The formation of comets by radiation pressure in the outer protosun. II - Dependence on the radiation-grain coupling. III - Dependence on the anisotropy of the radiation field

Astronomy and Astrophysics – Astronomy

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Comets, Evolution (Development), Protostars, Radiation Pressure, Backscattering, Cosmic Dust, Mie Scattering, Radiation Absorption

Scientific paper

Radiation pressure from the protosun and neighboring protostars may have caused the formation of the comets. Grains feel a net radiation pressure toward the center of the protocomet dust cloud due to the absorption and backscattering of radiation by the dust. Mie scattering is used to estimate the dust-radiation coupling. The dust-radiation coupling is sufficiently strong that the comets can form within the free fall time of the outer protosun.

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