Interstellar Dust in the Solar System

被引：72
作者：
Mann, Ingrid [1 ,2 ]
机构：
[1] Belgian Inst Space Aeron, B-1180 Brussels, Belgium
[2] Kindai Univ, Sch Sci & Engn, Osaka 5778502, Japan
来源：
ANNUAL REVIEW OF ASTRONOMY AND ASTROPHYSICS, VOL 48 | 2010年 / 48卷
关键词：
heliosphere; interplanetary medium; interstellar medium; MAJOR-ELEMENT COMPOSITION; INTERPLANETARY DUST; GRAIN DESTRUCTION; MASS-DISTRIBUTION; SIZE DISTRIBUTION; HELIOSPHERE; PENETRATION; DENSITY; CLOUD; WIND;
D O I：
10.1146/annurev-astro-081309-130846
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
A fraction of the dust in the interstellar medium (ISM) enters the heliosphere and is measured in situ from spacecraft. This review surveys the in situ measurements and discusses a hence derived model of dust in the local interstellar cloud (LTC). The LIC dust model bears similarities to pristine cometary dust and is characteristic of the warm ISM clouds that fill a part of the ISM in the vicinity of the Sun. Recent and future dust in situ measurements provide a basis for closely studying physical processes in the ISM surrounding the Solar System. The LIE dust is the only dust component measurable in the Solar System that was not previously incorporated in larger Solar System objects. Issues for future LIC dust studies are measuring dust fluxes at the outer heliosphere, measuring the mass distribution with meteor observations and observations from spacecraft, and measuring the LIC dust composition in situ in space.
引用
收藏
页码：173 / 203
页数：31
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