HST photometry of Trans-Neptunian Objects

D. C. Stephens, K. S. Noll, W. M. Grundy, R. L. Millis, J. R. Spencer, M. W. Buie, S. C. Tegler, W. Romanishin, D. P. Cruikshank

Research output: Contribution to journalArticle

11 Scopus citations

Abstract

From July 2001 to June 2002, an HST snapshot program obtained V, R and I photometry for 72 TNOs. The TNOs were sorted by dynamical class, and Spearman rank correlation statistics were calculated for each combination of color and orbital parameter. No strong correlations were found for the combined sample of TNOs, the resonant TNOs, or the non-resonant TNOs (classical). The results presented here suggest that if correlations reported by other authors are real, they are evident only at shorter wavelengths than observed in our survey.

Original languageEnglish (US)
Pages (from-to)251-260
Number of pages10
JournalEarth, Moon and Planets
Volume92
Issue number1-4
DOIs
StatePublished - Jun 1 2003

ASJC Scopus subject areas

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

Fingerprint Dive into the research topics of 'HST photometry of Trans-Neptunian Objects'. Together they form a unique fingerprint.

  • Cite this

    Stephens, D. C., Noll, K. S., Grundy, W. M., Millis, R. L., Spencer, J. R., Buie, M. W., Tegler, S. C., Romanishin, W., & Cruikshank, D. P. (2003). HST photometry of Trans-Neptunian Objects. Earth, Moon and Planets, 92(1-4), 251-260. https://doi.org/10.1023/B:MOON.0000031939.79962.f1