Event between (552678) 10JG210 and star GA0880:05357185 with event index number of 2222162
Geocentric closest approach at 2022/08/16 16:58:07 UTC
J2000 position of star is 17:13:52.1 -00:53:57
Equinox of date position of star is 17:14:59.5 -00:55:23
Stellar brightness G=14.4,
use SENSEUP=64 with the MallinCam and and exposure
time of 1 seconds with the QHY174 camera.
Star is 125 degrees from the moon.
Moon is 74% illuminated.
TNO apparent brightness V=21.6
TNO is 18.9 AU from the Sun
and 18.5 AU from the Earth.
The TNO is moving 12.9
km/sec on the sky relative to the star, or,
3.5 arcsec/hr.
The 1-sigma error in the time of the event is 55 seconds.
The 1-sigma cross-track error in the shadow position is
765 km.
The TNO has an absolute magnitude Hv=8.6
Diameter=113.2 km assuming a 5% albedo -- 8.9 sec chord
Diameter=46.2 km assuming a 30% albedo -- 3.6 sec chord
Dynamical classification is CENTAURR
Star training set for 552678, (2022/08/16 16:58UT) Object RA Dec mag sep mel Antares 16:30:47.9 -26:28:49 0.9 27.68 135 60Bet Oph 17:44:35.5 +04:33:34 2.8 9.20 117 PPM 180004 17:09:23.7 -01:06:27 6.5 1.42 126 PPM 180014 17:13:32.5 -00:47:59 8.4 0.39 125 PPM 180015 17:13:42.9 -01:02:13 8.9 0.35 125 PPM 180018 17:15:36.3 -00:43:58 10.1 0.24 125 552678 17:15:02.1 -00:55:26 14.4 125 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 552678, (2022/08/16 16:58UT) Object RA Dec mag sep mel Antares 16:29:24.4 -26:25:56 0.9 27.68 135 60Bet Oph 17:43:28.3 +04:34:06 2.8 9.20 117 PPM 180004 17:08:13.6 -01:04:47 6.5 1.42 126 PPM 180014 17:12:22.5 -00:46:27 8.4 0.39 125 PPM 180015 17:12:32.8 -01:00:41 8.9 0.35 125 PPM 180018 17:14:26.3 -00:42:30 10.1 0.24 125 552678 17:13:52.1 -00:53:57 14.4 125 Positions are for J2000
Event circumstances last updated at 2021/10/14 01:43:29 UT
Marc W. Buie, Southwest Research Institute