Bhawad LL6 chondrite: Chemistry, petrology, noble gases, nuclear tracks, and cosmogenic radionuclides

被引:14
|
作者
Bhandari, N
Murty, SVS [1 ]
Shukla, PN
Mahajan, RR
Shukla, AD
Suthar, KM
Parthasarathy, G
Paliwal, BS
机构
[1] Phys Res Lab, Ahmadabad 380009, Gujarat, India
[2] Natl Geophys Res Inst, Hyderabad 500007, Andhra Pradesh, India
[3] Jai Narain Vyas Univ, Jodhpur 342005, Rajasthan, India
关键词
D O I
10.1111/j.1945-5100.2005.tb00170.x
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
Chemical and mineral analysis of the Bhawad chondrite, which fell in Rajasthan in 2002, suggest that this stone belongs to LL6 group of chondrites. Based on helium, neon, and argon isotopes, it has a cosmic ray exposure age of 16.3 Ma. The track density in the olivines shows a narrow range of 1.7-6.8 x 10(6)/cm(2). The Na-22/(26) Al ratio of 1.13 is about 25% lower than the solar cycle average value of about 1.5, but is consistent with irradiation of the meteoroid to modulated galactic cosmic ray fluxes as expected for a fall around the solar maximum. The cosmogenic records indicate a pre-atmospheric radius of about 7.5 cm. Based on U/Th-(4) He and K-Ar-40, the gas retention ages are low (about 1.1 Ga), indicating a major thermal event or shock event that lead to the complete loss of radiogenic He-4 and Ar-40 and the partial loss of radiogenic Xe-129 and fission Xe from Pu-244.
引用
收藏
页码:1015 / 1021
页数:7
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