| Studies of meteorites
provide some of our most direct and detailed information on processes that
occurred in the earliest moments of solar system history.
Most meteorite research
projects at PSU are based on the chemical, mineralogic, and petrologic
analyses of meteorites, utilizing such equipment as petrographic microscopes,
scanning transmission electron microscopy, transmission electron microscopy,
electron microprobe, secondary-ionization-mass-spectrometry (SIMS), and
laser-ablation inductively-coupled-plasma-mass-
spectrometry (LA-ICPMS).
Some recent publications:
Hutson M., A. Ruzicka,
R. Pugh, L. Sloan and E. Thompson (2007). Complex brecciation and
shock effects in the Buck Mountain Wash (H3-5) chondrite. Meteorit.
Planet. Sci. 42, 963-978.
Ruzicka, A., H. Hiyagon,
M. Hutson and C. Floss (2007). Relict olivine, chondrule recycling, and
the evolution of nebular oxygen reservoirs. Earth Planetary Sci. Lett.
257, 274-289.
Schepker T.J. and A. Ruzicka
(2007) XRD as a tool to constrain olivine composition: Applications to
H- and L-chondrites. Meteorit. Planet. Sci. 42, Abstract #5316.
Hutson M. L. and A. Ruzicka
(2007) The case against Mercury as the angrite parent body. Meteorit.
Planet. Sci. 42, Abstract #5238.
Hutson, M., R. Hugo, A.
Ruzicka, and M. Killgore (2007) Annealing after shock: Evidence from olivine
microstructures in Portales Valley. Meteorit. Planet. Sci. 42, Abstract
#5072.
Ruzicka A. and M. Hutson
(2006) Differentiation and evolution of the IVA meteorite parent body:
Clues from pyroxene geochemistry in the Steinbach stony-iron.
Meteorit. Planet. Sci. 41, 1959-1987.
Ruzicka A., M. Hutson
and C. Floss (2006) Petrology of silicate inclusions in the Sombrerete
ungrouped iron meteorite: Implications for the origins of IIE-type silicate-bearing
irons . Meteorit Planet. Sci. 41, 1797-1831.
Ruzicka A. and M. Hutson
(2006) NWA 2999 and other angrites: No compelling evidence for a mercurian
origin. Meteorit. Planet. Sci., 41, Abstract #5080.
Ruzicka, A., C. Floss
and M. Hutson (2006) Trace-element compositions of normal, dusty, and clear
olivine in Chainpur chondrules. Meteorit. Planet. Sci., 41, Abstract #5266.
Hutson, M.L., R.N. Pugh
and A.M. Ruzicka (2006) Public outreach and education with meteorites involving
a museum exhibit, website, and teacher workshops. Lunar Planet. Sci. XXXVII,
Abstract #1095, Lunar and Planetary Institute.
Ruzicka A., M. Killgore,
D.W. Mittlefehldt, and M.D. Fries (2005) Portales Valley: Petrology of
a metallic-melt meteorite breccia. Meteorit. Planet. Sci. 40, 261-296.
(see also link:
http://www.psrd.hawaii.edu/Sept05/PortalesValley.html)
Fries, M., Steele A. and
A. Ruzicka (2005) Carbon and mineral phase distribution on a CV3 dark inclusion
boundary – A confocal raman imaging study. Meteorit. Planet. Sci., 40,
A52, Abstract #5236.
Ruzicka, A. and C. Floss
(2004) Forsterite and olivine in Sahara 97210 (LL3.2) and Chainpur (LL3.4)
chondrules: Compositional evolution and the influence of melting. Lunar
Planet. Sci. XXXV, Abstract #1422, Lunar and Planetary Institute (CD ROM).
Greeney, S. and A. Ruzicka
(2004) Relict forsterite in chondrules: Implications for cooling rates.
Lunar Planet. Sci. XXXV, Abstract #1426, Lunar and Planetary Institute
(CD ROM).
Lindsay, T., A. Ruzicka,
and M. Killgore (2003) Origin of silicate inclusions in the Miles (IIE)
iron: Minimal partial melting, maximal fractional crystallization. Meteorit.
Planet. Sci., 38, A102.
Ruzicka, A. and C. Floss
(2003) Relict forsterite and igneous olivine grains in Chainpur (LL3.5)
chondrules: Major and trace element evidence for vapor fractionation
and igneous partitioning. Lunar Planet Sci. XXXIV, Abstract #1243, Lunar
and Planetary Institute (CD ROM).
Hutson M. and A. Ruzicka
(2000) A multi-step model for the origin of E3 (enstatite) chondrites.
Meteorit. Planet. Sci. 35, 601-608.
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Close-up of a relict olivine
grain (grain with dark core) within a chondrule from the NWA 3127 chondrite.
SEM backscatterd electron image.
Silicate (dark) and metal
alloy (light) in the Udei Station silicate-bearing iron meteorite. The
scalebar increments at the bottom are 1 mm wide. Reflected light image
of acid-etched specimen.
Close-up of barred olivine
chondrule showing olivine bars (light) and silicate glass (dark) in the
newly-classified Buck Mountains Wash chondrite from Arizona. SEM backscatterd
electron image.
Close-up of unusual intergrowths
within FeNi-metal alloy in a newly-classified chondrite from Northwest
Africa, showing Ni-rich (bright) and Ni-poor (dark) regions. SEM
backscatterd electron image.
Dislocations (dark lines)
in an olivine crystal in the Portales Valley meteorite. HR-TEM image.
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