Accretion of Moon and Earth and the emergence of life

• Published in: Chemical geology Vol. 169; no. 1; pp. 69 - 82
• Main Authors: Arrhenius, G, Lepland, A
• Format: Journal Article
• Language: English
• Published: Netherlands Elsevier B.V 15-08-2000
• Subjects: Archean sediments; Chemofossils; Early Earth; Earth (Planet); Earth satellites; Emergence of life; Evolution, Planetary; Exobiology; Geologic Sediments - analysis; Lunar bombardment; Models, Theoretical; Moon; Origin of Life; Solar System; Space life sciences; Chemofossils; Archean sediments; Moon; Early Earth; Emergence of life; Lunar bombardment; Earth satellites; NASA Discipline Exobiology; Non-NASA Center
• ISSN: 0009-2541; 1872-6836
• DOI: 10.1016/S0009-2541(00)00333-8

The discrepancy between the impact records on the Earth and Moon in the time period, 4.0–3.5 Ga calls for a re-evaluation of the cause and localization of the late lunar bombardment. As one possible explanation, we propose that the time coverage in the ancient rock record is sufficiently fragmentary, so that the effects of giant, sterilizing impacts throughout the inner solar system, caused by marauding asteroids, could have escaped detection in terrestrial and Martian records.
Alternatively, the lunar impact record may reflect collisions of the receding Moon with a series of small, original satellites of the Earth and their debris in the time period about 4.0–3.5 Ga. The effects on Earth of such encounters could have been comparatively small. The location of these tellurian moonlets has been estimated to have been in the region around 40 Earth radii. Calculations presented here, indicate that this is the region that the Moon would traverse at 4.0–3.5 Ga, when the heavy and declining lunar bombardment took place.
The ultimate time limit for the emergence of life on Earth is determined by the effects of planetary accretion — existing models offer a variety of scenarios, ranging from low average surface temperature at slow accretion of the mantle, to complete melting of the planet followed by protracted cooling. The choice of accretion model affects the habitability of the planet by dictating the early evolution of the atmosphere and hydrosphere.
Further exploration of the sedimentary record on Earth and Mars, and of the chemical composition of impact-generated ejecta on the Moon, may determine the choice between the different interpretations of the late lunar bombardment and cast additional light on the time and conditions for the emergence of life.