Event between (533209) 14DR143 and star GA0880:04100107 with event index number of 2592355
Geocentric closest approach at 2022/05/31 17:51:31 UTC
J2000 position of star is 12:54:42.4 -00:51:15
Equinox of date position of star is 12:55:50.8 -00:58:27
Stellar brightness G=14.7,
use SENSEUP=128 with the MallinCam and and exposure
time of 2 seconds with the QHY174 camera.
Star is 109 degrees from the moon.
Moon is 2% illuminated.
TNO apparent brightness V=22.7
TNO is 49.2 AU from the Sun
and 48.6 AU from the Earth.
The TNO is moving 12.9
km/sec on the sky relative to the star, or,
1.3 arcsec/hr.
The 1-sigma error in the time of the event is 233 seconds.
The 1-sigma cross-track error in the shadow position is
2494 km.
The TNO has an absolute magnitude Hv=5.7
Diameter=436.5 km assuming a 5% albedo -- 33.9 sec chord
Diameter=178.2 km assuming a 30% albedo -- 13.8 sec chord
Dynamical classification is 3:2E
Star training set for 533209, (2022/05/31 17:38UT) Object RA Dec mag sep mel Spica 13:26:22.6 -11:16:39 1.0 12.79 120 Vindemiatrix 13:03:17.6 +10:50:21 2.8 11.96 105 38 Vir 12:54:20.1 -03:40:28 6.1 2.73 110 PPM 178912 12:57:35.7 -01:04:34 7.0 0.45 109 PPM 178911 12:57:06.5 -00:56:48 9.5 0.31 109 PPM 178905 12:55:22.1 -00:46:58 11.7 0.23 108 533209 12:55:51.4 -00:58:31 14.7 109 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 533209, (2022/05/31 17:38UT) Object RA Dec mag sep mel Spica 13:25:11.5 -11:09:41 1.0 12.79 120 Vindemiatrix 13:02:10.2 +10:57:33 2.8 11.96 105 38 Vir 12:53:10.8 -03:33:11 6.1 2.73 110 PPM 178912 12:56:26.6 -00:57:19 7.0 0.45 109 PPM 178911 12:55:57.5 -00:49:32 9.5 0.31 109 PPM 178905 12:54:13.1 -00:39:41 11.7 0.23 108 533209 12:54:42.4 -00:51:15 14.7 109 Positions are for J2000
Event circumstances last updated at 2022/03/12 01:41:22 UT
Marc W. Buie, Southwest Research Institute