RECON: TNO occultation with 13VO46

Event between 13VO46 and star GA0980:00307403 with event index number of 2676793

Geocentric closest approach at 2023/07/24 15:38:50 UTC

J2000 position of star is 03:32:19.2 +08:10:28
Equinox of date position of star is 03:33:29.5 +08:14:49
Stellar brightness G=13.4, use SENSEUP=32 with the MallinCam and and exposure time of 500 milli-seconds with the QHY174 camera.
Star is 143 degrees from the moon. Moon is 38% illuminated.
TNO apparent brightness V=23.4

TNO is 34.4 AU from the Sun and 34.7 AU from the Earth.
The TNO is moving 17.0 km/sec on the sky relative to the star, or, 2.4 arcsec/hr.
The 1-sigma error in the time of the event is 827 seconds.
The 1-sigma cross-track error in the shadow position is 5059 km.

The TNO has an absolute magnitude Hv=7.8
Diameter=140.6 km assuming a 5% albedo -- 9.9 sec chord
Diameter=57.4 km assuming a 30% albedo -- 4.0 sec chord
Dynamical classification is 2:1E
 
 
 
 
 
 
 
 

Star training set for 13VO46, (2023/07/24 15:39UT)
Object            RA         Dec     mag  sep  mel
Aldebaran      04:37:16.5 +16:33:17  0.8 17.61 127
Menkar         03:03:30.8 +04:10:51  2.5  8.51 151
6 Tau          03:33:52.6 +09:27:05  5.6  1.20 143
PPM 146677     03:35:02.7 +08:22:06  8.4  0.38 143
13VO46         03:33:35.3 +08:15:10 13.4       143
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 13VO46, (2023/07/24 15:39UT)
Object            RA         Dec     mag  sep  mel
Aldebaran      04:35:55.3 +16:30:29  0.8 17.61 127
Menkar         03:02:16.8 +04:05:21  2.5  8.51 151
6 Tau          03:32:35.9 +09:22:23  5.6  1.20 143
PPM 146677     03:33:46.5 +08:17:25  8.4  0.38 143
13VO46         03:32:19.2 +08:10:28 13.4       143
Positions are for J2000

Event circumstances last updated at 2021/10/08 01:05:15 UT

Marc W. Buie, Southwest Research Institute

RECON