RECON: TNO occultation with 613411

Event between (613411) 06HQ122 and star GA0780:05420545 with event index number of 2820830

Geocentric closest approach at 2026/06/11 18:14:21 UTC

J2000 position of star is 16:24:54.8 -10:13:22
Equinox of date position of star is 16:26:12.0 -10:16:30
Stellar brightness G=16.2, use SENSEUP=128 with the MallinCam and and exposure time of 2 seconds with the QHY174 camera.
Star is 144 degrees from the moon. Moon is 16% illuminated.
Apparent brightness V=22.8

Object is 42.3 AU from the Sun and 41.4 AU from the Earth.
Apparent velocity is 23.3 km/sec on the sky relative to the star, or, 2.8 arcsec/hr.
The 1-sigma error in the time of the event is 206 seconds.
The 1-sigma cross-track error in the shadow position is 1958 km.

The object has an absolute magnitude Hv=6.5
Diameter=295.1 km assuming a 5% albedo -- 12.7 sec chord
Diameter=120.5 km assuming a 30% albedo -- 5.2 sec chord
Dynamical classification is SCATNEAR
 
 
 
 
 
 
 
 

Star training set for 613411, (2026/06/11 18:07UT)
Object            RA         Dec     mag  sep  mel
Antares        16:31:02.0 -26:29:18  0.9 16.24 144
13Zet Oph      16:38:37.1 -10:37:07  2.6  3.03 141
3Ups Oph       16:29:14.1 -08:25:44  4.2  1.98 143
PPM 231679     16:27:05.3 -10:08:33  8.5  0.23 144
613411         16:26:22.0 -10:16:54 16.2       144
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 613411, (2026/06/11 18:07UT)
Object            RA         Dec     mag  sep  mel
Antares        16:29:24.4 -26:25:56  0.9 16.24 144
13Zet Oph      16:37:09.6 -10:34:01  2.6  3.03 141
3Ups Oph       16:27:48.0 -08:22:18  4.2  1.98 143
PPM 231679     16:25:38.2 -10:05:03  8.5  0.23 144
613411         16:24:54.8 -10:13:22 16.2       144
Positions are for J2000

Event circumstances last updated at 2023/05/29 02:45:30 UT

Marc W. Buie, Southwest Research Institute

RECON