RECON: TNO occultation with 14HX199

Event between 14HX199 and star GA0800:05029313 with event index number of 249371

Geocentric closest approach at 2020/02/12 22:38:41 UTC

J2000 position of star is 16:07:58.4 -09:24:15
Equinox of date position of star is 16:08:59.6 -09:27:11
Stellar brightness G=13.1, use SENSEUP=32
Star is 47 degrees from the moon. Moon is 82% illuminated.
TNO apparent brightness V=22.2

TNO is 30.6 AU from the Sun and 30.8 AU from the Earth.
The TNO is moving 11.7 km/sec on the sky relative to the star, or, 1.9 arcsec/hr.
The 1-sigma error in the time of the event is 353 seconds.
The 1-sigma cross-track error in the shadow position is 2314 km.

The TNO has an absolute magnitude Hv=7.1
Diameter=238.8 km assuming a 5% albedo -- 19.7 sec chord
Diameter=97.5 km assuming a 30% albedo -- 8.0 sec chord
Dynamical classification is 3:2E
 
 
 
 
 
 
 
 

Star training set for 14HX199, (2020/02/12 22:39UT)
Object            RA         Dec     mag  sep  mel
Antares        16:30:38.6 -26:28:30  0.9 17.77  56
1Del Oph       16:15:24.1 -03:44:41  2.7  5.92  49
15Psi Sco      16:13:06.1 -10:06:54  4.9  1.19  49
PPM 199342     16:10:08.0 -09:41:59  7.9  0.36  48
PPM 199322     16:08:44.8 -09:22:42  9.5  0.11  47
14HX199        16:09:04.2 -09:27:24 13.1        48
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 14HX199, (2020/02/12 22:39UT)
Object            RA         Dec     mag  sep  mel
Antares        16:29:24.4 -26:25:56  0.9 17.77  56
1Del Oph       16:14:20.7 -03:41:42  2.7  5.92  49
15Psi Sco      16:12:00.0 -10:03:51  4.9  1.19  49
PPM 199342     16:09:02.1 -09:38:53  7.9  0.36  48
PPM 199322     16:07:39.1 -09:19:33  9.5  0.11  47
14HX199        16:07:58.4 -09:24:15 13.1        47
Positions are for J2000

Event circumstances last updated at 2018/09/21 17:54:50 UT

Marc W. Buie, Southwest Research Institute

RECON