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

21 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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