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 | |
| State | Published - 2009 |
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ASJC Scopus subject areas
- Earth and Planetary Sciences (miscellaneous)
- Astronomy and Astrophysics
- Space and Planetary Science
Cite this
Solar system science with LSST. / Jones, R. L.; Chesley, S. R.; Connolly, A. J.; Harris, A. W.; Ivezic, Z.; Knezevic, Z.; Kubica, J.; Milani, A.; Trilling, David E.
In: Earth, Moon and Planets, Vol. 105, No. 2-4, 2009, p. 101-105.Research output: Contribution to journal › Article
}
TY - JOUR
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, David E
PY - 2009
Y1 - 2009
N2 - 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.
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.
UR - http://www.scopus.com/inward/record.url?scp=69049085531&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=69049085531&partnerID=8YFLogxK
U2 - 10.1007/s11038-009-9305-z
DO - 10.1007/s11038-009-9305-z
M3 - Article
AN - SCOPUS:69049085531
VL - 105
SP - 101
EP - 105
JO - Earth, Moon and Planets
JF - Earth, Moon and Planets
SN - 0167-9295
IS - 2-4
ER -