Document details

Low phase angle effects in photometry of trans-neptunian objects: 20000 Varuna ...

Author(s): Belskaya, I.N. cv logo 1 ; Ortiz, J.L. cv logo 2 ; Rousselot, P. cv logo 3 ; Ivanova, V. cv logo 4 ; Borisov, G. cv logo 5 ; Shevchenko, V.G. cv logo 6 ; Peixinho, N. cv logo 7

Date: 2006

Persistent ID: http://hdl.handle.net/10316/4395

Origin: Estudo Geral - Universidade de Coimbra

Subject(s): Trans-neptunian objects; Asteroids; Photometry


Description
We present the results of photometric observations of trans-neptunian object 20000 Varuna, which were obtained during 7 nights in November 2004-February 2005. The analysis of new and available photometric observations of Varuna reveals a pronounced opposition surge at phase angles less than 0.1 deg with amplitude of 0.2 mag relatively to the extrapolation of the linear part of magnitude-phase dependence to zero phase angle. The opposition surge of Varuna is markedly different from that of dark asteroids while quite typical for moderate albedo Solar System bodies. We find an indication of variations of the scattering properties over Varuna's surface that could result in an increase of the lightcurve amplitude toward zero phase angle. It is shown that a similar phase effect can be responsible for lightcurve changes found for TNO 19308 (1996 TO66) in 1997-1999. http://www.sciencedirect.com/science/article/B6WGF-4K4PSTX-2/1/447c751a99c7de80e8073e91841b1879
Document Type Article
Language English
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