Distinct Chlorine Isotope Reservoirs on Mars. Origins and Interactions

· by · in

Shearer C. K. * Messenger S. Sharp Z. D. Burger P. V. Nguyen N. McCubbin F. M.

80th Annual Meeting of the Meteoritical Society 2017 [#6364]

abstract (PDF)

“Chlorine isotopes measured in Chassigny provide evidence for two distinct Cl reservoirs on Mars that are linked to crust-atmosphere interactions and the nature of material accreting to form Mars.”

Related posts (automatically generated):

  1. The chlorine isotopic composition of Martian meteorites 1: Chlorine isotope composition of Martian mantle and crustal reservoirs and their interactions.
  2. The chlorine isotope composition of Martian meteorites 2. Implications for the early solar system and the formation of Mars
  3. Earth and Mars – distinct inner solar system products
  4. Chondritic late accretion to Mars and the nature of shergottite reservoirs
  5. Multiple early-formed water reservoirs in the interior of Mars
  6. Tracing martian surface interactions with the triple O isotope compositions of meteoritic phosphates
  7. Iron isotope systematics in planetary reservoirs
  8. Replacement of glass in the Nakhla meteorite by berthierine: Implications for understanding the origins of aluminum-rich phyllosilicates on Mars.OPEN ACCESS 
  9. Iron Isotope Compositions of Achondritic Meteorites from Distinct Parent Bodies
  10. Chlorine isotopic compositions of apatite in Apollo 14 rocks: Evidence for widespread vapor-phase metasomatism on the lunar nearside ∼4 billion years ago
Tags: , , ,