• DOI:10.1088/2041-8205/733/1/L4
• Corpus ID: 50809352

HUBBLE SPACE TELESCOPE OBSERVATIONS OF MAIN-BELT COMET (596) SCHEILA

@article{Jewitt2011HUBBLEST,
  title={HUBBLE SPACE TELESCOPE OBSERVATIONS OF MAIN-BELT COMET (596) SCHEILA},
  author={David C. Jewitt and H. Weaver and Max J. Mutchler and Stephen M. Larson and Jessica Agarwal},
  journal={The Astrophysical Journal Letters},
  year={2011},
  volume={733}
}

• D. Jewitt, H. Weaver, +2 authors J. Agarwal
• Published 28 March 2011
• Physics, Geology
• The Astrophysical Journal Letters

We present Hubble Space Telescope Observations of (596) Scheila during its recent dust outburst. The nucleus remained point-like with absolute magnitude HV = 8.85 ± 0.02 in our data, equal to the pre-outburst value, with no secondary fragments of diameter ⩾100 m (for assumed albedos 0.04). We find a coma having a peak scattering cross section ∼2.2×104 km2, corresponding to a mass in micron-sized particles of ∼4×107 kg. The particles are deflected by solar radiation pressure on projected spatial scales ∼2×104 km, in the sunward direction, and swept from the vicinity of the nucleus on timescales of weeks. The coma fades by ∼30% between observations on UT 2010 December 27 and 2011 January 4. The observed mass loss is inconsistent with an origin either by rotational instability of the nucleus or by electrostatic ejection of regolith charged by sunlight. Dust ejection could be caused by the sudden but unexplained exposure of buried ice. However, the data are most simply explained by the impact, at ∼5 km s−1, of a previously unknown asteroid ∼35 m in diameter.