Event between (535168) 14XU40 and star GA1120:02082313 with event index number of 2260032
Geocentric closest approach at 2027/09/14 18:24:37 UTC
J2000 position of star is 06:23:59.4 +22:03:29
Equinox of date position of star is 06:25:19.1 +22:02:42
Stellar brightness G=16.8,
use SENSEUP=128 with the MallinCam and and exposure
time of 2 seconds with the QHY174 camera.
Star is 117 degrees from the moon.
Moon is 99% illuminated.
TNO apparent brightness V=22.5
TNO is 33.3 AU from the Sun
and 33.5 AU from the Earth.
The TNO is moving 12.4
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 612 seconds.
The 1-sigma cross-track error in the shadow position is
1550 km.
The TNO has an absolute magnitude Hv=7.1
Diameter=229.1 km assuming a 5% albedo -- 18.5 sec chord
Diameter=93.5 km assuming a 30% albedo -- 7.5 sec chord
Dynamical classification is 3:2E
Star training set for 535168, (2027/09/14 18:40UT) Object RA Dec mag sep mel Betelgeuse 05:56:40.3 +07:24:35 0.4 16.21 110 Alhena 06:39:18.7 +16:22:24 1.9 6.52 121 PPM 095944 06:27:14.0 +23:18:34 6.0 1.32 117 PPM 095893 06:25:12.4 +23:04:05 8.4 1.03 117 PPM 095900 06:25:25.6 +22:22:39 9.3 0.34 117 PPM 095908 06:25:47.8 +22:03:18 10.2 0.04 117 535168 06:25:39.5 +22:02:29 16.8 117 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 535168, (2027/09/14 18:40UT) Object RA Dec mag sep mel Betelgeuse 05:55:10.3 +07:24:26 0.4 16.21 110 Alhena 06:37:42.8 +16:23:57 1.9 6.52 121 PPM 095944 06:25:33.0 +23:19:37 6.0 1.32 117 PPM 095893 06:23:31.6 +23:05:04 8.4 1.03 117 PPM 095900 06:23:45.2 +22:23:39 9.3 0.34 117 PPM 095908 06:24:07.7 +22:04:19 10.2 0.04 117 535168 06:23:59.4 +22:03:29 16.8 117 Positions are for J2000
Event circumstances last updated at 2022/01/28 23:47:02 UT
Marc W. Buie, Southwest Research Institute