The chlorine isotope fingerprint of the lunar magma ocean.
about
An asteroidal origin for water in the MoonLate-stage magmatic outgassing from a volatile-depleted MoonGallium isotopic evidence for extensive volatile loss from the Moon during its formation.The lunar core can be a major reservoir for volatile elements S, Se, Te and Sb.Depletion of potassium and sodium in mantles of Mars, Moon and Vesta by core formation.Volatile loss following cooling and accretion of the Moon revealed by chromium isotopes
P2860
The chlorine isotope fingerprint of the lunar magma ocean.
description
2015 nî lūn-bûn
@nan
2015年の論文
@ja
2015年論文
@yue
2015年論文
@zh-hant
2015年論文
@zh-hk
2015年論文
@zh-mo
2015年論文
@zh-tw
2015年论文
@wuu
2015年论文
@zh
2015年论文
@zh-cn
name
The chlorine isotope fingerprint of the lunar magma ocean.
@ast
The chlorine isotope fingerprint of the lunar magma ocean.
@en
type
label
The chlorine isotope fingerprint of the lunar magma ocean.
@ast
The chlorine isotope fingerprint of the lunar magma ocean.
@en
prefLabel
The chlorine isotope fingerprint of the lunar magma ocean.
@ast
The chlorine isotope fingerprint of the lunar magma ocean.
@en
P2093
P2860
P50
P356
P1433
P1476
The chlorine isotope fingerprint of the lunar magma ocean.
@en
P2093
James P Greenwood
Jeremy W Boyce
Juliane Gross
Yunbin Guan
P2860
P304
P356
10.1126/SCIADV.1500380
P577
2015-09-25T00:00:00Z