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.
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页数：103
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