Event between (523752) 14VU37 and star GA1060:00844521 with event index number of 2615285
Geocentric closest approach at 2026/09/22 06:39:27 UTC
J2000 position of star is 05:15:13.7 +17:42:40
Equinox of date position of star is 05:16:38.6 +17:44:13
Stellar brightness G=16.8,
use SENSEUP=128 with the MallinCam and and exposure
time of 2 seconds with the QHY174 camera.
Star is 132 degrees from the moon.
Moon is 80% illuminated.
Apparent brightness V=21.4
Object is 42.2 AU from the Sun
and 42.1 AU from the Earth.
Apparent velocity is 5.0
km/sec on the sky relative to the star, or,
0.6 arcsec/hr.
The 1-sigma error in the time of the event is 329 seconds.
The 1-sigma cross-track error in the shadow position is
1938 km.
The object has an absolute magnitude Hv=5.0
Diameter=586.2 km assuming a 5% albedo -- 121.5 sec chord
Diameter=239.3 km assuming a 30% albedo -- 49.6 sec chord
Dynamical classification is SCATEXTD
Star training set for 523752, (2026/09/22 06:41UT) Object RA Dec mag sep mel Aldebaran 04:37:27.4 +16:33:40 0.8 9.47 123 Alnath 05:27:59.0 +28:37:39 1.6 11.19 136 PPM 120692 05:13:13.8 +16:04:35 5.2 1.87 131 PPM 120798 05:19:05.0 +17:41:24 8.5 0.55 133 PPM 120758 05:16:39.8 +18:06:13 10.0 0.37 132 PPM 120737 05:15:42.5 +17:53:21 10.8 0.30 132 523752 05:16:47.0 +17:44:23 16.8 132 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 523752, (2026/09/22 06:41UT) Object RA Dec mag sep mel Aldebaran 04:35:55.3 +16:30:29 0.8 9.47 123 Alnath 05:26:17.6 +28:36:23 1.6 11.19 136 PPM 120692 05:11:41.6 +16:02:45 5.2 1.87 131 PPM 120798 05:17:31.6 +17:39:47 8.5 0.55 133 PPM 120758 05:15:06.2 +18:04:31 10.0 0.37 132 PPM 120737 05:14:09.0 +17:51:37 10.8 0.30 132 523752 05:15:13.7 +17:42:40 16.8 132 Positions are for J2000
Event circumstances last updated at 2024/04/23 03:25:02 UT
Marc W. Buie, Southwest Research Institute