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- W4232013704 abstract "A model of the interplanetary dust medium that includes two subsystems, a spherical component and a flat one, has been proposed by the author as a result of analysis of radar meteor orbits. The disintegration of short-period comets is the main source of the flat dust cloud, while the disintegration of long-period comets is the main source of the spherical cloud. Assuming that dust particles fall into the Sun due to the Poynting-Robertson effect, one can estimate the intensity of ejection of dust from long-period comets necessary for the maintenance of the observed density of interplanetary dust. It has been found that the long-period comets should eject between 7 × 10 14 and 2 × 10 15 g of meteoric dust per year." @default.
- W4232013704 created "2022-05-12" @default.
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- W4232013704 date "1972-01-01" @default.
- W4232013704 modified "2023-10-16" @default.
- W4232013704 title "On the Rate of Ejection of Dust by Long-Period Comets" @default.
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- W4232013704 doi "https://doi.org/10.1017/s0074180900006902" @default.
- W4232013704 hasPublicationYear "1972" @default.
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