RECON: TNO occultation with 330836

Event between (330836) Orius and star UC4-270-134054 with event index number of 68495

Geocentric closest approach at 2017/08/13 05:48:54 UTC

J2000 position of star is 17:57:46.5 -36:04:46
Equinox of date position of star is 17:58:56.8 -36:04:48
Stellar brightness R=14.6, use SENSEUP=128
Star is 116 degrees from the moon. Moon is 70% illuminated.
TNO apparent brightness V=22.3

TNO is 16.8 AU from the Sun and 16.2 AU from the Earth.
The TNO is moving 11.4 km/sec on the sky relative to the star, or, 3.5 arcsec/hr.
The 1-sigma error in the time of the event is 812 seconds.
The 1-sigma cross-track error in the shadow position is 4769 km.

The TNO has an absolute magnitude Hv=9.9
Diameter=63.1 km assuming a 5% albedo -- 5.5 sec chord
Diameter=25.8 km assuming a 30% albedo -- 2.3 sec chord
Dynamical classification is CENTAURR
 
 
 
 
 
 
 
 

Star training set for 330836, (2017/08/13 05:49UT)
Object            RA         Dec     mag  sep  mel
Antares        16:30:29.4 -26:28:11  0.9 21.14 136
Kap Sco        17:43:42.5 -39:02:15  2.4  4.23 118
PPM 296992     17:56:19.6 -36:28:39  6.3  0.66 116
PPM 297105     18:01:15.5 -35:55:39  7.7  0.49 115
PPM 297042     17:58:10.2 -36:16:25  8.7  0.25 116
330836         17:58:57.8 -36:04:48 14.6       115
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, (2017/08/13 05:49UT)
Object            RA         Dec     mag  sep  mel
Antares        16:29:24.4 -26:25:56  0.9 21.14 136
Kap Sco        17:42:29.3 -39:01:49  2.4  4.23 118
PPM 296992     17:55:08.1 -36:28:32  6.3  0.66 116
PPM 297105     18:00:04.3 -35:55:40  7.7  0.49 115
PPM 297042     17:56:58.8 -36:16:22  8.7  0.25 116
330836         17:57:46.5 -36:04:46 14.6       116
Positions are for J2000

Event circumstances last updated at 2017/05/16 18:31:29 UT

Marc W. Buie, Southwest Research Institute

RECON