the citation to the
 published
  data in about 30 seconds, just like I did:
 
  Consolmagno, G. J. and D. T. Britt, 1998, The Density
  and Porosity of Meteorites from the Vatican
 Collection,
   Meteoritics and Planetary Science, vol. 33, p.
 1231-1241.
 
  Getting unpaid internet access to a scholarly journal
 is
  another matter, though.
 
 
  Sterling K. Webb
 
 --
  - Original Message -
  From: David Gunning davidgunn...@fairpoint.net
  To: meteorite-list@meteoritecentral.com
  Cc: davidgunn...@fairpoint.net
  Sent: Thursday, September 30, 2010 7:08 AM
  Subject: [meteorite-list] [Fwd: RE: Specific Gravity
 Question]
 
 
  --- Original
  Message 
  Subject: RE: [meteorite-list] Specific Gravity
 Question
  

Re: [meteorite-list] Rocks from Space Picture of the Day - September 30, 2010

2010-09-30 Thread Greg Hupe

Hi Laurence,

Your Canyon Diablo diamonds on Picture of the Day are pretty cool! I 
appreciate your sharing images from the ASU collection.


Best regards,
Greg


Greg Hupe
The Hupe Collection
NaturesVault (eBay)
gmh...@htn.net
www.LunarRock.com
IMCA 3163

Click here for my current eBay auctions: 
http://search.ebay.com/_W0QQsassZnaturesvault


- Original Message - 
From: Michael Johnson mich...@rocksfromspace.org

To: meteorite-list@meteoritecentral.com
Sent: Thursday, September 30, 2010 1:21 PM
Subject: [meteorite-list] Rocks from Space Picture of the Day - September 
30,2010




http://www.rocksfromspace.org/September_30_2010.html
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[meteorite-list] Subject: Re: Habital Planet Discovery Announcement

2010-09-30 Thread countdeiro
Listees,

And now we have this to contemplate. 

http://www.dailymail.co.uk/sciencetech/article-1316538/Gliese-581g-mystery-Scientist-spotted-mysterious-pulse-light-direction-newEarth-planet-year.html

Best to all,

Count Deiro
IMCA 3536
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Re: [meteorite-list] Subject: Re: Habital Planet Discovery Announcement

2010-09-30 Thread Sterling K. Webb

Not to doubt the scientific trustworthiness of
the Daily Mail, but they state that the light pulse
was seen December, 2008, long before it was
announced that the star Gliese 581 has habitable
planets in orbit around it.

But Gliese 581 c, the first low mass extrasolar
planet found to be near its star's habitable zone,
was discovered in April 2007, and Gliese 581 b,
approximately Neptune-sized and the first planet
detected around Gliese 581, was discovered in
August 2005.

Discovered at the same time as Gliese 581 c, a third
planet, Gliese 581 d, has a mass of roughly 7 Earths,
or half a Uranus, and an orbit of 66.8 Earth days. It
orbits just within the outer limit of the habitable zone.

The fourth planet, Gliese 581 e, was announced on
21 April 2009. This planet, at an estimated minimum
mass of 1.9 Earths, is currently the lowest mass exoplanet
identified around a normal star. The more distant
Gliese 581 f was found at the same time.

Gliese 581 was much in the news by December, 2008.
It was known that there were low-mass planets and that
there were planets in the habitable zone. The BEBO
message had been sent just two months before, in
October, 2008.

It is certainly not true that the pulse was long before it was
announced that the star Gliese 581 has habitable planets
in orbit around it. It was well known.

Unrepeated signals don't count. Basic rule of SETI.


Sterling K. Webb
--
- Original Message - 
From: countde...@earthlink.net

To: meteorite-list@meteoritecentral.com
Sent: Thursday, September 30, 2010 10:40 PM
Subject: [meteorite-list] Subject: Re: Habital Planet Discovery 
Announcement




Listees,

And now we have this to contemplate.

http://www.dailymail.co.uk/sciencetech/article-1316538/Gliese-581g-mystery-Scientist-spotted-mysterious-pulse-light-direction-newEarth-planet-year.html

Best to all,

Count Deiro
IMCA 3536
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Re: [meteorite-list] Other Earths -- WAS: Re: Habitable Planet, etc.

2010-09-30 Thread Melanie Matthews
Hi Sterling, list. 
Thanks a bunch for your imput! I came up with a fictional (though as plausible 
as possible) rocky planet orbiting HIP 56948 - which I intend for it to have a 
somewhat higher gravity than Earth's, but wasn't sure whether to make it bigger 
like this new Super Earth. On it inhabits a sentient race of humanoids with 
their own languages (one of which I'm working on), cultures, etc. Many to which 
value meteorites as highly sacrad objects. I plan to publish this eventually.. 


So I'm kind of wondering in this point to make it it smaller than Earth (but 
perhaps denser?)so that the surface area would be closer to its center of 
gravity at the core. 


All the best 

 ---
-Melanie
IMCA: 2975
eBay: metmel2775
Known on SkyRock Cafe as SpaceCollector09

I eat, sleep and breath meteorites 24/7.



- Original Message 
From: Sterling K. Webb sterling_k_w...@sbcglobal.net
To: Carl 's carloselgua...@hotmail.com; meteorite-list@meteoritecentral.com
Sent: Wed, September 29, 2010 10:27:11 PM
Subject: [meteorite-list] Other Earths -- WAS: Re:  Habitable Planet, etc.

Hi, Carl, and Other Inquiring Minds,

 How much is slightly?

Well, I just answered that one, Carl, but the principle
involved is this: a bigger planet means that when you're
on the surface of it, you're much further away from the
center of its mass, hence gravity does not go up directly
as the diameter increases.

Imagine that we could build a spherical shell that com-
pletely enclosed the Earth, but was erected 4000 miles
above the Earth's surface. Massive as it would be, it would
be a minimal increase of the Earth's mass.

If you walked around on the outside of that shell, you
would be 8000 miles from the Earth's center instead of
the 4000 miles from the center we are down here. The
gravity would be only 25% of normal gravity on the
outside of that (imaginary) shell.

Imagine a planetary system where an Earth-like world
condenses from a heavy-metal-and-element-poor nebula,
like one that forms a calcium-rich or light-metal-rich star.
(They exist, BTW.)

Without an iron core of any great size, they would be made
of rock only, rich in silicon, calcium, magnesium, aluminum...
A lithophile planet, not a siderophile planet, is perfectly
possible. Basalt would be a rare deep-mantle stone and
iron a precious gem-metal, both almost never seen.

It would be a low-density world. It would not compress
as easily as iron-rich worlds. It would be much bigger for
its mass than a world like Earth, hence it would have a
much greater diameter but a LOWER surface gravity.

Imagine a two-Earth-mass world with a density of 3.26,
like a heavy rock; that's only 60% of the density of our Earth.
It would have 3.33 times the volume of Earth, 2.19 times
the surface area of Earth, and 1.49 times the diameter of
the Earth (11,840 miles in diameter).

Its surface gravity would only be 88% of the Earth's, despite
having twice the mass! It would have a deep siliac crust and
very high mountains, higher rates of erosion, no plate tectonics,
no volcanoes. The only vertical movements in the crust would
be isotasy; continents would be buoyant plutons of less dense
rock. There would be twice the water of the Earth spread out over
2.2 times the area --- the oceans should be similar to Earth's.

With twice the atmosphere of Earth and lower gravity, the air
would have a much greater scale height, meaning air pressure
would not fall off as rapidly with altitude as the Earth's. The
air would be denser and breathable (if it contain oxygen) at
much greater altitudes -- you could breath on top of a
52,000-foot-high mountain and fly a piston-engine aircraft
to 135,000 feet or more.

Sounds like an interesting place, doesn't it? (I've always
thought so.) There are millions of possible world-recipes
and likely billions of possible semi-Earth combinations that
could be made from them. It's NOT going to be the same old
solar system repeated over and over again.

What if Gliese 581g was made of low-density rock like my
sample world (above)? It would be 3 times the mass, 5 times
the volume, 1.70 times the diameter, 2.92 times the surface
area, and have a surface gravity of just 1.04 gees, ocean
depths the same as ours. But Gliese 581 doesn't seem to
be the right kind of star for that blend of materials. Some
K2 light-metal-rich dwarf somewhere...

Planet-building is fun.


Sterling K. Webb
--

- Original Message - From: Carl 's carloselgua...@hotmail.com
To: meteorite-list@meteoritecentral.com
Sent: Wednesday, September 29, 2010 7:46 PM
Subject: Re: [meteorite-list] (OT) Habital Planet Discovery Announcement


 
 Good evening All,
 
 Sorry for being really dense about stuff like this but I don't quite 
 understand 
how a planet with a mass three to four times and a diameter 1.2 to 1.4 times 
Earth will only have it's gravity only slightly higher? How much is 
slightly? 
Thanks for