RECON: TNO occultation with 543377

Event between (543377) 14BF70 and star GA0560:19161795 with event index number of 2254226

Geocentric closest approach at 2028/05/19 12:54:06 UTC

J2000 position of star is 17:11:42.3 -32:22:32
Equinox of date position of star is 17:13:17.9 -32:24:13
Stellar brightness G=16.5, use SENSEUP=128 with the MallinCam and and exposure time of 2 seconds with the QHY174 camera.
Star is 104 degrees from the moon. Moon is 22% illuminated.
Apparent brightness V=20.4

Object is 12.3 AU from the Sun and 11.4 AU from the Earth.
Apparent velocity is 16.3 km/sec on the sky relative to the star, or, 7.1 arcsec/hr.
The 1-sigma error in the time of the event is 154 seconds.
The 1-sigma cross-track error in the shadow position is 506 km.

The object has an absolute magnitude Hv=9.5
Diameter=75.5 km assuming a 5% albedo -- 4.7 sec chord
Diameter=30.8 km assuming a 30% albedo -- 1.9 sec chord
Dynamical classification is CENTAURR
 
 
 
 
 
 
 
 

Star training set for 543377, (2028/05/19 12:49UT)
Object            RA         Dec     mag  sep  mel
Antares        16:31:09.2 -26:29:33  0.9 10.95 113
26Eps Sco      16:52:00.8 -34:20:30  2.3  4.89 108
PPM 296042     17:14:49.4 -32:28:11  6.2  0.28 103
PPM 296007     17:13:07.8 -32:21:29  7.6  0.10 104
543377         17:13:33.2 -32:24:29 16.5       103
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 543377, (2028/05/19 12:49UT)
Object            RA         Dec     mag  sep  mel
Antares        16:29:24.4 -26:25:56  0.9 10.95 113
26Eps Sco      16:50:08.8 -34:17:41  2.3  4.89 108
PPM 296042     17:12:58.5 -32:26:18  6.2  0.28 103
PPM 296007     17:11:17.0 -32:19:31  7.6  0.10 104
543377         17:11:42.3 -32:22:32 16.5       104
Positions are for J2000

Event circumstances last updated at 2024/06/24 21:29:13 UT

Marc W. Buie, Southwest Research Institute

RECON