[meteorite-list] Hayabusa 2's first touchdown on NEA (162173) Ryugu

2019-03-06 Thread Katsu OHTSUKA via Meteorite-list

https://www.youtube.com/watch?v=-3hO58HFa1M

Katsu OHTSUKA

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[meteorite-list] Mukundpura CM2.0 (CM1) (aka Jaipur)

2019-02-22 Thread Katsu OHTSUKA via Meteorite-list
Mukundpura (formerly called Jaipur) seems CM2.0 (CM1) chondrite, 
according to the following open access paper: 
https://www.sciencedirect.com/science/article/pii/S1674987118300434


Katsu OHTSUKA
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Re: [meteorite-list] Meteorite Picture of the Day: Alais?

2018-02-22 Thread Katsu OHTSUKA via Meteorite-list

Thanks for a nice picture.
But, the texture of this meteorite looks not CI1 but CM or CR.
So, the meteorite may be not Alais (CI1) but Al Rais (CR2-an)?
But, I don't know whether or not the Paris museum houses a collection of Al 
Rais.


Katsu OHTSUKA

-Original Message- 
From: Paul Swartz via Meteorite-list

Sent: Wednesday, February 21, 2018 5:00 PM
To: meteorite-list@meteoritecentral.com
Subject: [meteorite-list] Meteorite Picture of the Day

Today's Meteorite Picture of the Day: Alais

Contributed by: Hanno Strufe

http://www.tucsonmeteorites.com/mpodmain.asp?DD=02/21/2018
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Re: [meteorite-list] New fall, Nkayi Zimbabwe

2015-02-09 Thread Katsu OHTSUKA via Meteorite-list

Hello Frank,
Tunguska, Russia and Kagarlyk, Ukraine (L6) would be another example.
http://adsabs.harvard.edu/abs/1995Obs...115..136S

Katsu

-Original Message- 
From: Frank Cressy via Meteorite-list

Sent: Tuesday, February 10, 2015 11:22 AM
To: Matthias Bärmann ; Sergey Vasiliev
Cc: Meteorite-list@meteoritecentral.com ; Michael Farmer ; Peter Scherff
Subject: Re: [meteorite-list] New fall, Nkayi Zimbabwe

Last week I noted that there were 9 instances of two meteorite falls 
occurring on the same day since 1865.  I found my data on these so here they 
are:


1. Aug. 25, 1865 - Aumale, Algeria (L6) and Shergotty, India (Martian)
2. Aug. 28, 1925 - Ellemeet, Netherlands (Diogenite) and Lanzenkirchen, 
Austria (L4)
3. Aug. 8, 1933 - Sioux County, USA (Eucrite) and Repeev Khuyor, Russia 
(Iron)

4. Sept. 17, 1945 - Atoka, USA (L6) and Soroti, Uganda (Iron)
5. Sept. 21, 1949 - Akaba, Jordon (L6) and Beddgeler, Wales (H5)
6. Oct. 20, 1951 - Manych, Russia (LL3.4) and Yambo, Congo (H5)
7. Oct. 30, 1994 - Devri-Khera, India (L6) and Lohawat, India (Howardite)
8. June 21, 2002 - Kilabo, Nigeria (LL6) and Thuathe, Lesotho (H4/5)
9. March 1, 2009 - Carterville, USA (chondrite) and Nkayi, Zimbabwe (L6)

Additionally, in two instances, falls occurred on the same day but in the 
same area, and are assumed to be from the same fall. They are:


Sept. 26, 1939 - Glabggang, Indonesia (H5/6) and Selakopi, Indonesia (H5) 
Both fell near Bandung
Nov. 13, 1952 - Galim (a), Cameroon (LL6) and Galim(b), Cameroon 
(EH3/4-an)Rubble Pile??


Enjoy,

Frank





On Saturday, February 7, 2015 3:16 AM, Matthias Bärmann majbaerm...@web.de 
wrote:





That's a great service indeed, Sergey, from which I have made use several 
times, always with pleasure.


Best - Matthias


Am 07.02.2015 um 11:37 schrieb Sergey Vasiliev via Meteorite-list:

Hello List,
If you are looking for the same day but different years then you can
use this service.
It is a bit outdated statistic based on MetBase data. MetBase has a
day of fall/find and MetBull doesn't. That's why not all the recent
falls are listed. But still you can play with this to see how many
falls/finds where recovered the particular day. Just choose the day
and check: http://sv-meteorites.com/play_with_statistic.aspx Best regards,
Sergey On Sat, Feb 7, 2015 at 1:55 AM, Frank Cressy via Meteorite-list 
meteorite-list@meteoritecentral.com wrote:
Actually with Cartersville and Nkayi, two recovered falls on the same day 
has happened 9 times since 1865.  Don't have the list readily available, 
though.  FYI, in 1933 the Sioux County eucrite fell about an hour and a 
half after the Repeev Khutor iron landed just north of the Caspian Sea.  I 
think Kilabo and Thuathe fell about 5 hours apart. Cheers, Frank On Friday, 
February 6, 2015 4:37 PM, Peter Scherff via Meteorite-list 
meteorite-list@meteoritecentral.com wrote: Hi, Ellemeet   Lanzenkirchen 
also fell on the same day. Thanks, Peter -Original Message-

From: Meteorite-list [mailto:meteorite-list-boun...@meteoritecentral.com] On
Behalf Of Michael Farmer via Meteorite-list
Sent: Friday, February 06, 2015 5:47 PM
To: Galactic Stone  Ironworks
Cc: meteorite-list@meteoritecentral.com; Raremeteorites
Subject: Re: [meteorite-list] New fall, Nkayi Zimbabwe Really? That's cool.
Thuathe and Kilabo fell same day. Lesotho and Nigeria. Michael Farmer

On Feb 6, 2015, at 3:46 PM, Galactic Stone  Ironworks
meteoritem...@gmail.com wrote:
This is the same day as the Cartersville Georgia fall. Have two different 
meteorites ever fallen on the same day in different

parts of the world and been recovered? Best regards, MikeG
--
-
Web - http://www.galactic-stone.com Facebook - 
http://www.facebook.com/galacticstone Twitter - 
http://twitter.com/galacticstone Pinterest - 
http://pinterest.com/galacticstone - 
On 2/6/15, Michael Farmer via Meteorite-list 
meteorite-list@meteoritecentral.com wrote:

New fall to announce,

Nkayi, Zimbabwe. Fell 1 March 2009. L6 Only 15 kilograms was saved
from a ~100 kilogram stone.
I bought the entire remaining mass which was a large fragment of 8
kilos and about 4 kilos of fragments.
For sale today $20 gram.
It is the only meteorite ever available from Zimbabwe.
Pieces from ~1 gram to 676 grams available. Michael Farmer
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[meteorite-list] The 5-th Symposium on Polar Science---Antarctic Meteorites Session

2014-11-28 Thread Katsu OHTSUKA via Meteorite-list
The proceeding papers are now available at the following link: 
http://www.nipr.ac.jp/symposium2014/program/e/OA.html


Katsu OHTSUKA
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Re: [meteorite-list] Meteorites with amino acids

2014-11-19 Thread Katsu OHTSUKA via Meteorite-list

and the Stardust (81P/Wild 2) Sample
http://adsabs.harvard.edu/abs/2009M%26PS...44.1323E.

Katsu
-Original Message- 
From: Matson, Rob D. via Meteorite-list 
Sent: Wednesday, November 19, 2014 12:07 PM 
To: meteorite-list@meteoritecentral.com 
Subject: [meteorite-list] Meteorites with amino acids 


Amino acids have been found in the following meteorites of which I'm aware:

Murray (CM2)
Murchison (CM2)
Tagish Lake (C2 ungrouped)
Almahata Sitta (anomalous ureilite)
Sutter's Mill (CM2)
Allan Hills 77306 (CM2)
Allan Hills 83100 (CM2)
Asuka 88120 (CM2)
Asuka 881334 (CM2)
Lewis Cliffs 90500 (CM2)
Lone Wolf Nunataks 94102 (CM2)
Yamato 74662 (CM2)
Yamato 791198 (CM2) - most amino-acid-rich meteorite known
Yamato 793321 (CM2)
Belgica 7904 (CM2)
Orgueil (CI1)
Ivuna (CI1)

I am sure there are others that I have missed.  --Rob
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[meteorite-list] EPS special issue Science of solar system materials examined from Hayabusa and future missions

2014-11-15 Thread Katsu OHTSUKA via Meteorite-list
Earth, Planets and Space (EPS) started working as an open access-style 
journal under SpringerOpen this year.
The EPS special issue Science of solar system materials examined from 
Hayabusa and future missions will be published soon,
as the proceedings of the HAYABUSA 2013 symposium 
http://hayabusaao.isas.jaxa.jp/symposium/2013/program.html,

papers of which are accessible now, as follows:

Mineralogy of four Itokawa particles collected from the first touchdown site
Takaaki Noguchi, John C Bridges, Leon J Hicks, Steven J Gurman, Makoto 
Kimura, Takahito Hashimoto, Mitsuru Konno, John P Bradley, Ryuji Okazaki, 
Masayuki Uesugi, Toru Yada, Yuzuru Karouji, Masanao Abe, Tatsuaki Okada, 
Takuya Mitsunari, Tomoki Nakamura, Hiroyuki Kagi

Earth, Planets and Space 2014, 66:124 (9 October 2014)
http://www.earth-planets-space.com/content/pdf/1880-5981-66-124.pdf

Mineralogy and defect microstructure of an olivine-dominated Itokawa dust 
particle: evidence for shock metamorphism, collisional fragmentation, and LL 
chondrite origin

Falko Langenhorst, Dennis Harries, Kilian Pollok, Peter A van Aken
Earth, Planets and Space 2014, 66:118 (17 September 2014)
http://www.earth-planets-space.com/content/pdf/1880-5981-66-118.pdf

Sequential analysis of carbonaceous materials in Hayabusa-returned samples 
for the determination of their origin
Masayuki Uesugi, Hiroshi Naraoka, Motoo Ito, Hikaru Yabuta, Fumio Kitajima, 
Yoshinori Takano, Hajime Mita, Ichiro Ohnishi, Yoko Kebukawa, Toru Yada, 
Yuzuru Karouji, Yukihiro Ishibashi, Takaaki Okada, Masanao Abe

Earth, Planets and Space 2014, 66:102 (26 August 2014)
http://www.earth-planets-space.com/content/pdf/1880-5981-66-102.pdf

Microchemical and structural evidence for space weathering in soils from 
asteroid Itokawa

Michelle S Thompson, Roy Christoffersen, Thomas J Zega, Lindsay P Keller
Earth, Planets and Space 2014, 66:89 (13 August 2014)
http://www.earth-planets-space.com/content/pdf/1880-5981-66-89.pdf

Mineralogy and crystallography of some Itokawa particles returned by the 
Hayabusa asteroidal sample return mission
Takashi Mikouchi, Mutsumi Komatsu, Kenji Hagiya, Kazumasa Ohsumi, Michael E 
Zolensky, Viktor Hoffmann, James Martinez, Rupert Hochleitner, Melanie 
Kaliwoda, Yasuko Terada, Naoto Yagi, Masaki Takata, Wataru Satake, Yuya 
Aoyagi, Atsushi Takenouchi, Yuzuru Karouji, Masayuki Uesugi, Toru Yada

Earth, Planets and Space 2014, 66:82 (1 August 2014)
http://www.earth-planets-space.com/content/pdf/1880-5981-66-82.pdf

A transmission electron microscope study of Itokawa regolith grains
Lindsay P Keller, Eve L Berger
Earth, Planets and Space 2014, 66:71 (15 July 2014)
http://www.earth-planets-space.com/content/pdf/1880-5981-66-71.pdf

Robotic systems for the determination of the composition of solar system 
materials by means of fireball spectroscopy

José M Madiedo
Earth, Planets and Space 2014, 66:70 (15 July 2014)
http://www.earth-planets-space.com/content/pdf/1880-5981-66-70.pdf

BTW, the HAYABUSA2014 symposium will be held on 4--5 December at JAXA/ISAS 
Sagamihara, Japan.

http://hayabusaao.isas.jaxa.jp/symposium/

Katsu




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Re: [meteorite-list] Ebay, again!

2014-11-03 Thread Katsu OHTSUKA via Meteorite-list

why CK4?
http://www.ebay.com/itm/Carbonaceous-chondrite-CK4-type-from-the-Lop-Nur-/141457699376?pt=LH_DefaultDomain_0hash=item20ef893230

Katsu 


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[meteorite-list] First known Terrestrial Impact of a Binary Asteroid from a Main Belt Breakup Event

2014-10-27 Thread Katsu OHTSUKA via Meteorite-list

Hello list,

An open access paper published in Scientific Reports is available at:
http://www.nature.com/srep/2014/141023/srep06724/full/srep06724.html

Katsu
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[meteorite-list] PDF version of Field Guide to Meteors and Meteorites

2014-10-20 Thread Katsu OHTSUKA via Meteorite-list

Hello list,

I found a PDF version of the classic book Field Guide to Meteors and 
Meteorites (by R. Norton  L. Chitwood)

in the following link:
http://museum-21.ru/files/video/Norton%20O.,%20Chitwood%20L.%20-%20Field%20Guide%20to%20Meteors%20and%20Meteorites%20-%202008.pdf

however this might be an illegal download site.

Katsu OHTSUKA

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Re: [meteorite-list] PDF version of Field Guide to Meteors and Meteorites

2014-10-20 Thread Katsu OHTSUKA via Meteorite-list

Hi Michael,

Oh, it was as I suspected.
I purchased this great book soon after publication,
but not autographed. I want their autographed copy, if any.

best regards,

Katsu

-Original Message- 
From: Anne Black

Sent: Tuesday, October 21, 2014 7:14 AM
To: linton...@earthlink.net ; mikest...@gmail.com ; ohts...@jb3.so-net.ne.jp
Cc: meteorite-list@meteoritecentral.com
Subject: Re: [meteorite-list] PDF version of Field Guide to Meteors 
andMeteorites


Thank you Linton, Thank You Michael.
And yes, Michael, you are right, that PDF version is illegal and has
now been reported to Springer.

Yes, neither author lived long enough to enjoy the result of their
work. In fact, Larry Chitwood died the very day the book was finished;
he had spent most of the day working with Richard and Dorothy Norton,
then decided to take a walk before dinner, and he was later found on a
hiking trail, apparently victim of a massive heart attack. Richard was
seriously affected by that death and did not last very long after that.

Thank you for supporting that excellent book, and yes the 2 widows do
get a (small) royalty check.
Right now that book is very hard to find but it is (or will shortly) be
re-printed, and Dorothy and I still hope very much to have available
during the Tucson show.

Any questions, just ask!


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


-Original Message-
From: Linton Rohr via Meteorite-list
meteorite-list@meteoritecentral.com
To: Michael Mulgrew mikest...@gmail.com; Katsu OHTSUKA
ohts...@jb3.so-net.ne.jp
Cc: meteorite-list meteorite-list@meteoritecentral.com
Sent: Mon, Oct 20, 2014 12:37 pm
Subject: Re: [meteorite-list] PDF version of Field Guide to Meteors
andMeteorites


Really!
It's a great book, which should be on every collector's shelf.
Sadly, neither author lived long enough to promote it's sale.
The least we can do is buy a copy in their honor.
Linton

- Original Message -
From: Michael Mulgrew via Meteorite-list
meteorite-list@meteoritecentral.com
To: Katsu OHTSUKA ohts...@jb3.so-net.ne.jp
Cc: meteorite-list meteorite-list@meteoritecentral.com
Sent: Monday, October 20, 2014 10:13 AM
Subject: Re: [meteorite-list] PDF version of Field Guide to Meteors
andMeteorites



Katsu,

The book is Copyright Springer-Verlag London Limited, the link your
provided is an illegal download (as you surmised, surprised you shared
it).

Please purchase the book and show your support.

-Michael in so. Cal.

On Mon, Oct 20, 2014 at 1:29 AM, Katsu OHTSUKA via Meteorite-list
meteorite-list@meteoritecentral.com wrote:

Hello list,

I found a PDF version of the classic book Field Guide to Meteors and
Meteorites (by R. Norton  L. Chitwood)
in the following link:


http://museum-21.ru/files/video/Norton%20O.,%20Chitwood%20L.%20-%20Field%20Guide%20to%20Meteors%20and%20Meteorites%20-%202008.pdf


however this might be an illegal download site.

Katsu OHTSUKA

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-
No virus found in this message.
Checked by AVG - www.avg.com
Version: 2015.0.5315 / Virus Database: 4181/8422 - Release Date:

10/20/14




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[meteorite-list] Ancient Asteroid Destroyer Finally Found, And It's a New Kind of Meteorite

2014-06-28 Thread Katsu OHTSUKA via Meteorite-list

Ancient Asteroid Destroyer Finally Found, And It's a New Kind of Meteorite
http://www.livescience.com/46563-new-meteorite-type-fossil-ordovician.html

Original paper (open access, freely downloadable):
A fossil winonaite-like meteorite in Ordovician limestone: A piece of the 
impactor that broke up the L-chondrite parent body?
Birger Schmitz, Gary R. Huss, Matthias M.M. Meiera, Bernhard 
Peucker-Ehrenbrink, Ross P. Church, Anders Cronholm, Melvyn B. Davies,
Philipp R. Heck, Anders Johansen, Klaus Keil, Per Kristiansson, Greg 
Ravizza, Mario Tassinari, Fredrik Terfelt

2014 EPSL, 400, 145
http://www.sciencedirect.com/science/article/pii/S0012821X14003367

Katsu OHTSUKA

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[meteorite-list] The Almahata Sitta polymict breccia and the late accretion of asteroid 2008 TC3

2014-06-12 Thread Katsu OHTSUKA via Meteorite-list

This review paper was published by Marian Horstmann  Addi Bischoff
in the latest issue of Chemie der Erde - Geochemistry.
http://www.sciencedirect.com/science/article/pii/S000928191463

Quite interesting and must-read paper for Almahata Sitta enthusiasts!

Katsu OHTSUKA

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[meteorite-list] Silicate-bearing iron meteorites and their implications for the evolution of asteroidal parent bodies

2014-04-16 Thread Katsu OHTSUKA

The review paper published in the latest Chem der Erde journal,
Silicate-bearing iron meteorites and their implications for the evolution 
of asteroidal parent bodies by Alex Ruzicka, 
is now freely downloadable: the link is

http://www.sciencedirect.com/science/article/pii/S0009281913001104

Regards,

Katsu OHTSUKA
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Re: [meteorite-list] Silicate-bearing iron meteorites and their implications for the evolution of asteroidal parent bodies

2014-04-16 Thread Katsu OHTSUKA

Sorry for wrong link.
If you would like to download the pdf file, you'd better browse first the 
following top page:

http://www.sciencedirect.com/science/journal/00092819?oldURL=y

Katsu

-Original Message- 
From: Katsu OHTSUKA

Sent: Wednesday, April 16, 2014 2:01 PM
To: meteorite-list@meteoritecentral.com
Subject: Silicate-bearing iron meteorites and their implications for the 
evolution of asteroidal parent bodies


The review paper published in the latest Chem der Erde journal,
Silicate-bearing iron meteorites and their implications for the evolution
of asteroidal parent bodies by Alex Ruzicka,
is now freely downloadable: the link is
http://www.sciencedirect.com/science/article/pii/S0009281913001104

Regards,

Katsu OHTSUKA 


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Re: [meteorite-list] NWA CI chondrite? in eBay

2013-11-02 Thread Katsu OHTSUKA

Thanks Gary, Michael and Graham!
Yes, no one in the list would purchase this fake CI.

Katsu

-Original Message- 
From: Graham Ensor

Sent: Friday, November 01, 2013 6:00 PM
To: Michael Mulgrew
Cc: Katsu OHTSUKA ; Meteorite List
Subject: Re: [meteorite-list] NWA CI chondrite? in eBay

My thoughts too Michael..

Graham

On Fri, Nov 1, 2013 at 8:08 AM, Michael Mulgrew mikest...@gmail.com wrote:
Based on the pictures and the description, I'd say it's not a meteorite at 
all.


Michael in so. Cal.

On Fri, Nov 1, 2013 at 12:09 AM, Katsu OHTSUKA ohts...@jb3.so-net.ne.jp 
wrote:

Hello list,

I have just viewed the eBay item NWA CI Carbonaceous ungrouped chondrite 
,

which is
http://www.ebay.com/itm//190950766886
but it looks different from typical CIs, such as Orgueil and Ivuna.
Does anyone hear the existence of NWA CI?

Regards,

Katsu

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[meteorite-list] NWA CI chondrite? in eBay

2013-11-01 Thread Katsu OHTSUKA

Hello list,

I have just viewed the eBay item NWA CI Carbonaceous ungrouped chondrite , 
which is

http://www.ebay.com/itm//190950766886
but it looks different from typical CIs, such as Orgueil and Ivuna.
Does anyone hear the existence of NWA CI?

Regards,

Katsu

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Re: [meteorite-list] Different colors of meteors/shooting stars

2013-09-10 Thread ohtsuka
Also the following Borovicka's paper may be useful for this problem-solving:
http://adsabs.harvard.edu/abs/1994A%26AS..103...83B

Katsu OHTSUKA
Tokyo, JAPAN

 -Original Message-
 From: Michael Mulgrew
 Sent: Tue, Sep 10 2013 17:19:20 JST
 To: Meteorite List
 Subject: Re: [meteorite-list] Different colors of meteors/shooting stars
 
 Perhaps this link is more relevant:
 http://laserstars.org/data/elements/ (please correct me if I'm wrong).
 
 Michael in so. Cal.
 
 On Mon, Sep 9, 2013 at 11:38 PM, Michael Mulgrew mikest...@gmail.com wrote:
  It was graciously pointed out to me that I erred and linked color
  spectra as produced by oxidation rather than by ionization, so feel
  free to disregard my link as it relates to meteors.
 
 
  My bad,
  Michael in so. Cal.
 
 
  
  From: Michael Mulgrew mikest...@gmail.com
  To: James Masny sciflye...@gmail.com
  Cc: Meteorite List Meteorite-list@meteoritecentral.com
  Sent: Monday, September 9, 2013 9:50 PM
  Subject: Re: [meteorite-list] Different colors of meteors/shooting stars
 
  Jim,
 
  This link should provide some additional info:
  http://webmineral.com/help/FlameTest.shtml
 
 
  Happy gazing,
  Michael in so. Cal.
 
  On Mon, Sep 9, 2013 at 9:38 PM, James Masny sciflye...@gmail.com wrote:
   Good evening list.  Sorry if this has been discussed before, but are
   different colors of meteors streaking through the atmosphere
   indicative of certain minerals burning up?  And what color represents
   what minerals?  I remember the 2001 Leonids, and seeing so many
   different colors - pink, blue, white, yellow, green, orange.  The
   other night, I was outside, and I caught 2 fireballs, 1 changed color
   from yellow to red, another from white to yellow.
  
   All the best
   Jim
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[meteorite-list] Asteroid Catalog Using AKARI: AKARI/IRC Mid-Infrared Asteroid Survey

2011-11-09 Thread Katsu OHTSUKA
Hello list, 


The following paper is freely downloadable for a limited time:
Asteroid Catalog Using AKARI: AKARI/IRC Mid-Infrared Asteroid Survey 
F. Usui, et. al., Publ. Astron. Soc. Japan 63, pp.1117-1138 (2011)

http://pasj.asj.or.jp/v63/n5/630526/630526.pdf

Katsu OHTSUKA, 
Tokyo Meteor Net

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[meteorite-list] The origin of the Martian moons revisited

2011-09-22 Thread Katsu OHTSUKA
The paper entitled was published in the latest AARv journal, 
and freely available at 
http://www.springerlink.com/content/q4783536445623t6/


Katsu OHTSUKA

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[meteorite-list] proceedings: NASA CP 2011-216469

2011-09-21 Thread Katsu OHTSUKA
Hello list, 

The proceedings of the Meteoroids2010 meeting is now available at 
http://www.nasa.gov/pdf/580931main_NASA_CP_2011_216469.pdf (size ~43 MB).


Katsu

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[meteorite-list] Particles brought back by Hayabusa identified as from Itokawa

2010-11-16 Thread Katsu OHTSUKA

like LL5--6?

http://www.jaxa.jp/press/2010/11/20101116_hayabusa_e.html

Katsu OHTSUKA
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Re: [meteorite-list] Habital Planet Discovery Announcement

2010-09-29 Thread Katsu OHTSUKA

Its preprint is in arXiv.org
http://lanl.arxiv.org/abs/1009.5733

Katsu
- Original Message - 
From: Sterling K. Webb sterling_k_w...@sbcglobal.net

To: countde...@earthlink.net; meteorite-list@meteoritecentral.com
Sent: Thursday, September 30, 2010 11:27 AM
Subject: Re: [meteorite-list] Habital Planet Discovery Announcement


Hi, Count, List,

Also reported here:
http://www.space.com/scienceastronomy/earth-like-exoplanet-possibly-habitable-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 a system to
fend outside radiation away from.

In general, M-class star systems seem to be quiet places.
Some theorists regard smaller stars as safer places (sort of
like being a stellar mouse; just keep quiet and no one will
notice you). M-class dwarfs are very, very common and often
very old, but their age is often hard to determine. [Their
stellar atmosphere is full of diatomic molecules and their
spectra are, like, scrambled eggs!]

   I looked 

[meteorite-list] 33rd NIPR symposium

2010-05-23 Thread Katsu OHTSUKA

The 33rd Symposium on Antarctic Meteorites (June 8 and 9, 2010)

National Institute of Polar Research,
Tachikawa City, Tokyo, Japan 


http://yamato.nipr.ac.jp/AMRC/symposium/2010/symposium3rd.html

The abstract papers are released and downloadable. 

Katsu 
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[meteorite-list] Extended High Circular Polarization in the Orion Massive Star Forming Region

2010-04-11 Thread Katsu OHTSUKA

Hello all,

The following paper may resolve the amino acid asymmetory in Murchison 
(CM2),


http://www.springerlink.com/content/q0k1k74u76451557/ ,

of which PDF is freely downloadable.

Katsu OHTSUKA 


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Re: [meteorite-list] Meteorite and meteoroid: New comprehensive definitions

2010-04-04 Thread Katsu OHTSUKA
Hello Larry and all, 


Thanks for this. Where was this published? Some of the numbers did not


Maybe in the next (2010 Jan.) issue of MAPS? 


Katsu OHTSUKA
Tokyo, JAPAN
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Re: [meteorite-list] The Perils of Type Collecting - A Guide

2010-03-03 Thread Katsu OHTSUKA

CM2 (Mighei-type)

Katsu

- Original Message - 
From: Greg Stanley stanleygr...@hotmail.com
To: cdtuc...@cox.net; meteorite-list@meteoritecentral.com; 
damoc...@yahoo.com; meteoritem...@gmail.com

Sent: Thursday, March 04, 2010 9:29 AM
Subject: Re: [meteorite-list] The Perils of Type Collecting - A Guide




Murchison is a CM2

Greg S.



Date: Wed, 3 Mar 2010 19:12:20 -0500
From: cdtuc...@cox.net
To: meteorite-list@meteoritecentral.com; damoc...@yahoo.com; 
meteoritem...@gmail.com

Subject: Re: [meteorite-list] The Perils of Type Collecting - A Guide

Good list,
missing is the division between
CBa Buencubbin
CBb HAH 237
CK3
and Tagish lake is not ungrouped but I think is a C2.
--
Carl or Debbie Esparza
Meteoritemax


 Richard Kowalski  wrote:

Thanks a lot Mike.

I thought I had pretty much completed my type set a few months ago, but 
now I see that I'm missed a few gradations that maybe I should pay 
attention to.


I think, for budgetary and sanity sake, I'll have to be selective in how 
fine my divisions are than to try to get every sub-type you mention!


--
Richard Kowalski
Full Moon Photography
IMCA #1081


--- On Wed, 3/3/10, Galactic Stone  Ironworks  wrote:


From: Galactic Stone  Ironworks
Subject: [meteorite-list] The Perils of Type Collecting - A Guide
To: Meteorite List
Date: Wednesday, March 3, 2010, 4:18 PM
Greetings Listees and fellow
collectors,

To the veteran collector, there will be little of interest
in this
post.  This post is directed at the silent newbie or
beginner lurkers
who are sorting through this List and trying to find their
way around
the world of collecting meteorites.

Many new collectors often want one of each type of
meteorite.  Many
veteran collectors abandon this pursuit because the task is
quite
daunting.   So when you hear talk about
type collecting, or building
a type collection, what exactly does that mean?  I
hope the
following brief article will answer those questions, or at
least point
the reader in the right general direction.  Note, I
gleaned much of
this type information from David Weir's authoritative
website
Meteorite Studies and from the Meteoritical
Bulletin.  I do not
claim that this list is 100% complete or without error, so
if the
reader spots an error or omission, please reply and correct
it.

-

The Perils of Type Collecting 

I started out collecting meteorites with a small sample of
NWA 4293 -
an ordinary high iron chondrite of the H6 type. It was
about the size
of a dog-food kibble and it looked like one. But I was
instantly
hooked, and I wanted to have one each of the different
types of
meteorite. This is known as type collecting or building a
type
collection.

The danger of type collecting (besides the damage to one's
checking
account) is that the various petrologic types are
subdivided into
various grades according to metamorphism.

For example, take the H chondrite group that my NWA 4293
sample belonged to.

There are H3 chondrites, H4 chondrites, H5 chondrites, and
H6
chondrites. Did I really need one each of these subtypes?
Well, it
depends on how deep a collector wants to go into the rabbit
hole.
There are distinct differences between the various H types.
The number
attached to each is more than just a simple weathering
grade or shock
grade. It represents a progession in the H-chondrite family
from least
altered to most altered. H3 chondrites are loaded with
chondrules, H4
have some chondrules, H5 has few chondrules, and H6 has
virtually no
visible chondrules. A new grade of H7 has been added as
well. So, a
collector could simply have a single Hx chondrite and say
that the
H-chondrites are represented. Or, the collector could have
one each of
the different subtypes from 3 to 7.

Another peril is the changing of nomenclature. For example,
the
K-subgroup of carbonaceous chondrites was only recognized
and
designated in 1990. Up until then, Karoonda was considered
a CV4
meteorite of the Vigarano family. Now Karoonda is
recognized as
distinctly different type of carbonaceous chondrite, so it
was made
into it's own group. Now we have CK4, CK5, and CK6
meteorites - all
represent a progression in metamorphism and have visible
(and
chemical) differences from other grades. There are standout
members of
each subgroup, so where does one draw the line? Should the
collector
acquire a sample of Karoonda and be done with it? Or should
the
collector go out and track down CK4, CK5 and CK6
meteorites? Again, it
depends on how extensive and exhaustive a collector wants
to be with
their type collection. Budget will also play a role as
well, because
an exhaustive type collection is a daunting project.

Lastly, one must consider the ungrouped meteorites. These
are oddball
meteorites that do not neatly fit into the pre-existing
meteorite
types. There are ungrouped chondrites, ungrouped
achondrites, and
ungrouped irons. No type collection can overlook these
meteorites
because some of them are types 

Re: [meteorite-list] Two extraterrestrial dust horizons found in theDome Fuji ice core

2010-01-03 Thread Katsu OHTSUKA

Dear Paul,

Thank you for sharing.
All the papers of EPSL Vol.289, issues1-2, 2010 (including Misawa's paper)
would be downloadable for everyone (non-subscriber, too), as free copies.

http://www.sciencedirect.com/science?_ob=PublicationURL_cdi=5801_auth=y_acct=C50221_version=1_urlVersion=0_userid=10_pubType=Jmd5=52c7e8b29221fe23b6fc7aa3ca3251f1

Katsu OHTSUKA

- Original Message - 
From: Paul Heinrich oxytropidoce...@cox.net

To: Meteorite List meteorite-list@meteoritecentral.com
Sent: Monday, January 04, 2010 10:31 AM
Subject: [meteorite-list] Two extraterrestrial dust horizons found in 
theDome Fuji ice core






Misawa, K., M. Kohno, T. Tomiyama, T. Noguchi, T. Nakamura,
K. Nagao, T.Mikouchi, and K. Nishiizumi, 2010, Two extraterrestrial
dust horizons found in the Dome Fuji ice core, East Antarctica. Earth
and Planetary Science Letters. vol. 289, no. 1-2, pp. 287-297.

http://dx.doi.org/10.1016/j.epsl.2009.11.016

In part the abstract reads,

Two silicate-rich dust layers were found in the Dome Fuji ice core
in East Antarctica, at Marine Isotope Stages 12 and 13. Morphologies,
textures, and chemical compositions of constituent particles reveal
that they are high-temperature melting products and are of
extraterrestrial origin. Because similar layers were found approximately
2000 km east of Dome Fuji, at EPICA (European Project for Ice
Coring in Antarctica)-Dome C, particles must have rained down
over a wide area 434 and 481 ka.

Mention is also made of these dust horizons in:

Narcisi, B., J. Robert Petit, and B. Delmonte, nd, Quaternary Science
Reviews, Article in Press, Corrected Proof

http://dx.doi.org/10.1016/j.quascirev.2009.07.009

A related paper that is available online as a PDF fils is:

Duprat , J., C. Engrand , M. Maurette , G. Kurat , M. Gounelle ,
and C. Hammer, 2007, Micrometeorites from Central Antarctic snow:
The CONCORDIA collection. Advances in Space Research. vol. 39,
pp. 605–611.

Abstract at http://dx.doi.org/10.1016/j.asr.2006.05.029

PDF file at:

http://www2.mnhn.fr/hdt205/leme/doc/2007%20Duprat%20et%20al.%20ASR.pdf

Yours,

Paul H.

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[meteorite-list] Solar-Radiation Heating Effects on 3200 Phaethon

2009-12-29 Thread Katsu OHTSUKA

Hello list,

My paper entitled Solar-Radiation Heating Effects on 3200 Phaethon
was finally published in the latest issue of PASJ, as follows,


http://pasj.asj.or.jp/v61/n6/610621/610621.pdf,

of which PDF file is freely downloadable now. 


Katsu OHTSUKA

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[meteorite-list] COMET P/1783 W1 = 2003 A 1 = 2009 R2 (PIGOTT-LINEAR-KOWALSKI)

2009-09-12 Thread ohtsuka
Great job! Congrats, Richard!

http://www.cfa.harvard.edu/mpec/K09/K09R40.html
http://www.comethunter.de/

Katsu OHTSUKA
Tokyo, JAPAN
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[meteorite-list] 32nd Symposium on Antarctic Meteorites

2009-05-30 Thread Katsu OHTSUKA
The 32nd Symposium on Antarctic Meteorites will be held at 
National Institute of Polar Research, Tachikawa City, Tokyo, Japan, 
on June 3 and 4, 2009.


http://www.metsoc2008.jp:80/nipr/symposium/2009/symposium3rd.html 

The program and abstracts are downloadable from 


http://www.metsoc2008.jp/nipr/symposium/2009/Program2009.pdf

Katsu
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Re: [meteorite-list] Kuiper Belt Meteorites?

2009-05-23 Thread Katsu OHTSUKA

Hello Eric, Larry, Matthias, and all

El-Quss Abu Said (CM2) seems to be a cometary (or KBO) meteorite
candidate:
http://adsabs.harvard.edu/abs/2008M%26PSA..43.5124N

Katsu OHTSUKA

- Original Message - 
From: Matthias Bärmann majbaerm...@web.de

To: lebof...@lpl.arizona.edu; Erik Fisler erikfw...@msn.com
Cc: meteorite-list meteorite-list@meteoritecentral.com
Sent: Saturday, May 23, 2009 8:31 AM
Subject: Re: [meteorite-list] Kuiper Belt Meteorites?



Hello Eric, Larry, list , -

Tagish Lake is supposed to be one candidate ...
http://www.scientificamerican.com/article.cfm?id=ancient-meteorites-from-o

Best regards,

Matthias Baermann


- Original Message - 
From: lebof...@lpl.arizona.edu

To: Erik Fisler erikfw...@msn.com
Cc: meteorite-list meteorite-list@meteoritecentral.com
Sent: Saturday, May 23, 2009 12:41 AM
Subject: Re: [meteorite-list] Kuiper Belt Meteorites?



Hi Erik:

If memory serves, the original reason that G. P. Kuiper proposed the
existance of the [Edgeworth] Kuiper Belt was as a source of comets with
relatively short period (under a hundred years or so?) comets.

So, if you believe that some meteorites ocme from comets, then these
probably originated in the Kuiper Belt.

Larry



Does anyone know if any meteorites on Earth are linked
to the Kuiper Belt Objects?
or is that too far away for a material to travel all the way to
Earth? or would Jupiter trap any parent bodies traveling past it?

[Erik]
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Re: [meteorite-list] Carancas paper

2008-06-20 Thread ohtsuka
Dear Starling and all, 

Thank you for your response.
I agree to your opinion. 
However, their computational results are 
correct if their (frangment) model is true. 
Anyway, you'd better send your comment to 
the authors. 

The Carancas session will be held in ACM 2008, 
Baltimore, July 15. The link is below: 

http://www.lpi.usra.edu/meetings/acm2008/pdf/sess305.pdf 

Does anyone in the list have a plan to attend this session? 

best,

Kastu OHTSUKA
Tokyo, JAPAN

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[meteorite-list] Carancas paper

2008-06-17 Thread ohtsuka
Hello list members, 

I have just downloaded a free PDF file of the letter paper on the Carancas 
event,  
published in AA yesterday. This seems to be very interesting and the 
link is below: 

http://www.aanda.org/index.php?option=articleaccess=standardItemid=129url=/articles/aa/abs/2008/26/aa09905-08/aa09905-08.html

Katsu
Tokyo, JAPAN

--

AA 485, L1-L4 (2008) 
DOI: 10.1051/0004-6361:200809905


Letter
The Carancas meteorite impact - Encounter with a monolithic meteoroid
J. Borovicka and P. Spurn? 

Astronomical Institute of the Academy of Sciences, Fricova 298, 25165 Ondrejov 
Observatory, Czech Republic 
e-mail: [EMAIL PROTECTED] 

Received 4 April 2008 / Accepted 4 May 2008

Abstract 
The formation of a 13-m wide impact crater by a stony meteorite near Carancas, 
Peru, on September 15, 2007 was an unexpected event. Stony meteoroids usually 
disintegrate in the atmosphere in many pieces, each landing at low velocity. We 
present examples of well-observed fireballs, which have all experienced 
atmospheric fragmentation. Using a simple model, we find that the Carancas 
meteoroid may have avoided fragmentation, if its strength was 20-40 MPa; such a 
strength would be comparable to the tensile strength of stony meteorites, but 
is higher than the strength of other observed meteoroids. We conclude that 
Carancas was a rare example of a monolithic meteoroid that was free of internal 
cracks. This example demonstrates that meteoroid strength can vary 
significantly from case to case and does not depend on meteoroid size. We 
estimate that the initial size of Carancas meteoroid was 0.9-1.7 m. Our model 
predicts an impact velocity that w
as in the range 2-4 km s-1. 


Key words: meteors, meteoroids -- Earth 

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[meteorite-list] The significance of mete orite density and porosity

2008-05-04 Thread ohtsuka
Dear List members,

Now you can freely download the PDF file of 
the title's paper in Chem Elde, which is very interesting.

http://www.sciencedirect.com/science?_ob=ArticleURL_udi=B7CW6-4S38C18-1_user=10_coverDate=04%2F30%2F2008_rdoc=2_fmt=high_orig=browse_srch=doc-info(%23toc%2318098%232008%23999319998%23684461%23FLA%23display%23Volume)_cdi=18098_sort=d_docanchor=_ct=10_acct=C50221_version=1_urlVersion=0_userid=10md5=5e4a816337b15ed7408ac5dc9403709b

Best

Katsu OHTSUKA, 
Tokyo, JAPAN
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Re: [meteorite-list] Fw: Comet 17P (Holmes) Visible Event !

2007-10-24 Thread K. Ohtsuka
Hello all,

I have just looked at the superoutburst of 17P/Holmes,
as follows:

2007 Oct. 24.72 UT: m1=2.8, Dia.=, DC=9, by NE

Katsu. OHTSUKA
Tokyo, JAPAN

- Original Message - 
From: giovannisostero [EMAIL PROTECTED]
To: mexicodoug [EMAIL PROTECTED]
Cc: meteorite-list meteorite-list@meteoritecentral.com
Sent: Thursday, October 25, 2007 1:22 AM
Subject: Re: [meteorite-list] Fw: Comet 17P (Holmes) Visible Event !


 Hi all,
 this is our BVR shot of 17P/Holmes in outburst (brightest object in the
field center):

 http://tinyurl.com/2mxrmx

 Cheers,
 Giovanni and Ernesto


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

2007-10-09 Thread K. Ohtsuka
Hello Sterling,

Thank you for letting me know your translation of
the Bolivian publications, which is very interesting.

Just before, I visited  http://spaceweather.com/,
where another latest infrasound analysis of the
Peruvian event by Peter Brown (Univ. W. Ontario)
is introduced. His team estimated the kinetic energy
of the impactor about 0.03 kton TNT.

Best wishes,

Kastu

- Original Message - 
From: Sterling K. Webb [EMAIL PROTECTED]
To: meteorite-list@meteoritecentral.com
Cc: Rob Matson [EMAIL PROTECTED]; K. Ohtsuka
[EMAIL PROTECTED]
Sent: Tuesday, October 09, 2007 9:14 AM
Subject: Re: [meteorite-list] Publications of the Carancas event ADDITIONAL


 Hi,

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

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

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

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


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


 Hello list members,

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

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

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

 Does anyone translate and introduce their summary?

 Best wishes,

 Katsu OHTSUKA
 Tokyo, JAPAN

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[meteorite-list] Publications of the Carancas event

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

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

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

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

Does anyone translate and introduce their summary?

Best wishes,

Katsu OHTSUKA
Tokyo, JAPAN

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

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

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


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

2007-01-18 Thread K. Ohtsuka
Amazing COMET!
COMET McNAUGHT is just reverse COMET WEST in 1976!

http://spaceweather.com/comets/mcnaught/17jan07/Crause2.jpg

http://www.spacew.com/gallery/image005564.html

Katsuhito
Tokyo, JAPAN
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Re: [meteorite-list] Week-Long Meteor Shower to Dazzle (Geminids)

2006-12-09 Thread K. Ohtsuka
Hello Sterling and all,

Please see also the following papers on Apollo asteroid 2005 UD, mini
Phaethon,
if you are interested in:

Title: Apollo asteroid 2005 UD: split nucleus of (3200) Phaethon?
Authors: Ohtsuka, K.; Sekiguchi, T.; Kinoshita, D.; Watanabe, J.-I.; Ito,
T.; Arakida, H.; Kasuga, Publication: Astronomy and Astrophysics, Volume
450, Issue 3, May II 2006, pp.L25-L28.

The PDF file of my paper is in paper folder in the following link:
http://briefcase.yahoo.co.jp/bc/tokyometeor/


Title: Physical Observations of 2005 UD: A Mini-Phaethon
Authors: Jewitt, David; Hsieh, Henry
Publication: The Astronomical Journal, Volume 132, Issue 4, pp. 1624-1629.

The PDF file of Jewitt's paper is in the following link:
http://www.ifa.hawaii.edu/faculty/jewitt/papers/2006/JH06.pdf

Both Phaethon and 2005 UD are F or B-type asteroids, thus linking to
thermally metamorphosed CI/CM.

Katsuhito OHTSUKA
Tokyo, JAPAN

- Original Message - 
From: Sterling K. Webb [EMAIL PROTECTED]
To: Ron Baalke [EMAIL PROTECTED]; Meteorite Mailing List
meteorite-list@meteoritecentral.com
Sent: Saturday, December 09, 2006 5:53 AM
Subject: Re: [meteorite-list] Week-Long Meteor Shower to Dazzle (Geminids)


 Hi,

 Nice timing, since we've been talking about
 chunks of comet:

  A final point to note are that Geminids stand apart from the other
  meteor showers in that they seem to have been spawned not by a comet,
  but by 3200 Phaeton, an Earth-crossing asteroid.  Then again, the
  Geminids may be comet debris after all, for some astronomers
  consider Phaeton to really be the dead nucleus of a burned-out comet
  that somehow got trapped into an unusually tight orbit.

 Discovered in 1983, Phaethon is 5100 meters
 in diameter and weighs in at 140,000,000 metric
 tons. It has a very dark surface and a density
 (vaguely) calculated at twice that of water.
 Despite being in a cometary orbit and being
 the parent body of a meteor stream in the same
 orbit, it has never shown any coma, dust, or
 gas outbursts. Dead comet? Asteroid? Or can
 we be sure there's really any difference? Yet?
 Phaethon approaches the Sun closer than
 any other numbered asteroid; its perihelion is
 only 0.140 AU, 58% of Mercury's orbital radius.
 The surface temperature at perihelion could
 reach ~1025 K.
 Obviously, it's not a ball of ice.
 If you plan on hanging around until 2093,
 it will closely approach the Earth, passing
 within 0.0198 AU, on December 14 of that
 year. Only a week and 87 years to go.
 3200 Phaethon is one of the objects that fit
 unto a pattern of a past breakup of a Comet
 Encke parent body, based on its orbital properties,
 an admittedly controversial idea (but a good one).
 The asteroid 3200 Phaethon was discovered
 as an asteroid, confirmed, plotted, and published,
 before Fred (Mr. Comet) Whipple pointed out
 that its orbit was identical with that of the
 Geminids.


 Sterling K. Webb
 --
-
 - Original Message - 
 From: Ron Baalke [EMAIL PROTECTED]
 To: Meteorite Mailing List meteorite-list@meteoritecentral.com
 Sent: Friday, December 08, 2006 1:46 PM
 Subject: [meteorite-list] Week-Long Meteor Shower to Dazzle (Geminids)


 
  http://www.space.com/spacewatch/061208_night_sky.html
 
  Week-Long Meteor Shower to Dazzle
  By Joe Rao
  SPACE.com
  08 December 2006
 
  The annual Geminid meteor shower is expected to produce a reliable
  shooting star show that will get going Sunday and peak the middle of
  next week.
 
  The Geminid event is known for producing one or two meteors every minute
  during the peak for viewers with dark skies willing to brave chilly
  nights.
 
  If the Geminid Meteor Shower occurred during a warmer month, it would be
  as familiar to most people as the famous August Perseids.
  Indeed, a night all snuggled-up in a sleeping bag under the stars is an
  attractive proposition in summer. But it's hard to imagine anything more
  bone chilling than lying on the ground in mid-December for several hours
  at night.
 
  But if you are willing to bundle up, late next Wednesday night into
  early Thursday morning will be when the Geminids are predicted to be at
  their peak.
 
  Most satisfying shower
 
  The Geminids are a very fine winter shower, and usually the most
  satisfying of all the annual showers, even surpassing the Perseids.
  Studies of past displays show that this shower has a reputation for
  being rich both in slow, bright, graceful meteors and fireballs as well
  as faint meteors, with relatively fewer objects of medium brightness.
  Many appear yellowish in hue. Some even appear to form jagged or divided
  paths.
 
  Unfortunately, as was the case this year with its summertime
  counterpart, this year's December Geminids will be hindered somewhat by
  moonlight, although to a much lesser degree than the brilliant gibbous
  Moon that wreaked havoc with the Perseids.
 
  On Thursday

Re: [meteorite-list] Meteorites Used To Study Solar Activity AT LAST!!!

2006-09-28 Thread K. Ohtsuka
Hello list members,

see the following link,

http://www.aanda.org/index.php?option=com_contenttask=viewid=181Itemid=42lang=en

where you can download the PDF file of the AA letter.

Katsuhito O.
Tokyo, JAPAN


- Original Message - 
From: Rob McCafferty [EMAIL PROTECTED]
To: meteorite-list@meteoritecentral.com
Sent: Thursday, September 28, 2006 7:00 AM
Subject: [meteorite-list] Meteorites Used To Study Solar Activity AT LAST!!!


 Hi all

 This phenomena of cosmic ray alteration of isotope
 concentration has been known to me for a long while.

 As solar activity increases, it deflects the cosmic
 rays which reduces the effect of cosmic rays.

 On earth, one of it's best effects is altering the
 amount of Carbon 14 (C14) prodced during periods of
 high solar activity. C14 has a known half-life of
 approx 5800 years and is created constantly so all
 things once living have a known amount of it. Once
 they die, this proportion decreases.

 Less well known is that year on year, the proportion
 of C12/C14 changes according to solar activity.
 Correction factors have to be made in carbon dating.

 Individual tree rings can be measured for actual vs
 predicted C12/C14 ratios and a picture of solar
 activity can be build up.

 This method shows several things

 Tree rings from 1640 to 1710 show a big increase in
 C14 vs predicted signifying a low solar activity. This
 roughly corresponds to a period of low temperature.
 The Thames in London used to freeze each winter and
 was so thick fairs could be held on the ice.

 It suggests that in Roman times, temperatures were
 even warmer than today. Grapes can only be grown in
 south east England today. Back then they could be
 grown North of York.

 It also suggests a general increase in solar activity
 over the last few hundred years, since the Maunder
 minimum, in fact. We're on a rise now, apparently.

 If meteorites are also showing this trend, some
 credence must be give to the The Human Race is a
 bunch of arrogant idiots who think they are more
 influential in the Grand Scheme of Things than they
 really are school of thought which I aspire to
 ascribe.

 Equally, I suggest that this blip in the epochs of
 time should be a timely reminder not to mess with
 things too much as we really have no idea how much
 influence we really have.

 Just my thoughts for the subject.

 (DISCLAIMER: this post was not sponsored by
 Shell/BP/XXon/FINA/Texaco or any other petrolium
 industry, etc. The author cannot discount the
 possibility that the original meteorite study may have
 been. He would like to distance himself from any
 suggestions to that effect

 I think that puts me in the clear)

 Anon (just in case)



 --- Matson, Robert [EMAIL PROTECTED] wrote:

  Hi All,
 
  Who'da thunk that global warming could become an
  on-topic
  subject for the meteorite list?!  --Rob
 
  -Original Message-
  From: [EMAIL PROTECTED]
  [mailto:[EMAIL PROTECTED]
  On Behalf Of Ron
  Baalke
  Sent: Tuesday, September 26, 2006 2:15 PM
  To: Meteorite Mailing List
  Subject: [meteorite-list] Meteorites Used To Study
  Solar Activity
 
 
 http://www.upi.com/NewsTrack/view.php?StoryID=20060926-015940-3936r
 
  Meteorites used to study solar activity
  UPI
  September 26, 2006
 
  OULU, Finland (UPI) -- A Finnish-led international
  team has used
  meteorites to investigate the sun's solar activity
  of past centuries.
 
  Ilya Usoskin at Finland's Sodankyla Geophysical
  Observatory and
  colleagues compared the amount of Titanium 44 in 19
  meteorites that have
  fallen to the Earth the past 240 years. They said
  their findings confirm
  that solar activity increased strongly during the
  20th century. They
  also find the sun has been particularly active
  during the past few
  decades.
 
  The scientists say studying the sun's activity is
  one of the oldest
  astrophysical projects, as astronomers began
  recording the number of
  sunspots to trace the sun's magnetic activity 400
  years ago.
 
  The team examined a set of 19 meteorites whose dates
  of fall are
  precisely known, measuring the amount of radioactive
  isotope Titanium 44
  in each meteorite. Titanium 44 is produced by the
  cosmic rays in the
  meteorites while they are outside the Earth's
  atmosphere. After the
  meteorite has fallen, it stops producing the
  isotope.
 
  By measuring the Titanium 44 in the meteorites, the
  scientists
  determined the level of solar activity at the time
  the meteorite fell.
 
  The study appears in the journal Astronomy 
  Astrophysics Letters.
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[meteorite-list] Great fireball in Japan

2006-08-10 Thread K. Ohtsuka
Hello list members,

A great fireball was witnessed by numerous people in Japan on the night of
August 9, 23:28:41 JST (=14:28:41 UT). Saturated images, due to its strong
luminosity, were recorded by several CCD cameras in the Fireball Network in
Japan, and now their data are processed. It maybe a member of the
Capricornid meteor shower with the geocentric velocity of around 20 km/sec.
If so, it is no meteorite dropping fireball.

http://sonotaco.jp/forum/viewtopic.php?t=1080

Katsuhito O.
Tokyo

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Re: [meteorite-list] Tokyo Area Boloide...info required

2006-04-12 Thread K. Ohtsuka
Hello Dirk-san,

This event? I could not see this bolide, too.

http://sonotaco.jp/forum/viewtopic.php?t=929

Katsuhito O.
Tokyo, JAPAN

- Original Message - 
From: drtanuki
To: meteorite-list@meteoritecentral.com
Sent: Wednesday, April 12, 2006 5:58 PM
Subject: [meteorite-list] Tokyo Area Boloide...info required


Dear List,
  A boloide  was seen and photographed in the Tokyo area while I was absent
from Japan (in the past two weeks).  My wife said film was shown on Japanese
TV but she was not paying attention.  I have done a websearch but found
nothing.  If I gain any information I will pass it on to the list.
  Best, Dirk Ross...Tokyo



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Re: [meteorite-list] Problems with ebay

2006-02-23 Thread K. Ohtsuka
I was also troubled as well as Matteo, some five hours before. But, now no
problem. That may be caused by the eBay website, I guess.

Katsuhito O.
Tokyo

- Original Message - 
From: Michael Farmer [EMAIL PROTECTED]
To: M come Meteorite Meteorites [EMAIL PROTECTED];
MeteoriteList meteorite-list@meteoritecentral.com
Sent: Friday, February 24, 2006 12:53 AM
Subject: Re: [meteorite-list] Problems with ebay


 That is very interesting, I have the same problem on my laptop when I go
to
 the Comcast homepage, it will not open and IU get high pitched clicks
 non-stop.
 Any computer guru out there know what this might be?
 mike
 - Original Message - 
 From: M come Meteorite Meteorites [EMAIL PROTECTED]
 To: MeteoriteList meteorite-list@meteoritecentral.com
 Sent: Thursday, February 23, 2006 12:58 AM
 Subject: [meteorite-list] Problems with ebay


  Hello
 
  its from yesterday I have problems to enter in My Ebay
  page on ebay.com. When I click this not open and it
  hears itself a continue click,click,click of
  background...you have the same problem? If I enter
  with ebay.it I not have this problem.
 
  Matteo
 
 
  M come Meteorite - Matteo Chinellato
  Via Triestina 126/A - 30030 - TESSERA, VENEZIA, ITALY
  Email: [EMAIL PROTECTED]
  Sale Site: http://www.mcomemeteorite.it
  Collection Site: http://www.mcomemeteorite.info
  MSN Messanger: spacerocks at hotmail.com
  EBAY.COM:http://members.ebay.com/aboutme/mcomemeteorite/
 
 
 
 
 
 
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Re: [meteorite-list] Harvey Awards - New Catagory

2006-01-25 Thread K. Ohtsuka
Yes from Tokyo, JAPAN

Katsuhito OHTSUKA
- Original Message - 
From: Greg Hupe [EMAIL PROTECTED]
To: meteorite-list@meteoritecentral.com
Sent: Wednesday, January 25, 2006 4:24 AM
Subject: [meteorite-list] Harvey Awards - New Catagory


 Dear List Members,

 A month or two ago I posted to the list that I felt that Steve Arnold -
IMB
 and Phil Mani should be nominated for a Harvey Award for their Huge
Brenham
 Main Mass discovery and also Geoff Notkin for his tireless work on behalf
of
 the Hurricane Katrina Fund Raiser among other too-numerous to list
 meteorite-related activities.

 I know that Geoff and Steve originally set up the Harvey Awards where they
 could not nominate themselves for an award. I would like all list members
to
 join me here on the list to nominate these fine gentleman for a Harvey
Award
 an encourage them to make a new category where they could receive an award
 if enough of us voted YES to this. Maybe they could create a People's
 Choice award or something along these lines.

 Everyone in favor, send the list a resounding YES and lets acknowledge
 their contributions and achievements in public.

 Consider this my YES vote...

 Best regards,

 Greg Hupe
 The Hupe Collection
 NaturesVault (eBay)
 [EMAIL PROTECTED]
 IMCA 3163

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[meteorite-list] NIPR meteorite newsletter

2005-10-08 Thread K. Ohtsuka
Hello list,

The latest NIPR meteorite newsletter ,vol.13 no.1 (pdf 17.0 Mb), was
published, which includes some color pictures of thin sections and PTS.

http://yamato.nipr.ac.jp/AMRC/AMRC/MeteoriteNewsletter_13-1.pdf

K. Ohtsuka, TOKYO


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Re: [meteorite-list] Unlocking the Organic Composition of AncientAsteroids

2005-10-07 Thread K. Ohtsuka
see also

http://ads.nao.ac.jp/cgi-bin/nph-bib_query?bibcode=2005P%26SS...53.1280Samp;db_key=ASTamp;data_type=HTMLamp;format=amp;high=411ea5d28b29620

Kat. O., TOKYO

- Original Message - 
From: Ron Baalke [EMAIL PROTECTED]
To: Meteorite Mailing List meteorite-list@meteoritecentral.com
Sent: Saturday, October 08, 2005 1:28 AM
Subject: [meteorite-list] Unlocking the Organic Composition of
AncientAsteroids



 http://www.physorg.com/news7056.html

 Unlocking the organic composition of ancient asteroids
 by Gina Buss
 PhysOrg.com
 October 07, 2005

 Meteorites contain fragments of asteroids brought about by collisions
 within the asteroid belt. These meteorites have not been exposed to
 geological processes experienced by planets and stars. Therefore, much
 of the matter in these meteorites originates from the formation of the
 Solar System some 4.5 billion years ago.

 Being the only record of the Solar System's pre-biotic chemical
 evolution, scientists have tried for years to extract and study this
 material. It is believed that discovering the composition of meteorites
 will reveal what the Solar System was made of at its birth and how those
 materials evolved into our current-day universe.

 Most of the methods used to extract this matter have failed leading to
 the destruction of the meteorite material or just the inability to
 extract any compounds.

 However, a recent study from the Planetary and Space Science Journal
 explains how scientists have developed a novel approach to extracting
 these meteoric materials. It's called hydropyrolysis.

 This new technology uses high hydrogen gas pressures, extreme
 temperature, and water as a non-destructive means for extracting organic
 and inorganic compounds from meteorites.

 This process has revealed high amounts of carbon and nitrogen- elements
 essential to life at the core of the meteorites. Also, this new
 technology revealed several never-before-seen organic molecules.

 The results of this study also contradict a common understanding to the
 origin of meteorites. It is thought that meteoric material originated
 from a molecular could that collapsed to form the Solar System.
 Scientists using hydropyrolysis believe this is a misconception and seek
 to use this technology to find the true origin of the organic matter in
 meteorites.

 Scientists hope that the use of this new technology will offer even more
 clues into the composition of the Solar System when it was forming.

 Finally researchers have a way to trace the evolutionary path of organic
 compounds which will ultimately lead to knowledge of the evolution of
 our universe.

 Reference:
 Sephton M, Love G, Meredith W, Snape C, Sun C, and Watson J. 2005.
 Planetary and Space Science Journal. Article in Press.


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Re: [meteorite-list] Hayabusa Begins Daring Close Encouter WithAsteroid

2005-09-14 Thread K. Ohtsuka
Hello Jeff-san
You can find Itokawa's latest image(s) at the following site:

http://www.isas.ac.jp/e/snews/index.shtml

K. Ohtsuka, Tokyo Meteor Network

- Original Message - 
From: Jeff Kuyken [EMAIL PROTECTED]
To: Ron Baalke [EMAIL PROTECTED]; Meteorite Mailing List
meteorite-list@meteoritecentral.com
Sent: Thursday, September 15, 2005 9:02 AM
Subject: Re: [meteorite-list] Hayabusa Begins Daring Close Encouter
WithAsteroid


 Hi List,

 Does anyone have a link to images that Hayabusa is sending back?

 Thanks,

 Jeff


 - Original Message -
 From: Ron Baalke
 To: Meteorite Mailing List
 Sent: Thursday, September 15, 2005 9:27 AM
 Subject: [meteorite-list] Hayabusa Begins Daring Close Encouter With
 Asteroid

 http://www.spaceflightnow.com/news/n0509/14hayabusa/

 Probe begins daring close encounter with asteroid
 BY STEPHEN CLARK
 SPACEFLIGHT NOW
 September 12, 2005

 A $100 million Japanese space explorer parked in the vicinity of an
 enigmatic asteroid this week, allowing scientists to get a first glimpse
 of the mid-sized rock that will become the source of the first samples
 of such an object to ever be returned to Earth.

 After methodically tweaking its course - first by electrical ion
 propulsion, then by conventional chemical thrusters - toward its target
 over the past few months, the Hayabusa probe finally arrived at its
 station keeping position some 12 miles from the asteroid early Monday.

 Officials timed the arrival by when the 1,000-pound craft's closure rate
 relative to the object reached zero, indicating the probe was now
 essentially anchored in the gate position located about 12 miles from
 the space rock. That moment occurred as the spacecraft commanded its
 maneuvering jets to fire one last time at about 0117 GMT Monday, or in
 the late-morning hours in Japan.

 Hayabusa's ion drive propulsion system took a the leading role for the
 rendezvous up until August 28, when control switched to the
 liquid-fueled chemical thrusters. That milestone left the four ion
 engines with a cumulative burn time of almost 26,000 hours, and the
 system will be re-started once the probe embarks on the last leg of its
 journey back to Earth.

 The delicate space ballet took place almost 200 million miles from
 controllers on Earth, who left responsibility for the rendezvous to an
 on-board navigation system that is designed to operate without ground
 intervention.

 The goal of the mission is to study asteroid 1998 SF36 - later named
 Itokawa in honor of an early Japanese pioneer in rocketry. The object
 was discovered in September 1998 by a joint team consisting of
 scientists from the U.S. Air Force, NASA, and the Massachusetts
 Institute of Technology.

 Details about Itokawa have largely remained elusive in the seven years
 since its discovery, but scientists now have a much clearer picture of
 the potato-shaped asteroid estimated to measure 2,000 feet by around 900
 feet. Its orbit stretches from inside Earth's out to a distance of 157
 million miles from the Sun, making it a member of the Apollo class of
 near-Earth asteroids that pose potential impact threats to our planet.

 Astronomers studied Itokawa via several ground-based telescopes during
 its last Earth fly-by in 2001, and they found evidence that the asteroid
 was brighter and more reflective than first expected. Scientists had a
 difficult time predicting what Hayabusa would find as it closed in on
 the object, and many questions were left unanswered.

 However, many of those issues can now be thoroughly remedied with the
 new higher resolution images Hayabusa's optical asteroid multi-band
 imaging camera has captured. The pictures show a contrast of rocky and
 hilly terrain with smooth regions, but detailed analysis and sample
 retrieval will be conducted before scientists can announce the results
 of their detailed study.

 A first look at the new images appears to show a loose layer of dust and
 dirt-like material covering the smooth surfaces of parts of the
 asteroid, which is a surprise to some project officials.

 According to a certain theory, small objects do not have regolith,
 said Hayabusa project manager Jun Kawaguchi. But this asteroid seems to
 have smooth portions that appear (to have) some regolith.

 Work with Hayabusa's science payload has already begun, with the
 near-infrared and X-ray spectrometers now gathering measurements. The
 craft's laser altimeter is also conducting observations to learn more
 details about Itokawa's terrain.

 The pair of spectrometers will labor to determine the elemental and
 mineral composition of Itokawa to help astronomers in their quest to
 link asteroids and comets to meteorites that have fallen to Earth and
 been recovered.

 The analysis has just started and no conclusive results (are) given
 until the measurements are detailed and analyzed, Kawaguchi told
 Spaceflight Now.

 When we talk about the shape just from impression and not from a
 scientific point

Re: [meteorite-list] Hayabusa Begins Daring Close EncouterWithAsteroid

2005-09-14 Thread K. Ohtsuka
P.S. Color composite images (but still looks like b/w image) of Itokawa are
released in Japanese page,
but not yet in English page.

 http://www.isas.ac.jp/j/snews/2005/0914.shtml

Katsu O.

- Original Message - 
From: K. Ohtsuka [EMAIL PROTECTED]
To: Meteorite Mailing List meteorite-list@meteoritecentral.com
Sent: Thursday, September 15, 2005 9:45 AM
Subject: Re: [meteorite-list] Hayabusa Begins Daring Close
EncouterWithAsteroid


 Hello Jeff-san
 You can find Itokawa's latest image(s) at the following site:

 http://www.isas.ac.jp/e/snews/index.shtml

 K. Ohtsuka, Tokyo Meteor Network

 - Original Message - 
 From: Jeff Kuyken [EMAIL PROTECTED]
 To: Ron Baalke [EMAIL PROTECTED]; Meteorite Mailing List
 meteorite-list@meteoritecentral.com
 Sent: Thursday, September 15, 2005 9:02 AM
 Subject: Re: [meteorite-list] Hayabusa Begins Daring Close Encouter
 WithAsteroid


  Hi List,
 
  Does anyone have a link to images that Hayabusa is sending back?
 
  Thanks,
 
  Jeff
 
 
  - Original Message -
  From: Ron Baalke
  To: Meteorite Mailing List
  Sent: Thursday, September 15, 2005 9:27 AM
  Subject: [meteorite-list] Hayabusa Begins Daring Close Encouter With
  Asteroid
 
  http://www.spaceflightnow.com/news/n0509/14hayabusa/
 
  Probe begins daring close encounter with asteroid
  BY STEPHEN CLARK
  SPACEFLIGHT NOW
  September 12, 2005
 
  A $100 million Japanese space explorer parked in the vicinity of an
  enigmatic asteroid this week, allowing scientists to get a first glimpse
  of the mid-sized rock that will become the source of the first samples
  of such an object to ever be returned to Earth.
 
  After methodically tweaking its course - first by electrical ion
  propulsion, then by conventional chemical thrusters - toward its target
  over the past few months, the Hayabusa probe finally arrived at its
  station keeping position some 12 miles from the asteroid early Monday.
 
  Officials timed the arrival by when the 1,000-pound craft's closure rate
  relative to the object reached zero, indicating the probe was now
  essentially anchored in the gate position located about 12 miles from
  the space rock. That moment occurred as the spacecraft commanded its
  maneuvering jets to fire one last time at about 0117 GMT Monday, or in
  the late-morning hours in Japan.
 
  Hayabusa's ion drive propulsion system took a the leading role for the
  rendezvous up until August 28, when control switched to the
  liquid-fueled chemical thrusters. That milestone left the four ion
  engines with a cumulative burn time of almost 26,000 hours, and the
  system will be re-started once the probe embarks on the last leg of its
  journey back to Earth.
 
  The delicate space ballet took place almost 200 million miles from
  controllers on Earth, who left responsibility for the rendezvous to an
  on-board navigation system that is designed to operate without ground
  intervention.
 
  The goal of the mission is to study asteroid 1998 SF36 - later named
  Itokawa in honor of an early Japanese pioneer in rocketry. The object
  was discovered in September 1998 by a joint team consisting of
  scientists from the U.S. Air Force, NASA, and the Massachusetts
  Institute of Technology.
 
  Details about Itokawa have largely remained elusive in the seven years
  since its discovery, but scientists now have a much clearer picture of
  the potato-shaped asteroid estimated to measure 2,000 feet by around 900
  feet. Its orbit stretches from inside Earth's out to a distance of 157
  million miles from the Sun, making it a member of the Apollo class of
  near-Earth asteroids that pose potential impact threats to our planet.
 
  Astronomers studied Itokawa via several ground-based telescopes during
  its last Earth fly-by in 2001, and they found evidence that the asteroid
  was brighter and more reflective than first expected. Scientists had a
  difficult time predicting what Hayabusa would find as it closed in on
  the object, and many questions were left unanswered.
 
  However, many of those issues can now be thoroughly remedied with the
  new higher resolution images Hayabusa's optical asteroid multi-band
  imaging camera has captured. The pictures show a contrast of rocky and
  hilly terrain with smooth regions, but detailed analysis and sample
  retrieval will be conducted before scientists can announce the results
  of their detailed study.
 
  A first look at the new images appears to show a loose layer of dust and
  dirt-like material covering the smooth surfaces of parts of the
  asteroid, which is a surprise to some project officials.
 
  According to a certain theory, small objects do not have regolith,
  said Hayabusa project manager Jun Kawaguchi. But this asteroid seems to
  have smooth portions that appear (to have) some regolith.
 
  Work with Hayabusa's science payload has already begun, with the
  near-infrared and X-ray spectrometers now gathering measurements. The
  craft's laser altimeter is also

Re: [meteorite-list] Fireball video

2005-08-04 Thread K. Ohtsuka
Hello list,

This image is of the possible meteorite-dropping fireball (more brighter
than full moon)
event observed on March 19, 2005, at 16:27:51 UT (not daytime but
nighttime),
in Japan. The image also shows terminal large-scale fragmentations.

However, I don't know the reason why the image is listed in wackyvids.com.

More detailed observational data are summarized in

http://sonotaco.jp/forum/viewtopic.php?t=369postdays=0postorder=ascstart=0

sorry, written in Japanese language.

K. Ohtsuka
TOKYO, JAPAN

- Original Message - 
From: Arizona Keith [EMAIL PROTECTED]
To: meteorite-list@meteoritecentral.com
Sent: Thursday, August 04, 2005 1:50 PM
Subject: [meteorite-list] Fireball video


 Hello List

 Check out this fireball video.

 Looks likes a daylight fireball.

 Anyone knows anything about it, there or when?

 http://www.wackyvids.com/movies/general/283/meteor.html

 or

 Wacky Vids web site
 http://www.wackyvids.com/

 pick Meteor


 Keith V.
 Chandler, AZ.


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Re: [meteorite-list] Fireball video

2005-08-04 Thread K. Ohtsuka
P.S.   This image was taken by SONOTACO at Tokyo using WATEC 100N CCD + CBC
6 mm f0.8.

The orbital determination was carried out by S. Nakano as follows:

http://www.oaa.gr.jp/~oaacs/yc/yc2475.htm

K. Ohtsuka

- Original Message - 
From: K. Ohtsuka [EMAIL PROTECTED]
To: Arizona Keith [EMAIL PROTECTED];
meteorite-list@meteoritecentral.com
Sent: Thursday, August 04, 2005 5:49 PM
Subject: Re: [meteorite-list] Fireball video


 Hello list,

 This image is of the possible meteorite-dropping fireball (more brighter
 than full moon)
 event observed on March 19, 2005, at 16:27:51 UT (not daytime but
 nighttime),
 in Japan. The image also shows terminal large-scale fragmentations.

 However, I don't know the reason why the image is listed in wackyvids.com.

 More detailed observational data are summarized in


http://sonotaco.jp/forum/viewtopic.php?t=369postdays=0postorder=ascstart=0

 sorry, written in Japanese language.

 K. Ohtsuka
 TOKYO, JAPAN

 - Original Message - 
 From: Arizona Keith [EMAIL PROTECTED]
 To: meteorite-list@meteoritecentral.com
 Sent: Thursday, August 04, 2005 1:50 PM
 Subject: [meteorite-list] Fireball video


  Hello List
 
  Check out this fireball video.
 
  Looks likes a daylight fireball.
 
  Anyone knows anything about it, there or when?
 
  http://www.wackyvids.com/movies/general/283/meteor.html
 
  or
 
  Wacky Vids web site
  http://www.wackyvids.com/
 
  pick Meteor
 
 
  Keith V.
  Chandler, AZ.
 
 
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Re: [meteorite-list] Japan Shoots For a Piece of an Asteroid(Hayabusa)

2005-06-08 Thread K. Ohtsuka
Hello Darren and list,

See details about the HAYABUSA mission to S-type Asteroid (25143) Itokawa:

http://www.hayabusa.isas.jaxa.jp/e/index.html

The Japanese spacecraft HAYABUSA will encounter Itokawa Oct.- Nov. this
year,
then will probe into and will retrieve the sample around only 1 gram in
total.

By the way, the reflectance spectral data of Itokawa corresponds to LL
chondrite (LL5 or 6),
so if this sample return mission succeeds in and the analyses of the Itokawa
sample prove Itokawa to be LL, then the market price to LL chondrites may
respond and
rise sharply.

Lets obtain LL chondrites now 

K. Ohtsuka

- Original Message - 
From: Darren Garrison [EMAIL PROTECTED]
To: Ron Baalke [EMAIL PROTECTED]
Cc: Meteorite Mailing List meteorite-list@meteoritecentral.com
Sent: Wednesday, June 08, 2005 6:12 AM
Subject: Re: [meteorite-list] Japan Shoots For a Piece of an
Asteroid(Hayabusa)


On Tue, 7 Jun 2005 13:45:53 -0700 (PDT), Ron Baalke
[EMAIL PROTECTED] wrote:

The Hayabusa probe is slowly closing in on a distant asteroid named
Itokawa. Within a few months, after surveying the asteroid thoroughly

Hadn't heard about this mission.  Anyone know what class of asteroid this is
supposed to be?
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Re: [meteorite-list] I am home from Tokyo

2005-06-07 Thread K. Ohtsuka
Hello Michael

I am living in near Tokyo, so I have often been to the Tokyo Mineral Fair
(TMF).
Indeed, it is rumored that it seems very closed show for non-regular dealers
like you.
Additionally saying is that Japanese people are in depression and in
deflation cycle under
silly economic policy, so the meteorite dealers cannot gained so much money
there now
I guess. I know other rumors concerning TMF, and I don't like TMF.

You had better participate the Tokyo Mineral Show (TMS) in December rather
than
this Tokyo Mineral Fair. Do you remember that I purchased a nice Allende
specimen
including DI from you in TMS last year? This is one of my favorite
specimens. Thanks.

K. Ohtsuka


- Original Message - 
From: Michael Farmer [EMAIL PROTECTED]
To: meteorite-list@meteoritecentral.com
Sent: Tuesday, June 07, 2005 3:29 PM
Subject: [meteorite-list] I am home from Tokyo


 Hi everyone,
 I am home a little early from Tokyo, and am preparing now for the
Ensishiem
 and St Marie aux Mines shows in France. Anyone who wants anything, let me
 know now so that I can prepare it, ship it, or bring it to France. I will
be
 traveling on from there back to Asia, and will not be bringing much at all
 to Europe. So please make your requests now.

 On to other business:

 Just a quick note about the Tokyo show, and just to squash any rumors
before
 they start, something occurred there that needs to be addressed now, not
 when people start spreading rumors.

 Hans Koser and I went to Tokyo, and managed to acquire a table at the
 show, directly from the show owner, when another dealers material was
stuck
 in customs.
 That table unfortunately was next to Marvin and Kitty Kilgore. We agreed
 from the start not to put meteorite specimens on the table (as this would
 compete too much with Marvin). Hans and I both had mineral specimens, and
 meteorite jewelry, spheres, and eggs made of meteorites.
 Within an hour of setting up the table (the show had already started)
there
 was a meeting with Marvin Kilgore and Bud Eisler. The complained to the
show
 owner several times, then Kitty Kilgore came in and saw us there and she
got
 the show owner, then they forced us to be kicked out of the show. There
was
 of course, an argument and although nothing serious, there was no
happiness
 between Hans, myself nor Marvin. He tried to explain that it was not
 personal, only business.
 Of course, any of you can imagine how much it costs to go to Tokyo,
shipping
 material, then being thrown out of the show barely two hours after it
 opened. This was not a nice thing to do, and we had only jewelry and
 manufactured items on our table, Kilgore had none of that, only large
 specimens for sale. Eisler did have lots of meteorite jewelry, but he was
 nowhere near us.
 This is a pretty bad situation, and no need to make it worse with
 rumors. It was several dealers being jealous and not wanting competition
at
 a show, and that was that. Since I have never attended that show, the show
 owner bowed to the complaints of Bruno and Carine, Marvin, and Eisler and
 kicked us out. Bruno complained to me the moment he saw me in Tokyo.
 Any of you who know Hans Koser knows that he is the nicest guy in the
 world, who works on very little money, and who this hurt extremely badly.
He
 did not deserve that sort of treatment, nor did I as I hardly know Bud
 Eisler (even though he lives in Tucson) and have always considered Marvin
a
 close friend. Needless to say, that is over with this action.

 There are two sides to every story, and Marvin tried to tell me that he
was
 kicked out of there before and it was then only fair that I got kicked out
 ( I don't buy that argument at all), and that there were too many
meteorite
 dealers there (again, so what) and those things made it ok to kick two
 friends to the curb and force them to lose $4000 to $6000 each in
expenses!
 There were many witnesses to what happened, and if you don't believe me,
ask
 Hans.

 I am a firm believer in what goes around, comes around.

 Mike Farmer


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Re: [meteorite-list] Final announcement of The 29th Symposium

2005-05-29 Thread K. Ohtsuka
Hello David-san,

 I appreciate your link to the Antarctic Meteorite Research #16 (NIPR)
 papers that you provided to the List some time ago, I was previously
 unaware of this online resource. I have also found the 2004 papers from
 this link by changing the numbers. Am I correct in presuming that the
 29th Symposium will result in the ARM #18, available later online?

Maybe, but, it will be published in AMR no.19.
AMR #18 has already been published.
AMR is the publication for the papers submitted to the Symposium on
Anterctic Meteorites held at NIPR every year,  as annual publication.

 I presently read papers published in MAPS and GCA and the abstracts from
 the MetSoc and LPSC conferences. I compile much of the relevant
 information onto my website meteoritestudies.com, perhaps you've
 visited this site before? Can you tell me how I may possibly purchase a
 copy of the International Symposium - Evolution of Solar System
 Materials, from September 2003, or access the published papers somehow?
 These 83 papers are listed in the AMR #17 but are not accessible, and
 I'd love to be able to read them. Please let me know if this is possible.

All the proceeding (PDF) papers of this Symposium, like LPSC-style, were
opened
in the NIPR web until last year, but, regrettably, now closed.
AMR #17 is not the same publication as this proceedings.
So, you should ask about the Proceedings to Dr. A. Yamaguchi
whose address appears in the end of the Final announcement of the Symposium.

By the way you can get the papers of AMRs from #4 to #16 through ADS.

 http://ads.nao.ac.jp//bib_abs.html#top

where you should fill AMR in Journal Name/code field along with
Volume number  4 - 16, that you want to browse, in Volume
field.

You can also accsess AMR #10 - #18 in NIPR website.

http://yamato.nipr.ac.jp/AMRC/EN/index1.html

Sincerely,

K. Ohtsuka

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[meteorite-list] Final announcement of The 29th Symposium on Antarctic Meteorites

2005-05-28 Thread K. Ohtsuka
Hello list members,
Does anyone participate this symposium (held in June 7-9, 2005) at NIPR,
Japan?

http://yamato.nipr.ac.jp/AMRC/researcher/symposium2.html

K. Ohtsuka, TMN

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Re: [meteorite-list] NWA 3118 CV3 Chondrule-Field Update

2005-02-23 Thread K. Ohtsuka
Hello List members,

See also Mineralogy of dark inclusions in CV by Brearly  Jones in
Planetary Materials, Reviews in Mineralogy vol. 36, p3-225, which is a
well-written review for CV DI, I guess.

K. Ohtsuka, Tokyo

- Original Message - 
From: [EMAIL PROTECTED]
To: Meteorite-list@meteoritecentral.com
Sent: Thursday, February 24, 2005 1:26 AM
Subject: [meteorite-list] NWA 3118 CV3 Chondrule-Field Update


  What does all this mean?

 Hello Walter, Bill, and List,

 I'll try to go through this in little steps:

  examination of the inclusion ...shows it to consist of small chondrules
  and chondrule fragments composed of very magnesian olivine (Fa1.1)

 The chondrules in the lower right part of the 32-gram slice are much
smaller
 than chondrules in the remaining CV3 matrix like chondrules in CO3
chondrites
 that are much smaller.

 See also O.R. Norton's Encyclopedia, pp. 135-136 and p. 136, Fig. 7.19:

 While the average chondrule-diameter of a CV is about 1 mm, the average
for
 a CO chondrite is about 0.15 mm.

  small chondrules ... composed of very magnesian olivine (Fa1.1)

 O.R. Norton, 135: most [chondrules in CO chondrites] are porphyritic
 olivine chondrules with olivine made of nearly pure forsterite.

 O.R. Norton, p. 312, Appendix C, Minerals in Meteorites:

 Forsterite = the magnesium end member of the olivine ... (Mg2SiO4)

 The chemical formula shows it is *magnesian* olivine and Fa1.1 shows there
 is hardly any trace of iron. The opposite end member is fayalite
(Fe2SiO4),
 the iron end member (here it is iron that is missing).

  with marginal Fe-rich reaction zones (Fa36.9)

 Imagine a small rim around the chondrules. These outer zones reacted with
 FeO-rich (iron-rich) olivine in the surronding matrix and thereby became
 enriched in Fe (not just Fa1.1 [iron-poor] but Fa36.9 [iron-rich]).

  against a porous matrix composed of felted blades of relatively
  ferroan olivine (Fa40.9-45.9) with accessory troilite and pentlandite.

 Here is what I already said the matrix is rich in olivine that contains
 a lot of iron and not as much magnesium as those magnesian chondrules.

  This clast has the attributes of Type A/B dark inclusions ...

 Dark inclusions are lithic fragments up to about 5 cm in size. They have
 been found in several CV3 chondrites, for example in Allende, Vigarano,
 Leoville, etc.). Their main mineral component is fayalitic olivine. Some
 are chondrule-rich, some are chondrule-free (consist almost entirely of
 matrix)*.

 *Reference:

 WEISBERG M.K. et al. (1998) Fayalitic olivine in CV3 chondrite matrix
 and dark inclusions: A nebular origin (MAPS 33-5, 1998, 1087-1099).

  This clast has the attributes of *Type A/B* dark inclusions ...

 HUTCHISON R. (2004) Meteorites: A Petrologic, Chemical, and
 Isotopic Synthesis (Cambridge Planetary Science Series, p. 62):

 Porphyritic chondrules may be type I and FeO-poor
   or type II and FeO-rich

 They may additionally be subdivided into two categories:

 - silica-poor A
 - silica-rich B

 AB is intermediate.

  Oxygen isotope analysis ... gave replicate (= duplicate) values of:

 d17O = +0.08, -0.18;
 d18O = 5.14, 4.99;
 D17O = -2.63, -2.81 per mil,  respectively, which plot on
the best fit line for whole rock CV chondrites.

 See O.R. Norton, p. 135 or McSWEEN H.Y. (1999) Meteorites and
 Their Parent Planets, p.51: The oxygen isotopic compositions
 provide one means of classifying chondrites into clans and groups.

 When you look at these plots in Norton or McSween, you'll see that
 these values are in the range for CV chondrites but very close to
 the area for CM chondrites (which are much more primitive than
 CVs and point toward aqueous activity and aqueous alteration on
 their parent bodies.

 So this clast may represent a more hydrated relict part of a CV parent
 body the other parts of which are more dehydrated due to parent body
 metamorphism.

 A piece from a boundary area between more and less dehydrated
 material?

 A pocket (or clast) of more primitive material embedded into the
 higher metamorphosed CV3 material?

  a specimen that clearly demonstrates what the above report describes:

  http://cgi.ebay.com/ws/eBayISAPI.dll?ViewItemitem=6513101418


 Best wishes,

 Bernd

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[meteorite-list] Antarctic Meteorite Research No.16

2005-02-16 Thread K. Ohtsuka
Hello List,

Now, you can download free papers of Antarctic Meteorite Research No.16,
featured the Yamato nakhlites: 

http://yamato.nipr.ac.jp/AMRC/amr16/amr16.html

Sincerely,

Katsuhito OHTSUKA
Tokyo, JAPAN
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