共查询到20条相似文献，搜索用时 0 毫秒
1.
2.
Schaefer BF 《Science (New York, N.Y.)》2005,308(5726):1267-1268
3.
Kerr RA 《Science (New York, N.Y.)》2008,319(5862):401
4.
5.
6.
Eiler JM 《Science (New York, N.Y.)》2007,317(5841):1046-1047
7.
Weyer S 《Science (New York, N.Y.)》2008,320(5883):1600-1601
8.
9.
Rodrigues AS 《Science (New York, N.Y.)》2006,313(5790):1051-1052
10.
Woods P 《Science (New York, N.Y.)》2001,291(5506):995-997
11.
12.
Balter M 《Science (New York, N.Y.)》2005,309(5732):234-237
13.
Mervis J 《Science (New York, N.Y.)》2004,304(5675):1280
14.
Significant abundances of trapped argon, krypton, and xenon have been measured in shock-altered phases of the achondritic meteorite Elephant Moraine 79001 from Antarctica. The relative elemental abundances, the high ratios of argon-40 to argon-36 (>/= 2000), and the high ratios of xenon-129 to xenon-132 (>/= 2.0) of the trapped gas more closely resemble Viking data for the martian atmosphere than data for noble gas components typically found in meteorites. These findings support earlier suggestions, made on the basis of geochemical evidence, that shergottites and related rare meteorites may have originated from the planet Mars. 相似文献
15.
Normile D 《Science (New York, N.Y.)》2005,310(5747):426-428
16.
17.
18.
Kerr RA 《Science (New York, N.Y.)》2001,291(5510):1875-1876
19.
Grimm D 《Science (New York, N.Y.)》2011,332(6029):526-529
20.