RECON: TNO occultation with 307251

Event between (307251) 02KW14 and star GA0640:09674084 with event index number of 356721

Geocentric closest approach at 2019/06/04 03:23:33 UTC

J2000 position of star is 16:58:37.8 -25:31:40
Equinox of date position of star is 16:59:48.4 -25:33:21
Stellar brightness G=15.4, use SENSEUP=128
Star is 172 degrees from the moon. Moon is 1% illuminated.
TNO apparent brightness V=21.8

TNO is 42.4 AU from the Sun and 41.4 AU from the Earth.
The TNO is moving 24.7 km/sec on the sky relative to the star, or, 3.0 arcsec/hr.
The 1-sigma error in the time of the event is 254 seconds.
The 1-sigma cross-track error in the shadow position is 2614 km.

The TNO has an absolute magnitude Hv=5.6
Diameter=457.1 km assuming a 5% albedo -- 18.5 sec chord
Diameter=186.6 km assuming a 30% albedo -- 7.6 sec chord
Dynamical classification is SCATEXTD
 
 
 
 
 
 
 
 

Star training set for 307251, (2019/06/04 03:24UT)
Object            RA         Dec     mag  sep  mel
Antares        16:30:36.1 -26:28:24  0.9  6.63 166
23Tau Sco      16:37:05.7 -28:15:17  2.8  5.74 166
26 Oph         17:01:21.1 -25:01:01  5.8  0.64 172
PPM 266202     16:59:28.7 -26:05:14  7.4  0.54 172
PPM 266236     17:00:40.3 -25:43:39  9.2  0.26 172
307251         16:59:49.5 -25:33:22 15.4       172
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, (2019/06/04 03:24UT)
Object            RA         Dec     mag  sep  mel
Antares        16:29:24.4 -26:25:56  0.9  6.63 166
23Tau Sco      16:35:53.0 -28:12:58  2.8  5.74 166
26 Oph         17:00:09.6 -24:59:22  5.8  0.64 172
PPM 266202     16:58:16.7 -26:03:32  7.4  0.54 172
PPM 266236     16:59:28.5 -25:41:58  9.2  0.26 172
307251         16:58:37.8 -25:31:40 15.4       172
Positions are for J2000

Event circumstances last updated at 2019/02/12 08:20:48 UT

Marc W. Buie, Southwest Research Institute

RECON