loading page

Identifying Biosignatures in a Mars-Analogue Volcanic Rock: the ~3.5 Ga Kitty’s Gap Chert
  • +4
  • Laura Clodoré,
  • Frédéric Foucher,
  • Keyron Hickman-Lewis,
  • Stéphanie Sorieul,
  • Matthieu Réfrégiers,
  • Guillaume Collet,
  • Frances Westall
Laura Clodoré
CNRS

Corresponding Author:[email protected]

Author Profile
Frédéric Foucher
CNRS
Author Profile
Keyron Hickman-Lewis
Natural History Museum
Author Profile
Stéphanie Sorieul
Université de Bordeaux CNRS CENBG
Author Profile
Matthieu Réfrégiers
CNRS
Author Profile
Guillaume Collet
CNRS
Author Profile
Frances Westall
CNRS CBM
Author Profile

Abstract

Documentation of primitive terrestrial life signatures and the methods used to characterize them will be relevant to identify signatures of biological origin at the surface of Mars. In this respect, fossils of chemolithotrophic microorganisms found in ancient volcanic rocks on Earth are used as analogues for the kinds of microorganisms that could be found on Mars. Indeed, chemolithotrophs are the ancient forms of life thought to inhabit the first habitats on Earth and potentially on Mars when the two planets had similar conditions in their early history, i.e. an atmosphere, geological activity and enough liquid water in specific habitable localities for a prolonged period of time.