RECON: TNO occultation with 469442

Event between (469442) 02GG166 and star GA0600:31301659 with event index number of 1297998

Geocentric closest approach at 2024/02/24 11:39:52 UTC

J2000 position of star is 18:02:16.9 -29:32:51
Equinox of date position of star is 18:03:49.3 -29:32:44
Stellar brightness G=16.5, use SENSEUP=128 with the MallinCam and and exposure time of 2 seconds with the QHY174 camera.
Star is 116 degrees from the moon. Moon is 100% illuminated.
Apparent brightness V=20.5

Object is 15.5 AU from the Sun and 15.9 AU from the Earth.
Apparent velocity is 22.8 km/sec on the sky relative to the star, or, 7.1 arcsec/hr.
The 1-sigma error in the time of the event is 93 seconds.
The 1-sigma cross-track error in the shadow position is 689 km.

The object has an absolute magnitude Hv=8.2
Diameter=136.1 km assuming a 5% albedo -- 6.0 sec chord
Diameter=55.6 km assuming a 30% albedo -- 2.4 sec chord
Dynamical classification is CENTAURR
 
 
 
 
 
 
 
 

Star training set for 469442, (2024/02/24 11:40UT)
Object            RA         Dec     mag  sep  mel
Antares        16:30:53.5 -26:29:01  0.9 20.70  95
34Ups Sco      17:32:24.5 -37:18:46  2.7 10.15 109
Gam1Sgr        18:06:33.8 -29:34:36  4.7  0.60 116
PPM 267733     18:04:16.0 -29:32:04  8.5  0.10 116
469442         18:03:49.5 -29:32:44 16.5       116
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 469442, (2024/02/24 11:40UT)
Object            RA         Dec     mag  sep  mel
Antares        16:29:24.4 -26:25:56  0.9 20.70  95
34Ups Sco      17:30:45.8 -37:17:46  2.7 10.15 109
Gam1Sgr        18:05:01.2 -29:34:48  4.7  0.60 116
PPM 267733     18:02:43.4 -29:32:11  8.5  0.10 116
469442         18:02:16.9 -29:32:51 16.5       116
Positions are for J2000

Event circumstances last updated at 2024/02/12 04:17:45 UT

Marc W. Buie, Southwest Research Institute

RECON