RECON: TNO occultation with 538691

Event between (538691) 16FW59 and star GA0800:04229942 with event index number of 1624424

Geocentric closest approach at 2020/02/21 02:02:16 UTC

J2000 position of star is 12:26:31.5 -09:43:02
Equinox of date position of star is 12:27:32.0 -09:49:30
Stellar brightness G=15.8, use SENSEUP=128
Star is 113 degrees from the moon. Moon is 6% illuminated.
TNO apparent brightness V=22.7

TNO is 45.3 AU from the Sun and 44.5 AU from the Earth.
The TNO is moving 19.2 km/sec on the sky relative to the star, or, 2.1 arcsec/hr.
The 1-sigma error in the time of the event is 314 seconds.
The 1-sigma cross-track error in the shadow position is 3176 km.

The TNO has an absolute magnitude Hv=6.1
Diameter=363.1 km assuming a 5% albedo -- 18.9 sec chord
Diameter=148.2 km assuming a 30% albedo -- 7.7 sec chord
Dynamical classification is CLASSICAL
 
 
 
 
 
 
 
 

Star training set for 538691, (2020/02/21 02:02UT)
Object            RA         Dec     mag  sep  mel
Spica          13:26:15.4 -11:15:57  1.0 14.49  99
4Gam Crv       12:16:50.7 -17:39:13  2.6  8.25 111
21 Vir         12:34:49.2 -09:33:46  5.6  1.81 111
PPM 225875     12:28:53.5 -10:16:42  8.5  0.56 112
PPM 195483     12:27:32.9 -10:04:33  9.5  0.25 113
538691         12:27:34.0 -09:49:43 15.8       113
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 538691, (2020/02/21 02:02UT)
Object            RA         Dec     mag  sep  mel
Spica          13:25:11.5 -11:09:41  1.0 14.49  99
4Gam Crv       12:15:48.2 -17:32:31  2.6  8.25 111
21 Vir         12:33:46.6 -09:27:07  5.6  1.81 111
PPM 225875     12:27:51.0 -10:10:01  8.5  0.56 112
PPM 195483     12:26:30.4 -09:57:52  9.5  0.25 113
538691         12:26:31.5 -09:43:02 15.8       113
Positions are for J2000

Event circumstances last updated at 2019/07/02 02:29:59 UT

Marc W. Buie, Southwest Research Institute

RECON