RECON: TNO occultation with 533396

Event between (533396) 14GQ53 and star GA0860:04989114 with event index number of 1606186

Geocentric closest approach at 2020/09/05 21:44:31 UTC

J2000 position of star is 16:42:49.7 -02:46:17
Equinox of date position of star is 16:43:54.0 -02:48:32
Stellar brightness G=14.2, use SENSEUP=64
Star is 134 degrees from the moon. Moon is 88% illuminated.
TNO apparent brightness V=23.3

TNO is 19.8 AU from the Sun and 19.9 AU from the Earth.
The TNO is moving 14.7 km/sec on the sky relative to the star, or, 3.7 arcsec/hr.
The 1-sigma error in the time of the event is 59 seconds.
The 1-sigma cross-track error in the shadow position is 1066 km.

The TNO has an absolute magnitude Hv=10.0
Diameter=83.2 km assuming a 5% albedo -- 4.1 sec chord
Diameter=34.0 km assuming a 30% albedo -- 1.7 sec chord
Dynamical classification is CENTAURR
 
 
 
 
 
 
 
 

Star training set for 533396, (2020/09/05 21:45UT)
Object            RA         Dec     mag  sep  mel
Antares        16:30:40.7 -26:28:34  0.9 23.88 134
1Del Oph       16:15:25.9 -03:44:46  2.7  7.17 141
12 Oph         16:37:26.7 -02:22:02  5.8  1.67 135
PPM 199899     16:42:13.1 -02:53:54  7.6  0.43 134
PPM 199936     16:44:54.8 -02:45:34  9.1  0.26 133
533396         16:43:54.5 -02:48:33 14.2       133
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 533396, (2020/09/05 21:45UT)
Object            RA         Dec     mag  sep  mel
Antares        16:29:24.4 -26:25:56  0.9 23.88 134
1Del Oph       16:14:20.7 -03:41:42  2.7  7.17 141
12 Oph         16:36:22.1 -02:19:35  5.8  1.67 135
PPM 199899     16:41:08.2 -02:51:35  7.6  0.43 134
PPM 199936     16:43:50.0 -02:43:19  9.1  0.26 133
533396         16:42:49.7 -02:46:17 14.2       134
Positions are for J2000

Event circumstances last updated at 2020/07/03 21:28:06 UT

Marc W. Buie, Southwest Research Institute

RECON