Late delivery of exotic chromium to the crust of Mars by water-rich carbonaceous asteroids

Research output: Contribution to journalJournal articleResearchpeer-review

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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 journalJournal articleResearchpeer-review

Harvard

Zhu, K, Schiller, M, Pan, L, Saji, NS, Larsen, KK, Amsellem, E, Rundhaug, C, Sossi, P, Leya, I, Moynier, F & Bizzarro, M 2022, 'Late delivery of exotic chromium to the crust of Mars by water-rich carbonaceous asteroids', Science Advances, vol. 8, no. 46, eabp8415. https://doi.org/10.1126/sciadv.abp8415

APA

Zhu, K., Schiller, M., Pan, L., Saji, N. S., Larsen, K. K., Amsellem, E., Rundhaug, C., Sossi, P., Leya, I., Moynier, F., & Bizzarro, M. (2022). Late delivery of exotic chromium to the crust of Mars by water-rich carbonaceous asteroids. Science Advances, 8(46), [eabp8415]. https://doi.org/10.1126/sciadv.abp8415

Vancouver

Zhu K, Schiller M, Pan L, Saji NS, Larsen KK, Amsellem E et al. Late delivery of exotic chromium to the crust of Mars by water-rich carbonaceous asteroids. Science Advances. 2022;8(46). eabp8415. https://doi.org/10.1126/sciadv.abp8415

Author

Zhu, Ke ; Schiller, Martin ; Pan, Lu ; Saji, Nikitha Susan ; Larsen, Kirsten K. ; Amsellem, Elsa ; Rundhaug, Courtney ; Sossi, Paolo ; Leya, Ingo ; Moynier, Frederic ; Bizzarro, Martin. / Late delivery of exotic chromium to the crust of Mars by water-rich carbonaceous asteroids. In: Science Advances. 2022 ; Vol. 8, No. 46.

Bibtex

@article{b39a97a8cada421f8f26cf599052cfa6,
title = "Late delivery of exotic chromium to the crust of Mars by water-rich carbonaceous asteroids",
abstract = "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.",
author = "Ke Zhu and Martin Schiller and Lu Pan and Saji, {Nikitha Susan} and Larsen, {Kirsten K.} and Elsa Amsellem and Courtney Rundhaug and Paolo Sossi and Ingo Leya and Frederic Moynier and Martin Bizzarro",
year = "2022",
doi = "10.1126/sciadv.abp8415",
language = "English",
volume = "8",
journal = "Science advances",
issn = "2375-2548",
publisher = "American Association for the Advancement of Science",
number = "46",

}

RIS

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