In-Situ Monitoring of Interstellar Dust in the Inner Solar System

Altobelli, Nicolas; Kempf, Sascha; Krüger, Harald; Landgraf, Markus; Srama, Ralf; Grün, Eberhard

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In-Situ Monitoring of Interstellar Dust in the Inner Solar System

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Altobelli, Nicolas
Ralf Srama - Heidelberg Dust Group, Research Groups, MPI for Nuclear Physics, Max Planck Society;

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Kempf, Sascha
Ralf Srama - Heidelberg Dust Group, Research Groups, MPI for Nuclear Physics, Max Planck Society;

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Krüger, Harald
Ralf Srama - Heidelberg Dust Group, Research Groups, MPI for Nuclear Physics, Max Planck Society;

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Srama, Ralf
Ralf Srama - Heidelberg Dust Group, Research Groups, MPI for Nuclear Physics, Max Planck Society;

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Grün, Eberhard
Ralf Srama - Heidelberg Dust Group, Research Groups, MPI for Nuclear Physics, Max Planck Society;

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引用

Altobelli, N., Kempf, S., Krüger, H., Landgraf, M., Srama, R., & Grün, E. (2005). In-Situ Monitoring of Interstellar Dust in the Inner Solar System. In C. C., Popescu, & R. J. (., Tuffs (Eds.), The Spectral Energy Distributions of Gas-Rich Galaxies: Confronting Models with Data (pp. 149-152). Melville: American Institute of Physics.

引用: https://hdl.handle.net/11858/00-001M-0000-0011-8A08-9

要旨

We present in this paper new interstellar dust data obtained in the inner solar system by the dust instruments on-board the Cassini, Galileo and Helios spacecraft. While the Ulysses dust instrument provided an in-situ monitoring of the interstellar dust stream at high ecliptic latitude between 3 AU and 5 AU, the new data cover an heliocentric distance range between 0.3 AU and 3 AU in the ecliptic plane. Furthermore, the data provide evidence of the interstellar dust stream alteration in the inner solar system, caused by radiation pressure forces and gravitation focusing.