RECON: TNO occultation with 535988

Event between (535988) 15BU518 and star GA0740:05361981 with event index number of 2559570

Geocentric closest approach at 2023/03/23 18:01:29 UTC

J2000 position of star is 15:07:11.8 -14:32:58
Equinox of date position of star is 15:08:27.5 -14:38:09
Stellar brightness G=16.3, use SENSEUP=128 with the MallinCam and and exposure time of 2 seconds with the QHY174 camera.
Star is 161 degrees from the moon. Moon is 5% illuminated.
TNO apparent brightness V=22.8

TNO is 32.9 AU from the Sun and 32.2 AU from the Earth.
The TNO is moving 14.8 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 158 seconds.
The 1-sigma cross-track error in the shadow position is 1584 km.

The TNO has an absolute magnitude Hv=7.5
Diameter=190.6 km assuming a 5% albedo -- 12.9 sec chord
Diameter=77.8 km assuming a 30% albedo -- 5.2 sec chord
Dynamical classification is SCATNEAR
 
 
 
 
 
 
 
 

Star training set for 535988, (2023/03/23 18:03UT)
Object            RA         Dec     mag  sep  mel
Antares        16:30:50.1 -26:28:53  0.9 22.57 140
27Bet Lib      15:18:15.6 -09:28:02  2.6  5.70 159
21Nu Lib       15:07:55.6 -16:20:44  5.2  1.71 161
PPM 229783     15:08:42.8 -14:46:02  8.0  0.14 161
535988         15:08:29.1 -14:38:15 16.3       161
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 535988, (2023/03/23 18:03UT)
Object            RA         Dec     mag  sep  mel
Antares        16:29:24.4 -26:25:56  0.9 22.57 140
27Bet Lib      15:17:00.3 -09:22:59  2.6  5.70 159
21Nu Lib       15:06:37.6 -16:15:25  5.2  1.71 161
PPM 229783     15:07:25.4 -14:40:44  8.0  0.14 161
535988         15:07:11.8 -14:32:58 16.3       161
Positions are for J2000

Event circumstances last updated at 2022/10/03 04:24:29 UT

Marc W. Buie, Southwest Research Institute

RECON