Interplanetary Dust, Meteoroids, Meteors and Meteorites

Detlef Koschny; Rachel Soja; Cecile Engrand; George Flynn; Jérémie Lasue; Anny Chantal Levasseur-Regourd; David Malaspina; Tomoki Nakamura; Andrew R. Poppe; Veerle J. Sterken; Josep M. Trigo-Rodríguez

doi:10.1007/s11214-019-0597-7

Journal articles

Interplanetary Dust, Meteoroids, Meteors and Meteorites

Detlef Koschny ^{1, 2} Rachel Soja ³ Cecile Engrand ⁴ George Flynn ⁵ Jérémie Lasue ⁶ Anny Chantal Levasseur-Regourd ⁷ David Malaspina ⁸ Tomoki Nakamura ⁹ Andrew R. Poppe ¹⁰ Veerle J. Sterken ^{11, 12} Josep M. Trigo-Rodríguez ¹³

1 ESA - Agence Spatiale Européenne

2 Lehrstuhl für Raumfahrttechnik [Garching]

3 IRS - Institut für Raumfahrtsysteme

4 CSNSM - Centre de Sciences Nucléaires et de Sciences de la Matière

5 SUNY Plattsburgh - State University of New York at Plattsburgh

6 IRAP - Institut de recherche en astrophysique et planétologie

7 PLANETO - LATMOS

LATMOS - Laboratoire Atmosphères, Milieux, Observations Spatiales

8 LASP - Laboratory for Atmospheric and Space Physics [Boulder]

9 Tohoku University [Sendai]

10 SSL - Space Sciences Laboratory [Berkeley]

11 IAP - Institute of Applied Physics [Bern]

12 Astronomical Institute [Bern]

13 IEEC-CSIC - Institute for Space Studies of Catalonia [Barcelona]

Abstract : Interplanetary dust particles and meteoroids mostly originate from comets and asteroids. Understanding their distribution in the Solar system, their dynamical behavior and their properties, sheds light on the current state and the dynamical behavior of the Solar system. Dust particles can endanger Earth-orbiting satellites and deep-space probes, and a good understanding of the spatial density and velocity distribution of dust and meteoroids in the Solar system is important for designing proper spacecraft shielding. The study of interplanetary dust and meteoroids provides clues to the formation of the Solar system. Particles having formed 4.5 billion years ago can survive planetary accretion and those that survived until now did not evolve significantly since then. Meteoroids and interplanetary dust can be observed by measuring the intensity and polarization of the zodiacal light, by observing meteors entering the Earth’s atmosphere, by collecting them in the upper atmosphere, polar ices and snow, and by detecting them with in-situ detectors on space probes.

Keywords : Interplanetary dust Meteors Meteorites Zodiacal light

Document type :

Journal articles

Domain :

Sciences of the Universe [physics] / Astrophysics [astro-ph]

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https://hal-insu.archives-ouvertes.fr/insu-02151293
Contributor : Catherine Cardon <>
Submitted on : Friday, June 7, 2019 - 8:35:52 PM
Last modification on : Friday, July 2, 2021 - 3:14:23 AM

Interplanetary Dust, Meteoroids, Meteors and Meteorites

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