RECON: TNO occultation with 14JL80

Event between 14JL80 and star GA0740:05802090 with event index number of 269907

Geocentric closest approach at 2020/06/08 20:17:02 UTC

J2000 position of star is 16:06:42.2 -14:54:32
Equinox of date position of star is 16:07:45.7 -14:57:29
Stellar brightness G=16.4, use SENSEUP=128
Star is 56 degrees from the moon. Moon is 89% illuminated.
TNO apparent brightness V=21.8

TNO is 28.4 AU from the Sun and 27.4 AU from the Earth.
The TNO is moving 22.0 km/sec on the sky relative to the star, or, 4.0 arcsec/hr.
The 1-sigma error in the time of the event is 155 seconds.
The 1-sigma cross-track error in the shadow position is 1710 km.

The TNO has an absolute magnitude Hv=7.3
Diameter=219.8 km assuming a 5% albedo -- 9.3 sec chord
Diameter=89.7 km assuming a 30% albedo -- 3.8 sec chord
Dynamical classification is 3:2E
 
 
 
 
 
 
 
 

Star training set for 14JL80, (2020/06/08 20:17UT)
Object            RA         Dec     mag  sep  mel
Antares        16:30:39.8 -26:28:32  0.9 12.68  48
8Bet1Sco       16:06:37.7 -19:51:35  2.6  4.91  54
11 Sco         16:08:44.6 -12:47:56  6.1  2.17  56
PPM 231252     16:09:07.6 -14:55:36  8.4  0.31  55
PPM 231236     16:08:34.9 -14:48:40  8.7  0.23  55
14JL80         16:07:51.5 -14:57:45 16.4        55
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 14JL80, (2020/06/08 20:17UT)
Object            RA         Dec     mag  sep  mel
Antares        16:29:24.4 -26:25:56  0.9 12.68  48
8Bet1Sco       16:05:26.2 -19:48:20  2.6  4.91  54
11 Sco         16:07:36.3 -12:44:44  6.1  2.17  56
PPM 231252     16:07:58.4 -14:52:25  8.4  0.31  55
PPM 231236     16:07:25.6 -14:45:28  8.7  0.23  55
14JL80         16:06:42.2 -14:54:32 16.4        55
Positions are for J2000

Event circumstances last updated at 2018/09/21 18:00:10 UT

Marc W. Buie, Southwest Research Institute

RECON