Event between (523601) 03UY413 and star GA1200:00338219 with event index number of 2626854
Geocentric closest approach at 2024/09/29 23:21:07 UTC
J2000 position of star is 02:03:42.0 +31:54:27
Equinox of date position of star is 02:05:06.0 +32:01:18
Stellar brightness G=14.7,
use SENSEUP=128 with the MallinCam and and exposure
time of 2 seconds with the QHY174 camera.
Star is 115 degrees from the moon.
Moon is 7% illuminated.
Apparent brightness V=21.8
Object is 42.8 AU from the Sun
and 42.0 AU from the Earth.
Apparent velocity is 21.4
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 86 seconds.
The 1-sigma cross-track error in the shadow position is
1661 km.
The object has an absolute magnitude Hv=5.4
Diameter=483.1 km assuming a 5% albedo -- 23.5 sec chord
Diameter=197.2 km assuming a 30% albedo -- 9.6 sec chord
Dynamical classification is SCATNEAR
Star training set for 523601, (2024/09/29 23:22UT) Object RA Dec mag sep mel Aldebaran 04:37:20.6 +16:33:26 0.8 37.71 87 Hamal 02:08:34.4 +23:34:42 2.0 8.48 118 3Eps Tri 02:04:25.1 +33:24:09 5.5 1.39 114 PPM 066820 01:59:29.7 +31:15:14 8.2 1.43 116 PPM 066898 02:03:52.8 +31:40:47 9.7 0.44 115 PPM 066918 02:05:03.5 +32:00:24 10.1 0.03 114 523601 02:05:08.7 +32:01:32 14.7 114 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 523601, (2024/09/29 23:22UT) Object RA Dec mag sep mel Aldebaran 04:35:55.3 +16:30:29 0.8 37.71 87 Hamal 02:07:10.7 +23:27:41 2.0 8.48 118 3Eps Tri 02:02:57.8 +33:17:04 5.5 1.39 114 PPM 066820 01:58:03.7 +31:08:03 8.2 1.43 116 PPM 066898 02:02:26.3 +31:33:41 9.7 0.44 115 PPM 066918 02:03:36.7 +31:53:20 10.1 0.03 114 523601 02:03:42.0 +31:54:27 14.7 114 Positions are for J2000
Event circumstances last updated at 2023/12/22 05:48:36 UT
Marc W. Buie, Southwest Research Institute