Issue |
A&A
Volume 391, Number 3, September I 2002
|
|
---|---|---|
Page(s) | 1133 - 1139 | |
Section | Celestial mechanics and astrometry | |
DOI | https://doi.org/10.1051/0004-6361:20020903 | |
Published online | 09 August 2002 |
Coordinated thermal and optical observations of Trans-Neptunian object (20 000)Varuna from Sierra Nevada
1
Observatoire de Paris, 5 place J. Janssen, 92195 Meudon, France
2
I.R.A.M. 300 Av. de la Piscine, 38406 St-Martin d'Hères Cedex, France
3
Instituto de Astrofísica de Andalucia, CSIC, Camino Bajo de Huetor 24, 18080 Granada, Spain
4
I.R.A.M. Avda. Divina Pastora 7, 18012 Granada, Spain
5
Centro de Astronomia e Astrofísica da Universidade de Lisboa, 1349-018 Lisboa, Portugal
Corresponding author: E. Lellouch, emmanuel.lellouch@obspm.fr
Received:
11
June
2002
Accepted:
14
June
2002
We report on coordinated thermal and optical measurements of
trans-Neptunian object (20 000)Varuna obtained in January–February 2002,
respectively from the IRAM 30-m and IAA 1.5 m telescopes. The optical
data show a lightcurve with a period of hr, a mean V
magnitude of
and a
magnitude
amplitude. They also tentatively indicate that the lightcurve
is asymmetric and double-peaked. The thermal observations
indicate a
mJy flux, averaged over the object's
rotation. Combining the two datasets, we
infer that Varuna has a mean 1060
km diameter and
a mean 0.038
V geometric albedo, in general agreement with
an earlier determination using the same technique.
Key words: kuiper belt / planets and satellites: general / techniques: photometric / submillimeter
© ESO, 2002
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