Event between (535026) 14WV509 and star GA0920:00458151 with event index number of 2337867
Geocentric closest approach at 2024/03/29 05:07:15 UTC
J2000 position of star is 04:40:00.8 +03:46:16
Equinox of date position of star is 04:41:13.5 +03:48:53
Stellar brightness G=16.8,
use SENSEUP=128 with the MallinCam and and exposure
time of 2 seconds with the QHY174 camera.
Star is 153 degrees from the moon.
Moon is 86% illuminated.
Apparent brightness V=22.8
Object is 39.3 AU from the Sun
and 39.7 AU from the Earth.
Apparent velocity is 20.3
km/sec on the sky relative to the star, or,
2.5 arcsec/hr.
The 1-sigma error in the time of the event is 210 seconds.
The 1-sigma cross-track error in the shadow position is
2186 km.
The object has an absolute magnitude Hv=6.7
Diameter=275.4 km assuming a 5% albedo -- 13.3 sec chord
Diameter=112.4 km assuming a 30% albedo -- 5.4 sec chord
Dynamical classification is SCATEXTD
Star training set for 535026, (2024/03/29 05:16UT) Object RA Dec mag sep mel Aldebaran 04:37:18.9 +16:33:22 0.8 12.78 161 67Bet Eri 05:09:02.6 -05:03:25 2.8 11.26 142 PPM 147685 04:35:25.7 +05:37:04 5.8 2.32 155 PPM 147832 04:43:31.4 +03:50:51 8.5 0.56 153 PPM 147818 04:42:38.4 +03:42:15 8.6 0.36 153 PPM 147808 04:42:03.1 +03:43:56 10.5 0.21 153 535026 04:41:17.4 +03:49:01 16.8 153 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 535026, (2024/03/29 05:16UT) Object RA Dec mag sep mel Aldebaran 04:35:55.3 +16:30:29 0.8 12.78 161 67Bet Eri 05:07:50.8 -05:05:13 2.8 11.26 142 PPM 147685 04:34:08.2 +05:34:08 5.8 2.32 155 PPM 147832 04:42:14.8 +03:48:11 8.5 0.56 153 PPM 147818 04:41:21.9 +03:39:32 8.6 0.36 153 PPM 147808 04:40:46.6 +03:41:12 10.5 0.21 153 535026 04:40:00.8 +03:46:16 16.8 153 Positions are for J2000
Event circumstances last updated at 2023/01/13 03:56:57 UT
Marc W. Buie, Southwest Research Institute