Event between 09DL143 and star GA0900:04003673 with event index number of 2034346
Geocentric closest approach at 2024/01/14 19:31:58 UTC
J2000 position of star is 13:37:26.7 +01:42:16
Equinox of date position of star is 13:38:35.0 +01:35:28
Stellar brightness G=16.7,
use SENSEUP=128 with the MallinCam and and exposure
time of 2 seconds with the QHY174 camera.
Star is 138 degrees from the moon.
Moon is 15% illuminated.
TNO apparent brightness V=24.1
TNO is 44.7 AU from the Sun
and 44.6 AU from the Earth.
The TNO is moving 6.7
km/sec on the sky relative to the star, or,
0.8 arcsec/hr.
The 1-sigma error in the time of the event is 679 seconds.
The 1-sigma cross-track error in the shadow position is
2402 km.
The TNO has an absolute magnitude Hv=7.5
Diameter=193.2 km assuming a 5% albedo -- 28.6 sec chord
Diameter=78.9 km assuming a 30% albedo -- 11.7 sec chord
Dynamical classification is CLASSICAL
Star training set for 09DL143, (2024/01/14 19:32UT) Object RA Dec mag sep mel Spica 13:26:27.8 -11:17:10 1.0 13.22 136 Vindemiatrix 13:03:22.4 +10:49:50 2.8 12.74 148 78 Vir 13:35:21.1 +03:32:10 4.9 2.12 139 PPM 159933 13:39:44.8 +01:08:00 7.9 0.52 137 PPM 159934 13:39:46.9 +01:20:58 9.1 0.36 137 PPM 159906 13:38:01.8 +01:45:48 10.1 0.24 138 09DL143 13:38:40.2 +01:34:57 16.7 137 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 09DL143, (2024/01/14 19:32UT) Object RA Dec mag sep mel Spica 13:25:11.5 -11:09:41 1.0 13.22 136 Vindemiatrix 13:02:10.2 +10:57:33 2.8 12.74 148 78 Vir 13:34:08.0 +03:39:32 4.9 2.12 139 PPM 159933 13:38:31.2 +01:15:18 7.9 0.52 137 PPM 159934 13:38:33.3 +01:28:16 9.1 0.36 137 PPM 159906 13:36:48.3 +01:53:07 10.1 0.24 138 09DL143 13:37:26.7 +01:42:16 16.7 138 Positions are for J2000
Event circumstances last updated at 2022/05/03 01:49:16 UT
Marc W. Buie, Southwest Research Institute