RECON: TNO occultation with 536922

Event between (536922) 15FP345 and star GA0820:04885169 with event index number of 2724509

Geocentric closest approach at 2029/03/04 05:54:52 UTC

J2000 position of star is 15:16:22.5 -07:42:33
Equinox of date position of star is 15:17:37.1 -07:47:37
Stellar brightness G=15.9, use SENSEUP=128 with the MallinCam and and exposure time of 2 seconds with the QHY174 camera.
Star is 21 degrees from the moon. Moon is 82% illuminated.
Apparent brightness V=22.7

Object is 37.9 AU from the Sun and 37.5 AU from the Earth.
Apparent velocity is 8.5 km/sec on the sky relative to the star, or, 1.1 arcsec/hr.
The 1-sigma error in the time of the event is 487 seconds.
The 1-sigma cross-track error in the shadow position is 3816 km.

The object has an absolute magnitude Hv=6.8
Diameter=257.0 km assuming a 5% albedo -- 30.4 sec chord
Diameter=104.9 km assuming a 30% albedo -- 12.4 sec chord
Dynamical classification is 7:4EEE+7:4EII
 
 
 
 
 
 
 
 

Star training set for 536922, (2029/03/04 05:55UT)
Object            RA         Dec     mag  sep  mel
Antares        16:31:12.1 -26:29:39  0.9 25.52  36
27Bet Lib      15:18:34.9 -09:29:19  2.6  1.68  21
PPM 198488     15:22:40.3 -05:55:42  5.4  2.22  23
PPM 198427     15:18:47.5 -07:57:44  7.7  0.26  21
536922         15:17:56.2 -07:48:54 15.9        21
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 536922, (2029/03/04 05:55UT)
Object            RA         Dec     mag  sep  mel
Antares        16:29:24.4 -26:25:56  0.9 25.52  36
27Bet Lib      15:17:00.3 -09:22:59  2.6  1.68  21
PPM 198488     15:21:07.5 -05:49:30  5.4  2.22  23
PPM 198427     15:17:13.7 -07:51:24  7.7  0.26  21
536922         15:16:22.5 -07:42:33 15.9        21
Positions are for J2000

Event circumstances last updated at 2023/03/27 23:25:30 UT

Marc W. Buie, Southwest Research Institute

RECON