RECON: TNO occultation with 281371

Event between (281371) 08FC76 and star UC4-523-013266 with event index number of 165828

Geocentric closest approach at 2018/12/06 17:59:00 UTC

J2000 position of star is 05:27:35.9 +14:33:27
Equinox of date position of star is 05:28:35.4 +14:34:16
Stellar brightness R=16.4, use SENSEUP=128
Star is 165 degrees from the moon. Moon is 0% illuminated.
TNO apparent brightness V=19.8

TNO is 11.3 AU from the Sun and 10.4 AU from the Earth.
The TNO is moving 21.9 km/sec on the sky relative to the star, or, 10.5 arcsec/hr.
The 1-sigma error in the time of the event is 39 seconds.
The 1-sigma cross-track error in the shadow position is 529 km.

The TNO has an absolute magnitude Hv=9.3
Diameter=83.2 km assuming a 5% albedo -- 3.8 sec chord
Diameter=34.0 km assuming a 30% albedo -- 1.5 sec chord
Dynamical classification is CENTAURR
 
 
 
 
 
 
 
 

Star training set for 281371, (2018/12/06 17:59UT)
Object            RA         Dec     mag  sep  mel
Betelgeuse     05:56:11.8 +07:24:33  0.4  9.84 156
Bellatrix      05:26:08.8 +06:21:55  1.6  8.23 162
PPM 120962     05:28:18.9 +15:16:21  6.1  0.71 166
PPM 120966     05:28:26.2 +14:02:38  8.0  0.53 165
PPM 120952     05:27:26.5 +14:24:56  9.6  0.34 166
281371         05:28:40.7 +14:34:20 16.4       165
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 281371, (2018/12/06 17:59UT)
Object            RA         Dec     mag  sep  mel
Betelgeuse     05:55:10.3 +07:24:26  0.4  9.84 156
Bellatrix      05:25:07.8 +06:20:58  1.6  8.23 162
PPM 120962     05:27:13.9 +15:15:27  6.1  0.71 166
PPM 120966     05:27:21.7 +14:01:45  8.0  0.53 165
PPM 120952     05:26:21.8 +14:24:01  9.6  0.34 166
281371         05:27:35.9 +14:33:27 16.4       165
Positions are for J2000

Event circumstances last updated at 2017/05/19 18:07:47 UT

Marc W. Buie, Southwest Research Institute

RECON