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There is a lot of
information on the web about Lunar Meteorites. A Google.com search on the term
“Lunar Meteorites” yields 390,000 sites on that search engine alone.
As a geologist, I find it
fascinating that impacts on the moon’s surface can produce meteorites on the
Earth. The moon has a small gravitational field and low escape velocity. Any
rocks dislodged by a surface impact on the moon have a chance to escape the
moon’s gravitational field. This has also happened on Mars, and there are Mars
Meteorites.
Some
Definitions:
First here are some
definitions related to lunar meteorites, meteoroids, asteroids and planets. From
the NASA website:
"Shooting stars" or meteors are bits of material falling
through Earth's atmosphere; they are heated to incandescence by the friction of
the air. The bright trails as they are coming through the Earth's atmosphere are
termed meteors, and these chunks as they are hurtling through space are called
meteoroids. Large pieces that do not vaporize completely and reach the surface
of the Earth are termed meteorites.
Asteroids are essentially
chunks of rock ranging in size from dust particles to 1,000 km across.
Planetoids are planet sized asteroids.
For more information about
meteors, meteorites and asteroids I have produced a CD-ROM entitled
Falling from the Sky: A Meteorite Resource.
This CD includes hundreds of pages of information and many interactive web page
links.
Introduction
The following information
was taken from the Washington University in St. Louis, Department of Earth and
Planetary Sciences website:
http://epsc.wustl.edu/admin/resources/moon_meteorites.html
Meteoroids strike the Moon
every day. Lunar escape velocity averages 2.38 km/s (1.48 miles per second),
only a few times the muzzle velocity of a rifle (0.7-1.0 km/s). Any rock on the
lunar surface that is accelerated by the impact of a meteoroid to lunar escape
velocity or greater will leave the Moon’s gravitational influence. Some ejected
material becomes captured by the Earth’s gravitational field and lands on Earth
within a few hundred thousands of years (much shorter for some). Other ejected
material, however, assumes an orbit around the Sun. Some of that material may
eventually strike Earth. This can take a long time. Lunar meteorites
Yamato-82192/82193/86032 and Dhofar 025 remained in space for 10 and 20 million
years before finally landing on Earth.
Lunar meteorites look a lot like some Earth rocks. We know that they came from
space, however, because like asteroidal meteorites, lunar meteorites have
fusion crusts from the melting that
occurs as they enter the Earth’s atmosphere (the olive-green crusts on the
photos above). Also, they contain certain isotopes that can only be produced by
reactions with cosmic rays while outside the Earth’s atmosphere.
Chemical compositions,
isotope ratios, minerals, and textures of the lunar meteorites are all similar
to those of samples collected on the Moon during the Apollo missions. Taken
together, these various characteristics are different from those of any other
type of meteorite or terrestrial rock. For example, all of those meteorites in
the
List that are classified as
feldspathic breccias
are rich in the mineral
anorthite,
which is plagioclase feldspar, mineralogically, and a calcium aluminum silicate,
chemically. Consequently, these meteorites all have high concentrations of
aluminum and calcium. Because of some unique aspects about how the Moon formed,
the lunar highlands are composed predominantly of anorthite. Anorthite is much
less common on asteroids and, to the best of our knowledge, on the surface of
any other planet or planetary satellite.
The largest single stone is
Kalahari 009 at 13.5 kg (30 lbs.). The rest
are much smaller. The next biggest are
Dar al Gani 400 (1425 grams = 3.1 lbs) and
LAP 02205 (1226 grams = 2.7 lbs).
Together, the five stones of the LAP 02xxx "pairing" are the second largest
lunar meteorite (1875 grams = 4.1 lbs.). Several of the lunar meteorite
fragments found in Antarctica and Oman only weigh a few grams (a U.S. nickel
weighs 5 grams).
While impact
cratering on the Moon can be a very destructive process, it also has the
capacity to throw new samples of rock our way. As an impact crater is being
excavated, some rocky material can be thrown out of the crater with enough
velocity to escape the Moon's gravity and fall to Earth. Since impact craters
occur at random locations, lunar meteorites provide a set of samples from all
portions of the Moon, including the farside and polar regions, which Apollo
astronauts and Luna spacecraft were unable to visit.
Thus far
15 lunar meteorites have been discovered
(see table below). Many of these have been
recovered in Antarctica, where they can be preserved in glacial ice for
thousands of years after they fall. Some lunar meteorites, however, have also
been found in other parts of the world. Generally these are hot desert regions
where the meteorites are preserved because there is so little rain to affect
them.
Even though
the lunar meteorites sample different regions of the Moon than the Apollo and
Luna programs, they have some similarities. One common type of lunar meteorite
is an anorthositic breccia. The word "anorthositic" indicates the
rock contains lots of bright white fragments of anorthosite (a
plagioclase-rich rock containing some pyroxene, with or without olivine),
the type of rock found in the lunar highlands. A "breccia" is a rock that
contains the broken fragments of older rocks. These breccias are usually
produced by the impact processes, which crush rock, move it around the surface
of the Moon, and mix it with broken fragments of other types of rock. There are
different types of impact breccias, including fragmental breccias, polymict
breccias, and regolith breccias.
Of the >26,000 meteorites listed in the
Catalogue of Meteorites, only 1
in 1200 are lunar. Meteorites are very rare rocks; lunar meteorites are
exceedingly rare. No lunar meteorites have yet been found in North America,
South America, or Europe.
Lunar Meteorites
Table
A table of
Lunar Meteorites has been compiled by the University of Arizona Space Imagery
Center, from the following website:
http://www.lpl.arizona.edu/sic/moon/lunar_meteorites/table_record_impact.html
|
Impact
# |
Age
of
Impact
(MA) |
Transit
Time
(MA) |
Terrestrial
Age
(MA) |
Meteorite(s) |
Classification |
Terrane
at
the Impact
Site |
|
1 |
9 ± 2 |
9±2 |
~0.08 |
Y82192/3
Y86032 |
Anorthositic fragmental breccia
Anorthositic fragmental breccia |
Highlands
Highlands |
|
2 |
0.9± 0.1
1.1±0.2 |
0.9±0.1
1.1±0.2 |
<0.07
<0.05 |
Asuka-881757
Y793169 |
Mare gabbro
Mare gabbro |
Mare
Mare |
|
3 |
~0.27 |
0.04 |
0.21 to
0.25 |
MAC88104/5 |
Anorthositic breccia (r/f) |
Highlands |
|
4 to 5 |
<0.07
<0.04 |
<0.01
<0.02 |
<0.06
<0.02 |
EET87521
Y793274 |
Basaltic
fragmental breccia
Basaltic regolith breccia |
Mare
Mare |
|
5 to 6 |
0.06±0.03 |
<0.019 |
0.06 ±0.04 |
Y791197 |
Anorthositic regolith breccia |
Highlands |
|
6 to 7 |
0.0115 |
0.025 |
0.009 |
ALHA81005 |
Anorthositic regolith breccia |
Highlands |
|
7 to 8 |
-------- |
<0.2 |
<0.07 |
Calcalong
Creek |
KREEP-rich
microbreccia |
Highlands |
|
7 to 9 |
0.025-0.06 |
0.02-0.05 |
0.005-0.01 |
QUE93069
QUE94269 |
Anorthositic regolith breccia
Anorthositic regolith breccia |
Highlands
Highlands |
|
7 to 10* |
- |
- |
- |
QUE94281 |
Basaltic
fragmental breccia |
Mare |
|
7 to 11* |
- |
- |
- |
Dar al Gani
262 |
Anorthositic polymict breccia |
Highlands |
|
7 to 12* |
- |
- |
- |
EET96008 |
Basaltic
breccia |
Mare |
|
7 to 13* |
- |
- |
- |
Dar al Gani
400 |
Anorthositic polymict breccia |
Highlands |
|
7 to 14* |
- |
- |
- |
Dhofar 025 |
Anorthositic regolith breccia |
Highlands |
|
7 to 15* |
- |
- |
- |
Dhofar 026 |
Anorth.
crystalline melt breccia |
Highlands |
|
7 to 16* |
- |
- |
- |
NWA 032 |
Olivine-pyroxene basalt |
Mare |
|
7 to 17* |
- |
- |
- |
Dhofar 081 |
Feldspathic
fragmental breccia |
Highlands |
Based on
information presented by Eugster et al. (1991), Nishiizumi et al. (1991), Vogt
et al. (1991), Hill et al. (1991), Nishiizumi et al. 1992, Warren (1994), Grier
et al. (1995), Kring et al. (1995), Swindle et al. 1995, Kring et al.
(1996), Nishiizumi et al. (1996), Bischoff and Weber (1997), Grossman (2000),
Grossman and Zipfel (2001).
References
The following
list of references about lunar meteorites has been compiled by Washington
University – St. Louis, Department of Earth and Planetary Sciences. The web site
is:
http://epsc.wustl.edu/admin/resources/meteorites/references.html
Anand M., Misra
K., Taylor L. A., Nazarov M. A., Clayton R. N., and Mayeda T. K. (2002)
Apparently KREEPy lunar meteorite Dhofar 287a: The
residual melt tapped from a fractionating magma chamber (abstract).
In Lunar and Planetary Science XXXIII,
abstract no. 1635, Lunar and Planetary Institute, Houston.
Anand M., Taylor
L. A., Nazarov M. A., and Patchen A. (2003)
Petrologic comparisons of lunar mare basalt meteorites
Dh-287A and NWA 032 (abstract). In Lunar and Planetary Science
IIIIV, abstract #1787, Lunar and Planetary Institute, Houston.
Anand M., Taylor
L. A., Misra K. C., Demidova S. I., and Nazarov M. A. (2003)
KREEPy lunar meteorite Dhofar 287A: A new lunar mare
basalt, Meteorit. Planet. Sci.
38, 485-499.
Anand M., Taylor
L. A., Neal C. R., Snyder G. A., Patchen A., Sano Y., and Terada K. (2003)
Petrogenesis of lunar meteorite EET 96008,
Geochim. Cosmochim. Acta
67, 3499–3518.
Anand M., Taylor
L. A., Neal C., Patchen A. and Kramer G. (2004)
Petrology and geochemistry of LAP 02 205: A new low-Ti
mare-basalt meteorite (abstract). In
Lunar and Planetary Science XXXV, abstract no. 1626, Lunar
and Planetary Institute, Houston.
Anand, M.,
Taylor, L. A., Nazarov, M. A., Shu, J., Mao H.-K., and Hemley, R. J. (2004)
Space weathering on airless planetary bodies: clues
from the lunar mineral hapkeite.
Proceedings of the National Academy of Sciences
101, no. 18, 6847-6851.
Arai T. (2001)
Mineralogical study of lunar meteorite EET 96008 (abstract), In Antarctic
Meteorites XXVI, 3-6, National Institute of Polar Research, Tokyo.
Arai T (2003)
Yamato 983885: Lunar highland breccia with alkali anorthosite (abstract).
Evolution of Solar System Materials: A New
Perspective from Antarctic Meteorites, 7-8, National Institute of
Polar Research, Tokyo.
Arai T. and
Warren P. H. (1999)
Lunar meteorite Queen Alexandra Range 94281: Glass
compositions and other evidence for launch pairing with Yamato 793274,
Meteorit. Planet. Sci. 34, 209-234.
Arai T., Takeda
H., and Warren P. H. (1996)
Four lunar meteorites: Crystallization trends of
pyroxenes and spinels, Meteorit. Planet. Sci. 31, 877-892.
Arai T., Ishi
T., and Otsuki M. (2002)
Mineralogical study of new lunar meteorite Yamato
981031 (abstract). In Lunar and Planetary Science
XXXIII, abstract no. 2064, Lunar and Planetary Institute,
Houston.
Arai T., Ishi
T., and Otsuki M. (2002) A new lunar meteorite Yamato 981031: A possible link
between two lunar meteorite source craters (abstract). In Antarctic
Meteorites XXVII, 4-6, National Institute of Polar Research, Tokyo.
Arai T., Otsuki
M., Ishii T., Mikouchi T., and Miyamoto M. (2004)
Mineralogy of Yamato 983885 lunar polymict breccia
with alkali-rich and Mg-rich rocks (abstract). In
Lunar and Planetary Science XXXV,
abstract no. 2155, Lunar and Planetary Institute, Houston.
Arai T., Misawa
K. and Kojima H. (2005)
A new lunar meteorite MET 01210: Mare breccia with a
low-Ti ferrobasalt (abstract). In Lunar and Planetary Science XXXVI,
abstract no. 2361, Lunar and Planetary Institute, Houston.
Arai T., Shimoda
H., Kita N., Morishita Y., and Kojima H. (2005)
Source magma compositions for basalt clasts of lunar
meteorite EET 87521 in connection to KREEP (abstract). 68th Annual
Meeting of the Meteoritical Society, number #5196.
Arai T., Shimoda
H., Kita N., and Morishita Y. (2005) Petrogenesis of basaltic clasts with
extreme compositional variations in a brecciated lunar meteorite EET 87521
(abstract), Antarctic Meteorites XXIX, 1–2, National Institute of Polar
Research, Tokyo.
Arai T., Otsuki
M., Ishii T., Mikouchi T., and Miyamoto M. (2005) Mineralogy of Yamato 983885
lunar polymict breccia with KREEP basalt, a high-Al basalt, a very low-Ti basalt
and Mg-rich rocks. Antarct. Meteorite Res.
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Barrat J. A.,
Gillet Ph., Jambon A., Sautter V., Javoy M., Petit E., and Lesourd M. (2001)
News from the Moon and Mars: preliminary examinations
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Science XXXII, abstract no.
1713, Lunar and Planetary Institute, Houston.
Bartoschewitz
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Kurtz Th. (2005)
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Bartoschewitz
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(2005)
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Bartoschewitz
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(1996)
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(2001) Fantastic new chondrites, achondrites, and lunar meteorites as the result
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Weber D. (1997)
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Korschinek G., Kubik P. W., Mayeda T. K., Merchel S., Michel R., Neumann S.,
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major lithologies (abstract). Meteorit. Planet. Sci.
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B. A., Taylor L. A., and Nazarov M. A. (2001)
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Dhofar 025 (abstract).In Lunar and Planetary Science
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Houston.
Cahill J. T.,
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Cohen B. A.
(2005)
More impact-melt clasts in feldspathic lunar
meteorites (abstract). 68th Annual Meeting of the Meteoritical
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Cohen B. A.,
Kring D. A., and Swindle T. D. (1999)
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Cohen B. A.,
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Cohen B. A.,
Taylor L. A., and Nazarov M. A. (2001)
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Taylor L. A., and Nazarov M. A. (2001)
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James O. B., Taylor L. A., Nazarov M. A., and Barsukova L. D. (2004) Lunar
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Taylor G. J., Keil K., Bunch T. E., Wittke J. H., Korotev R. L., Jolliff B. L.,
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Fernandes V. A., Burgess R., Turner G., Eugster O., and Lorenzetti S. (2002)
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