RECON: TNO occultation with 533398

Event between (533398) 14GA54 and star GA0740:17477508 with event index number of 2164864

Geocentric closest approach at 2028/03/09 16:56:32 UTC

J2000 position of star is 18:22:05.6 -14:14:01
Equinox of date position of star is 18:23:29.1 -14:13:13
Stellar brightness G=14.2, use SENSEUP=64 with the MallinCam and and exposure time of 1 seconds with the QHY174 camera.
Star is 125 degrees from the moon. Moon is 97% illuminated.
Apparent brightness V=22.3

Object is 31.0 AU from the Sun and 31.3 AU from the Earth.
Apparent velocity is 14.9 km/sec on the sky relative to the star, or, 2.4 arcsec/hr.
The 1-sigma error in the time of the event is 508 seconds.
The 1-sigma cross-track error in the shadow position is 2210 km.

The object has an absolute magnitude Hv=7.2
Diameter=215.8 km assuming a 5% albedo -- 14.5 sec chord
Diameter=88.1 km assuming a 30% albedo -- 5.9 sec chord
Dynamical classification is CENTAURR
 
 
 
 
 
 
 
 

Star training set for 533398, (2028/03/09 16:57UT)
Object            RA         Dec     mag  sep  mel
Antares        16:31:08.4 -26:29:31  0.9 29.00  99
Nunki          18:57:00.7 -26:15:32  2.0 14.34 131
PPM 234386     18:21:46.2 -15:49:03  5.2  1.67 124
PPM 234435     18:23:52.3 -14:22:23  7.7  0.16 125
533398         18:23:41.8 -14:13:05 14.2       125
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 533398, (2028/03/09 16:57UT)
Object            RA         Dec     mag  sep  mel
Antares        16:29:24.4 -26:25:56  0.9 29.00  99
Nunki          18:55:15.9 -26:17:49  2.0 14.34 131
PPM 234386     18:20:08.9 -15:49:55  5.2  1.67 124
PPM 234435     18:22:16.0 -14:23:19  7.7  0.16 125
533398         18:22:05.6 -14:14:01 14.2       125
Positions are for J2000

Event circumstances last updated at 2024/06/23 21:29:30 UT

Marc W. Buie, Southwest Research Institute

RECON