Polarimetry of Solar System minor bodies and planets

被引：0

作者：

Bagnulo, Stefano ^{[1
]}

Belskaya, Irina ^{[2
]}

Cellino, Alberto ^{[3
]}

Kwon, Yuna G. ^{[4
]}

Munoz, Olga ^{[5
]}

Stam, Daphne M. ^{[6
]}

机构：

[1] Armagh Observ & Planetarium, Coll Hill, Armagh BT61 9DG, North Ireland

[2] V N Karazin Kharkiv Natl Univ, Inst Astron, 35 Sumska str, UA-61022 Kharkiv, Ukraine

[3] INAF Osservatorio Astrofisico Torino, I-10025 Turin, Italy

[4] CALTECH, Infrared Proc & Anal Ctr IPAC, 1200 Calif Blvd, MC 100-22, Pasadena, CA 91125 USA

[5] CSIC, Inst Astrofis Andalucia, Glorieta Astron S-N, Granada 18008, Spain

[6] Leiden Observ, Einsteinweg 55, NL-2333 CC Leiden, Netherlands

来源：

ASTRONOMY AND ASTROPHYSICS REVIEW | 2024年 / 32卷 / 01期

基金：

新加坡国家研究基金会;

关键词：

Solar System astronomy; Polarimetry; Laboratory astrophysics; PHASE-ANGLE OBSERVATIONS; ASTEROID; 3200; PHAETHON; COMET WEST 1975N; LIGHT-SCATTERING; IMAGING POLARIMETRY; CIRCULAR-POLARIZATION; LINEAR-POLARIZATION; OPTICAL-PROPERTIES; MICROWAVE ANALOG; NEGATIVE POLARIZATION;

D O I：

10.1007/s00159-024-00157-w

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The study of the polarisation of light is a powerful tool for probing the physical and compositional properties of astrophysical sources, including Solar System objects. In this article, we provide a comprehensive overview of the state-of-the-art in polarimetric studies of various celestial bodies within our Solar System: planets, moons, asteroids, and comets. Additionally, we review relevant laboratory measurements and summarise the fundamental principles of polarimetric observational techniques.

引用

页数：103

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