RECON: TNO occultation with 517717

Event between (517717) 15KZ120 and star GA1240:03949171 with event index number of 267210

Geocentric closest approach at 2018/09/01 00:25:21 UTC

J2000 position of star is 16:52:00.5 +34:12:22
Equinox of date position of star is 16:52:41.1 +34:10:34
Stellar brightness G=16.9, use SENSEUP=128
Star is 126 degrees from the moon. Moon is 72% illuminated.
TNO apparent brightness V=19.8

TNO is 8.4 AU from the Sun and 8.4 AU from the Earth.
The TNO is moving 10.8 km/sec on the sky relative to the star, or, 6.4 arcsec/hr.
The 1-sigma error in the time of the event is 68 seconds.
The 1-sigma cross-track error in the shadow position is 316 km.

The TNO has an absolute magnitude Hv=10.0
Diameter=60.3 km assuming a 5% albedo -- 5.6 sec chord
Diameter=24.6 km assuming a 30% albedo -- 2.3 sec chord
Dynamical classification is CENTAURR
 
 
 
 
 
 
 
 

Star training set for 517717, (2018/09/01 00:25UT)
Object            RA         Dec     mag  sep  mel
Vega           18:37:34.3 +38:48:07  0.0 21.50 107
27Bet Her      16:31:01.4 +21:27:00  2.8 13.59 139
PPM 079591     16:44:33.1 +34:00:19  6.0  1.69 127
PPM 079694     16:51:14.4 +33:46:00  7.9  0.51 127
PPM 079745     16:54:07.9 +34:04:54  9.5  0.31 126
517717         16:52:41.6 +34:10:33 16.9       126
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 517717, (2018/09/01 00:25UT)
Object            RA         Dec     mag  sep  mel
Vega           18:36:56.6 +38:47:06  0.0 21.50 107
27Bet Her      16:30:13.1 +21:29:22  2.8 13.59 139
PPM 079591     16:43:51.6 +34:02:21  6.0  1.69 127
PPM 079694     16:50:32.9 +33:47:51  7.9  0.51 127
PPM 079745     16:53:26.7 +34:06:41  9.5  0.31 126
517717         16:52:00.5 +34:12:22 16.9       126
Positions are for J2000

Event circumstances last updated at 2018/06/05 16:22:40 UT

Marc W. Buie, Southwest Research Institute

RECON