Late delivery of exotic chromium to the crust of Mars by water-rich carbonaceous asteroids
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Late delivery of exotic chromium to the crust of Mars by water-rich carbonaceous asteroids. / Zhu, Ke; Schiller, Martin; Pan, Lu; Saji, Nikitha Susan; Larsen, Kirsten K.; Amsellem, Elsa; Rundhaug, Courtney; Sossi, Paolo; Leya, Ingo; Moynier, Frederic; Bizzarro, Martin.
In: Science Advances, Vol. 8, No. 46, eabp8415, 2022.Research output: Contribution to journal › Journal article › Research › peer-review
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TY - JOUR
T1 - Late delivery of exotic chromium to the crust of Mars by water-rich carbonaceous asteroids
AU - Zhu, Ke
AU - Schiller, Martin
AU - Pan, Lu
AU - Saji, Nikitha Susan
AU - Larsen, Kirsten K.
AU - Amsellem, Elsa
AU - Rundhaug, Courtney
AU - Sossi, Paolo
AU - Leya, Ingo
AU - Moynier, Frederic
AU - Bizzarro, Martin
PY - 2022
Y1 - 2022
N2 - The terrestrial planets endured a phase of bombardment following their accretion, but the nature of this late accreted material is debated, preventing a full understanding of the origin of inner solar system volatiles. We report the discovery of nucleosynthetic chromium isotope variability (μ54Cr) in Martian meteorites that represent mantle-derived magmas intruded in the Martian crust. The μ54Cr variability, ranging from −33.1 ± 5.4 to +6.8 ± 1.5 parts per million, correlates with magma chemistry such that samples having assimilated crustal material define a positive μ54Cr endmember. This compositional endmember represents the primordial crust modified by impacting outer solar system bodies of carbonaceous composition. Late delivery of this volatile-rich material to Mars provided an exotic water inventory corresponding to a global water layer >300 meters deep, in addition to the primordial water reservoir from mantle outgassing. This carbonaceous material may also have delivered a source of biologically relevant molecules to early Mars.
AB - The terrestrial planets endured a phase of bombardment following their accretion, but the nature of this late accreted material is debated, preventing a full understanding of the origin of inner solar system volatiles. We report the discovery of nucleosynthetic chromium isotope variability (μ54Cr) in Martian meteorites that represent mantle-derived magmas intruded in the Martian crust. The μ54Cr variability, ranging from −33.1 ± 5.4 to +6.8 ± 1.5 parts per million, correlates with magma chemistry such that samples having assimilated crustal material define a positive μ54Cr endmember. This compositional endmember represents the primordial crust modified by impacting outer solar system bodies of carbonaceous composition. Late delivery of this volatile-rich material to Mars provided an exotic water inventory corresponding to a global water layer >300 meters deep, in addition to the primordial water reservoir from mantle outgassing. This carbonaceous material may also have delivered a source of biologically relevant molecules to early Mars.
U2 - 10.1126/sciadv.abp8415
DO - 10.1126/sciadv.abp8415
M3 - Journal article
C2 - 36383650
VL - 8
JO - Science advances
JF - Science advances
SN - 2375-2548
IS - 46
M1 - eabp8415
ER -
ID: 326331893