Event between 10WM75 and star GA0940:01069471 with event index number of 2109482
Geocentric closest approach at 2024/02/11 16:15:22 UTC
J2000 position of star is 06:02:04.0 +05:53:36
Equinox of date position of star is 06:03:14.3 +05:53:31
Stellar brightness G=13.8,
use SENSEUP=64 with the MallinCam and and exposure
time of 1 seconds with the QHY174 camera.
Star is 102 degrees from the moon.
Moon is 5% illuminated.
TNO apparent brightness V=22.5
TNO is 43.2 AU from the Sun
and 42.6 AU from the Earth.
The TNO is moving 15.5
km/sec on the sky relative to the star, or,
1.8 arcsec/hr.
The 1-sigma error in the time of the event is 317 seconds.
The 1-sigma cross-track error in the shadow position is
2431 km.
The TNO has an absolute magnitude Hv=6.0
Diameter=373.3 km assuming a 5% albedo -- 24.3 sec chord
Diameter=152.4 km assuming a 30% albedo -- 9.9 sec chord
Dynamical classification is SCATEXTD
Star training set for 10WM75, (2024/02/11 16:09UT) Object RA Dec mag sep mel Betelgeuse 05:56:28.7 +07:24:34 0.4 2.29 101 Bellatrix 05:26:25.5 +06:22:10 1.6 9.19 93 63 Ori 06:06:15.4 +05:25:00 6.4 0.86 103 PPM 149763 06:02:01.1 +05:48:07 8.4 0.35 102 PPM 149820 06:04:24.8 +05:43:34 9.4 0.31 103 PPM 149817 06:04:10.9 +05:43:13 11.2 0.27 103 10WM75 06:03:21.5 +05:53:30 13.8 103 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 10WM75, (2024/02/11 16:09UT) Object RA Dec mag sep mel Betelgeuse 05:55:10.3 +07:24:26 0.4 2.29 101 Bellatrix 05:25:07.8 +06:20:58 1.6 9.19 93 63 Ori 06:04:58.1 +05:25:12 6.4 0.86 103 PPM 149763 06:00:43.7 +05:48:10 8.4 0.35 102 PPM 149820 06:03:07.5 +05:43:42 9.4 0.31 103 PPM 149817 06:02:53.6 +05:43:21 11.2 0.27 103 10WM75 06:02:04.0 +05:53:36 13.8 102 Positions are for J2000
Event circumstances last updated at 2021/11/16 00:48:38 UT
Marc W. Buie, Southwest Research Institute