RECON: TNO occultation with 612891

Event between (612891) 04TT357 and star GA1060:01388126 with event index number of 2804619

Geocentric closest approach at 2026/02/09 20:08:24 UTC

J2000 position of star is 05:49:44.0 +17:38:17
Equinox of date position of star is 05:51:02.2 +17:38:36
Stellar brightness G=11.2, use SENSEUP=8 with the MallinCam and and exposure time of 125 milli-seconds with the QHY174 camera.
Star is 145 degrees from the moon. Moon is 47% illuminated.
TNO apparent brightness V=23.4

TNO is 34.6 AU from the Sun and 34.0 AU from the Earth.
The TNO is moving 12.7 km/sec on the sky relative to the star, or, 1.9 arcsec/hr.
The 1-sigma error in the time of the event is 613 seconds.
The 1-sigma cross-track error in the shadow position is 2079 km.

The TNO has an absolute magnitude Hv=7.9
Diameter=157.8 km assuming a 5% albedo -- 12.5 sec chord
Diameter=64.4 km assuming a 30% albedo -- 5.1 sec chord
Dynamical classification is 5:2EEE
 
 
 
 
 
 
 
 

Star training set for 612891, (2026/02/09 20:08UT)
Object            RA         Dec     mag  sep  mel
Betelgeuse     05:56:35.2 +07:24:35  0.4 10.32 140
Alhena         06:39:13.2 +16:22:29  1.9 11.53 134
126 Tau        05:42:48.3 +16:32:42  4.6  2.30 147
PPM 121438     05:51:01.0 +17:31:28  8.3  0.13 145
612891         05:51:15.4 +17:38:38 11.2       145
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 612891, (2026/02/09 20:08UT)
Object            RA         Dec     mag  sep  mel
Betelgeuse     05:55:10.3 +07:24:26  0.4 10.32 140
Alhena         06:37:42.8 +16:23:56  1.9 11.53 134
126 Tau        05:41:17.7 +16:32:02  4.6  2.30 147
PPM 121438     05:49:29.7 +17:31:06  8.3  0.13 145
612891         05:49:44.0 +17:38:17 11.2       145
Positions are for J2000

Event circumstances last updated at 2022/05/04 23:24:42 UT

Marc W. Buie, Southwest Research Institute

RECON