RECON: TNO occultation with 307251

Event between (307251) 02KW14 and star GA0600:33902597 with event index number of 2754125

Geocentric closest approach at 2029/05/20 03:59:14 UTC

J2000 position of star is 17:57:27.8 -28:17:31
Equinox of date position of star is 17:59:00.7 -28:17:35
Stellar brightness G=15.7, 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 39% illuminated.
Apparent brightness V=22.0

Object is 44.2 AU from the Sun and 43.4 AU from the Earth.
Apparent velocity is 20.9 km/sec on the sky relative to the star, or, 2.4 arcsec/hr.
The 1-sigma error in the time of the event is 1274 seconds.
The 1-sigma cross-track error in the shadow position is 4689 km.

The object has an absolute magnitude Hv=5.5
Diameter=457.1 km assuming a 5% albedo -- 22.8 sec chord
Diameter=186.6 km assuming a 30% albedo -- 9.3 sec chord
Dynamical classification is SCATEXTD
 
 
 
 
 
 
 
 

Star training set for 307251, (2029/05/20 03:59UT)
Object            RA         Dec     mag  sep  mel
Antares        16:31:12.8 -26:29:40  0.9 19.61 113
34Ups Sco      17:32:45.9 -37:18:58  2.7 10.60 125
Gam1Sgr        18:06:53.8 -29:34:33  4.7  2.10 134
PPM 267596     18:00:30.9 -28:45:34  6.6  0.54 132
307251         17:59:19.3 -28:17:35 15.7       133
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 307251, (2029/05/20 03:59UT)
Object            RA         Dec     mag  sep  mel
Antares        16:29:24.4 -26:25:56  0.9 19.61 113
34Ups Sco      17:30:45.8 -37:17:46  2.7 10.60 125
Gam1Sgr        18:05:01.2 -29:34:48  4.7  2.10 134
PPM 267596     17:58:39.0 -28:45:33  6.6  0.54 132
307251         17:57:27.8 -28:17:31 15.7       132
Positions are for J2000

Event circumstances last updated at 2024/06/26 21:35:29 UT

Marc W. Buie, Southwest Research Institute

RECON