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

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页码：101 / 105

页数：5

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