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The Varuna stellar occultation
of 19 February 2010
On 19 February 2010 around 23:00 -- 23:10 UT (night of Friday February 19th to Saturday February 20th, 2010),
the Trans-Neptunian-Object Varuna may occult the star UCAC2 410140042, or UCAC3: 3UC 233-085933
with Vmag~ 11.1
Such an event, if observed at various sites, could allow us to:
- pin down Varuna's radius to km-accuracy, while its diameter is presently poorly constrained between ~ 500 and 1000 km.
- provide its shape, if non-spherical
- detect a possible faint atmosphere around that body.
Independent predictions are posted on:
the MIT page.
Update as of
06 February 2010
by the Rio group,
using star position derived from observations made at Pico dos Dias:
α= 07h 29mn 22.4714 sec +/- 26 mas
δ= +26d 07' 23.173" +/- 31 mas (J2000/UCAC2)
and the following offset for Varuna wrt JPL#18 ephemeris:
Δα cos(δ)= -2 +/- 66 mas
Δδ = -74 +/- 26 mas.
click to enhance:
Click on images for enhancement
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Shadow moves from right to left. Dots are spaced by 1 mn, with larger dot marking geocentric C/A
(23:07:24 UT).
Dotted lines are typical errors on global path, roughly +/-1700 km, or about +/-40 mas.
Dark gray: astronomical night.
Light gray: astronomical twilight.
Charts
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Charts prepared by Felipe Braga Ribas (Rio de Janeiro). Left 30x30 arcmin, right 5x5 arcmin.
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