Speckle interferometry observations of main belt asteroids at TNG

Details Speckle interferometry observations of main belt asteroids at TNG Speckle interferometry observations of main belt asteroids at TNG

Nov 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002esasp.500..497c&link_type=abstract

In: Proceedings of Asteroids, Comets, Meteors - ACM 2002. International Conference, 29 July - 2 August 2002, Berlin, Germany. Ed

Physics

Asteroids, Speckle Interferometry

Scientific paper

Speckle interferometry observations of eight main belt asteroids (3 Juno, 12 Victoria, 16 Psyche, 30 Urania, 88 Thisbe, 135 Hertha, 230 Athamantis, and 324 Bamberga) were obtained at the Telescopio Nazionale Galileo in La Palma (Canary Islands, Spain). Average sizes and apparent shapes were measured, and were found to fit reasonably the predictions of indirect techniques for size and shape determination (radiometry and photometry). No new binary objects were discovered.

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