RECON: TNO occultation with 492338

Event between (492338) 14FW and star UC4-411-060327 with event index number of 193976

Geocentric closest approach at 2018/02/11 08:32:38 UTC

J2000 position of star is 15:21:46.0 -07:48:35
Equinox of date position of star is 15:22:42.1 -07:52:17
Stellar brightness R=15.7, use SENSEUP=128
Star is 43 degrees from the moon. Moon is 18% illuminated.
TNO apparent brightness V=20.7

TNO is 10.8 AU from the Sun and 10.7 AU from the Earth.
The TNO is moving 11.1 km/sec on the sky relative to the star, or, 5.1 arcsec/hr.
The 1-sigma error in the time of the event is 107 seconds.
The 1-sigma cross-track error in the shadow position is 667 km.

The TNO has an absolute magnitude Hv=10.0
Diameter=60.3 km assuming a 5% albedo -- 5.4 sec chord
Diameter=24.6 km assuming a 30% albedo -- 2.2 sec chord
Dynamical classification is CENTAURR
 
 
 
 
 
 
 
 

Star training set for 492338, (2018/02/11 08:33UT)
Object            RA         Dec     mag  sep  mel
Antares        16:30:31.3 -26:28:14  0.9 24.59  25
27Bet Lib      15:17:59.1 -09:26:55  2.6  1.96  44
PPM 198488     15:22:05.2 -05:53:21  5.4  1.99  44
PPM 198502     15:22:38.6 -08:43:14  8.5  0.85  43
PPM 198493     15:22:19.0 -07:49:31  9.3  0.11  43
492338         15:22:44.3 -07:52:26 15.7        43
Positions are for equinox of date

Azimuth is measured in degrees eastward from north. North is at an azimuth of 0, due East is at an azimuth of 90 degrees, due South is 180, and due West is 270.

Do not use the listing below for the RECON CPC 1100 telescopes. This is provided for other non-team facilities.

Star training set for 492338, (2018/02/11 08:33UT)
Object            RA         Dec     mag  sep  mel
Antares        16:29:24.4 -26:25:56  0.9 24.59  25
27Bet Lib      15:17:00.3 -09:22:59  2.6  1.96  44
PPM 198488     15:21:07.5 -05:49:30  5.4  1.99  44
PPM 198502     15:21:40.0 -08:39:24  8.5  0.85  43
PPM 198493     15:21:20.8 -07:45:40  9.3  0.11  43
492338         15:21:46.0 -07:48:35 15.7        43
Positions are for J2000

Event circumstances last updated at 2017/06/14 17:00:06 UT

Marc W. Buie, Southwest Research Institute

RECON