2014 | 2013 | 2012 | 2011 | 2010 | 2009 | 2008 | 2007 | 2006 | 2005 | 2004 | 2003 | 2002 | 2001 | 2000 | 1999 | 1998 | 1997 | 1996 | 1995 | 1994 | 1993 | 1992 | 1991 | 1990 | 1989 | 1988 | 1987 | 1986 | 1985 | 1984 | 1983 | 1982 | 1981 | 1980 | 1979 | 1978 | 1977 | 1976 | 1975 | 1974 | 1973 | 1972 | 1971 | 1970 | 1969 | 1968 | 1967 | 1966 | 1965 | 1964 | 1963 | 1962 | 1961 | 500 | 76 | 0
Observations of Varuna at millimeter and optical wavelength
Authors: Moreno, R.; Lellouch, E.; Ortiz, J. L.; Paubert, G.; Doressoundiram, A.; Peixinho, N.
Ref.: American Astronomical Society, DPS Meeting #34, #17.01; Bulletin of the American Astronomical Society 34 (2002)
Abstract: We report observations of trans-Neptunian object (20000) Varuna at millimeter(mm) and optical wavelengths, obtained in January-February 2002 from the IRAM 30m and IAA 1.5m telescopes. The bolometric measurement from IRAM indicates a flux at 1.2 mm of 1.12+/-0.41 mJy, averaged over the object's rotation. The optical measurements show a lightcurve with a period of 3.176+/-0.010 hr, a mean V magnitude of 20.37+/-0.08 and a 0.42+/-0.01 magnitude amplitude. These data tentatively indicate that the lightcure is asymmetric and double-peaked. The joint analysis of these two datasets, has permitted to infer a mean 1060+180-220 km diameter, and a mean 0.038+0.022-0.010 V geometric albedo, fully consistent with the canonical 4% value assumed in size distribution studies.