Bibliography: p. 28-30.
|Statement||Brian Mason and S.R. Taylor.|
|Series||Smithsonian contributions to the earth sciences ;, no. 25|
|Contributions||Taylor, Stuart Ross, 1925-|
|LC Classifications||QE1 .S227 no. 25, QB756.A44 .S227 no. 25|
|The Physical Object|
|Pagination||iii, 30 p. :|
|Number of Pages||30|
|LC Control Number||82600091|
Inclusions in the Allende meteorite. 1 online resource (iii, 30 p.) (OCoLC) Print version: Mason, Brian Harold, Inclusions in the Allende meteorite. iii, 30 p. (DLC) (OCoLC) Material Type: Government publication, National government publication: Document Type: Book: All Authors / Contributors. REFRACTORY INCLUSIONS x IN THE ALLENDE METEORITE Lawrence 1 Grossrnan Department of the Geophysical Sciences, The University of Chicago, South Ellis Avenue, Chicago, Illinois INTRODUCTION The fall of the Allende Type 3 carbonaceous chondrite in Chihuahua,File Size: 3MB. Inclusions in the Allende meteorite (Smithsonian contributions to the earth sciences) [Brian Harold Mason] on *FREE* shipping on qualifying : Brian Harold Mason. The Allende meteorite, which is classified as a carbonaceous chondrite, consists of large, irregularly shaped white inclusions and rounded chondrules in a dark matrix. The inclusions are composed of minerals believed to have condensed at high temperatures from a gas having the composition of the Sun, and their time of formation is older than.
Inclusions in the Allende Meteorite Brian Mason and S.R. Taylor Introduction The fall of the Allende meteorite in northern Mexico on 8 February was a unique event in the history of meteoritics. One of us (BM) was in the field immediately after the event, and even a . Stone meteorite: Detail of prepared slice of the carbonaceous chondrite Allende, which was seen to fall in Chihuahua, Mexico on the night of February 8, , following a massive fireball. Allende contains carbonaceous compounds as well as calcium-rich inclusions (large white circle near center). Coarse-grained, calcium-rich inclusions in the Allende meteorite are enclosed by sequences of very thin, mineralogically distinct rim layers. A number of questions arise in connection with the. Alteration qf Al-rich inclusions inside amoeboid olivine aggregates in the Allende meteorite AIUHIKO HASHIMOTO’ and LAWRENCE GROSSMAN’ Department of the Geophysical Sciences, The University of Chicago, South Ellis Avenue, Chicago, IL , U.S.A. (Received November ; accepted in revised,rorm Ma ).
The "Allende strewn field" is the area where the meteorites were found. The long line with the arrow is the direction of the flight of the meteorite. (The curvy line is the highway.) The meteorite is named after the small nearby town of Pueblito de Allende (shown as Allende on the map). A meteorite is a fragment of rock or iron from outer space, usually a meteoroid or asteroid, which survives passage through the atmosphere as a meteor to impact the surface of the ites are believed to originate in the asteroid belt between the planets of Mars and Jupiter. A meteorite may range in size from less than a gram to more than 60 tons. Meteorites are characterized as either meteorite falls or meteorite finds. A meteorite fall is a meteorite that was observed falling from the sky. The Chelyabinsk meteorite, which fell in Russia in , and the Allende meteorite, which fell in Mexico in , are typical meteorite falls. A meteorite find is not the same as a meteorite fall. Refractory Inclusions in the Allende Meteorite. Annual Review of Earth and Planetary Sciences Vol. (Volume publication date May ) Annual Review of Earth and Planetary Sciences Mass Fractionation Laws, Mass-Independent Effects, and Isotopic AnomaliesCited by: