RECON: TNO occultation with 523773

Event between (523773) 14XS40 and star GA0840:03823768 with event index number of 2356810

Geocentric closest approach at 2026/02/23 16:40:20 UTC

J2000 position of star is 09:39:30.1 -05:08:17
Equinox of date position of star is 09:40:43.2 -05:14:57
Stellar brightness G=17.0, use SENSEUP=128 with the MallinCam and and exposure time of 2 seconds with the QHY174 camera.
Star is 96 degrees from the moon. Moon is 41% illuminated.
Apparent brightness V=21.1

Object is 37.8 AU from the Sun and 36.9 AU from the Earth.
Apparent velocity is 25.4 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 65 seconds.
The 1-sigma cross-track error in the shadow position is 1451 km.

The object has an absolute magnitude Hv=5.3
Diameter=517.6 km assuming a 5% albedo -- 20.8 sec chord
Diameter=211.3 km assuming a 30% albedo -- 8.5 sec chord
Dynamical classification is SCATEXTD
 
 
 
 
 
 
 
 

Star training set for 523773, (2026/02/23 16:42UT)
Object            RA         Dec     mag  sep  mel
Regulus        10:09:45.8 +11:50:18  1.3 18.55  96
Alphard        09:28:52.3 -08:46:24  2.0  4.60  95
33 Hya         09:35:50.9 -06:01:58  5.6  1.46  95
PPM 192590     09:39:30.6 -05:17:08  8.0  0.33  96
523773         09:40:48.7 -05:15:27 17.0        96
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 523773, (2026/02/23 16:42UT)
Object            RA         Dec     mag  sep  mel
Regulus        10:08:21.9 +11:58:02  1.3 18.55  96
Alphard        09:27:35.2 -08:39:30  2.0  4.60  95
33 Hya         09:34:32.7 -05:54:55  5.6  1.46  95
PPM 192590     09:38:12.0 -05:10:00  8.0  0.33  96
523773         09:39:30.1 -05:08:17 17.0        96
Positions are for J2000

Event circumstances last updated at 2024/04/23 03:23:20 UT

Marc W. Buie, Southwest Research Institute

RECON