RECON: TNO occultation with 524179

Event between (524179) 01FQ185 and star GA0720:05593270 with event index number of 1911956

Geocentric closest approach at 2028/06/28 21:34:59 UTC

J2000 position of star is 15:36:27.7 -16:01:18
Equinox of date position of star is 15:37:50.1 -16:06:03
Stellar brightness G=16.2, use SENSEUP=128 with the MallinCam and and exposure time of 2 seconds with the QHY174 camera.
Star is 57 degrees from the moon. Moon is 43% illuminated.
Apparent brightness V=22.8

Object is 37.9 AU from the Sun and 37.1 AU from the Earth.
Apparent velocity is 16.7 km/sec on the sky relative to the star, or, 2.2 arcsec/hr.
The 1-sigma error in the time of the event is 356 seconds.
The 1-sigma cross-track error in the shadow position is 2024 km.

The object has an absolute magnitude Hv=6.9
Diameter=251.2 km assuming a 5% albedo -- 15.2 sec chord
Diameter=102.6 km assuming a 30% albedo -- 6.2 sec chord
Dynamical classification is 2:1E
 
 
 
 
 
 
 
 

Star training set for 524179, (2028/06/28 21:35UT)
Object            RA         Dec     mag  sep  mel
Antares        16:31:09.6 -26:29:34  0.9 16.12  70
8Bet1Sco       16:07:05.9 -19:52:52  2.6  7.86  64
35Zet4Lib      15:34:32.1 -16:56:51  5.6  1.19  56
PPM 230463     15:37:32.5 -16:03:51  8.2  0.14  56
524179         15:38:04.2 -16:06:51 16.2        57
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 524179, (2028/06/28 21:35UT)
Object            RA         Dec     mag  sep  mel
Antares        16:29:24.4 -26:25:56  0.9 16.12  70
8Bet1Sco       16:05:26.2 -19:48:20  2.6  7.86  64
35Zet4Lib      15:32:55.2 -16:51:11  5.6  1.19  56
PPM 230463     15:35:56.0 -15:58:17  8.2  0.14  56
524179         15:36:27.7 -16:01:18 16.2        57
Positions are for J2000

Event circumstances last updated at 2024/05/05 03:40:49 UT

Marc W. Buie, Southwest Research Institute

RECON