RECON: TNO occultation with 330836

Event between (330836) Orius and star GA0520:31060281 with event index number of 155583

Geocentric closest approach at 2018/10/26 17:28:22 UTC

J2000 position of star is 18:26:45.3 -36:28:40
Equinox of date position of star is 18:28:01.5 -36:27:55
Stellar brightness G=16.9, use SENSEUP=128
Star is 139 degrees from the moon. Moon is 95% illuminated.
TNO apparent brightness V=22.7

TNO is 17.6 AU from the Sun and 18.0 AU from the Earth.
The TNO is moving 21.8 km/sec on the sky relative to the star, or, 6.0 arcsec/hr.
The 1-sigma error in the time of the event is 528 seconds.
The 1-sigma cross-track error in the shadow position is 4445 km.

The TNO has an absolute magnitude Hv=9.9
Diameter=63.1 km assuming a 5% albedo -- 2.9 sec chord
Diameter=25.8 km assuming a 30% albedo -- 1.2 sec chord
Dynamical classification is CENTAURR
 
 
 
 
 
 
 
 

Star training set for 330836, (2018/10/26 17:28UT)
Object            RA         Dec     mag  sep  mel
Antares        16:30:33.9 -26:28:20  0.9 26.83 166
Kap Sco        17:43:47.5 -39:02:16  2.4  9.11 146
PPM 297683     18:26:37.6 -35:58:48  5.9  0.56 140
PPM 297748     18:29:03.2 -36:28:21  8.4  0.21 139
PPM 297712     18:27:40.4 -36:18:14  9.4  0.18 140
330836         18:28:01.6 -36:27:55 16.9       139
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 330836, (2018/10/26 17:28UT)
Object            RA         Dec     mag  sep  mel
Antares        16:29:24.4 -26:25:56  0.9 26.83 166
Kap Sco        17:42:29.3 -39:01:49  2.4  9.11 146
PPM 297683     18:25:21.6 -35:59:31  5.9  0.56 140
PPM 297748     18:27:46.9 -36:29:08  8.4  0.21 139
PPM 297712     18:26:24.1 -36:18:58  9.4  0.18 140
330836         18:26:45.3 -36:28:40 16.9       139
Positions are for J2000

Event circumstances last updated at 2018/10/23 20:41:35 UT

Marc W. Buie, Southwest Research Institute

RECON