Event between (612243) 01QR322 and star GA1060:00386409 with event index number of 2811938
Geocentric closest approach at 2027/11/23 13:04:13 UTC
J2000 position of star is 03:30:12.8 +17:35:40
Equinox of date position of star is 03:31:34.4 +17:40:30
Stellar brightness G=16.6,
use SENSEUP=128 with the MallinCam and and exposure
time of 2 seconds with the QHY174 camera.
Star is 129 degrees from the moon.
Moon is 23% illuminated.
Apparent brightness V=22.9
Object is 30.4 AU from the Sun
and 29.4 AU from the Earth.
Apparent velocity is 24.6
km/sec on the sky relative to the star, or,
4.1 arcsec/hr.
The 1-sigma error in the time of the event is 290 seconds.
The 1-sigma cross-track error in the shadow position is
2221 km.
The object has an absolute magnitude Hv=8.1
Diameter=143.2 km assuming a 5% albedo -- 5.9 sec chord
Diameter=58.5 km assuming a 30% albedo -- 2.4 sec chord
Dynamical classification is 1:1
Star training set for 612243, (2027/11/23 12:58UT) Object RA Dec mag sep mel Aldebaran 04:37:31.5 +16:33:48 0.8 15.74 113 Menkar 03:03:44.5 +04:11:51 2.5 15.14 136 PPM 119253 03:41:00.7 +16:37:31 6.2 2.44 127 PPM 119148 03:32:56.5 +18:01:54 8.3 0.44 128 PPM 119147 03:32:50.6 +17:38:13 9.7 0.25 128 PPM 119124 03:31:36.0 +17:40:42 10.3 0.05 129 612243 03:31:48.0 +17:41:18 16.6 128 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 612243, (2027/11/23 12:58UT) Object RA Dec mag sep mel Aldebaran 04:35:55.3 +16:30:29 0.8 15.74 113 Menkar 03:02:16.8 +04:05:21 2.5 15.14 136 PPM 119253 03:39:25.8 +16:32:11 6.2 2.44 127 PPM 119148 03:31:21.1 +17:56:18 8.3 0.44 128 PPM 119147 03:31:15.4 +17:32:37 9.7 0.25 128 PPM 119124 03:30:00.8 +17:35:04 10.3 0.05 129 612243 03:30:12.8 +17:35:40 16.6 129 Positions are for J2000
Event circumstances last updated at 2023/11/28 04:18:30 UT
Marc W. Buie, Southwest Research Institute