RECON: TNO occultation with 308460

Event between (308460) 05SC278 and star GA1020:00178391 with event index number of 2185897

Geocentric closest approach at 2022/12/18 17:40:11 UTC

J2000 position of star is 01:56:32.5 +12:04:07
Equinox of date position of star is 01:57:45.7 +12:10:45
Stellar brightness G=12.3, use SENSEUP=16 with the MallinCam and and exposure time of 250 milli-seconds with the QHY174 camera.
Star is 173 degrees from the moon. Moon is 27% illuminated.
TNO apparent brightness V=22.6

TNO is 33.1 AU from the Sun and 32.6 AU from the Earth.
The TNO is moving 11.9 km/sec on the sky relative to the star, or, 1.8 arcsec/hr.
The 1-sigma error in the time of the event is 164 seconds.
The 1-sigma cross-track error in the shadow position is 1340 km.

The TNO has an absolute magnitude Hv=7.3
Diameter=208.9 km assuming a 5% albedo -- 17.4 sec chord
Diameter=85.3 km assuming a 30% albedo -- 7.1 sec chord
Dynamical classification is 5:4E
 
 
 
 
 
 
 
 

Star training set for 308460, (2022/12/18 17:40UT)
Object            RA         Dec     mag  sep  mel
Aldebaran      04:37:14.5 +16:33:13  0.8 38.81 135
6Bet Ari       01:55:54.8 +20:55:10  2.6  8.75 166
PPM 117850     02:00:39.9 +12:24:19  6.1  0.74 172
PPM 117791     01:57:17.6 +12:24:03  8.5  0.25 173
308460         01:57:46.4 +12:10:49 12.3       173
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 308460, (2022/12/18 17:40UT)
Object            RA         Dec     mag  sep  mel
Aldebaran      04:35:55.3 +16:30:29  0.8 38.81 135
6Bet Ari       01:54:38.5 +20:48:26  2.6  8.75 166
PPM 117850     01:59:25.9 +12:17:40  6.1  0.74 172
PPM 117791     01:56:03.7 +12:17:21  8.5  0.25 173
308460         01:56:32.5 +12:04:07 12.3       173
Positions are for J2000

Event circumstances last updated at 2022/10/02 04:11:35 UT

Marc W. Buie, Southwest Research Institute

RECON