RECON: TNO occultation with 82155

Event between (82155) 01FZ173 and star UC4-339-067729 with event index number of 110435

Geocentric closest approach at 2018/03/17 15:10:14 UTC

J2000 position of star is 14:20:13.8 -22:15:28
Equinox of date position of star is 14:21:12.5 -22:20:12
Stellar brightness R=15.4, use SENSEUP=128
Star is 136 degrees from the moon. Moon is 0% illuminated.
TNO apparent brightness V=21.4

TNO is 33.0 AU from the Sun and 32.3 AU from the Earth.
The TNO is moving 15.5 km/sec on the sky relative to the star, or, 2.4 arcsec/hr.
The 1-sigma error in the time of the event is 603 seconds.
The 1-sigma cross-track error in the shadow position is 5591 km.

The TNO has an absolute magnitude Hv=6.1
Diameter=346.7 km assuming a 5% albedo -- 23.4 sec chord
Diameter=141.6 km assuming a 30% albedo -- 9.6 sec chord
Dynamical classification is SCATNEAR
 
 
 
 
 
 
 
 

Star training set for 82155, (2018/03/17 15:10UT)
Object            RA         Dec     mag  sep  mel
Spica          13:26:09.3 -11:15:21  1.0 17.21 154
5The Cen       14:07:45.6 -36:27:31  2.1 14.42 130
PPM 262884     14:25:51.2 -24:53:17  5.3  2.76 134
PPM 262742     14:18:43.2 -21:54:45  7.6  0.73 137
PPM 262801     14:22:03.7 -21:59:31  9.5  0.40 136
82155          14:21:15.6 -22:20:26 15.4       136
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 82155, (2018/03/17 15:10UT)
Object            RA         Dec     mag  sep  mel
Spica          13:25:11.5 -11:09:41  1.0 17.21 154
5The Cen       14:06:40.2 -36:22:21  2.1 14.42 130
PPM 262884     14:24:48.6 -24:48:23  5.3  2.76 134
PPM 262742     14:17:41.7 -21:49:44  7.6  0.73 137
PPM 262801     14:21:02.1 -21:54:34  9.5  0.40 136
82155          14:20:13.8 -22:15:28 15.4       136
Positions are for J2000

Event circumstances last updated at 2017/04/24 16:20:50 UT

Marc W. Buie, Southwest Research Institute

RECON