RECON: TNO occultation with 11HF103

Event between 11HF103 and star UC4-349-167914 with event index number of 202052

Geocentric closest approach at 2018/03/17 15:12:21 UTC

J2000 position of star is 19:08:41.3 -20:14:49
Equinox of date position of star is 19:09:43.6 -20:13:04
Stellar brightness R=13.9, use SENSEUP=64
Star is 72 degrees from the moon. Moon is 0% illuminated.
TNO apparent brightness V=24.9

TNO is 43.1 AU from the Sun and 43.4 AU from the Earth.
The TNO is moving 14.9 km/sec on the sky relative to the star, or, 1.7 arcsec/hr.
The 1-sigma error in the time of the event is 1159 seconds.
The 1-sigma cross-track error in the shadow position is 4727 km.

The TNO has an absolute magnitude Hv=8.4
Diameter=123.0 km assuming a 5% albedo -- 8.2 sec chord
Diameter=50.2 km assuming a 30% albedo -- 3.4 sec chord
Dynamical classification is CLASSICAL
 
 
 
 
 
 
 
 

Star training set for 11HF103, (2018/03/17 15:12UT)
Object            RA         Dec     mag  sep  mel
Antares        16:30:31.6 -26:28:15  0.9 36.94 108
Nunki          18:56:23.6 -26:16:21  2.0  6.79  75
PPM 235581     19:10:52.5 -19:46:24  6.4  0.51  72
PPM 269374     19:10:05.9 -19:58:18  8.4  0.26  72
PPM 269376     19:10:09.6 -20:09:07  9.4  0.11  72
11HF103        19:09:45.8 -20:13:00 13.9        72
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 11HF103, (2018/03/17 15:12UT)
Object            RA         Dec     mag  sep  mel
Antares        16:29:24.4 -26:25:56  0.9 36.94 108
Nunki          18:55:15.9 -26:17:49  2.0  6.79  75
PPM 235581     19:09:48.2 -19:48:15  6.4  0.51  72
PPM 269374     19:09:01.5 -20:00:07  8.4  0.26  72
PPM 269376     19:09:05.1 -20:10:56  9.4  0.11  72
11HF103        19:08:41.3 -20:14:49 13.9        72
Positions are for J2000

Event circumstances last updated at 2017/08/01 16:35:04 UT

Marc W. Buie, Southwest Research Institute

RECON