RECON: TNO occultation with 38628

Event between (38628) Huya and star GA0820:07775302 with event index number of 2433303

Geocentric closest approach at 2028/07/09 03:31:03 UTC

J2000 position of star is 18:07:40.5 -07:49:49
Equinox of date position of star is 18:09:00.3 -07:49:31
Stellar brightness G=15.9, use SENSEUP=128 with the MallinCam and and exposure time of 2 seconds with the QHY174 camera.
Star is 44 degrees from the moon. Moon is 95% illuminated.
Apparent brightness V=19.5

Object is 29.7 AU from the Sun and 28.7 AU from the Earth.
Apparent velocity is 22.3 km/sec on the sky relative to the star, or, 3.9 arcsec/hr.
The 1-sigma error in the time of the event is 104 seconds.
The 1-sigma cross-track error in the shadow position is 1077 km.

The object has an absolute magnitude Hv=4.8
Diameter=648.7 km assuming a 5% albedo -- 29.4 sec chord
Diameter=264.8 km assuming a 30% albedo -- 12.0 sec chord
Dynamical classification is 3:2E+6:4II
 
 
 
 
 
 
 
 

Star training set for 38628, (2028/07/09 03:30UT)
Object            RA         Dec     mag  sep  mel
Antares        16:31:09.7 -26:29:34  0.9 29.84  65
60Bet Oph      17:44:53.0 +04:33:26  2.8 13.79  54
PPM 201392     18:07:40.6 -08:19:10  6.1  0.63  44
PPM 201422     18:09:40.9 -07:58:25  9.5  0.19  44
38628          18:09:13.4 -07:49:28 15.9        44
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 38628, (2028/07/09 03:30UT)
Object            RA         Dec     mag  sep  mel
Antares        16:29:24.4 -26:25:56  0.9 29.84  65
60Bet Oph      17:43:28.3 +04:34:06  2.8 13.79  54
PPM 201392     18:06:07.4 -08:19:27  6.1  0.63  44
PPM 201422     18:08:07.9 -07:58:47  9.5  0.19  44
38628          18:07:40.5 -07:49:49 15.9        44
Positions are for J2000

Event circumstances last updated at 2024/06/24 21:30:42 UT

Marc W. Buie, Southwest Research Institute

RECON