RECON: TNO occultation with 523659

Event between (523659) 12HG84 and star GA0640:07618028 with event index number of 309124

Geocentric closest approach at 2020/09/24 23:19:31 UTC

J2000 position of star is 16:12:18.8 -24:48:50
Equinox of date position of star is 16:13:30.6 -24:51:49
Stellar brightness G=15.9, use SENSEUP=128
Star is 38 degrees from the moon. Moon is 60% illuminated.
TNO apparent brightness V=21.6

TNO is 40.2 AU from the Sun and 40.6 AU from the Earth.
The TNO is moving 18.6 km/sec on the sky relative to the star, or, 2.3 arcsec/hr.
The 1-sigma error in the time of the event is 641 seconds.
The 1-sigma cross-track error in the shadow position is 1995 km.

The TNO has an absolute magnitude Hv=5.4
Diameter=501.2 km assuming a 5% albedo -- 27.0 sec chord
Diameter=204.6 km assuming a 30% albedo -- 11.0 sec chord
Dynamical classification is CLASSICAL
 
 
 
 
 
 
 
 

Star training set for 523659, (2020/09/24 23:20UT)
Object            RA         Dec     mag  sep  mel
Antares        16:30:40.9 -26:28:34  0.9  4.18  34
7Del Sco       16:01:33.8 -22:40:45  2.3  3.51  41
PPM 265182     16:09:58.3 -23:44:21  5.9  1.39  39
PPM 265227     16:12:17.2 -25:10:13  8.1  0.42  38
PPM 265235     16:12:45.2 -24:48:31  9.0  0.19  38
523659         16:13:34.0 -24:51:57 15.9        37
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 523659, (2020/09/24 23:20UT)
Object            RA         Dec     mag  sep  mel
Antares        16:29:24.4 -26:25:56  0.9  4.18  34
7Del Sco       16:00:20.0 -22:37:18  2.3  3.51  41
PPM 265182     16:08:43.7 -23:41:08  5.9  1.39  39
PPM 265227     16:11:01.8 -25:07:04  8.1  0.42  38
PPM 265235     16:11:30.1 -24:45:22  9.0  0.19  38
523659         16:12:18.8 -24:48:50 15.9        38
Positions are for J2000

Event circumstances last updated at 2019/10/16 21:26:14 UT

Marc W. Buie, Southwest Research Institute

RECON