RECON: TNO occultation with 60558

Event between (60558) Echeclus and star GA1060:03063079 with event index number of 2337526

Geocentric closest approach at 2024/11/23 04:00:39 UTC

J2000 position of star is 08:13:19.7 +16:07:04
Equinox of date position of star is 08:14:42.0 +16:02:36
Stellar brightness G=14.5, use SENSEUP=128 with the MallinCam and and exposure time of 2 seconds with the QHY174 camera.
Star is 31 degrees from the moon. Moon is 49% illuminated.
Apparent brightness V=20.7

Object is 13.2 AU from the Sun and 12.7 AU from the Earth.
Apparent velocity is 8.7 km/sec on the sky relative to the star, or, 3.4 arcsec/hr.
The 1-sigma error in the time of the event is 57 seconds.
The 1-sigma cross-track error in the shadow position is 465 km.

The object has an absolute magnitude Hv=9.2
Diameter=88.3 km assuming a 5% albedo -- 10.0 sec chord
Diameter=36.1 km assuming a 30% albedo -- 4.1 sec chord
Dynamical classification is CENTAURR
 
 
 
 
 
 
 
 

Star training set for 60558, (2024/11/23 04:01UT)
Object            RA         Dec     mag  sep  mel
Pollux         07:46:50.3 +27:57:51  1.1 13.56  39
16Zet2Cnc      08:13:38.3 +17:34:17  5.2  1.55  32
PPM 125010     08:14:53.0 +16:21:12  8.5  0.31  31
PPM 124988     08:13:50.2 +15:52:02 10.7  0.28  31
60558          08:14:44.3 +16:02:28 14.5        31
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, (2024/11/23 04:01UT)
Object            RA         Dec     mag  sep  mel
Pollux         07:45:17.9 +28:01:33  1.1 13.56  39
16Zet2Cnc      08:12:13.0 +17:38:50  5.2  1.55  32
PPM 125010     08:13:28.2 +16:25:47  8.5  0.31  31
PPM 124988     08:12:25.7 +15:56:36 10.7  0.28  31
60558          08:13:19.7 +16:07:04 14.5        31
Positions are for J2000

Event circumstances last updated at 2024/03/19 03:36:06 UT

Marc W. Buie, Southwest Research Institute

RECON