40Ar/39Ar and (U-Th)/He model age signatures of elusive Mercurian and Venusian meteorites

Fred Jourdan, Ela Eroglu

Research output: Contribution to journalArticle

6 Citations (Scopus)

Abstract

No meteorites from Mercury and Venus have been conclusively identified so far. In this study, we develop an original approach based on extensive Monte Carlo simulations and diffusion models to explore the radiogenic argon (40Ar*) and helium (4He*) loss behavior and the range of 40Ar/39Ar and (U-Th)/He age signatures expected for a range of crystals if meteorites from these planets were ever to be found. We show that we can accurately date the crystallization age of a meteorite from both Mercury and Venus using the 40Ar/39Ar technique on clinopyroxene (± orthopyroxene) and that its 40Ar/39Ar age should match the Pb-Pb age. At the surface of Mercury, phases like albite and anorthite will exhibit a complete range of 40Ar* loss ranging from 0% to 100%, whereas merrillite and apatite will show 100% 4He* loss. By measuring the crystal size and diffusion parameters of a series of plagioclase crystals, one can inverse the 40Ar* loss value to estimate the maximum temperature experienced by a rock, and narrow down the possible pre-ejection location of the meteorite at the surface of Mercury. At the surface of Venus, plagioclase and phosphate phases will only record the age of ejection. The (U-Th)/He systematics of merrillite and apatite will be, respectively, moderately and strongly affected by 4He* loss during the transit of the meteorite from its host planet to Earth. Finally, meteorites from Mercury or Venus will each have their own 40Ar/39Ar and (U-Th)/He isotopic age and 38Arc cosmic ray exposure age signatures over a series of different crystal types, allowing to unambiguously recognize a meteorite for any of these two planets using radiogenic and cosmogenic noble gases.

Original languageEnglish
Pages (from-to)884-905
Number of pages22
JournalMeteoritics and Planetary Science
Volume52
Issue number5
DOIs
Publication statusPublished - May 2017
Externally publishedYes

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meteorites
meteorite
signatures
Venus (planet)
Venus
crystal
planets
planet
apatites
plagioclase
ejection
apatite
crystals
anorthite
noble gas
transit
argon
albite
orthopyroxene
cosmic ray

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title = "40Ar/39Ar and (U-Th)/He model age signatures of elusive Mercurian and Venusian meteorites",
abstract = "No meteorites from Mercury and Venus have been conclusively identified so far. In this study, we develop an original approach based on extensive Monte Carlo simulations and diffusion models to explore the radiogenic argon (40Ar*) and helium (4He*) loss behavior and the range of 40Ar/39Ar and (U-Th)/He age signatures expected for a range of crystals if meteorites from these planets were ever to be found. We show that we can accurately date the crystallization age of a meteorite from both Mercury and Venus using the 40Ar/39Ar technique on clinopyroxene (± orthopyroxene) and that its 40Ar/39Ar age should match the Pb-Pb age. At the surface of Mercury, phases like albite and anorthite will exhibit a complete range of 40Ar* loss ranging from 0{\%} to 100{\%}, whereas merrillite and apatite will show 100{\%} 4He* loss. By measuring the crystal size and diffusion parameters of a series of plagioclase crystals, one can inverse the 40Ar* loss value to estimate the maximum temperature experienced by a rock, and narrow down the possible pre-ejection location of the meteorite at the surface of Mercury. At the surface of Venus, plagioclase and phosphate phases will only record the age of ejection. The (U-Th)/He systematics of merrillite and apatite will be, respectively, moderately and strongly affected by 4He* loss during the transit of the meteorite from its host planet to Earth. Finally, meteorites from Mercury or Venus will each have their own 40Ar/39Ar and (U-Th)/He isotopic age and 38Arc cosmic ray exposure age signatures over a series of different crystal types, allowing to unambiguously recognize a meteorite for any of these two planets using radiogenic and cosmogenic noble gases.",
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40Ar/39Ar and (U-Th)/He model age signatures of elusive Mercurian and Venusian meteorites. / Jourdan, Fred; Eroglu, Ela.

In: Meteoritics and Planetary Science, Vol. 52, No. 5, 05.2017, p. 884-905.

Research output: Contribution to journalArticle

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AU - Jourdan, Fred

AU - Eroglu, Ela

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SN - 1086-9379

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