RECON: TNO occultation with 14JT80

Event between 14JT80 and star GA0780:06539269 with event index number of 1045692

Geocentric closest approach at 2019/10/12 04:58:02 UTC

J2000 position of star is 17:28:04.5 -10:28:21
Equinox of date position of star is 17:29:09.0 -10:29:14
Stellar brightness G=14.4, use SENSEUP=128
Star is 99 degrees from the moon. Moon is 97% illuminated.
TNO apparent brightness V=22.6

TNO is 31.9 AU from the Sun and 32.4 AU from the Earth.
The TNO is moving 20.4 km/sec on the sky relative to the star, or, 3.1 arcsec/hr.
The 1-sigma error in the time of the event is 338 seconds.
The 1-sigma cross-track error in the shadow position is 3151 km.

The TNO has an absolute magnitude Hv=7.4
Diameter=203.2 km assuming a 5% albedo -- 9.9 sec chord
Diameter=83.0 km assuming a 30% albedo -- 4.1 sec chord
Dynamical classification is 3:2E
 
 
 
 
 
 
 
 

Star training set for 14JT80, (2019/10/12 04:58UT)
Object            RA         Dec     mag  sep  mel
Antares        16:30:37.4 -26:28:27  0.9 21.13 110
35Eta Oph      17:11:30.8 -15:44:53  2.6  6.79 103
PPM 233365     17:39:15.4 -10:56:12  5.7  2.52  96
PPM 200710     17:30:22.2 -10:00:18  7.8  0.57  99
PPM 233108     17:29:02.2 -10:27:00  9.4  0.05  99
14JT80         17:29:10.2 -10:29:15 14.4        99
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 14JT80, (2019/10/12 04:58UT)
Object            RA         Dec     mag  sep  mel
Antares        16:29:24.4 -26:25:56  0.9 21.13 110
35Eta Oph      17:10:22.7 -15:43:29  2.6  6.79 103
PPM 233365     17:38:09.5 -10:55:35  5.7  2.52  96
PPM 200710     17:29:16.7 -09:59:26  7.8  0.57  99
PPM 233108     17:27:56.6 -10:26:05  9.4  0.05  99
14JT80         17:28:04.5 -10:28:21 14.4        99
Positions are for J2000

Event circumstances last updated at 2019/06/07 22:44:47 UT

Marc W. Buie, Southwest Research Institute

RECON