RECON: TNO occultation with 31824

Event between (31824) Elatus and star GA0720:05670920 with event index number of 2195794

Geocentric closest approach at 2028/03/31 03:29:03 UTC

J2000 position of star is 15:45:39.5 -16:50:09
Equinox of date position of star is 15:47:02.1 -16:54:36
Stellar brightness G=15.9, use SENSEUP=128 with the MallinCam and and exposure time of 2 seconds with the QHY174 camera.
Star is 168 degrees from the moon. Moon is 23% illuminated.
Apparent brightness V=21.8

Object is 13.7 AU from the Sun and 13.0 AU from the Earth.
Apparent velocity is 12.8 km/sec on the sky relative to the star, or, 4.9 arcsec/hr.
The 1-sigma error in the time of the event is 249 seconds.
The 1-sigma cross-track error in the shadow position is 1360 km.

The object has an absolute magnitude Hv=10.3
Diameter=56.5 km assuming a 5% albedo -- 4.1 sec chord
Diameter=23.1 km assuming a 30% albedo -- 1.7 sec chord
Dynamical classification is CENTAURR
 
 
 
 
 
 
 
 

Star training set for 31824, (2028/03/31 03:28UT)
Object            RA         Dec     mag  sep  mel
Antares        16:31:08.7 -26:29:32  0.9 13.97 178
8Bet1Sco       16:07:05.1 -19:52:49  2.6  5.55 173
44Eta Lib      15:45:40.0 -15:45:38  5.4  1.22 167
PPM 230708     15:47:26.9 -17:02:14  8.0  0.12 168
31824          15:47:16.0 -16:55:21 15.9       168
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 31824, (2028/03/31 03:28UT)
Object            RA         Dec     mag  sep  mel
Antares        16:29:24.4 -26:25:56  0.9 13.97 178
8Bet1Sco       16:05:26.2 -19:48:20  2.6  5.55 173
44Eta Lib      15:44:04.4 -15:40:24  5.4  1.22 167
PPM 230708     15:45:50.4 -16:57:03  8.0  0.12 168
31824          15:45:39.5 -16:50:09 15.9       168
Positions are for J2000

Event circumstances last updated at 2024/03/07 04:20:31 UT

Marc W. Buie, Southwest Research Institute

RECON