RECON: TNO occultation with 534161

Event between (534161) 14RQ63 and star GA1080:01451455 with event index number of 2175369

Geocentric closest approach at 2026/10/17 04:13:58 UTC

J2000 position of star is 05:53:08.5 +18:21:56
Equinox of date position of star is 05:54:26.1 +18:22:08
Stellar brightness G=16.7, use SENSEUP=128 with the MallinCam and and exposure time of 2 seconds with the QHY174 camera.
Star is 167 degrees from the moon. Moon is 36% illuminated.
TNO apparent brightness V=22.5

TNO is 31.8 AU from the Sun and 31.3 AU from the Earth.
The TNO is moving 7.5 km/sec on the sky relative to the star, or, 1.2 arcsec/hr.
The 1-sigma error in the time of the event is 851 seconds.
The 1-sigma cross-track error in the shadow position is 1842 km.

The TNO has an absolute magnitude Hv=7.3
Diameter=208.9 km assuming a 5% albedo -- 27.7 sec chord
Diameter=85.3 km assuming a 30% albedo -- 11.3 sec chord
Dynamical classification is 3:2E
 
 
 
 
 
 
 
 

Star training set for 534161, (2026/10/17 03:53UT)
Object            RA         Dec     mag  sep  mel
Betelgeuse     05:56:37.4 +07:24:35  0.4 10.97 158
Alhena         06:39:15.6 +16:22:27  1.9 10.81 169
57 Ori         05:56:31.8 +19:45:08  5.6  1.45 169
PPM 121541     05:55:01.0 +18:10:25  8.2  0.21 167
534161         05:54:42.8 +18:22:10 16.7       168
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 534161, (2026/10/17 03:53UT)
Object            RA         Dec     mag  sep  mel
Betelgeuse     05:55:10.3 +07:24:26  0.4 10.97 158
Alhena         06:37:42.8 +16:23:57  1.9 10.81 169
57 Ori         05:54:56.6 +19:44:58  5.6  1.45 169
PPM 121541     05:53:26.9 +18:10:12  8.2  0.21 167
534161         05:53:08.5 +18:21:56 16.7       167
Positions are for J2000

Event circumstances last updated at 2022/01/17 23:43:01 UT

Marc W. Buie, Southwest Research Institute

RECON