Arecibo radar observations of Phobos and Deimos

Michael W. Busch, Steven J. Ostro, Lance A.M. Benner, Jon D. Giorgini, Christopher Magri, Ellen S. Howell, Michael C. Nolan, Alice A. Hine, Donald B. Campbell, Irwin I. Shapiro, John F. Chandler

Research output: Contribution to journalArticlepeer-review

16 Scopus citations

Abstract

In November 2005, we observed the moons of Mars using the Arecibo 2380-MHz (13-cm) radar, obtaining a result for the OC radar albedo of Phobos (0.056 ± 0.014) consistent with its previously reported radar albedo and implying an upper bound on its near-surface bulk density of 1.6 ± 0.3   g cm-3. We detected Deimos by radar for the first time, finding its OC radar albedo to be 0.021 ± 0.006, implying an upper bound on its near-surface density of 1.1 ± 0.3   g cm-3, consistent with a high-porosity regolith. We briefly discuss reasons for these low radar albedos, Deimos' being possibly the lowest of any Solar System body yet observed by radar.

Original languageEnglish (US)
Pages (from-to)581-584
Number of pages4
JournalIcarus
Volume186
Issue number2
DOIs
StatePublished - Feb 2007
Externally publishedYes

Keywords

  • Mars
  • Radar observations
  • Regoliths
  • satellites

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

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