Temporal changes in the solar system meteoroid complex

Details Temporal changes in the solar system meteoroid complex Temporal changes in the solar system meteoroid complex

Apr 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998exdu.work..101b&link_type=abstract

Exozodiacal Dust Workshop, p. 101

Other

Meteoroids, Zodiacal Dust, Planetary Systems, Solar System, Planetary Craters, Lunar Craters, Temporal Distribution

Scientific paper

Temporal changes of the dust population in the inner planet region of the solar system can in principle be detected by the study of ancient impact crater records and by the study of tracers of interplanetary material in sediments. The evidence for change is poor but existing information on the present state of the zodiacal dust complex can be used to predict temporal variations of dust density in the inner regions of other planetary systems. It is likely that the evolution of dust in the inner regions of planetary systems can be approximated by an initial period of long term decline followed by a period of relative constancy with superimposed short term fluctuations.

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