Event between 13TU187 and star GA0960:00248536 with event index number of 2676405
Geocentric closest approach at 2022/10/30 19:35:11 UTC
J2000 position of star is 02:55:41.5 +06:02:42
Equinox of date position of star is 02:56:50.6 +06:07:55
Stellar brightness G=16.5,
use SENSEUP=128 with the MallinCam and and exposure
time of 2 seconds with the QHY174 camera.
Star is 114 degrees from the moon.
Moon is 34% illuminated.
TNO apparent brightness V=22.9
TNO is 33.5 AU from the Sun
and 32.5 AU from the Earth.
The TNO is moving 24.5
km/sec on the sky relative to the star, or,
3.7 arcsec/hr.
The 1-sigma error in the time of the event is 249 seconds.
The 1-sigma cross-track error in the shadow position is
4125 km.
The TNO has an absolute magnitude Hv=7.7
Diameter=141.9 km assuming a 5% albedo -- 7.2 sec chord
Diameter=57.9 km assuming a 30% albedo -- 2.9 sec chord
Dynamical classification is 3:2E
Star training set for 13TU187, (2022/10/30 19:35UT) Object RA Dec mag sep mel Aldebaran 04:37:14.0 +16:33:12 0.8 26.67 140 Menkar 03:03:28.5 +04:10:41 2.5 2.55 114 PPM 146085 02:58:16.5 +04:35:31 6.1 1.58 113 PPM 145993 02:53:26.8 +05:36:02 8.3 1.01 113 PPM 146074 02:57:29.9 +06:05:22 9.3 0.16 114 PPM 146053 02:56:43.2 +06:01:29 10.9 0.12 114 13TU187 02:56:54.0 +06:08:10 16.5 114 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 13TU187, (2022/10/30 19:35UT) Object RA Dec mag sep mel Aldebaran 04:35:55.3 +16:30:29 0.8 26.67 140 Menkar 03:02:16.8 +04:05:21 2.5 2.55 114 PPM 146085 02:57:04.6 +04:30:04 6.1 1.58 113 PPM 145993 02:52:14.6 +05:30:28 8.3 1.01 113 PPM 146074 02:56:17.5 +05:59:54 9.3 0.16 114 PPM 146053 02:55:30.8 +05:56:00 10.9 0.12 114 13TU187 02:55:41.5 +06:02:42 16.5 114 Positions are for J2000
Event circumstances last updated at 2021/10/05 01:13:27 UT
Marc W. Buie, Southwest Research Institute