RECON: TNO occultation with 32532

Event between (32532) Thereus and star GA0800:04340471 with event index number of 2196098

Geocentric closest approach at 2027/04/30 01:41:48 UTC

J2000 position of star is 13:13:41.8 -09:05:50
Equinox of date position of star is 13:14:58.3 -09:13:31
Stellar brightness G=16.7, use SENSEUP=128 with the MallinCam and and exposure time of 2 seconds with the QHY174 camera.
Star is 122 degrees from the moon. Moon is 39% illuminated.
Apparent brightness V=19.3

Object is 10.2 AU from the Sun and 9.2 AU from the Earth.
Apparent velocity is 19.8 km/sec on the sky relative to the star, or, 10.6 arcsec/hr.
The 1-sigma error in the time of the event is 33 seconds.
The 1-sigma cross-track error in the shadow position is 465 km.

The object has an absolute magnitude Hv=9.2
Diameter=86.3 km assuming a 5% albedo -- 4.4 sec chord
Diameter=35.2 km assuming a 30% albedo -- 1.8 sec chord
Dynamical classification is CENTAURR
 
 
 
 
 
 
 
 

Star training set for 32532, (2027/04/30 01:43UT)
Object            RA         Dec     mag  sep  mel
Spica          13:26:38.2 -11:18:11  1.0  3.50 119
PPM 196204     13:09:58.2 -09:07:48  5.5  1.28 124
PPM 196325     13:16:56.6 -08:11:55  8.2  1.13 122
PPM 196286     13:14:38.7 -09:04:34  8.9  0.20 123
32532          13:15:07.7 -09:14:29 16.7       122
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 32532, (2027/04/30 01:43UT)
Object            RA         Dec     mag  sep  mel
Spica          13:25:11.5 -11:09:41  1.0  3.50 119
PPM 196204     13:08:32.4 -08:59:05  5.5  1.28 124
PPM 196325     13:15:30.8 -08:03:18  8.2  1.13 122
PPM 196286     13:13:12.9 -08:55:55  8.9  0.20 123
32532          13:13:41.8 -09:05:50 16.7       122
Positions are for J2000

Event circumstances last updated at 2024/04/23 03:27:50 UT

Marc W. Buie, Southwest Research Institute

RECON