RECON: TNO occultation with 04KC19

Event between 04KC19 and star GA0680:15225770 with event index number of 258961

Geocentric closest approach at 2018/06/18 19:18:05 UTC

J2000 position of star is 17:38:22.8 -20:55:37
Equinox of date position of star is 17:39:28.8 -20:56:10
Stellar brightness G=16.9, use SENSEUP=128
Star is 109 degrees from the moon. Moon is 32% illuminated.
TNO apparent brightness V=23.2

TNO is 30.3 AU from the Sun and 29.3 AU from the Earth.
The TNO is moving 23.3 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 197 seconds.
The 1-sigma cross-track error in the shadow position is 1084 km.

The TNO has an absolute magnitude Hv=8.5
Diameter=121.3 km assuming a 5% albedo -- 5.2 sec chord
Diameter=49.5 km assuming a 30% albedo -- 2.1 sec chord
Dynamical classification is 3:2E
 
 
 
 
 
 
 
 

Star training set for 04KC19, (2018/06/18 19:18UT)
Object            RA         Dec     mag  sep  mel
Antares        16:30:32.5 -26:28:17  0.9 16.71  94
35Eta Oph      17:11:26.3 -15:44:48  2.6  8.44 101
PPM 267109     17:39:51.5 -21:55:19  6.4  0.99 109
PPM 267087     17:38:56.7 -20:40:38  8.4  0.29 108
PPM 267110     17:39:51.8 -20:58:11  9.4  0.09 109
04KC19         17:39:29.0 -20:56:11 16.9       109
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 04KC19, (2018/06/18 19:18UT)
Object            RA         Dec     mag  sep  mel
Antares        16:29:24.4 -26:25:56  0.9 16.71  94
35Eta Oph      17:10:22.7 -15:43:29  2.6  8.44 101
PPM 267109     17:38:44.8 -21:54:46  6.4  0.99 109
PPM 267087     17:37:50.6 -20:40:03  8.4  0.29 108
PPM 267110     17:38:45.6 -20:57:37  9.4  0.09 109
04KC19         17:38:22.8 -20:55:37 16.9       109
Positions are for J2000

Event circumstances last updated at 2018/06/05 16:09:23 UT

Marc W. Buie, Southwest Research Institute

RECON