RECON: TNO occultation with 11JY31

Event between 11JY31 and star UC4-349-168014 with event index number of 203192

Geocentric closest approach at 2018/06/21 23:42:07 UTC

J2000 position of star is 19:08:56.0 -20:18:44
Equinox of date position of star is 19:09:59.5 -20:16:57
Stellar brightness R=15.8, use SENSEUP=128
Star is 87 degrees from the moon. Moon is 66% illuminated.
TNO apparent brightness V=25.1

TNO is 42.4 AU from the Sun and 41.5 AU from the Earth.
The TNO is moving 23.5 km/sec on the sky relative to the star, or, 2.8 arcsec/hr.
The 1-sigma error in the time of the event is 599 seconds.
The 1-sigma cross-track error in the shadow position is 2281 km.

The TNO has an absolute magnitude Hv=8.8
Diameter=103.8 km assuming a 5% albedo -- 4.4 sec chord
Diameter=42.4 km assuming a 30% albedo -- 1.8 sec chord
Dynamical classification is CLASSICAL
 
 
 
 
 
 
 
 

Star training set for 11JY31, (2018/06/21 23:42UT)
Object            RA         Dec     mag  sep  mel
Antares        16:30:32.6 -26:28:17  0.9 36.97  51
Nunki          18:56:24.6 -26:16:20  2.0  6.76  83
PPM 235581     19:10:53.5 -19:46:23  6.4  0.55  87
PPM 269374     19:10:06.8 -19:58:17  8.4  0.31  87
PPM 269376     19:10:10.5 -20:09:05  9.4  0.13  87
11JY31         19:10:01.5 -20:16:54 15.8        87
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 11JY31, (2018/06/21 23:42UT)
Object            RA         Dec     mag  sep  mel
Antares        16:29:24.4 -26:25:56  0.9 36.97  51
Nunki          18:55:15.9 -26:17:49  2.0  6.76  83
PPM 235581     19:09:48.2 -19:48:15  6.4  0.55  87
PPM 269374     19:09:01.5 -20:00:07  8.4  0.31  87
PPM 269376     19:09:05.1 -20:10:56  9.4  0.13  87
11JY31         19:08:56.0 -20:18:44 15.8        86
Positions are for J2000

Event circumstances last updated at 2017/12/04 18:46:31 UT

Marc W. Buie, Southwest Research Institute

RECON