RECON: TNO occultation with 04TF282

Event between 04TF282 and star GA1020:00742974 with event index number of 1189639

Geocentric closest approach at 2022/12/22 12:57:08 UTC

J2000 position of star is 05:16:50.2 +12:41:48
Equinox of date position of star is 05:18:05.0 +12:43:10
Stellar brightness G=14.6, use SENSEUP=128 with the MallinCam and and exposure time of 2 seconds with the QHY174 camera.
Star is 167 degrees from the moon. Moon is 1% illuminated.
TNO apparent brightness V=22.4

TNO is 42.0 AU from the Sun and 41.1 AU from the Earth.
The TNO is moving 24.6 km/sec on the sky relative to the star, or, 3.0 arcsec/hr.
The 1-sigma error in the time of the event is 206 seconds.
The 1-sigma cross-track error in the shadow position is 2211 km.

The TNO has an absolute magnitude Hv=6.2
Diameter=346.7 km assuming a 5% albedo -- 14.1 sec chord
Diameter=141.6 km assuming a 30% albedo -- 5.8 sec chord
Dynamical classification is SCATNEAR
 
 
 
 
 
 
 
 

Star training set for 04TF282, (2022/12/22 12:57UT)
Object            RA         Dec     mag  sep  mel
Aldebaran      04:37:14.5 +16:33:13  0.8 10.60 168
Bellatrix      05:26:21.9 +06:22:07  1.6  6.67 160
18 Ori         05:17:20.8 +11:21:55  5.6  1.37 165
PPM 120787     05:18:22.8 +12:35:20  7.7  0.15 166
04TF282        05:18:07.7 +12:43:13 14.6       167
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 04TF282, (2022/12/22 12:57UT)
Object            RA         Dec     mag  sep  mel
Aldebaran      04:35:55.3 +16:30:29  0.8 10.60 168
Bellatrix      05:25:07.8 +06:20:58  1.6  6.67 160
18 Ori         05:16:04.1 +11:20:29  5.6  1.37 165
PPM 120787     05:17:05.5 +12:33:56  7.7  0.15 166
04TF282        05:16:50.2 +12:41:48 14.6       167
Positions are for J2000

Event circumstances last updated at 2022/03/13 02:19:00 UT

Marc W. Buie, Southwest Research Institute

RECON