RECON: TNO occultation with 523723

Event between (523723) 14MY69 and star GA0800:21852004 with event index number of 2615577

Geocentric closest approach at 2026/08/06 16:07:17 UTC

J2000 position of star is 23:24:17.9 -08:27:15
Equinox of date position of star is 23:25:32.1 -08:19:21
Stellar brightness G=16.6, use SENSEUP=128 with the MallinCam and and exposure time of 2 seconds with the QHY174 camera.
Star is 64 degrees from the moon. Moon is 44% illuminated.
Apparent brightness V=22.1

Object is 42.1 AU from the Sun and 41.3 AU from the Earth.
Apparent velocity is 20.0 km/sec on the sky relative to the star, or, 2.4 arcsec/hr.
The 1-sigma error in the time of the event is 108 seconds.
The 1-sigma cross-track error in the shadow position is 2092 km.

The object has an absolute magnitude Hv=5.8
Diameter=409.3 km assuming a 5% albedo -- 20.9 sec chord
Diameter=167.1 km assuming a 30% albedo -- 8.5 sec chord
Dynamical classification is SCATEXTD
 
 
 
 
 
 
 
 

Star training set for 523723, (2026/08/06 16:09UT)
Object            RA         Dec     mag  sep  mel
Fomalhaut      22:59:06.8 -29:28:50  1.2 22.07  81
Diphda         00:44:55.3 -17:50:28  2.0 21.50  55
PPM 207606     23:30:23.2 -09:07:10  6.4  1.42  63
PPM 207503     23:25:08.0 -08:18:52  6.7  0.13  64
523723         23:25:40.5 -08:18:28 16.6        64
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 523723, (2026/08/06 16:09UT)
Object            RA         Dec     mag  sep  mel
Fomalhaut      22:57:39.6 -29:37:24  1.2 22.07  81
Diphda         00:43:35.7 -17:59:11  2.0 21.50  55
PPM 207606     23:29:00.6 -09:15:59  6.4  1.42  63
PPM 207503     23:23:45.5 -08:27:39  6.7  0.13  64
523723         23:24:17.9 -08:27:15 16.6        64
Positions are for J2000

Event circumstances last updated at 2023/11/20 04:27:28 UT

Marc W. Buie, Southwest Research Institute

RECON