Event between (535019) 14WE509 and star GA1000:03562311 with event index number of 2345505
Geocentric closest approach at 2022/12/03 08:10:17 UTC
J2000 position of star is 12:00:06.6 +11:20:22
Equinox of date position of star is 12:01:14.8 +11:12:57
Stellar brightness G=16.0,
use SENSEUP=128 with the MallinCam and and exposure
time of 2 seconds with the QHY174 camera.
Star is 159 degrees from the moon.
Moon is 78% illuminated.
TNO apparent brightness V=22.8
TNO is 33.9 AU from the Sun
and 34.1 AU from the Earth.
The TNO is moving 14.0
km/sec on the sky relative to the star, or,
2.0 arcsec/hr.
The 1-sigma error in the time of the event is 194 seconds.
The 1-sigma cross-track error in the shadow position is
1554 km.
The TNO has an absolute magnitude Hv=7.3
Diameter=207.0 km assuming a 5% albedo -- 14.8 sec chord
Diameter=84.5 km assuming a 30% albedo -- 6.1 sec chord
Dynamical classification is 4:3E
Star training set for 535019, (2022/12/03 08:07UT) Object RA Dec mag sep mel Regulus 10:09:35.4 +11:51:15 1.3 27.36 135 Denebola 11:50:13.7 +14:26:38 2.1 4.21 155 9Omi Vir 12:06:22.6 +08:36:20 4.1 2.89 162 PPM 128719 12:02:24.2 +12:15:00 7.0 1.07 158 PPM 128722 12:02:31.9 +11:11:48 9.6 0.31 159 PPM 128702 12:01:04.1 +11:09:23 11.3 0.08 159 535019 12:01:17.0 +11:12:42 16.0 159 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 535019, (2022/12/03 08:07UT) Object RA Dec mag sep mel Regulus 10:08:21.9 +11:58:02 1.3 27.36 135 Denebola 11:49:02.9 +14:34:17 2.1 4.21 155 9Omi Vir 12:05:12.2 +08:44:00 4.1 2.89 162 PPM 128719 12:01:13.7 +12:22:39 7.0 1.07 158 PPM 128722 12:01:21.4 +11:19:28 9.6 0.31 159 PPM 128702 11:59:53.6 +11:17:02 11.3 0.08 159 535019 12:00:06.6 +11:20:22 16.0 159 Positions are for J2000
Event circumstances last updated at 2022/03/12 01:49:58 UT
Marc W. Buie, Southwest Research Institute