Event between 10XE91 and star GA0980:01620085 with event index number of 2110115
Geocentric closest approach at 2022/11/02 04:35:08 UTC
J2000 position of star is 06:19:44.4 +08:41:33
Equinox of date position of star is 06:20:58.9 +08:40:52
Stellar brightness G=16.0,
use SENSEUP=128 with the MallinCam and and exposure
time of 2 seconds with the QHY174 camera.
Star is 130 degrees from the moon.
Moon is 60% illuminated.
TNO apparent brightness V=22.9
TNO is 40.5 AU from the Sun
and 40.0 AU from the Earth.
The TNO is moving 13.3
km/sec on the sky relative to the star, or,
1.7 arcsec/hr.
The 1-sigma error in the time of the event is 278 seconds.
The 1-sigma cross-track error in the shadow position is
2134 km.
The TNO has an absolute magnitude Hv=6.7
Diameter=280.6 km assuming a 5% albedo -- 21.1 sec chord
Diameter=114.5 km assuming a 30% albedo -- 8.6 sec chord
Dynamical classification is SCATNEAR
Star training set for 10XE91, (2022/11/02 04:35UT) Object RA Dec mag sep mel Betelgeuse 05:56:24.5 +07:24:34 0.4 6.22 123 Alhena 06:39:01.9 +16:22:40 1.9 8.87 136 PPM 150426 06:25:17.2 +08:52:17 6.2 1.08 131 PPM 150265 06:19:55.4 +09:02:10 7.0 0.44 129 PPM 150284 06:20:45.5 +09:00:24 8.7 0.33 130 PPM 150297 06:21:14.4 +08:38:29 10.4 0.07 130 10XE91 06:20:59.2 +08:40:52 16.0 130 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 10XE91, (2022/11/02 04:35UT) Object RA Dec mag sep mel Betelgeuse 05:55:10.3 +07:24:26 0.4 6.22 123 Alhena 06:37:42.8 +16:23:57 1.9 8.87 136 PPM 150426 06:24:02.3 +08:53:06 6.2 1.08 131 PPM 150265 06:18:40.3 +09:02:49 7.0 0.44 129 PPM 150284 06:19:30.5 +09:01:04 8.7 0.33 130 PPM 150297 06:19:59.5 +08:39:10 10.4 0.07 130 10XE91 06:19:44.4 +08:41:33 16.0 130 Positions are for J2000
Event circumstances last updated at 2022/10/01 04:16:00 UT
Marc W. Buie, Southwest Research Institute