RECON: TNO occultation with 90568

Event between (90568) 04GV9 and star GA0660:06851817 with event index number of 2309313

Geocentric closest approach at 2028/09/10 15:26:41 UTC

J2000 position of star is 15:57:05.5 -23:23:20
Equinox of date position of star is 15:58:33.0 -23:27:30
Stellar brightness G=16.8, use SENSEUP=128 with the MallinCam and and exposure time of 2 seconds with the QHY174 camera.
Star is 179 degrees from the moon. Moon is 64% illuminated.
Apparent brightness V=20.2

Object is 40.2 AU from the Sun and 40.4 AU from the Earth.
Apparent velocity is 13.4 km/sec on the sky relative to the star, or, 1.7 arcsec/hr.
The 1-sigma error in the time of the event is 175 seconds.
The 1-sigma cross-track error in the shadow position is 1519 km.

The object has an absolute magnitude Hv=4.0
Diameter=946.3 km assuming a 5% albedo -- 72.0 sec chord
Diameter=386.3 km assuming a 30% albedo -- 29.4 sec chord
Dynamical classification is SCATEXTD
 
 
 
 
 
 
 
 

Star training set for 90568, (2028/09/10 15:27UT)
Object            RA         Dec     mag  sep  mel
Antares        16:31:10.3 -26:29:35  0.9  7.93 172
7Del Sco       16:02:02.1 -22:42:03  2.3  1.07 178
PPM 264830     15:55:38.7 -24:03:41  5.4  0.93 179
PPM 264924     15:59:31.5 -23:36:29  7.1  0.22 179
90568          15:58:48.1 -23:28:12 16.8       179
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 90568, (2028/09/10 15:27UT)
Object            RA         Dec     mag  sep  mel
Antares        16:29:24.4 -26:25:56  0.9  7.93 172
7Del Sco       16:00:20.0 -22:37:19  2.3  1.07 178
PPM 264830     15:53:55.9 -23:58:42  5.4  0.93 179
PPM 264924     15:57:48.8 -23:31:39  7.1  0.22 179
90568          15:57:05.5 -23:23:20 16.8       179
Positions are for J2000

Event circumstances last updated at 2024/06/24 21:33:58 UT

Marc W. Buie, Southwest Research Institute

RECON