Volume 415, Number 2, February IV 2004
|Page(s)||771 - 775|
|Section||Planets and planetary systems|
|Published online||11 February 2004|
Size estimates of some optically bright KBOs
Max-Planck-Institut für Radioastronomie (MPIfR), Auf dem Hügel 69, 53121 Bonn, Germany e-mail: firstname.lastname@example.org
Corresponding author: W. J. Altenhoff, email@example.com
Accepted: 10 November 2003
Seven recently detected optically “bright” Kuiper-Belt-Objects (KBOs) were observed at 250 GHz using the Max-Planck Millimeter Bolometer (MAMBO) array at the IRAM 30 m telescope. Only the optical binary KBO (47 171) 1999 TC36 was detected, whose components differ optically by mag. Assuming that the derived mean geometric albedo of is identical for both, the component diameters become 566 and 225 km. For the other six objects upper limits to their sizes and lower limits for their albedos were obtained. The geometric albedo, p, for (28978) Ixion is surprisingly large, ≥0.15. For a consistent comparison all published radio photometric data of KBOs and Centaurs were analyzed again: the average geometric albedo is found to be ≈0.08.
Key words: minor planets / radio continuum: solar system
© ESO, 2004
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