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Giant impact-induced atmospheric blow-off

Thomas J. Ahrens

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Abstract

Abstract. Previous calculations indicate that the Earth suffered impacts from objects up to Mars size. Such a giant impact may have produced a temporary ejecta-based ring that accreted to form the Moon. To simulate the surface waves from such events we approximated the cratering source as a buried pressurized sphere. For a 1027 J impactor we calculated the resulting surface wave using the mode summation method of Sato et al. [1]. For such an impact, the solid Earth free-surface velocity above, and antipodal to, the source achieves 2.6 and 1.9 km/s. Such large ground motions pump the atmosphere and result in upward particle motions which cause the atmosphere to be accelerated to excess of the escape velocity (11.2 km/s) at high altitudes. For a 1.3 x 1032 J Moon-forming impact we calculate that ~50 % of the Earth’s atmosphere is accelerated to escape.

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Abstract. Previous calculations indicate that the Earth suffered impacts from objects up to Mars size. Such a giant impact may have produced a temporary ejecta-based ring that accreted to form the Moon. To simulate the surface waves from such events we approximated the cratering source as a buried pressurized sphere. For a 1027 J impactor we calculated the resulting surface wave using the mode summation method of Sato et al. [1]. For such an impact, the solid Earth free-surface velocity above, and antipodal to, the source achieves 2.6 and 1.9 km/s. Such large ground motions pump the atmosphere and result in upward particle motions which cause the atmosphere to be accelerated to excess of the escape velocity (11.2 km/s) at high altitudes. For a 1.3 x 1032 J Moon-forming impact we calculate that ~50 % of the Earth’s atmosphere is accelerated to escape.

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Available abstract

Abstract. Previous calculations indicate that the Earth suffered impacts from objects up to Mars size. Such a giant impact may have produced a temporary ejecta-based ring that accreted to form the Moon. To simulate the surface waves from such events we approximated the cratering source as a buried pressurized sphere. For a 1027 J impactor we calculated the resulting surface wave using the mode summation method of Sato et al. [1]. For such an impact, the solid Earth free-surface velocity above, and antipodal to, the source achieves 2.6 and 1.9 km/s. Such large ground motions pump the atmosphere and result in upward particle motions which cause the atmosphere to be accelerated to excess of the escape velocity (11.2 km/s) at high altitudes. For a 1.3 x 1032 J Moon-forming impact we calculate that ~50 % of the Earth’s atmosphere is accelerated to escape.

Key concepts: Planetesimal, Astrobiology, Atmosphere (unit), Atmosphere of Mars, Atmosphere of Venus, Planet, Mars Exploration Program, Terrestrial planet

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