4.7 Article

H and Cl isotope characteristics of indigenous and late hydrothermal fluids on the differentiated asteroidal parent body of Grave Nunataks 06128

Journal

GEOCHIMICA ET COSMOCHIMICA ACTA
Volume 266, Issue -, Pages 529-543

Publisher

PERGAMON-ELSEVIER SCIENCE LTD
DOI: 10.1016/j.gca.2019.01.024

Keywords

Apatite; Merrillite; Asteroids; H isotopes; Cl isotopes; Secondary ion mass spectrometry

Funding

  1. UK Science and Technology Facilities Council (STFC) [ST/I001298/1, ST/P005225/1]
  2. UK Cosmochemical Analysis Network (UKCAN) [ST/I001964/1]
  3. UK Research Partnership Investment Funding (UKRPIF) Manchester RPIF Round 2
  4. EPSRC [EP/S019367/1, EP/P025021/1] Funding Source: UKRI
  5. STFC [ST/I001298/1, ST/I001964/1, ST/P000657/1, ST/P005225/1] Funding Source: UKRI

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The paired achondrites Graves Nunataks (GRA) 06128 and 06129 are samples of an asteroid that underwent partial melting within a few million years after the start of Solar System formation. In order to better constrain the origin and processing of volatiles in the early Solar System, we have investigated the abundance of H, F and Cl and the isotopic composition of H and Cl in phosphates in GRA 06128 using secondary ion mass spectrometry. Indigenous H in GRA 06128, as recorded in magmatic merrillite, is characterised by an average delta D of ca. -152 +/- 330%, which is broadly similar to estimates of the H isotope composition of indigenous H in other differentiated asteroidal and planetary bodies such as Mars, the Moon and the angrite and eucrite meteorite parent bodies. The merrillite data thus suggest that early accretion of locally-derived volatiles was widespread for the bodies currently populating the asteroid belt. Apatite formed at the expense of merrillite around 100 million years after the differentiation of the GRA 06128/9 parent body, during hydrothermal alteration, which was probably triggered by an impact event. Apatite in GRA 06128 contains 5.4-5.7 wt.% Cl, 0.6-0.8 wt.% F, and similar to 20 to 60 ppm H2O, which is similar to the H2O abundance in merrillite from which apatite formed. The apatite delta D values range between around +100 parts per thousand and +2000 parts per thousand and are inversely correlated with apatite H2O contents. The Cl isotope composition of apatite appears to be homogeneous across various grains, with an average delta Cl-37 value of 3.2 +/- 0.7 parts per thousand. A possible scenario to account for the apatite chemical and isotopic characteristics involves interaction of GRA 06128/9 with fumarole-like fluids derived from D- and HCl-rich ices delivered to the GRA 06128/9 parent-body by an ice-rich impactor. (C) 2019 The Author(s). Published by Elsevier Ltd.

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