RECON: TNO occultation with 547893

Event between (547893) 10WN75 and star GA0860:01315884 with event index number of 2399253

Geocentric closest approach at 2025/08/28 14:24:22 UTC

J2000 position of star is 06:29:36.6 -02:19:34
Equinox of date position of star is 06:30:50.5 -02:20:39
Stellar brightness G=15.6, use SENSEUP=128 with the MallinCam and and exposure time of 2 seconds with the QHY174 camera.
Star is 113 degrees from the moon. Moon is 26% illuminated.
Apparent brightness V=21.7

Object is 37.1 AU from the Sun and 37.6 AU from the Earth.
Apparent velocity is 22.9 km/sec on the sky relative to the star, or, 3.0 arcsec/hr.
The 1-sigma error in the time of the event is 125 seconds.
The 1-sigma cross-track error in the shadow position is 2038 km.

The object has an absolute magnitude Hv=5.8
Diameter=436.5 km assuming a 5% albedo -- 18.6 sec chord
Diameter=178.2 km assuming a 30% albedo -- 7.6 sec chord
Dynamical classification is SCATEXTD
 
 
 
 
 
 
 
 

Star training set for 547893, (2025/08/28 14:24UT)
Object            RA         Dec     mag  sep  mel
Betelgeuse     05:56:33.7 +07:24:35  0.4 12.98 125
Saiph          05:48:58.5 -09:39:45  2.1 12.73 120
PPM 176266     06:27:57.6 -01:31:28  5.9  1.10 114
PPM 176287     06:30:40.3 -02:14:13  8.5  0.12 113
547893         06:30:54.1 -02:20:42 15.6       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 547893, (2025/08/28 14:24UT)
Object            RA         Dec     mag  sep  mel
Betelgeuse     05:55:10.3 +07:24:26  0.4 12.98 125
Saiph          05:47:45.4 -09:40:11  2.1 12.73 120
PPM 176266     06:26:39.6 -01:30:27  5.9  1.10 114
PPM 176287     06:29:22.7 -02:13:06  8.5  0.12 113
547893         06:29:36.6 -02:19:34 15.6       113
Positions are for J2000

Event circumstances last updated at 2024/06/18 02:53:25 UT

Marc W. Buie, Southwest Research Institute

RECON