RECON: TNO occultation with 523717

Event between (523717) 14KY101 and star GA0680:12531985 with event index number of 2616292

Geocentric closest approach at 2023/05/23 21:39:07 UTC

J2000 position of star is 17:29:00.4 -20:48:11
Equinox of date position of star is 17:30:23.8 -20:49:13
Stellar brightness G=15.6, use SENSEUP=128 with the MallinCam and and exposure time of 2 seconds with the QHY174 camera.
Star is 150 degrees from the moon. Moon is 17% illuminated.
Apparent brightness V=22.1

Object is 35.8 AU from the Sun and 34.9 AU from the Earth.
Apparent velocity is 22.4 km/sec on the sky relative to the star, or, 3.2 arcsec/hr.
The 1-sigma error in the time of the event is 317 seconds.
The 1-sigma cross-track error in the shadow position is 2324 km.

The object has an absolute magnitude Hv=6.5
Diameter=316.2 km assuming a 5% albedo -- 13.5 sec chord
Diameter=129.1 km assuming a 30% albedo -- 5.5 sec chord
Dynamical classification is 3:2E
 
 
 
 
 
 
 
 

Star training set for 523717, (2023/05/23 21:39UT)
Object            RA         Dec     mag  sep  mel
Antares        16:30:50.7 -26:28:55  0.9 14.75 138
35Eta Oph      17:11:43.3 -15:45:08  2.6  6.73 144
PPM 266825     17:26:06.1 -21:27:41  6.1  1.19 150
PPM 266907     17:29:40.0 -20:58:52  8.3  0.24 150
523717         17:30:24.1 -20:49:13 15.6       151
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 523717, (2023/05/23 21:39UT)
Object            RA         Dec     mag  sep  mel
Antares        16:29:24.4 -26:25:56  0.9 14.75 138
35Eta Oph      17:10:22.7 -15:43:29  2.6  6.73 144
PPM 266825     17:24:42.0 -21:26:30  6.1  1.19 150
PPM 266907     17:28:16.2 -20:57:49  8.3  0.24 150
523717         17:29:00.4 -20:48:11 15.6       150
Positions are for J2000

Event circumstances last updated at 2023/04/20 03:43:03 UT

Marc W. Buie, Southwest Research Institute

RECON