TY - JOUR
T1 - A new source of basaltic meteorites inferred from Northwest Africa 011
AU - Yamaguchi, Akira
AU - Clayton, Robert N.
AU - Mayeda, Toshiko K.
AU - Ebihara, Mitsuru
AU - Oura, Yasuji
AU - Miura, Yayoi N.
AU - Haramura, Hiroshi
AU - Misawa, Keiji
AU - Kojima, Hideyasu
AU - Nagao, Keisuke
PY - 2002/4/12
Y1 - 2002/4/12
N2 - Eucrites are a class of basaltic meteorites that share common mineralogical, isotopic, and chemical properties and are thought to have been derived from the same parent body, possibly asteroid 4 Vesta. The texture, mineralogy, and noble gas data of the recently recovered meteorite, Northwest Africa (NWA) 011, are similar to those of basaltic eucrites. However, the oxygen isotopic composition of NWA011 is different from that of other eucrites, indicating that NWA011 may be derived from a different parent body. The presence of basaltic meteorites with variable oxygen isotopic composition suggests the occurrence of multiple basaltic meteorite parent bodies, perhaps similar to 4 Vesta, in the early solar system.
AB - Eucrites are a class of basaltic meteorites that share common mineralogical, isotopic, and chemical properties and are thought to have been derived from the same parent body, possibly asteroid 4 Vesta. The texture, mineralogy, and noble gas data of the recently recovered meteorite, Northwest Africa (NWA) 011, are similar to those of basaltic eucrites. However, the oxygen isotopic composition of NWA011 is different from that of other eucrites, indicating that NWA011 may be derived from a different parent body. The presence of basaltic meteorites with variable oxygen isotopic composition suggests the occurrence of multiple basaltic meteorite parent bodies, perhaps similar to 4 Vesta, in the early solar system.
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U2 - 10.1126/science.1069408
DO - 10.1126/science.1069408
M3 - Article
C2 - 11951042
AN - SCOPUS:0037066519
SN - 0036-8075
VL - 296
SP - 334
EP - 336
JO - Science
JF - Science
IS - 5566
ER -