RECON: TNO occultation with 10VE253

Event between 10VE253 and star GA1180:02793908 with event index number of 2106089

Geocentric closest approach at 2022/10/21 23:11:40 UTC

J2000 position of star is 06:58:08.9 +29:53:10
Equinox of date position of star is 06:59:35.8 +29:51:14
Stellar brightness G=16.8, use SENSEUP=128 with the MallinCam and and exposure time of 2 seconds with the QHY174 camera.
Star is 63 degrees from the moon. Moon is 13% illuminated.
TNO apparent brightness V=23.3

TNO is 20.2 AU from the Sun and 19.9 AU from the Earth.
The TNO is moving 3.3 km/sec on the sky relative to the star, or, 0.8 arcsec/hr.
The 1-sigma error in the time of the event is 282 seconds.
The 1-sigma cross-track error in the shadow position is 3614 km.

The TNO has an absolute magnitude Hv=10.0
Diameter=61.1 km assuming a 5% albedo -- 18.5 sec chord
Diameter=24.9 km assuming a 30% albedo -- 7.6 sec chord
Dynamical classification is CENTAURR
 
 
 
 
 
 
 
 

Star training set for 10VE253, (2022/10/21 23:12UT)
Object            RA         Dec     mag  sep  mel
Pollux         07:46:42.6 +27:58:09  1.1 10.48  53
PPM 097053     07:08:50.5 +28:08:22  6.2  2.65  61
PPM 096723     06:56:14.0 +29:47:49  8.0  0.73  64
PPM 072258     06:58:27.5 +29:59:53  9.4  0.29  63
10VE253        06:59:36.0 +29:51:14 16.8        63
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 10VE253, (2022/10/21 23:12UT)
Object            RA         Dec     mag  sep  mel
Pollux         07:45:17.9 +28:01:33  1.1 10.48  53
PPM 097053     07:07:24.8 +28:10:36  6.2  2.65  61
PPM 096723     06:54:46.9 +29:49:39  8.0  0.73  64
PPM 072258     06:57:00.3 +30:01:47  9.4  0.29  63
10VE253        06:58:08.9 +29:53:10 16.8        63
Positions are for J2000

Event circumstances last updated at 2022/10/01 04:15:34 UT

Marc W. Buie, Southwest Research Institute

RECON