Event between (576257) 12JD68 and star GA0960:07017802 with event index number of 2529261
Geocentric closest approach at 2028/05/27 19:15:08 UTC
J2000 position of star is 18:25:10.5 +06:40:31
Equinox of date position of star is 18:26:15.1 +06:41:21
Stellar brightness G=14.9,
use SENSEUP=128 with the MallinCam and and exposure
time of 2 seconds with the QHY174 camera.
Star is 147 degrees from the moon.
Moon is 14% illuminated.
TNO apparent brightness V=22.8
TNO is 28.2 AU from the Sun
and 27.4 AU from the Earth.
The TNO is moving 20.2
km/sec on the sky relative to the star, or,
3.7 arcsec/hr.
The 1-sigma error in the time of the event is 359 seconds.
The 1-sigma cross-track error in the shadow position is
2503 km.
The TNO has an absolute magnitude Hv=8.2
Diameter=138.0 km assuming a 5% albedo -- 6.8 sec chord
Diameter=56.4 km assuming a 30% albedo -- 2.8 sec chord
Dynamical classification is 3:2E+6:4II
Star training set for 576257, (2028/05/27 19:15UT) Object RA Dec mag sep mel Vega 18:37:54.0 +38:48:40 0.0 32.22 118 60Bet Oph 17:44:52.6 +04:33:26 2.8 10.59 143 PPM 165790 18:27:00.8 +08:03:00 5.6 1.36 146 PPM 165794 18:27:12.8 +07:07:13 8.5 0.46 147 PPM 165773 18:26:28.9 +06:48:09 9.2 0.11 147 PPM 165787 18:26:57.9 +06:40:30 10.3 0.10 147 576257 18:26:33.4 +06:41:35 14.9 147 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 576257, (2028/05/27 19:15UT) Object RA Dec mag sep mel Vega 18:36:56.7 +38:47:07 0.0 32.22 118 60Bet Oph 17:43:28.3 +04:34:06 2.8 10.59 143 PPM 165790 18:25:38.8 +08:01:55 5.6 1.36 146 PPM 165794 18:25:50.1 +07:06:07 8.5 0.46 147 PPM 165773 18:25:06.0 +06:47:05 9.2 0.11 147 PPM 165787 18:25:34.9 +06:39:25 10.3 0.10 147 576257 18:25:10.5 +06:40:31 14.9 147 Positions are for J2000
Event circumstances last updated at 2022/02/13 02:37:06 UT
Marc W. Buie, Southwest Research Institute