RECON: TNO occultation with 432949

Event between (432949) 12HH2 and star GA0840:04438205 with event index number of 2437735

Geocentric closest approach at 2023/08/09 09:00:59 UTC

J2000 position of star is 14:29:22.0 -04:39:56
Equinox of date position of star is 14:30:35.8 -04:46:10
Stellar brightness G=16.3, use SENSEUP=128 with the MallinCam and and exposure time of 2 seconds with the QHY174 camera.
Star is 156 degrees from the moon. Moon is 40% illuminated.
Apparent brightness V=21.5

Object is 31.3 AU from the Sun and 31.5 AU from the Earth.
Apparent velocity is 12.5 km/sec on the sky relative to the star, or, 2.0 arcsec/hr.
The 1-sigma error in the time of the event is 102 seconds.
The 1-sigma cross-track error in the shadow position is 1271 km.

The object has an absolute magnitude Hv=6.3
Diameter=322.1 km assuming a 5% albedo -- 26.0 sec chord
Diameter=131.5 km assuming a 30% albedo -- 10.6 sec chord
Dynamical classification is 5:4E+10:8II
 
 
 
 
 
 
 
 

Star training set for 432949, (2023/08/09 09:00UT)
Object            RA         Dec     mag  sep  mel
Spica          13:26:26.4 -11:17:02  1.0 17.16 146
27Bet Lib      15:18:16.8 -09:28:07  2.6 12.72 166
105Phi Vir     14:29:25.3 -02:19:58  4.8  2.45 154
PPM 197596     14:30:24.0 -05:02:26  8.5  0.28 156
432949         14:30:36.1 -04:46:11 16.3       156
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 432949, (2023/08/09 09:00UT)
Object            RA         Dec     mag  sep  mel
Spica          13:25:11.5 -11:09:41  1.0 17.16 146
27Bet Lib      15:17:00.3 -09:22:59  2.6 12.72 166
105Phi Vir     14:28:11.9 -02:13:41  4.8  2.45 154
PPM 197596     14:29:09.7 -04:56:10  8.5  0.28 156
432949         14:29:22.0 -04:39:56 16.3       156
Positions are for J2000

Event circumstances last updated at 2023/07/04 04:03:37 UT

Marc W. Buie, Southwest Research Institute

RECON