RECON: TNO occultation with 14GK54

Event between 14GK54 and star GA0700:06122697 with event index number of 1046691

Geocentric closest approach at 2020/02/08 02:53:17 UTC

J2000 position of star is 16:02:22.9 -18:02:13
Equinox of date position of star is 16:03:30.1 -18:05:24
Stellar brightness G=15.8, use SENSEUP=128
Star is 120 degrees from the moon. Moon is 98% illuminated.
TNO apparent brightness V=22.7

TNO is 26.6 AU from the Sun and 26.8 AU from the Earth.
The TNO is moving 14.1 km/sec on the sky relative to the star, or, 2.6 arcsec/hr.
The 1-sigma error in the time of the event is 322 seconds.
The 1-sigma cross-track error in the shadow position is 1365 km.

The TNO has an absolute magnitude Hv=8.2
Diameter=140.0 km assuming a 5% albedo -- 10.0 sec chord
Diameter=57.1 km assuming a 30% albedo -- 4.1 sec chord
Dynamical classification is 3:2E
 
 
 
 
 
 
 
 

Star training set for 14GK54, (2020/02/08 02:53UT)
Object            RA         Dec     mag  sep  mel
Antares        16:30:38.6 -26:28:30  0.9 10.46 127
8Bet1Sco       16:06:36.6 -19:51:32  2.6  1.91 121
49 Lib         16:01:27.5 -16:35:28  5.5  1.58 119
PPM 231132     16:04:27.5 -18:19:25  7.9  0.32 120
PPM 231113     16:03:48.0 -18:13:35  8.9  0.15 120
14GK54         16:03:32.4 -18:05:30 15.8       120
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 14GK54, (2020/02/08 02:53UT)
Object            RA         Dec     mag  sep  mel
Antares        16:29:24.4 -26:25:56  0.9 10.46 127
8Bet1Sco       16:05:26.2 -19:48:20  2.6  1.91 121
49 Lib         16:00:18.7 -16:32:08  5.5  1.58 119
PPM 231132     16:03:17.9 -18:16:09  7.9  0.32 120
PPM 231113     16:02:38.5 -18:10:18  8.9  0.15 120
14GK54         16:02:22.9 -18:02:13 15.8       119
Positions are for J2000

Event circumstances last updated at 2019/06/07 23:15:06 UT

Marc W. Buie, Southwest Research Institute

RECON