RECON: TNO occultation with 517717

Event between (517717) 15KZ120 and star GA1420:02352393 with event index number of 2628014

Geocentric closest approach at 2025/01/20 19:13:09 UTC

J2000 position of star is 03:25:20.8 +52:40:58
Equinox of date position of star is 03:27:02.2 +52:45:42
Stellar brightness G=15.8, use SENSEUP=128 with the MallinCam and and exposure time of 2 seconds with the QHY174 camera.
Star is 129 degrees from the moon. Moon is 60% illuminated.
TNO apparent brightness V=21.7

TNO is 13.7 AU from the Sun and 13.2 AU from the Earth.
The TNO is moving 26.9 km/sec on the sky relative to the star, or, 10.1 arcsec/hr.
The 1-sigma error in the time of the event is 115 seconds.
The 1-sigma cross-track error in the shadow position is 2082 km.

The TNO has an absolute magnitude Hv=10.1
Diameter=57.5 km assuming a 5% albedo -- 2.1 sec chord
Diameter=23.5 km assuming a 30% albedo -- 0.9 sec chord
Dynamical classification is CENTAURR
 
 
 
 
 
 
 
 

Star training set for 517717, (2025/01/20 19:13UT)
Object            RA         Dec     mag  sep  mel
Pollux         07:46:50.9 +27:57:49  1.1 53.13  87
Mirphak        03:26:07.5 +49:56:54  1.8  2.83 131
PPM 028555     03:35:34.5 +55:03:28  5.9  2.60 126
PPM 028463     03:27:35.2 +52:50:19  7.9  0.09 129
517717         03:27:12.3 +52:46:10 15.8       128
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 517717, (2025/01/20 19:13UT)
Object            RA         Dec     mag  sep  mel
Pollux         07:45:17.9 +28:01:33  1.1 53.13  87
Mirphak        03:24:19.4 +49:51:40  1.8  2.83 131
PPM 028555     03:33:39.0 +54:58:30  5.9  2.60 126
PPM 028463     03:25:43.5 +52:45:08  7.9  0.09 129
517717         03:25:20.8 +52:40:58 15.8       129
Positions are for J2000

Event circumstances last updated at 2022/10/23 03:29:19 UT

Marc W. Buie, Southwest Research Institute

RECON