RECON: TNO occultation with 469442

Event between (469442) 02GG166 and star GA0620:08675497 with event index number of 1103422

Geocentric closest approach at 2021/05/09 14:04:56 UTC

J2000 position of star is 16:32:17.9 -26:48:06
Equinox of date position of star is 16:33:36.8 -26:50:44
Stellar brightness G=15.1, use SENSEUP=128 with the MallinCam and and exposure time of 2 seconds with the QHY174 camera.
Star is 134 degrees from the moon. Moon is 4% illuminated.
TNO apparent brightness V=20.6

TNO is 17.2 AU from the Sun and 16.3 AU from the Earth.
The TNO is moving 19.1 km/sec on the sky relative to the star, or, 5.8 arcsec/hr.
The 1-sigma error in the time of the event is 44 seconds.
The 1-sigma cross-track error in the shadow position is 616 km.

The TNO has an absolute magnitude Hv=8.2
Diameter=136.1 km assuming a 5% albedo -- 7.1 sec chord
Diameter=55.6 km assuming a 30% albedo -- 2.9 sec chord
Dynamical classification is CENTAURR
 
 
 
 
 
 
 
 

Star training set for 469442, (2021/05/09 14:05UT)
Object            RA         Dec     mag  sep  mel
Antares        16:30:43.2 -26:28:39  0.9  0.74 135
23Tau Sco      16:37:12.9 -28:15:31  2.8  1.62 133
PPM 265618     16:32:41.7 -26:34:56  6.1  0.33 134
PPM 265651     16:33:54.0 -26:37:14  9.3  0.23 134
469442         16:33:37.0 -26:50:45 15.1       134
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, (2021/05/09 14:05UT)
Object            RA         Dec     mag  sep  mel
Antares        16:29:24.4 -26:25:56  0.9  0.74 135
23Tau Sco      16:35:52.9 -28:12:58  2.8  1.62 133
PPM 265618     16:31:22.9 -26:32:16  6.1  0.33 134
PPM 265651     16:32:35.1 -26:34:35  9.3  0.23 134
469442         16:32:17.9 -26:48:06 15.1       134
Positions are for J2000

Event circumstances last updated at 2021/04/25 22:58:16 UT

Marc W. Buie, Southwest Research Institute

RECON