2 edition of Crystallization history of lunar feldspathic basalt 14310. found in the catalog.
Crystallization history of lunar feldspathic basalt 14310.
Odette B. James
"Prepared on behalf of the National Aeronautics and Space Administration".
|Series||Geological Survey professional paper -- 841|
Dynamic crystallization experiments were initiated on a synthetic composition to study the crystallization behavior of a feldspathic member of the lunar basalt suite and to determine what factors in the cooling history might produce ophitic basaltic textures versus the poikilitic breccia matrix. to a pristine mare basalt () (Fig. 1c). Furthermore, although basaltic sample was originally classiﬁed as a pristine high-Al mare basalt (e.g., Longhi et al., ; Ridley et al., ; Crawford and Hollister, ), subsequent experimental studies of dynamic crystallization demonstrated its impact origin (e.g., Usselman and.
basin-scale impacts into a highly feldspathic crust. Basin-sized impacts would likely form a melt with a unique cooling rate and crystallization history relative to smaller-scale impacts. Impact melting of a highly feldspathic target material may also lead to an initial . We have continued our efforts in understanding the crystalliza- tion history of feldspathic basalt , A KmEP basalt, in the hopes that we might arrive at an interpretation of its origin and hence the origin of other lunar samples with the composition.
Gmnite. Compositional term used for lunar rocks or glasses rich in Si and,^. Common composition is approximately Si02 70, A 14, FeO 2, MgO 1, CaO 2, Na20 1, K2 0 7 (weight per cent). The term rhyolite has been used in the same compositional sense. High-alumina basalt. Lunar rocks with % modal (or normative). NWA Lunar Feldspathic Breccia NWA is a jaw-dropping spectacular meteorite! It displays dozens of mm anorthosite and basalt clasts easily seen with the naked eye, and hundreds of mm clasts easily seen with a simple magnifying glass. and the large crystal size indicates an extended cooling period in a thick lava flow.
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Get this from a library. Crystallization history of lunar feldspathic basalt [Odette B James; Geological Survey (U.S.),; United States.
National Aeronautics and Space Administration.] -- Additional title page description: An account of the crystallization history of an unusual type of lunar basalt, deduced from detailed petrographic studies and microprobe mineral analyses. Get this from a library.
Crystallization history of lunar feldspathic basalt [Odette B James; Geological Survey (U.S.),; United States. National Aeronautics and Space Administration,].
CRYSTALLIZATION HISTORY OF LUNAR FELDSP ATHIC BASALT ' By ODETTE B. JAMES ABSTRACT Lunar feldspathic basalt crystallized at or near the lunar surface from a melt of virtually the same bulk composition as the rock now by: Odette B. James, author of Crystallization History of Lunar Feldspathic Basalton LibraryThing Odette B.
James, author of Crystallization History of Lunar Feldspathic Basalton LibraryThing LibraryThing is a cataloging and social networking site. MIL is a feldspathic, basalt bearing, regolith breccia lunar meteorite likely paired to Yamato We discuss the petrography and crystallization history of several very low-Ti basalt.
O.B. James, Crystallization history of lunar feldspathic basaltU.S.G.S. Prof. Paper () in press.  G.M. Brown and A.
Peckett, Selective volatilization on the lunar surface: evidence from Apollo 14 feldspar phyric basalts, Nature () . Crystallization history of lunar feldspathic basalt 14310. book history of lunar feldspathic basalt USGS Professional Paper (This sample was collected by Apollo 14) Geology of the Apollo 14 landing site in the Fra Mauro highlands USGS Professional Paper (This is a large report with maps and lots of panoramas of the site.
Lunar feldspathic basalt crystallized at or near the lunar surface from a melt of virtually the same bulk composition as the rock now has. This melt contained no silicate xenoliths or. We report an age of crystallization for spinel-troctolite (VHA basalt) of ± × 10 9 yr (I = ± 6) and an age of crystallization for KREEP-rich basalt of [ ± × 10 9 yr (I = ± 5).
The ages probably date the cooling of shock melts. Zoned lunar pyroxenes have been examined by high voltage (– kV) transmission electron microscopy and electron diffraction, with the particular aim of providing information on the cooling history of individual pyroxenes.
Microstructures resulting from composition discontinuities occurring during continuous crystallization, exsolution lamellae of pigeonite and augite and the development. Date: Jun From: Archaeology in New Zealand, By: Moore, P.
R., (Phillip R.), INNZNA Description: Notes basalt rock was essentially the only rock type used for adzes in eastern Polynesia. Reveals the Tahanga basalt at Opito although widely used for adze manufacturing it was not the only fine grained volcanic rock exploited in the north eastern North Island.
Breccias Dhofar (18°54'52" N, 54°20'42" E) Oman Found January Lunar (feldspathic fragmental breccia) History: M. Farmer recovered a specimen in the Dhofar region of Oman.
Physical characteristics: The g meteorite has an odd external shape akin to a thick-bladed talon. Petrography: (T. Bunch and J. Wittke, NAU) The sample is a feldspathic fragmental breccia that.
Sample was found as a separate sample without adhering matrix and thus, may or may not have been a clast within the Fra Mauro Formation. It was apparently not photographed on the lunar surface, but it was apparently half buried and the soil line separating the cratered and uncratered surfaces can be easily distinguished.
This is USGS Professional Paper ,Crystallization History of Lunar Feldspathic Basalt Published inthis is one of only a few rare publications the USGS did on behalf of NASA on Lunar geology.
USGS APOLLO FORMATION of APOLLO 14 SAMPLE Vintage Report | eBay Skip to main contentSeller Rating: % positive. The early history and broad-scale petrogenesis of the Moon were glimpsed from the first manned and unmanned missions to the Moon that returned ~ kg of lunar rocks and soils from the lunar surface (Vaniman et al.
).These were collected by the Apollo and Luna missions from the central and eastern nearside of the Moon (Fig. 1).Based on numerous studies of these returned. Zhuqing Xue, Long Xiao, Clive R. Neal, Yigang Xu, Oldest high-Ti basalt and magnesian crustal materials in feldspathic lunar meteorite DhofarGeochimica et Cosmochimica Acta, /, ().
(2) Evidence for liquid immiscibility on the Moon has been documented in MIs in minerals and mesostasis in Apollo mare basalts (e.g., high‐Ti basaltlow‐Ti ilmenite basaltand olivine basalt ; Roedder et al.,; Roedder, ) as well. 2 kg of rocks >1 cm in size (Lunar Sourcebook, Table ).
Lunar Sourcebook () G. Heiken, D. Vaniman, and B. French, eds., Cambridge University Press Thanks to Erich H. Haiderer, Norbert Classen, and Tony Irving for providing samples, images, and opinions that help sort out possible pairing relationships among the many Dhofar.
Fukang meteorite — rectilinear section of the most beautiful extraterrestrial substance known, Pallasite-PAL, Fukang, Xinjiang Uyghur Autonomous Region. 64 x 64 x 42 mm ( x x in).Estimate: $25, Offered in The Moon and Beyond: Meteorites. Crystallization History of Lunar Feldspathic Basalt by Odette B.
James: Daring American Heroes of Flight: 9 Brave Fliers (Great Scientists and Famous Inventors) by Jennifer Reed: Luna: Dark Side of the Moon: The Magnificent Madness of the American Lunar Quest by Gerard DeGroot: The Decision to Go to the Moon by John M.
Logsdon. Lunar breccias preserve the records of geologic processes on the Moon. In this study, we report the occurrence, petrography, mineralogy, and geologic significance of the observed secondary olivine veinlets in lunar feldspathic breccia meteorite Northwest Africa (NWA) Three major groups of Lunar basalt based on titanium concentrations (1, pg ).
They can be further divided based on other chemical parameters. High-Ti (>9% by weight TiO2) (Apollo 11 and 17) (Apollo 16 had a few fragments but they were probably the. Sm–Nd isochron diagram for NWAyielding the youngest lunar crystallization age of ± Gyr and the most negative ɛ Nd value of ±