RECON: TNO occultation with 15KK178

Event between 15KK178 and star GA0720:07531731 with event index number of 1992859

Geocentric closest approach at 2023/02/24 10:18:46 UTC

J2000 position of star is 17:10:02.9 -16:21:07
Equinox of date position of star is 17:11:22.5 -16:22:45
Stellar brightness G=16.9, use SENSEUP=128 with the MallinCam and and exposure time of 2 seconds with the QHY174 camera.
Star is 133 degrees from the moon. Moon is 22% illuminated.
Apparent brightness V=22.4

Object is 37.1 AU from the Sun and 37.3 AU from the Earth.
Apparent velocity is 12.6 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 344 seconds.
The 1-sigma cross-track error in the shadow position is 1858 km.

The object has an absolute magnitude Hv=6.5
Diameter=306.2 km assuming a 5% albedo -- 24.3 sec chord
Diameter=125.0 km assuming a 30% albedo -- 9.9 sec chord
Dynamical classification is SCATEXTD
 
 
 
 
 
 
 
 

Star training set for 15KK178, (2023/02/24 10:19UT)
Object            RA         Dec     mag  sep  mel
Antares        16:30:49.8 -26:28:53  0.9 13.81 141
35Eta Oph      17:11:42.4 -15:45:07  2.6  0.63 133
PPM 232651     17:09:35.6 -17:38:16  6.0  1.33 133
PPM 232687     17:11:10.4 -16:20:26  8.5  0.06 133
15KK178        17:11:23.0 -16:22:46 16.9       132
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 15KK178, (2023/02/24 10:19UT)
Object            RA         Dec     mag  sep  mel
Antares        16:29:24.4 -26:25:56  0.9 13.81 141
35Eta Oph      17:10:22.7 -15:43:29  2.6  0.63 133
PPM 232651     17:08:14.9 -17:36:33  6.0  1.33 133
PPM 232687     17:09:50.4 -16:18:47  8.5  0.06 133
15KK178        17:10:02.9 -16:21:07 16.9       133
Positions are for J2000

Event circumstances last updated at 2023/01/08 03:30:45 UT

Marc W. Buie, Southwest Research Institute

RECON