Solar system science with LSST

R. L. Jones; S. R. Chesley; A. J. Connolly; A. W. Harris; Z. Ivezic; Z. Knezevic; J. Kubica; A. Milani; D. E. Trilling

doi:10.1007/s11038-009-9305-z

Solar system science with LSST

R. L. Jones, S. R. Chesley, A. J. Connolly, A. W. Harris, Z. Ivezic, Z. Knezevic, J. Kubica, A. Milani, D. E. Trilling

Physics and Astronomy

Research output: Contribution to journal › Article › peer-review

27 Scopus citations

Abstract

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.

Original language	English (US)
Pages (from-to)	101-105
Number of pages	5
Journal	Earth, Moon and Planets
Volume	105
Issue number	2-4
DOIs	https://doi.org/10.1007/s11038-009-9305-z
State	Published - 2009

ASJC Scopus subject areas

Astronomy and Astrophysics
Earth and Planetary Sciences (miscellaneous)
Space and Planetary Science

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10.1007/s11038-009-9305-z

Cite this

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title = "Solar system science with LSST",

abstract = "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.",

author = "Jones, {R. L.} and Chesley, {S. R.} and Connolly, {A. J.} and Harris, {A. W.} and Z. Ivezic and Z. Knezevic and J. Kubica and A. Milani and Trilling, {D. E.}",

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T1 - Solar system science with LSST

AU - Jones, R. L.

AU - Chesley, S. R.

AU - Connolly, A. J.

AU - Harris, A. W.

AU - Ivezic, Z.

AU - Knezevic, Z.

AU - Kubica, J.

AU - Milani, A.

AU - Trilling, D. E.

PY - 2009

Y1 - 2009

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AB - 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.

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Solar system science with LSST

Abstract

ASJC Scopus subject areas

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