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Area of Science:

  • Astrobiology
  • Geochemistry
  • Origin of Life studies

Background:

  • Asteroids are hypothesized to have delivered prebiotic compounds crucial for life's origin on early Earth.
  • Pristine asteroid samples offer a unique opportunity to assess their chemical potential for supporting life.
  • The interaction between asteroidal chemistry and early metabolic pathways remains largely unquantified.

Purpose of the Study:

  • To computationally evaluate the metabolic viability of primitive life forms on asteroid material.
  • To determine the capacity of different asteroid compositions to support early Earth metabolisms.
  • To identify critical substrates required for life within asteroidal samples.

Main Methods:

  • Metabolic network expansion was used to test biochemical network viability.
  • Computational analysis was performed on the known chemistry of asteroids (Itokawa, Ryugu, Bennu) and meteorites (Murchison, Murray).
  • Focus was placed on acetogenic and methanogenic metabolisms, representing primitive life.

Main Results:

  • The chemistry of Murchison and Bennu samples appears to support acetogenic and methanogenic metabolisms.
  • Murray, Ryugu, and Itokawa samples lack essential substrates like adenine and D-ribose, vital for ATP production.
  • Significant compositional variation exists among carbonaceous bodies regarding their capacity to support primitive metabolisms.

Conclusions:

  • Asteroidal composition significantly influences their potential to support early life.
  • Asteroids rich in carbon, nitrogen, and phosphate, like Bennu, hold astrobiological relevance.
  • The findings suggest potential past or present habitability on some parent asteroid bodies.