RECON: TNO occultation with 05UN524

Event between 05UN524 and star GA1260:03296754 with event index number of 1957771

Geocentric closest approach at 2023/04/08 15:42:56 UTC

J2000 position of star is 08:25:23.9 +37:39:45
Equinox of date position of star is 08:26:50.5 +37:35:20
Stellar brightness G=14.9, use SENSEUP=128 with the MallinCam and and exposure time of 2 seconds with the QHY174 camera.
Star is 108 degrees from the moon. Moon is 93% illuminated.
TNO apparent brightness V=21.9

TNO is 19.1 AU from the Sun and 18.8 AU from the Earth.
The TNO is moving 8.6 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 82 seconds.
The 1-sigma cross-track error in the shadow position is 1032 km.

The TNO has an absolute magnitude Hv=8.8
Diameter=102.8 km assuming a 5% albedo -- 12.2 sec chord
Diameter=42.0 km assuming a 30% albedo -- 5.0 sec chord
Dynamical classification is CENTAURR
 
 
 
 
 
 
 
 

Star training set for 05UN524, (2023/04/08 15:43UT)
Object            RA         Dec     mag  sep  mel
Pollux         07:46:44.3 +27:58:05  1.1 12.78 115
PPM 073770     08:32:50.1 +37:11:05  6.0  1.24 107
PPM 073689     08:26:54.2 +37:18:39  8.1  0.27 108
PPM 073703     08:27:51.0 +37:28:03  8.8  0.22 108
05UN524        08:26:54.7 +37:35:07 14.9       108
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 05UN524, (2023/04/08 15:43UT)
Object            RA         Dec     mag  sep  mel
Pollux         07:45:17.9 +28:01:33  1.1 12.78 115
PPM 073770     08:31:20.0 +37:15:52  6.0  1.24 107
PPM 073689     08:25:23.6 +37:23:17  8.1  0.27 108
PPM 073703     08:26:20.4 +37:32:42  8.8  0.22 108
05UN524        08:25:23.9 +37:39:45 14.9       108
Positions are for J2000

Event circumstances last updated at 2022/03/12 01:56:51 UT

Marc W. Buie, Southwest Research Institute

RECON