RECON: TNO occultation with 14GT53

Event between 14GT53 and star GA0680:06135905 with event index number of 274395

Geocentric closest approach at 2020/06/17 00:21:58 UTC

J2000 position of star is 15:10:06.5 -21:45:11
Equinox of date position of star is 15:11:13.9 -21:49:33
Stellar brightness G=15.0, use SENSEUP=128
Star is 164 degrees from the moon. Moon is 17% illuminated.
TNO apparent brightness V=22.3

TNO is 45.4 AU from the Sun and 44.6 AU from the Earth.
The TNO is moving 19.8 km/sec on the sky relative to the star, or, 2.2 arcsec/hr.
The 1-sigma error in the time of the event is 168 seconds.
The 1-sigma cross-track error in the shadow position is 2457 km.

The TNO has an absolute magnitude Hv=5.7
Diameter=438.5 km assuming a 5% albedo -- 22.2 sec chord
Diameter=179.0 km assuming a 30% albedo -- 9.1 sec chord
Dynamical classification is CLASSICAL
 
 
 
 
 
 
 
 

Star training set for 14GT53, (2020/06/17 00:22UT)
Object            RA         Dec     mag  sep  mel
Antares        16:30:39.9 -26:28:32  0.9 18.67 146
7Del Sco       16:01:32.8 -22:40:42  2.3 11.66 154
PPM 264038     15:17:34.4 -22:28:26  5.5  1.59 163
PPM 263852     15:09:32.7 -22:10:30  8.0  0.53 164
PPM 263887     15:10:56.7 -21:49:05  8.9  0.08 164
14GT53         15:11:17.5 -21:49:47 15.0       164
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 14GT53, (2020/06/17 00:22UT)
Object            RA         Dec     mag  sep  mel
Antares        16:29:24.4 -26:25:56  0.9 18.67 146
7Del Sco       16:00:20.0 -22:37:18  2.3 11.66 154
PPM 264038     15:16:23.0 -22:23:58  5.5  1.59 163
PPM 263852     15:08:21.7 -22:05:51  8.0  0.53 164
PPM 263887     15:09:45.8 -21:44:28  8.9  0.08 164
14GT53         15:10:06.5 -21:45:11 15.0       164
Positions are for J2000

Event circumstances last updated at 2019/06/07 23:51:52 UT

Marc W. Buie, Southwest Research Institute

RECON