RECON: TNO occultation with 15KN173

Event between 15KN173 and star GA0720:05952317 with event index number of 1012588

Geocentric closest approach at 2019/05/04 01:25:45 UTC

J2000 position of star is 16:12:17.2 -16:52:14
Equinox of date position of star is 16:13:22.9 -16:55:07
Stellar brightness G=12.4, use SENSEUP=16
Star is 149 degrees from the moon. Moon is 1% illuminated.
TNO apparent brightness V=23.5

TNO is 31.9 AU from the Sun and 31.0 AU from the Earth.
The TNO is moving 21.7 km/sec on the sky relative to the star, or, 3.5 arcsec/hr.
The 1-sigma error in the time of the event is 484 seconds.
The 1-sigma cross-track error in the shadow position is 5680 km.

The TNO has an absolute magnitude Hv=8.4
Diameter=124.7 km assuming a 5% albedo -- 5.8 sec chord
Diameter=50.9 km assuming a 30% albedo -- 2.4 sec chord
Dynamical classification is 3:2E
 
 
 
 
 
 
 
 

Star training set for 15KN173, (2019/05/04 01:26UT)
Object            RA         Dec     mag  sep  mel
Antares        16:30:35.8 -26:28:24  0.9 10.35 142
8Bet1Sco       16:06:33.9 -19:51:25  2.6  3.35 149
PPM 231413     16:15:46.4 -18:35:02  6.1  1.76 148
PPM 231403     16:15:22.6 -16:35:19  8.3  0.58 148
PPM 231338     16:13:07.8 -16:51:18  9.1  0.09 149
15KN173        16:13:23.7 -16:55:09 12.4       148
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 15KN173, (2019/05/04 01:26UT)
Object            RA         Dec     mag  sep  mel
Antares        16:29:24.4 -26:25:56  0.9 10.35 142
8Bet1Sco       16:05:26.2 -19:48:20  2.6  3.35 149
PPM 231413     16:14:39.1 -18:32:11  6.1  1.76 148
PPM 231403     16:14:16.3 -16:32:27  8.3  0.58 148
PPM 231338     16:12:01.4 -16:48:23  9.1  0.09 149
15KN173        16:12:17.2 -16:52:14 12.4       149
Positions are for J2000

Event circumstances last updated at 2019/02/12 07:34:44 UT

Marc W. Buie, Southwest Research Institute

RECON