Event between (545293) 11FX62 and star GA0560:08139625 with event index number of 2398278
Geocentric closest approach at 2026/07/07 20:53:37 UTC
J2000 position of star is 15:44:15.2 -33:43:03
Equinox of date position of star is 15:45:45.0 -33:47:24
Stellar brightness G=15.3,
use SENSEUP=128 with the MallinCam and and exposure
time of 2 seconds with the QHY174 camera.
Star is 135 degrees from the moon.
Moon is 49% illuminated.
Apparent brightness V=22.0
Object is 29.2 AU from the Sun
and 28.5 AU from the Earth.
Apparent velocity is 16.5
km/sec on the sky relative to the star, or,
2.9 arcsec/hr.
The 1-sigma error in the time of the event is 147 seconds.
The 1-sigma cross-track error in the shadow position is
1913 km.
The object has an absolute magnitude Hv=7.2
Diameter=219.8 km assuming a 5% albedo -- 13.4 sec chord
Diameter=89.7 km assuming a 30% albedo -- 5.5 sec chord
Dynamical classification is CENTAURR
Star training set for 545293, (2026/07/07 20:55UT) Object RA Dec mag sep mel Antares 16:31:02.3 -26:29:18 0.9 12.17 127 Eta Lup 16:01:53.3 -38:28:11 2.8 5.67 130 PPM 294249 15:48:26.2 -34:45:47 5.8 1.09 134 PPM 294129 15:42:35.8 -33:13:47 8.3 0.90 135 PPM 294212 15:46:35.6 -33:42:10 8.8 0.17 134 PPM 294187 15:45:11.6 -33:47:19 10.2 0.16 135 545293 15:45:56.5 -33:47:58 15.3 134 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 545293, (2026/07/07 20:55UT) Object RA Dec mag sep mel Antares 16:29:24.4 -26:25:56 0.9 12.17 127 Eta Lup 16:00:07.3 -38:23:48 2.8 5.67 130 PPM 294249 15:46:44.1 -34:40:57 5.8 1.09 134 PPM 294129 15:40:55.2 -33:08:45 8.3 0.90 135 PPM 294212 15:44:54.5 -33:37:16 8.8 0.17 134 PPM 294187 15:43:30.4 -33:42:22 10.2 0.16 135 545293 15:44:15.2 -33:43:03 15.3 135 Positions are for J2000
Event circumstances last updated at 2023/07/05 02:59:50 UT
Marc W. Buie, Southwest Research Institute