Call for Observation
2002TC302 occults UCAC4-593-005847 (15m8) on 2018 Jan 28 around 21h55min UTC
A new update for the astrometry has been issued by Josselin Desmars. Important for European observers: The occultation track remains in central Europe.
Observations were made in Sierra Nevada and Calar Alto led by Jose Luis Ortiz and reduced by Marcelo Assafin and Julio Camargo.
The prediction is now much more accurate and remains very favourable for Europe but keep in mind that the event can occur everywhere in Europe/North Africa
so observations, even outside the path, are welcome.
Here a map centered on Europe (the shadow goes from North to South).
Each blue dot is spaced by one minute and the big blue dot corresponds to the nominal occultation. The red dotted lines represent the 1 sigma uncertainty.
A projection onto the whole earth is givcen in the following:
Areas in dark grey correspond to full night (Sun elevation below -18 degrees) and areas in light grey correspond to twilight (Sun elevation between -18 and 0 degrees) while daytime is in white.
Keep in mind the new prediction has a slightly earlier central time
for the occultation as compared with former predictions, around 21h55min UTC.
Observations are requested at least 15min before and after the occultation time (around 21:55 TU depending on your location).
Here more informations about the occultation.
The TNO 2002TC302 occults the star UCAC4-593-005847 (15m8) for Europe on 2018 January 28 around 21h55min UTC. The TNO has an approx. diameter of around 580km. The prediction has been made by the LuckyStar team (J. Desmars and B. Sicardy and the RIO team). It is based on a GAIA DR1 catalogue position, the proper motion has been taken from the UCAC5 catalogue. The ephemeris of 2002TC302 is from NIMAv10.
The star G* and J* magnitudes in the graphics are the G (from Gaia) and J (from 2MASS) magnitudes, normalized to a body moving at 20km/s in order to enhance very slow events. In this case, the movement of the shadow is slow, around 4.8 km/sec. This allows the use of even slow cameras, the spacial resolution of the measurement is around 5 km, if a 1 sec exposure time is used. This makes it an easy event, even for instruments of the 30cm class or less.
The event is very favourable, even if the uncertainty of the prediction is low. Keep in mind, that the possible occultation area covers one of the most higly populated area with telescopes in the world. Many experienced observers are in this region!
This is a unique chance to get more infos about this object in a distance of more than 44 astronomical units. The scientific rationale
of the observation is to determine a precise deiameter and shape of the body. This would allow a more precise determination of its volume and consecutively of its mass and density.
More information will come shortly before the occultation, perhaps a new prediction.
If you observe the event, please report either to myself
or to J. Desmars or B. Sicardy.
With many thanks to J. Desmars
and B. Sicardy
Wolfgang Beisker, IOTA-ES