Event between (524834) 03YL179 and star GA1100:02606578 with event index number of 2218100
Geocentric closest approach at 2026/12/23 23:47:21 UTC
J2000 position of star is 07:02:16.0 +21:41:33
Equinox of date position of star is 07:03:43.7 +21:39:20
Stellar brightness G=16.4,
use SENSEUP=128 with the MallinCam and and exposure
time of 2 seconds with the QHY174 camera.
Star is 14 degrees from the moon.
Moon is 100% illuminated.
Apparent brightness V=23.3
Object is 38.8 AU from the Sun
and 37.8 AU from the Earth.
Apparent velocity is 24.8
km/sec on the sky relative to the star, or,
3.3 arcsec/hr.
The 1-sigma error in the time of the event is 1250 seconds.
The 1-sigma cross-track error in the shadow position is
5418 km.
The object has an absolute magnitude Hv=7.4
Diameter=208.9 km assuming a 5% albedo -- 8.2 sec chord
Diameter=85.3 km assuming a 30% albedo -- 3.4 sec chord
Dynamical classification is CLASSICAL
Star training set for 524834, (2026/12/23 23:47UT) Object RA Dec mag sep mel Pollux 07:46:58.0 +27:57:32 1.1 11.63 22 Alhena 06:39:16.2 +16:22:26 1.9 7.85 13 44 Gem 07:06:55.7 +22:35:41 5.9 1.18 14 PPM 096913 07:03:31.1 +21:59:55 8.2 0.36 14 PPM 096928 07:03:53.6 +21:56:28 9.4 0.29 14 PPM 096937 07:04:21.4 +21:42:34 10.1 0.13 14 524834 07:03:52.7 +21:39:06 16.4 15 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 524834, (2026/12/23 23:47UT) Object RA Dec mag sep mel Pollux 07:45:17.9 +28:01:33 1.1 11.63 22 Alhena 06:37:42.8 +16:23:57 1.9 7.85 13 44 Gem 07:05:18.4 +22:38:15 5.9 1.18 14 PPM 096913 07:01:54.2 +22:02:21 8.2 0.36 14 PPM 096928 07:02:16.7 +21:58:55 9.4 0.29 14 PPM 096937 07:02:44.6 +21:45:02 10.1 0.13 14 524834 07:02:16.0 +21:41:33 16.4 14 Positions are for J2000
Event circumstances last updated at 2024/06/20 21:26:07 UT
Marc W. Buie, Southwest Research Institute