RECON: TNO occultation with 02GB32

Event between 02GB32 and star GA0820:04835001 with event index number of 1266262

Geocentric closest approach at 2024/06/11 18:55:18 UTC

J2000 position of star is 15:45:27.0 -06:56:06
Equinox of date position of star is 15:46:42.4 -07:00:25
Stellar brightness G=14.6, use SENSEUP=128 with the MallinCam and and exposure time of 2 seconds with the QHY174 camera.
Star is 90 degrees from the moon. Moon is 28% illuminated.
Apparent brightness V=23.5

Object is 36.7 AU from the Sun and 35.8 AU from the Earth.
Apparent velocity is 20.2 km/sec on the sky relative to the star, or, 2.8 arcsec/hr.
The 1-sigma error in the time of the event is 449 seconds.
The 1-sigma cross-track error in the shadow position is 1944 km.

The object has an absolute magnitude Hv=7.8
Diameter=168.3 km assuming a 5% albedo -- 8.3 sec chord
Diameter=68.7 km assuming a 30% albedo -- 3.4 sec chord
Dynamical classification is SCATNEAR
 
 
 
 
 
 
 
 

Star training set for 02GB32, (2024/06/11 19:25UT)
Object            RA         Dec     mag  sep  mel
Antares        16:30:54.6 -26:29:03  0.9 22.13 105
27Bet Lib      15:18:19.6 -09:28:18  2.6  7.45  84
PPM 198946     15:48:03.5 -06:11:41  6.5  0.88  90
PPM 198923     15:46:30.3 -07:16:34  9.0  0.27  90
02GB32         15:46:45.5 -07:00:36 14.6        90
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 02GB32, (2024/06/11 19:25UT)
Object            RA         Dec     mag  sep  mel
Antares        16:29:24.4 -26:25:56  0.9 22.13 105
27Bet Lib      15:17:00.3 -09:22:59  2.6  7.45  84
PPM 198946     15:46:45.4 -06:07:13  6.5  0.88  90
PPM 198923     15:45:11.6 -07:12:04  9.0  0.27  90
02GB32         15:45:27.0 -06:56:06 14.6        90
Positions are for J2000

Event circumstances last updated at 2023/07/04 04:13:07 UT

Marc W. Buie, Southwest Research Institute

RECON