RECON: TNO occultation with 459865

Event between (459865) 13XZ8 and star GA0680:18886012 with event index number of 2284720

Geocentric closest approach at 2026/09/28 21:37:06 UTC

J2000 position of star is 17:48:55.8 -20:54:05
Equinox of date position of star is 17:50:23.5 -20:54:27
Stellar brightness G=11.8, use SENSEUP=8 with the MallinCam and and exposure time of 125 milli-seconds with the QHY174 camera.
Star is 126 degrees from the moon. Moon is 94% illuminated.
Apparent brightness V=20.3

Object is 10.7 AU from the Sun and 10.8 AU from the Earth.
Apparent velocity is 13.8 km/sec on the sky relative to the star, or, 6.3 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 513 km.

The object has an absolute magnitude Hv=9.5
Diameter=70.8 km assuming a 5% albedo -- 5.5 sec chord
Diameter=28.9 km assuming a 30% albedo -- 2.2 sec chord
Dynamical classification is CENTAURR
 
 
 
 
 
 
 
 

Star training set for 459865, (2026/09/28 21:31UT)
Object            RA         Dec     mag  sep  mel
Antares        16:31:03.1 -26:29:20  0.9 19.01 144
35Eta Oph      17:11:54.8 -15:45:22  2.6 10.51 135
58 Oph         17:45:02.1 -21:41:37  4.9  1.50 128
PPM 267354     17:51:03.0 -20:50:14  8.0  0.14 126
459865         17:50:31.6 -20:54:29 11.8       126
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 459865, (2026/09/28 21:31UT)
Object            RA         Dec     mag  sep  mel
Antares        16:29:24.4 -26:25:56  0.9 19.01 144
35Eta Oph      17:10:22.7 -15:43:29  2.6 10.51 135
58 Oph         17:43:25.7 -21:41:00  4.9  1.50 128
PPM 267354     17:49:27.2 -20:49:51  8.0  0.14 126
459865         17:48:55.8 -20:54:05 11.8       126
Positions are for J2000

Event circumstances last updated at 2024/06/20 21:25:09 UT

Marc W. Buie, Southwest Research Institute

RECON