James Webb Space Telescope Observations of Stellar Occultations by Solar System Bodies and Rings

被引:8
作者
Santos-Sanz, P. [1 ]
French, R. G. [2 ]
Pinilla-Alonso, N. [3 ]
Stansberry, J. [4 ]
Lin, Z-Y. [5 ]
Zhang, Z-W. [6 ]
Vilenius, E. [7 ,8 ]
Mueller, Th. [7 ]
Ortiz, J. L. [1 ]
Braga-Ribas, F. [9 ]
Bosh, A. [10 ]
Duffard, R. [1 ]
Lellouch, E. [11 ]
Tancredi, G. [12 ]
Young, L. [13 ]
Milam, Stefanie N. [14 ]
机构
[1] CSIC, IAA, Glorieta Astron S-N, E-18008 Granada, Spain
[2] Wellesley Coll, Dept Astron, Wellesley, MA 02481 USA
[3] Univ Tennessee, Dept Earth & Planetary Sci, Knoxville, TN 37996 USA
[4] Space Telescope Sci Inst, 3700 San Martin Dr, Baltimore, MD 21218 USA
[5] Natl Cent Univ, Inst Astron, Taoyuan 32001, Taiwan
[6] Acad Sinica, Inst Astron & Astrophys, POB 23-141, Taipei 10617, Taiwan
[7] Max Planck Inst Extraterr Phys, D-85748 Garching, Germany
[8] Max Planck Inst Solar Syst Res, Gottingen, Germany
[9] Fed Univ Technol Parana UTFPR DAFIS, Curitiba, Parana, Brazil
[10] MIT, Dept Earth Atmospher & Planetary Sci, Cambridge, MA USA
[11] Univ Paris 06, CNRS, Observ Paris, Univ Paris Diderot,LESIA, Meudon, France
[12] Fac Ciencias, Dept Astron, Montevideo, Uruguay
[13] SwRI, 1050 Walnut St, Boulder, CO 80302 USA
[14] NASA, Goddard Space Flight Ctr, Greenbelt, MD USA
关键词
Kuiper belt: general; methods: observational; occultations; planets and satellites: rings; techniques: photometric; telescopes; KUIPER-BELT OBJECTS; ICE RICH SURFACE; SIZE DISTRIBUTION; COLLISIONAL EVOLUTION; VISIBLE SPECTROSCOPY; LUMINOSITY FUNCTION; HERSCHEL-PACS; TNOS; COOL; ACCRETION;
D O I
10.1088/1538-3873/128/959/018011
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In this paper, we investigate the opportunities provided by the James Webb Space Telescope (JWST) for significant scientific advances in the study of Solar System bodies and rings using stellar occultations. The strengths and weaknesses of the stellar occultation technique are evaluated in light of JWST's unique capabilities. We identify several possible JWST occultation events by minor bodies and rings and evaluate their potential scientific value. These predictions depend critically on accurate a priori knowledge of the orbit of JWST near the Sun-Earth Lagrange point 2 (L2). We also explore the possibility of serendipitous stellar occultations by very small minor bodies as a byproduct of other JWST observing programs. Finally, to optimize the potential scientific return of stellar occultation observations, we identify several characteristics of JWST's orbit and instrumentation that should be taken into account during JWST's development.
引用
收藏
页码:1 / 16
页数:16
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