RECON: TNO occultation with 14KD102

Event between 14KD102 and star GA0720:15109157 with event index number of 1050322

Geocentric closest approach at 2020/06/17 02:10:20 UTC

J2000 position of star is 17:47:48.2 -16:21:20
Equinox of date position of star is 17:48:55.5 -16:21:39
Stellar brightness G=15.6, use SENSEUP=128
Star is 131 degrees from the moon. Moon is 17% illuminated.
TNO apparent brightness V=22.2

TNO is 30.8 AU from the Sun and 29.8 AU from the Earth.
The TNO is moving 23.4 km/sec on the sky relative to the star, or, 3.9 arcsec/hr.
The 1-sigma error in the time of the event is 548 seconds.
The 1-sigma cross-track error in the shadow position is 1710 km.

The TNO has an absolute magnitude Hv=7.4
Diameter=200.5 km assuming a 5% albedo -- 8.6 sec chord
Diameter=81.8 km assuming a 30% albedo -- 3.5 sec chord
Dynamical classification is 3:2E
 
 
 
 
 
 
 
 

Star training set for 14KD102, (2020/06/17 02:10UT)
Object            RA         Dec     mag  sep  mel
Antares        16:30:39.9 -26:28:32  0.9 20.81 147
35Eta Oph      17:11:33.2 -15:44:56  2.6  9.01 140
PPM 233599     17:48:46.8 -14:43:55  5.9  1.63 131
PPM 233581     17:47:47.2 -16:00:36  8.4  0.45 132
PPM 233621     17:50:12.0 -16:15:19  8.9  0.31 131
14KD102        17:48:59.1 -16:21:40 15.6       131
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 14KD102, (2020/06/17 02:10UT)
Object            RA         Dec     mag  sep  mel
Antares        16:29:24.4 -26:25:56  0.9 20.81 147
35Eta Oph      17:10:22.7 -15:43:29  2.6  9.01 140
PPM 233599     17:47:36.7 -14:43:33  5.9  1.63 131
PPM 233581     17:46:36.4 -16:00:13  8.4  0.45 132
PPM 233621     17:49:01.1 -16:15:01  8.9  0.31 131
14KD102        17:47:48.2 -16:21:20 15.6       131
Positions are for J2000

Event circumstances last updated at 2019/06/07 23:51:57 UT

Marc W. Buie, Southwest Research Institute

RECON