Magnetite in CI carbonaceous meteorites: Origin by aqueous activity on a planetesimal surface

John F. Kerridge; Alan L. Mackay; William V. Boynton

doi:10.1126/science.205.4404.395

Magnetite in CI carbonaceous meteorites: Origin by aqueous activity on a planetesimal surface

John F. Kerridge, Alan L. Mackay, William V. Boynton

Lunar and Planetary Lab

Research output: Contribution to journal › Article › peer-review

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Abstract

The composition and morphology of magnetite in CI carbonaceous meteorites appear incompatible with a nebular origin. Mineralization on the meteorite parent body is a more plausible mode of formation. The iodine-xenon age of this material therefore dates an episode of secondary mineralization on a planetesimal rather than the epoch of condensation in the primitive solar nebula.

Original language	English (US)
Pages (from-to)	395-397
Number of pages	3
Journal	Science
Volume	205
Issue number	4404
DOIs	https://doi.org/10.1126/science.205.4404.395
State	Published - 1979

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@article{6237c309ad9c460fa47756a34436bf57,

title = "Magnetite in CI carbonaceous meteorites: Origin by aqueous activity on a planetesimal surface",

abstract = "The composition and morphology of magnetite in CI carbonaceous meteorites appear incompatible with a nebular origin. Mineralization on the meteorite parent body is a more plausible mode of formation. The iodine-xenon age of this material therefore dates an episode of secondary mineralization on a planetesimal rather than the epoch of condensation in the primitive solar nebula.",

author = "Kerridge, \{John F.\} and Mackay, \{Alan L.\} and Boynton, \{William V.\}",

year = "1979",

doi = "10.1126/science.205.4404.395",

language = "English (US)",

volume = "205",

pages = "395--397",

journal = "Science",

issn = "0036-8075",

publisher = "American Association for the Advancement of Science",

number = "4404",

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T1 - Magnetite in CI carbonaceous meteorites

T2 - Origin by aqueous activity on a planetesimal surface

AU - Kerridge, John F.

AU - Mackay, Alan L.

AU - Boynton, William V.

PY - 1979

Y1 - 1979

N2 - The composition and morphology of magnetite in CI carbonaceous meteorites appear incompatible with a nebular origin. Mineralization on the meteorite parent body is a more plausible mode of formation. The iodine-xenon age of this material therefore dates an episode of secondary mineralization on a planetesimal rather than the epoch of condensation in the primitive solar nebula.

AB - The composition and morphology of magnetite in CI carbonaceous meteorites appear incompatible with a nebular origin. Mineralization on the meteorite parent body is a more plausible mode of formation. The iodine-xenon age of this material therefore dates an episode of secondary mineralization on a planetesimal rather than the epoch of condensation in the primitive solar nebula.

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UR - https://www.scopus.com/inward/citedby.url?scp=0000406715&partnerID=8YFLogxK

U2 - 10.1126/science.205.4404.395

DO - 10.1126/science.205.4404.395

M3 - Article

AN - SCOPUS:0000406715

SN - 0036-8075

VL - 205

SP - 395

EP - 397

JO - Science

JF - Science

IS - 4404

ER -

Magnetite in CI carbonaceous meteorites: Origin by aqueous activity on a planetesimal surface

Abstract

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