Radar imaging of asteroid 654 Zelinda

C. Magri, M. C. Nolan, S. J. Ostro, J. D. Giorgini

Research output: Contribution to journalArticlepeer-review

1 Scopus citations


Radar observations of main-belt asteroid 654 Zelinda were made at the Arecibo Observatory in February 2002. Echoes were several times stronger than for any previous main-belt radar experiment; delay-Doppler imaging resolution was 1.2 km. one percent of Zelinda's diameter. Zelinda is topographically complex. The most prominent feature is a quasispecular "glint" probably produced by a flat facet 15 km across. This facet may connect in turn to a second feature, perhaps 30 km long and fairly straight. Shape reconstruction is in progress; rotation phase coverage is probably the limiting factor in obtaining a unique model. Any such limitation could be removed at Zelinda's next strong radar apparition in 2009.

Original languageEnglish (US)
Pages (from-to)485-488
Number of pages4
JournalEuropean Space Agency, (Special Publication) ESA SP
Issue number500
StatePublished - Jul 2002
Externally publishedYes

ASJC Scopus subject areas

  • Aerospace Engineering
  • Space and Planetary Science


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