Abstract
We imaged the region around Asteroid (4) Vesta in nine long exposures using the Wide Field Planetary Camera 2 on the Hubble Space Telescope on May 14 and 16, 2007 to conduct a deep search for satellites in support of NASA's Dawn mission that orbited (4) Vesta in 2011-2012. Several previous search efforts have been undertaken, but no satellites were detected. Our search covered distances from 14 to 260 Vesta radii and searched to a limiting magnitude of 22.5 ± 0.4 in HST's wide-band red filter (F702W). Our upper limit for possible satellites corresponds to a satellite just 22 ± 4. m in radius, assuming the same optical properties as Vesta. Our upper limit is ~10 times smaller than the best limit of previous searches. In situ satellite searches by NASA's Dawn spacecraft will probe regions closer to Vesta than our effort reported here.
Original language | English (US) |
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Pages (from-to) | 305-310 |
Number of pages | 6 |
Journal | Icarus |
Volume | 220 |
Issue number | 2 |
DOIs | |
State | Published - Aug 2012 |
All Science Journal Classification (ASJC) codes
- Astronomy and Astrophysics
- Space and Planetary Science