RECON: TNO occultation with 538690

Event between (538690) 16FP59 and star GA0820:04223455 with event index number of 1624363

Geocentric closest approach at 2020/03/27 18:15:46 UTC

J2000 position of star is 12:23:35.9 -07:10:57
Equinox of date position of star is 12:24:36.2 -07:17:26
Stellar brightness G=16.8, use SENSEUP=128
Star is 143 degrees from the moon. Moon is 10% illuminated.
TNO apparent brightness V=22.6

TNO is 47.8 AU from the Sun and 46.8 AU from the Earth.
The TNO is moving 25.6 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 115 seconds.
The 1-sigma cross-track error in the shadow position is 2033 km.

The TNO has an absolute magnitude Hv=5.8
Diameter=416.9 km assuming a 5% albedo -- 16.3 sec chord
Diameter=170.2 km assuming a 30% albedo -- 6.6 sec chord
Dynamical classification is CLASSICAL
 
 
 
 
 
 
 
 

Star training set for 538690, (2020/03/27 18:16UT)
Object            RA         Dec     mag  sep  mel
Spica          13:26:15.7 -11:15:59  1.0 15.71 159
4Gam Crv       12:16:51.0 -17:39:15  2.6 10.53 142
PPM 195518     12:28:54.0 -04:43:37  6.2  2.78 144
PPM 195429     12:24:12.1 -07:24:40  7.1  0.16 143
PPM 195436     12:24:27.7 -07:09:55  9.3  0.14 143
538690         12:24:38.5 -07:17:41 16.8       143
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 538690, (2020/03/27 18:16UT)
Object            RA         Dec     mag  sep  mel
Spica          13:25:11.5 -11:09:41  1.0 15.71 159
4Gam Crv       12:15:48.2 -17:32:31  2.6 10.53 142
PPM 195518     12:27:51.4 -04:36:55  6.2  2.78 144
PPM 195429     12:23:09.5 -07:17:57  7.1  0.16 143
PPM 195436     12:23:25.1 -07:03:12  9.3  0.14 143
538690         12:23:35.9 -07:10:57 16.8       143
Positions are for J2000

Event circumstances last updated at 2019/07/02 02:34:26 UT

Marc W. Buie, Southwest Research Institute

RECON