RECON: TNO occultation with 95626

Event between (95626) 02GZ32 and star GA0700:21578467 with event index number of 1118150

Geocentric closest approach at 2021/06/03 22:52:13 UTC

J2000 position of star is 18:15:37.7 -19:16:13
Equinox of date position of star is 18:16:52.4 -19:15:43
Stellar brightness G=15.3, use SENSEUP=128 with the MallinCam and and exposure time of 2 seconds with the QHY174 camera.
Star is 89 degrees from the moon. Moon is 34% illuminated.
TNO apparent brightness V=19.5

TNO is 18.1 AU from the Sun and 17.1 AU from the Earth.
The TNO is moving 20.0 km/sec on the sky relative to the star, or, 5.8 arcsec/hr.
The 1-sigma error in the time of the event is 93 seconds.
The 1-sigma cross-track error in the shadow position is 778 km.

The TNO has an absolute magnitude Hv=6.9
Diameter=251.2 km assuming a 5% albedo -- 12.6 sec chord
Diameter=102.6 km assuming a 30% albedo -- 5.1 sec chord
Dynamical classification is CENTAURR
 
 
 
 
 
 
 
 

Star training set for 95626, (2021/06/03 22:52UT)
Object            RA         Dec     mag  sep  mel
Antares        16:30:43.5 -26:28:40  0.9 25.44 112
Nunki          18:56:35.5 -26:16:06  2.0 11.52  80
PPM 234244     18:16:46.3 -18:39:11  6.1  0.61  89
PPM 234237     18:16:32.5 -18:59:04  7.6  0.29  89
95626          18:16:53.5 -19:15:43 15.3        89
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 95626, (2021/06/03 22:52UT)
Object            RA         Dec     mag  sep  mel
Antares        16:29:24.4 -26:25:56  0.9 25.44 112
Nunki          18:55:15.9 -26:17:49  2.0 11.52  80
PPM 234244     18:15:30.8 -18:39:42  6.1  0.61  89
PPM 234237     18:15:16.8 -18:59:34  7.6  0.29  89
95626          18:15:37.7 -19:16:13 15.3        89
Positions are for J2000

Event circumstances last updated at 2021/02/06 21:04:31 UT

Marc W. Buie, Southwest Research Institute

RECON