RECON: TNO occultation with 469442

Event between (469442) 02GG166 and star GA0660:06598218 with event index number of 310246

Geocentric closest approach at 2019/07/03 01:49:07 UTC

J2000 position of star is 15:35:45.8 -22:59:37
Equinox of date position of star is 15:36:54.5 -23:03:25
Stellar brightness G=17.3, use SENSEUP=128
Star is 132 degrees from the moon. Moon is 0% illuminated.
TNO apparent brightness V=20.7

TNO is 18.5 AU from the Sun and 17.7 AU from the Earth.
The TNO is moving 13.8 km/sec on the sky relative to the star, or, 3.9 arcsec/hr.
The 1-sigma error in the time of the event is 151 seconds.
The 1-sigma cross-track error in the shadow position is 1143 km.

The TNO has an absolute magnitude Hv=7.9
Diameter=158.5 km assuming a 5% albedo -- 11.5 sec chord
Diameter=64.7 km assuming a 30% albedo -- 4.7 sec chord
Dynamical classification is CENTAURR
 
 
 
 
 
 
 
 

Star training set for 469442, (2019/07/03 01:49UT)
Object            RA         Dec     mag  sep  mel
Antares        16:30:36.4 -26:28:25  0.9 12.65 145
7Del Sco       16:01:29.4 -22:40:33  2.3  5.67 138
PPM 264469     15:38:57.1 -23:12:18  5.8  0.49 133
PPM 264491     15:39:53.6 -23:06:43  7.1  0.69 133
PPM 264428     15:36:54.1 -23:03:52  9.4  0.01 132
469442         15:36:54.8 -23:03:26 17.3       133
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 469442, (2019/07/03 01:49UT)
Object            RA         Dec     mag  sep  mel
Antares        16:29:24.4 -26:25:56  0.9 12.65 145
7Del Sco       16:00:20.0 -22:37:18  2.3  5.67 138
PPM 264469     15:37:48.0 -23:08:32  5.8  0.49 133
PPM 264491     15:38:44.6 -23:02:58  7.1  0.69 133
PPM 264428     15:35:45.1 -23:00:03  9.4  0.01 132
469442         15:35:45.8 -22:59:37 17.3       132
Positions are for J2000

Event circumstances last updated at 2019/06/07 22:21:55 UT

Marc W. Buie, Southwest Research Institute

RECON