RECON: TNO occultation with 459865

Event between (459865) 13XZ8 and star GA0640:10054850 with event index number of 2283035

Geocentric closest approach at 2025/09/25 03:46:38 UTC

J2000 position of star is 17:01:12.3 -24:33:49
Equinox of date position of star is 17:02:42.0 -24:35:52
Stellar brightness G=14.9, use SENSEUP=128 with the MallinCam and and exposure time of 2 seconds with the QHY174 camera.
Star is 37 degrees from the moon. Moon is 10% illuminated.
Apparent brightness V=20.0

Object is 10.1 AU from the Sun and 10.3 AU from the Earth.
Apparent velocity is 18.5 km/sec on the sky relative to the star, or, 8.9 arcsec/hr.
The 1-sigma error in the time of the event is 38 seconds.
The 1-sigma cross-track error in the shadow position is 411 km.

The object has an absolute magnitude Hv=9.5
Diameter=70.8 km assuming a 5% albedo -- 4.1 sec chord
Diameter=28.9 km assuming a 30% albedo -- 1.7 sec chord
Dynamical classification is CENTAURR
 
 
 
 
 
 
 
 

Star training set for 459865, (2025/09/25 03:43UT)
Object            RA         Dec     mag  sep  mel
Antares        16:30:59.4 -26:29:13  0.9  7.41  30
23Tau Sco      16:37:29.3 -28:16:02  2.8  6.74  32
26 Oph         17:01:44.3 -25:01:33  5.8  0.49  37
PPM 266306     17:03:50.0 -24:32:20  8.2  0.25  38
459865         17:02:46.7 -24:35:58 14.9        38
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, (2025/09/25 03:43UT)
Object            RA         Dec     mag  sep  mel
Antares        16:29:24.4 -26:25:56  0.9  7.41  30
23Tau Sco      16:35:52.9 -28:12:58  2.8  6.74  32
26 Oph         17:00:09.6 -24:59:22  5.8  0.49  37
PPM 266306     17:02:15.6 -24:30:13  8.2  0.25  38
459865         17:01:12.3 -24:33:49 14.9        37
Positions are for J2000

Event circumstances last updated at 2024/06/18 02:54:15 UT

Marc W. Buie, Southwest Research Institute

RECON