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- W3048504741 abstract "The only type of concentration of cometary dust with a reasonable probability of being detected by deep-space probes, are the dust tails emanating from passing comets. Essentially all the dust released from long-period comets leaves the solar system on hyperbolic orbits, because the radiation pressure limit is high (corresponding to centimetre-sized grains emitted in the vicinity of the Earth’s orbit by comets of the Oort’s Cloud). For the short-period comets the dynamical conditions for retention of emitted particles within the solar system are much more favourable, but those which remain in circumsolar orbits tend to disperse rather rapidly (Kresák, 1976a)." @default.
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- W3048504741 date "1976-01-01" @default.
- W3048504741 modified "2023-10-14" @default.
- W3048504741 title "4.9 On the Structure of Hyperbolic Interplanetary Dust Streams" @default.
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- W3048504741 doi "https://doi.org/10.1017/s0252921100052088" @default.
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