Event between 14JQ92 and star GA0880:08085034 with event index number of 2491315
Geocentric closest approach at 2024/04/23 20:50:57 UTC
J2000 position of star is 18:26:56.8 -00:45:13
Equinox of date position of star is 18:28:07.3 -00:44:19
Stellar brightness G=16.3,
use SENSEUP=128 with the MallinCam and and exposure
time of 2 seconds with the QHY174 camera.
Star is 67 degrees from the moon.
Moon is 100% illuminated.
TNO apparent brightness V=23.0
TNO is 27.6 AU from the Sun
and 27.2 AU from the Earth.
The TNO is moving 11.2
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 225 seconds.
The 1-sigma cross-track error in the shadow position is
2569 km.
The TNO has an absolute magnitude Hv=8.4
Diameter=127.6 km assuming a 5% albedo -- 11.4 sec chord
Diameter=52.1 km assuming a 30% albedo -- 4.7 sec chord
Dynamical classification is 3:2E+6:4II
Star training set for 14JQ92, (2024/04/23 21:04UT) Object RA Dec mag sep mel Antares 16:30:54.1 -26:29:02 0.9 38.18 37 60Bet Oph 17:44:40.5 +04:33:32 2.8 12.09 58 59 Ser 18:28:27.2 +00:12:45 5.6 0.95 67 PPM 180318 18:25:38.8 -01:03:00 8.5 0.71 66 PPM 180338 18:29:10.1 -01:04:36 8.7 0.42 67 PPM 180331 18:27:25.6 -00:30:28 10.2 0.30 67 14JQ92 18:28:12.0 -00:44:15 16.3 67 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 14JQ92, (2024/04/23 21:04UT) Object RA Dec mag sep mel Antares 16:29:24.4 -26:25:56 0.9 38.18 37 60Bet Oph 17:43:28.3 +04:34:06 2.8 12.09 58 59 Ser 18:27:12.5 +00:11:46 5.6 0.95 67 PPM 180318 18:24:23.4 -01:03:53 8.5 0.71 66 PPM 180338 18:27:54.7 -01:05:37 8.7 0.42 67 PPM 180331 18:26:10.5 -00:31:25 10.2 0.30 67 14JQ92 18:26:56.8 -00:45:13 16.3 67 Positions are for J2000
Event circumstances last updated at 2022/10/11 04:28:02 UT
Marc W. Buie, Southwest Research Institute