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Interplanetary dust (1979)

Millman, Peter M.

Springer

Naturwissenschaften 66 (1979), S. 134-139

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ISSN: 1432-1904

Source: Springer Online Journal Archives 1860-2000

Topics: Biology , Chemistry and Pharmacology , Natural Sciences in General

Notes: Abstract The interplanetary dust cloud, total mass 1010–1020 g in round figures, originates as fragments of comets and produces a mean flux at the earth-moon system in the range 10−13–10−12 g m−2 s−1. Over 2/3 of the mass consists of particles with individual weights 10−3 to 10−6 g. They are fragile, are continually broken up into smaller pieces by collisions, and have a chemical composition similar to that assumed as the average for the entire solar system. The cloud extends to roughly 3 a.u. from the sun in the ecliptic plane, with a particle space density falling off as r −v , where r is distance from the sun and v is in the range 1 to 1.5.

Type of Medium: Electronic Resource

URL: http://dx.doi.org/10.1007/BF00368706

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