RECON: TNO occultation with 500832

Event between (500832) 13GZ136 and star GA0760:05406996 with event index number of 2328286

Geocentric closest approach at 2025/02/21 01:07:25 UTC

J2000 position of star is 15:51:14.8 -12:37:49
Equinox of date position of star is 15:52:33.0 -12:41:59
Stellar brightness G=15.7, use SENSEUP=128 with the MallinCam and and exposure time of 2 seconds with the QHY174 camera.
Star is 15 degrees from the moon. Moon is 47% illuminated.
Apparent brightness V=23.7

Object is 34.2 AU from the Sun and 34.1 AU from the Earth.
Apparent velocity is 7.3 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 378 seconds.
The 1-sigma cross-track error in the shadow position is 3045 km.

The object has an absolute magnitude Hv=8.2
Diameter=138.0 km assuming a 5% albedo -- 19.0 sec chord
Diameter=56.4 km assuming a 30% albedo -- 7.8 sec chord
Dynamical classification is SCATNEAR
 
 
 
 
 
 
 
 

Star training set for 500832, (2025/02/21 01:07UT)
Object            RA         Dec     mag  sep  mel
Antares        16:30:57.2 -26:29:08  0.9 16.46   4
8Bet1Sco       16:06:54.2 -19:52:20  2.6  7.94   7
PPM 230856     15:53:02.9 -14:12:27  6.2  1.51  13
PPM 230863     15:53:20.6 -12:36:41  7.7  0.20  15
500832         15:52:38.5 -12:42:16 15.7        14
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 500832, (2025/02/21 01:07UT)
Object            RA         Dec     mag  sep  mel
Antares        16:29:24.4 -26:25:56  0.9 16.46   4
8Bet1Sco       16:05:26.2 -19:48:20  2.6  7.94   7
PPM 230856     15:51:38.4 -14:08:01  6.2  1.51  13
PPM 230863     15:51:57.0 -12:32:15  7.7  0.20  15
500832         15:51:14.8 -12:37:49 15.7        14
Positions are for J2000

Event circumstances last updated at 2023/07/04 04:27:52 UT

Marc W. Buie, Southwest Research Institute

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