RECON: TNO occultation with 126619

Event between (126619) 02CX154 and star GA0760:04685701 with event index number of 1055294

Geocentric closest approach at 2021/02/10 17:27:08 UTC

J2000 position of star is 12:42:24.2 -12:38:00
Equinox of date position of star is 12:43:30.1 -12:44:54
Stellar brightness G=16.2, use SENSEUP=128 with the MallinCam and and exposure time of 2 seconds with the QHY174 camera.
Star is 114 degrees from the moon. Moon is 1% illuminated.
TNO apparent brightness V=23.5

TNO is 42.1 AU from the Sun and 41.5 AU from the Earth.
The TNO is moving 13.7 km/sec on the sky relative to the star, or, 1.6 arcsec/hr.
The 1-sigma error in the time of the event is 515 seconds.
The 1-sigma cross-track error in the shadow position is 5597 km.

The TNO has an absolute magnitude Hv=7.2
Diameter=218.8 km assuming a 5% albedo -- 16.0 sec chord
Diameter=89.3 km assuming a 30% albedo -- 6.5 sec chord
Dynamical classification is SCATNEAR
 
 
 
 
 
 
 
 

Star training set for 126619, (2021/02/10 17:27UT)
Object            RA         Dec     mag  sep  mel
Spica          13:26:18.5 -11:16:15  1.0 10.57 105
4Gam Crv       12:16:53.7 -17:39:33  2.6  8.08 116
PPM 226198     12:42:21.8 -13:07:47  6.0  0.47 114
PPM 226222     12:43:28.7 -12:49:48  9.7  0.08 113
126619         12:43:30.3 -12:44:56 16.2       113
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 126619, (2021/02/10 17:27UT)
Object            RA         Dec     mag  sep  mel
Spica          13:25:11.5 -11:09:41  1.0 10.57 105
4Gam Crv       12:15:48.1 -17:32:30  2.6  8.08 116
PPM 226198     12:41:15.7 -13:00:51  6.0  0.47 114
PPM 226222     12:42:22.6 -12:42:52  9.7  0.08 113
126619         12:42:24.2 -12:38:00 16.2       114
Positions are for J2000

Event circumstances last updated at 2021/01/18 21:27:46 UT

Marc W. Buie, Southwest Research Institute

RECON