RECON: TNO occultation with 525461

Event between (525461) 05EN302 and star GA0760:04955145 with event index number of 1813653

Geocentric closest approach at 2028/01/03 19:08:40 UTC

J2000 position of star is 14:19:09.0 -13:13:41
Equinox of date position of star is 14:20:21.8 -13:19:48
Stellar brightness G=16.8, use SENSEUP=128 with the MallinCam and and exposure time of 2 seconds with the QHY174 camera.
Star is 142 degrees from the moon. Moon is 38% illuminated.
TNO apparent brightness V=24.0

TNO is 48.4 AU from the Sun and 48.8 AU from the Earth.
The TNO is moving 16.6 km/sec on the sky relative to the star, or, 1.7 arcsec/hr.
The 1-sigma error in the time of the event is 563 seconds.
The 1-sigma cross-track error in the shadow position is 5165 km.

The TNO has an absolute magnitude Hv=7.0
Diameter=251.2 km assuming a 5% albedo -- 14.6 sec chord
Diameter=102.6 km assuming a 30% albedo -- 6.0 sec chord
Dynamical classification is CLASSICAL
 
 
 
 
 
 
 
 

Star training set for 525461, (2028/01/03 19:09UT)
Object            RA         Dec     mag  sep  mel
Spica          13:26:40.4 -11:18:24  1.0 13.34 155
2 Lib          14:24:56.3 -11:50:26  6.2  1.84 141
PPM 228678     14:23:22.7 -13:18:32  8.4  0.66 141
PPM 228633     14:21:24.6 -13:22:33  9.7  0.18 141
525461         14:20:40.1 -13:21:21 16.8       141
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 525461, (2028/01/03 19:09UT)
Object            RA         Dec     mag  sep  mel
Spica          13:25:11.5 -11:09:41  1.0 13.34 155
2 Lib          14:23:25.6 -11:42:52  6.2  1.84 141
PPM 228678     14:21:51.4 -13:10:56  8.4  0.66 141
PPM 228633     14:19:53.4 -13:14:54  9.7  0.18 141
525461         14:19:09.0 -13:13:41 16.8       142
Positions are for J2000

Event circumstances last updated at 2022/05/20 23:01:33 UT

Marc W. Buie, Southwest Research Institute

RECON