Mapping the interstellar dust flow into the solar system

Details Mapping the interstellar dust flow into the solar system Mapping the interstellar dust flow into the solar system

Nov 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001esasp.495..663b&link_type=abstract

In: Proceedings of the Meteoroids 2001 Conference, 6 - 10 August 2001, Kiruna, Sweden. Ed.: Barbara Warmbein. ESA SP-495, Noordw

Physics

3

Interstellar Dust, Meteor Radar

Scientific paper

The Advanced Meteor Orbit Radar facility (AMOR) monitors the dynamcial properties of meteoroids of sizes down to about 40 μm. The oprbital data set secured to date contains about 106 orbits. The population of inner Solar System meteoroids sampled contains a significant proportion of particles that are moving in unbound solar orbits. Maps the far-sun inflow directions of this extra-Solar System population show the presence of both a broad interstellar inflow and discrete sources.

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