RECON: TNO occultation with 60558

Event between (60558) Echeclus and star GA1040:03159075 with event index number of 2337610

Geocentric closest approach at 2026/01/13 00:14:14 UTC

J2000 position of star is 08:28:27.1 +15:28:09
Equinox of date position of star is 08:29:48.7 +15:23:15
Stellar brightness G=16.5, use SENSEUP=128 with the MallinCam and and exposure time of 2 seconds with the QHY174 camera.
Star is 103 degrees from the moon. Moon is 29% illuminated.
Apparent brightness V=20.6

Object is 13.9 AU from the Sun and 12.9 AU from the Earth.
Apparent velocity is 23.2 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 22 seconds.
The 1-sigma cross-track error in the shadow position is 473 km.

The object has an absolute magnitude Hv=9.2
Diameter=88.3 km assuming a 5% albedo -- 3.7 sec chord
Diameter=36.1 km assuming a 30% albedo -- 1.5 sec chord
Dynamical classification is CENTAURR
 
 
 
 
 
 
 
 

Star training set for 60558, (2026/01/13 00:14UT)
Object            RA         Dec     mag  sep  mel
Pollux         07:46:54.5 +27:57:40  1.1 16.05 116
29 Cnc         08:30:04.3 +14:07:22  6.0  1.26 102
PPM 125327     08:31:19.4 +15:26:51  8.2  0.35 102
PPM 125324     08:31:04.9 +15:34:56 10.0  0.35 102
60558          08:29:54.8 +15:22:53 16.5       102
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 60558, (2026/01/13 00:14UT)
Object            RA         Dec     mag  sep  mel
Pollux         07:45:17.9 +28:01:33  1.1 16.05 116
29 Cnc         08:28:37.3 +14:12:39  6.0  1.26 102
PPM 125327     08:29:51.7 +15:32:09  8.2  0.35 102
PPM 125324     08:29:37.1 +15:40:14 10.0  0.35 102
60558          08:28:27.1 +15:28:09 16.5       102
Positions are for J2000

Event circumstances last updated at 2024/03/19 03:41:11 UT

Marc W. Buie, Southwest Research Institute

RECON