Event between (523764) 14WC510 and star GA0920:02181551 with event index number of 2613298
Geocentric closest approach at 2024/12/29 01:43:18 UTC
J2000 position of star is 07:02:11.6 +02:22:44
Equinox of date position of star is 07:03:27.2 +02:20:33
Stellar brightness G=16.3,
use SENSEUP=128 with the MallinCam and and exposure
time of 2 seconds with the QHY174 camera.
Star is 141 degrees from the moon.
Moon is 4% illuminated.
Apparent brightness V=22.0
Object is 29.8 AU from the Sun
and 28.9 AU from the Earth.
Apparent velocity is 23.9
km/sec on the sky relative to the star, or,
4.1 arcsec/hr.
The 1-sigma error in the time of the event is 96 seconds.
The 1-sigma cross-track error in the shadow position is
1071 km.
The object has an absolute magnitude Hv=7.2
Diameter=212.8 km assuming a 5% albedo -- 9.0 sec chord
Diameter=86.9 km assuming a 30% albedo -- 3.7 sec chord
Dynamical classification is 3:2E+6:4II
Star training set for 523764, (2024/12/29 01:45UT) Object RA Dec mag sep mel Betelgeuse 05:56:31.5 +07:24:35 0.4 17.43 155 Alhena 06:39:09.3 +16:22:33 1.9 15.26 154 PPM 151661 07:00:15.9 +03:33:59 6.0 1.47 142 PPM 151829 07:04:52.8 +02:23:56 7.9 0.35 140 PPM 151808 07:04:11.1 +02:34:40 9.2 0.29 141 PPM 151757 07:02:45.7 +02:18:17 11.1 0.19 141 523764 07:03:29.8 +02:20:28 16.3 140 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 523764, (2024/12/29 01:45UT) Object RA Dec mag sep mel Betelgeuse 05:55:10.3 +07:24:26 0.4 17.43 155 Alhena 06:37:42.8 +16:23:57 1.9 15.26 154 PPM 151661 06:58:57.0 +03:36:08 6.0 1.47 142 PPM 151829 07:03:34.6 +02:26:14 7.9 0.35 140 PPM 151808 07:02:52.8 +02:36:57 9.2 0.29 141 PPM 151757 07:01:27.5 +02:20:31 11.1 0.19 141 523764 07:02:11.6 +02:22:44 16.3 141 Positions are for J2000
Event circumstances last updated at 2024/03/02 06:05:00 UT
Marc W. Buie, Southwest Research Institute