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Nearly Carbon‐Saturated Magma Oceans in Planetary Embryos During Core Formation
Author(s) -
Kuwahara Hideharu,
Itoh Shoichi,
Suzumura Akimasa,
Nakada Ryoichi,
Irifune Tetsuo
Publication year - 2021
Publication title -
geophysical research letters
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.007
H-Index - 273
eISSN - 1944-8007
pISSN - 0094-8276
DOI - 10.1029/2021gl092389
Subject(s) - astrobiology , enstatite , silicate , geology , terrestrial planet , carbon fibers , chondrite , mantle (geology) , saturation (graph theory) , hadean , geochemistry , earth science , materials science , meteorite , chemistry , planet , astrophysics , physics , mathematics , organic chemistry , composite material , combinatorics , composite number
Abstract A planetary mantle after core formation has been thought to be highly depleted in carbon due to its strong siderophile behavior. However, the carbon contents in lunar and terrestrial mantles are much greater than experimental predictions; thus, how the carbon contents in terrestrial mantles were established is puzzling and poorly understood. Here, we present high‐pressure experiments on the metal‐silicate partitioning of carbon at 2 GPa and 1923 K in a system containing 0.2 wt% C, which is close to that in enstatite chondrites, and show that a magma ocean made of chondritic materials is nearly saturated with carbon even under metal saturation. The consistency between the solubility of carbon in silicate melts and the carbon contents in lunar and terrestrial mantles also supports a nearly carbon‐saturated magma ocean during core formation and suggests that carbon contents in terrestrial mantles may have been established during the main accretion phase.