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Stellar Occultation by Transneptunian Object (208996) 2003 AZ84

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Electronic Telegram No. 2675 Central Bureau for Astronomical Telegrams

INTERNATIONAL ASTRONOMICAL UNION

CBAT Director: Daniel W. E. Green; Hoffman Lab 209; Harvard University; 20 Oxford St.; Cambridge, MA 02138; U.S.A.

e-mail: [email protected] (alternate [email protected]) URL http://www.cbat.eps.harvard.edu/index.html

Prepared using the Tamkin Foundation Computer Network

STELLAR OCCULTATION BY TRANSNEPTUNIAN OBJECT (208996) 2003 AZ84

F. Braga-Ribas, B. Sicardy, F. Colas, and J. Lecacheux, Observatoire de Paris; A. Maury, San Pedro de Atacama Celestial Explorations Observatory (SPACE); J. L. Ortiz, N. Morales, and I. de la Cueva, Instituto de Astrofisica de Andalucia (IAA), Granada; E. Jehin, J. Manfroid, and M. Gillon, Institut d'Astrophysique de l'Universite de Liege; M. Assafin, Observatorio do Valongo, UFRJ, Rio de Janeiro; and R. Vieira-Martins and J. I. B. Camargo, Observatorio Nacional, Rio de Janeiro, report on the positive detection of an occultation of a faint star (magnitude R about 18) by the transneptunian object (208996) 2003 AZ84 on Jan. 8d06h29m59s UT (mid-time), from the SPACE Observatory. The occultation was recorded by A. Maury with the C. Harlinten 0.5-m Planewave telescope there, and also by J. L. Ortiz with the remotely operated 0.4-m ASH2 telescope of the IAA in Spain. E. Jehin and J. Manfroid report that no drop of the flux was observed with the 0.6-m robotic TRAPPIST telescope of Liege University, which is located 610 km from San Pedro. Using a

diffracting model, F. Braga-Ribas determined the times of immersion and emersion of the star. The occultation lasted for 21.7 +/- 0.8 seconds, corresponding to a chord length of 573 +/- 21 km. This result gives a lower limit to the diameter of the TNO, and can be compared to the estimated diameter from Stansberry et al. (2008, *Physical Properties of Kuiper Belt and Centaur Objects*, University of Arizona Press, pp. 161ff; 685.8 +/- 95.5 km, based on Spitzer data) and Mueller et al. (2010, A.Ap. 518, L146; 910 +/- 60 km, based on Herschel data).

NOTE: These 'Central Bureau Electronic Telegrams' are sometimes superseded by text appearing later in the printed IAU Circulars. (C) Copyright 2011 CBAT

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