Event between 10BK118 and star GA0360:16305296 with event index number of 1090078
Geocentric closest approach at 2021/06/08 14:02:02 UTC
J2000 position of star is 14:52:11.7 -52:47:39
Equinox of date position of star is 14:53:42.8 -52:52:50
Stellar brightness G=16.0,
use SENSEUP=128 with the MallinCam and and exposure
time of 2 seconds with the QHY174 camera.
Star is 144 degrees from the moon.
Moon is 3% illuminated.
TNO apparent brightness V=23.3
TNO is 20.0 AU from the Sun
and 19.2 AU from the Earth.
The TNO is moving 33.3
km/sec on the sky relative to the star, or,
8.6 arcsec/hr.
The 1-sigma error in the time of the event is 64 seconds.
The 1-sigma cross-track error in the shadow position is
1466 km.
The TNO has an absolute magnitude Hv=10.2
Diameter=55.2 km assuming a 5% albedo -- 1.7 sec chord
Diameter=22.5 km assuming a 30% albedo -- 0.7 sec chord
Dynamical classification is CENTAURR
Star training set for 10BK118, (2021/06/08 14:02UT) Object RA Dec mag sep mel PPM 360911 14:41:04.4 -60:55:21 0.0 8.22 136 Alp Lup 14:43:22.0 -47:28:44 2.3 5.65 149 PPM 343284 14:57:49.7 -52:53:42 5.5 0.62 144 PPM 343260 14:55:06.0 -53:19:25 7.7 0.49 144 PPM 343250 14:54:28.4 -52:58:03 9.7 0.14 144 PPM 343234 14:53:14.8 -52:59:35 10.2 0.13 144 10BK118 14:53:43.5 -52:52:52 16.0 144 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 10BK118, (2021/06/08 14:02UT) Object RA Dec mag sep mel PPM 360911 14:39:25.4 -60:49:53 0.0 8.22 136 Alp Lup 14:41:55.7 -47:23:18 2.3 5.65 149 PPM 343284 14:56:17.4 -52:48:34 5.5 0.62 144 PPM 343260 14:53:33.6 -53:14:14 7.7 0.49 144 PPM 343250 14:52:56.4 -52:52:51 9.7 0.14 144 PPM 343234 14:51:43.0 -52:54:22 10.2 0.13 144 10BK118 14:52:11.7 -52:47:39 16.0 144 Positions are for J2000
Event circumstances last updated at 2021/04/08 23:40:05 UT
Marc W. Buie, Southwest Research Institute