RECON: TNO occultation with 14JQ80

Event between 14JQ80 and star GA0740:05924997 with event index number of 256256

Geocentric closest approach at 2020/02/02 09:10:01 UTC

J2000 position of star is 16:17:46.3 -15:34:07
Equinox of date position of star is 16:18:49.2 -15:36:46
Stellar brightness G=14.6, use SENSEUP=128
Star is 161 degrees from the moon. Moon is 53% illuminated.
TNO apparent brightness V=22.5

TNO is 32.0 AU from the Sun and 32.3 AU from the Earth.
The TNO is moving 17.6 km/sec on the sky relative to the star, or, 2.7 arcsec/hr.
The 1-sigma error in the time of the event is 554 seconds.
The 1-sigma cross-track error in the shadow position is 5072 km.

The TNO has an absolute magnitude Hv=7.3
Diameter=206.1 km assuming a 5% albedo -- 11.8 sec chord
Diameter=84.1 km assuming a 30% albedo -- 4.8 sec chord
Dynamical classification is 3:2E
 
 
 
 
 
 
 
 

Star training set for 14JQ80, (2020/02/02 09:10UT)
Object            RA         Dec     mag  sep  mel
Antares        16:30:38.5 -26:28:30  0.9 11.20 155
8Bet1Sco       16:06:36.5 -19:51:32  2.6  5.16 163
PPM 231511     16:20:08.6 -14:55:13  5.8  0.76 161
PPM 231466     16:18:29.4 -15:22:35  7.9  0.26 161
PPM 231475     16:19:05.7 -15:36:13  9.7  0.05 161
14JQ80         16:18:54.8 -15:37:00 14.6       161
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 14JQ80, (2020/02/02 09:10UT)
Object            RA         Dec     mag  sep  mel
Antares        16:29:24.4 -26:25:56  0.9 11.20 155
8Bet1Sco       16:05:26.2 -19:48:20  2.6  5.16 163
PPM 231511     16:19:00.4 -14:52:22  5.8  0.76 161
PPM 231466     16:17:21.0 -15:19:41  7.9  0.26 161
PPM 231475     16:17:57.1 -15:33:20  9.7  0.05 161
14JQ80         16:17:46.3 -15:34:07 14.6       161
Positions are for J2000

Event circumstances last updated at 2018/06/12 19:52:15 UT

Marc W. Buie, Southwest Research Institute

RECON