Solar System Science with LSST

被引：42
|
作者：
Jones, R. L. [1 ]
Chesley, S. R. [2 ]
Connolly, A. J. [1 ]
Harris, A. W. [3 ]
Ivezic, Z. [1 ]
Knezevic, Z. [4 ]
Kubica, J. [5 ]
Milani, A. [6 ]
Trilling, D. E. [7 ]
机构：
[1] Univ Washington, Washington, DC USA
[2] JPL Caltech, Pasadena, CA USA
[3] SSI, Princeton, NJ USA
[4] AO Belgrade, Belgrade, Serbia
[5] Google, Mountain View, CA USA
[6] Univ Pisa, Pisa, Italy
[7] No Arizona Univ, Flagstaff, AZ 86011 USA
来源：
EARTH MOON AND PLANETS | 2009年 / 105卷 / 2-4期
关键词：
SKY SURVEY;
D O I：
10.1007/s11038-009-9305-z
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The Large Synoptic Survey Telescope (LSST) will provide a unique tool to study moving objects throughout the solar system, creating massive catalogs of Near Earth Objects (NEOs), asteroids, Trojans, TransNeptunian Objects (TNOs), comets and planetary satellites with well-measured orbits and high quality, multi-color photometry accurate to 0.005 magnitudes for the brightest objects. In the baseline LSST observing plan, back-to-back 15-second images will reach a limiting magnitude as faint as r = 24.7 in each 9.6 square degree image, twice per night; a total of approximately 20,000 square degrees of the sky will be imaged in multiple filters, with revisits about every 3 nights over several months of each year.
引用
收藏
页码：101 / 105
页数：5
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