RECON: TNO occultation with 119951

Event between (119951) 02KX14 and star GA0660:11716378 with event index number of 277547

Geocentric closest approach at 2020/07/12 00:16:58 UTC

J2000 position of star is 17:20:13.6 -23:18:02
Equinox of date position of star is 17:21:24.4 -23:19:09
Stellar brightness G=13.4, use SENSEUP=32
Star is 109 degrees from the moon. Moon is 59% illuminated.
TNO apparent brightness V=20.6

TNO is 39.0 AU from the Sun and 38.1 AU from the Earth.
The TNO is moving 20.8 km/sec on the sky relative to the star, or, 2.7 arcsec/hr.
The 1-sigma error in the time of the event is 111 seconds.
The 1-sigma cross-track error in the shadow position is 1480 km.

The TNO has an absolute magnitude Hv=4.7
Diameter=691.9 km assuming a 5% albedo -- 33.2 sec chord
Diameter=282.4 km assuming a 30% albedo -- 13.6 sec chord
Dynamical classification is CLASSICAL
 
 
 
 
 
 
 
 

Star training set for 119951, (2020/07/12 00:17UT)
Object            RA         Dec     mag  sep  mel
Antares        16:30:40.2 -26:28:33  0.9 11.94 119
35Eta Oph      17:11:33.4 -15:44:56  2.6  7.92 112
PPM 266836     17:26:21.6 -24:15:39  6.4  1.46 107
PPM 266759     17:23:21.3 -23:35:33  8.2  0.51 108
PPM 266724     17:22:18.7 -23:11:07  9.3  0.23 108
119951         17:21:28.4 -23:19:12 13.4       108
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 119951, (2020/07/12 00:17UT)
Object            RA         Dec     mag  sep  mel
Antares        16:29:24.4 -26:25:56  0.9 11.94 119
35Eta Oph      17:10:22.7 -15:43:29  2.6  7.92 112
PPM 266836     17:25:06.3 -24:14:37  6.4  1.46 107
PPM 266759     17:22:06.4 -23:34:26  8.2  0.51 108
PPM 266724     17:21:04.0 -23:09:59  9.3  0.23 108
119951         17:20:13.6 -23:18:02 13.4       109
Positions are for J2000

Event circumstances last updated at 2019/06/08 00:02:42 UT

Marc W. Buie, Southwest Research Institute

RECON