RECON: TNO occultation with 15BE568

Event between 15BE568 and star GA0740:05068802 with event index number of 2643608

Geocentric closest approach at 2024/01/05 02:35:54 UTC

J2000 position of star is 13:50:18.3 -14:34:01
Equinox of date position of star is 13:51:30.6 -14:40:37
Stellar brightness G=12.1, use SENSEUP=16 with the MallinCam and and exposure time of 250 milli-seconds with the QHY174 camera.
Star is 7 degrees from the moon. Moon is 41% illuminated.
TNO apparent brightness V=23.1

TNO is 22.8 AU from the Sun and 23.1 AU from the Earth.
The TNO is moving 15.7 km/sec on the sky relative to the star, or, 3.4 arcsec/hr.
The 1-sigma error in the time of the event is 166 seconds.
The 1-sigma cross-track error in the shadow position is 1102 km.

The TNO has an absolute magnitude Hv=9.2
Diameter=88.7 km assuming a 5% albedo -- 5.6 sec chord
Diameter=36.2 km assuming a 30% albedo -- 2.3 sec chord
Dynamical classification is CENTAURR
 
 
 
 
 
 
 
 

Star training set for 15BE568, (2024/01/05 02:32UT)
Object            RA         Dec     mag  sep  mel
Spica          13:26:27.7 -11:17:09  1.0  7.00   2
83 Vir         13:45:47.8 -16:17:56  5.6  2.13   7
PPM 227883     13:50:38.0 -14:52:50  8.4  0.30   7
PPM 227889     13:50:50.1 -14:28:25  9.8  0.28   6
15BE568        13:51:36.0 -14:41:07 12.1         7
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 15BE568, (2024/01/05 02:32UT)
Object            RA         Dec     mag  sep  mel
Spica          13:25:11.5 -11:09:41  1.0  7.00   2
83 Vir         13:44:29.9 -16:10:45  5.6  2.13   7
PPM 227883     13:49:20.2 -14:45:43  8.4  0.30   7
PPM 227889     13:49:32.5 -14:21:18  9.8  0.28   6
15BE568        13:50:18.3 -14:34:01 12.1         7
Positions are for J2000

Event circumstances last updated at 2022/05/03 01:46:13 UT

Marc W. Buie, Southwest Research Institute

RECON