Event between (523682) 14CN23 and star GA0520:14631897 with event index number of 2649259
Geocentric closest approach at 2024/09/19 12:27:19 UTC
J2000 position of star is 16:59:20.9 -36:39:34
Equinox of date position of star is 17:00:59.6 -36:41:41
Stellar brightness G=14.4,
use SENSEUP=64 with the MallinCam and and exposure
time of 1 seconds with the QHY174 camera.
Star is 119 degrees from the moon.
Moon is 97% illuminated.
Apparent brightness V=21.4
Object is 16.5 AU from the Sun
and 16.7 AU from the Earth.
Apparent velocity is 13.7
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 345 seconds.
The 1-sigma cross-track error in the shadow position is
2076 km.
The object has an absolute magnitude Hv=8.9
Diameter=104.7 km assuming a 5% albedo -- 7.3 sec chord
Diameter=42.8 km assuming a 30% albedo -- 3.0 sec chord
Dynamical classification is CENTAURR
Star training set for 523682, (2024/09/19 12:27UT) Object RA Dec mag sep mel Antares 16:30:55.6 -26:29:05 0.9 12.04 127 26Eps Sco 16:51:46.3 -34:20:08 2.3 3.02 121 PPM 295772 17:02:16.2 -35:58:10 5.7 0.77 119 PPM 295827 17:04:34.5 -36:53:42 8.3 0.74 118 PPM 295733 17:00:19.4 -36:33:30 9.7 0.19 119 PPM 295760 17:01:36.7 -36:40:56 10.1 0.12 119 523682 17:01:00.7 -36:41:42 14.4 119 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 523682, (2024/09/19 12:27UT) Object RA Dec mag sep mel Antares 16:29:24.4 -26:25:56 0.9 12.04 127 26Eps Sco 16:50:08.7 -34:17:41 2.3 3.02 121 PPM 295772 17:00:37.0 -35:56:05 5.7 0.77 119 PPM 295827 17:02:54.5 -36:51:42 8.3 0.74 118 PPM 295733 16:58:39.7 -36:31:21 9.7 0.19 119 PPM 295760 16:59:57.0 -36:38:50 10.1 0.12 119 523682 16:59:20.9 -36:39:34 14.4 119 Positions are for J2000
Event circumstances last updated at 2024/06/11 03:50:35 UT
Marc W. Buie, Southwest Research Institute