RECON: TNO occultation with 523746

Event between (523746) 14UT114 and star GA1180:02995450 with event index number of 2323141

Geocentric closest approach at 2024/09/16 18:40:39 UTC

J2000 position of star is 07:32:40.0 +29:57:38
Equinox of date position of star is 07:34:12.1 +29:54:24
Stellar brightness G=13.1, use SENSEUP=32 with the MallinCam and and exposure time of 500 milli-seconds with the QHY174 camera.
Star is 135 degrees from the moon. Moon is 97% illuminated.
Apparent brightness V=21.3

Object is 16.5 AU from the Sun and 16.9 AU from the Earth.
Apparent velocity is 21.1 km/sec on the sky relative to the star, or, 6.2 arcsec/hr.
The 1-sigma error in the time of the event is 42 seconds.
The 1-sigma cross-track error in the shadow position is 664 km.

The object has an absolute magnitude Hv=8.8
Diameter=95.5 km assuming a 5% albedo -- 5.0 sec chord
Diameter=39.0 km assuming a 30% albedo -- 2.0 sec chord
Dynamical classification is CENTAURR
 
 
 
 
 
 
 
 

Star training set for 523746, (2024/09/16 18:34UT)
Object            RA         Dec     mag  sep  mel
Pollux         07:46:49.6 +27:57:52  1.1  3.37 138
PPM 072946     07:36:42.8 +30:54:18  6.3  1.13 135
PPM 097585     07:31:55.3 +29:08:17  8.5  0.92 134
PPM 097636     07:33:56.1 +29:55:02  9.8  0.06 134
523746         07:34:13.4 +29:54:21 13.1       135
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 523746, (2024/09/16 18:34UT)
Object            RA         Dec     mag  sep  mel
Pollux         07:45:17.9 +28:01:33  1.1  3.37 138
PPM 072946     07:35:08.7 +30:57:40  6.3  1.13 135
PPM 097585     07:30:22.3 +29:11:29  8.5  0.92 134
PPM 097636     07:32:22.7 +29:58:18  9.8  0.06 134
523746         07:32:40.0 +29:57:38 13.1       135
Positions are for J2000

Event circumstances last updated at 2024/05/05 03:29:12 UT

Marc W. Buie, Southwest Research Institute

RECON