RECON: TNO occultation with 501214

Event between (501214) 13TC146 and star GA0780:22010109 with event index number of 2453222

Geocentric closest approach at 2023/08/19 21:39:40 UTC

J2000 position of star is 22:24:22.5 -11:36:15
Equinox of date position of star is 22:25:35.3 -11:29:15
Stellar brightness G=14.4, use SENSEUP=64 with the MallinCam and and exposure time of 1 seconds with the QHY174 camera.
Star is 149 degrees from the moon. Moon is 11% illuminated.
TNO apparent brightness V=21.0

TNO is 27.6 AU from the Sun and 26.6 AU from the Earth.
The TNO is moving 24.1 km/sec on the sky relative to the star, or, 4.5 arcsec/hr.
The 1-sigma error in the time of the event is 43 seconds.
The 1-sigma cross-track error in the shadow position is 980 km.

The TNO has an absolute magnitude Hv=6.6
Diameter=279.3 km assuming a 5% albedo -- 11.8 sec chord
Diameter=114.0 km assuming a 30% albedo -- 4.8 sec chord
Dynamical classification is CENTAURR
 
 
 
 
 
 
 
 

Star training set for 501214, (2023/08/19 21:40UT)
Object            RA         Dec     mag  sep  mel
Fomalhaut      22:58:57.0 -29:29:47  1.2 19.61 144
50 Aqr         22:25:42.9 -13:24:32  5.8  1.93 148
PPM 240220     22:25:46.1 -11:02:10  8.1  0.45 149
PPM 240224     22:25:51.9 -11:27:33  9.6  0.06 149
501214         22:25:37.8 -11:29:01 14.4       149
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 501214, (2023/08/19 21:40UT)
Object            RA         Dec     mag  sep  mel
Fomalhaut      22:57:39.6 -29:37:24  1.2 19.61 144
50 Aqr         22:24:27.1 -13:31:46  5.8  1.93 148
PPM 240220     22:24:30.9 -11:09:23  8.1  0.45 149
PPM 240224     22:24:36.6 -11:34:47  9.6  0.06 149
501214         22:24:22.5 -11:36:15 14.4       149
Positions are for J2000

Event circumstances last updated at 2022/11/13 03:31:14 UT

Marc W. Buie, Southwest Research Institute

RECON