RECON: TNO occultation with 13EM149

Event between 13EM149 and star GA0740:05353221 with event index number of 2047900

Geocentric closest approach at 2023/08/12 10:48:54 UTC

J2000 position of star is 15:05:26.3 -15:02:36
Equinox of date position of star is 15:06:45.0 -15:08:01
Stellar brightness G=16.2, use SENSEUP=128 with the MallinCam and and exposure time of 2 seconds with the QHY174 camera.
Star is 132 degrees from the moon. Moon is 14% illuminated.
Apparent brightness V=23.2

Object is 43.3 AU from the Sun and 43.3 AU from the Earth.
Apparent velocity is 5.5 km/sec on the sky relative to the star, or, 0.6 arcsec/hr.
The 1-sigma error in the time of the event is 2106 seconds.
The 1-sigma cross-track error in the shadow position is 3408 km.

The object has an absolute magnitude Hv=6.7
Diameter=274.2 km assuming a 5% albedo -- 49.8 sec chord
Diameter=111.9 km assuming a 30% albedo -- 20.3 sec chord
Dynamical classification is CLASSICAL
 
 
 
 
 
 
 
 

Star training set for 13EM149, (2023/08/12 10:49UT)
Object            RA         Dec     mag  sep  mel
Antares        16:30:51.5 -26:28:56  0.9 22.64 154
27Bet Lib      15:18:16.9 -09:28:07  2.6  6.33 132
21Nu Lib       15:07:56.9 -16:20:49  5.2  1.25 132
PPM 229720     15:06:03.2 -15:05:17  8.1  0.17 131
13EM149        15:06:45.1 -15:08:01 16.2       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 13EM149, (2023/08/12 10:49UT)
Object            RA         Dec     mag  sep  mel
Antares        16:29:24.4 -26:25:56  0.9 22.64 154
27Bet Lib      15:17:00.3 -09:22:59  2.6  6.33 132
21Nu Lib       15:06:37.6 -16:15:25  5.2  1.25 132
PPM 229720     15:04:44.4 -14:59:51  8.1  0.17 131
13EM149        15:05:26.3 -15:02:36 16.2       132
Positions are for J2000

Event circumstances last updated at 2023/07/28 03:52:47 UT

Marc W. Buie, Southwest Research Institute

RECON