RECON: TNO occultation with 01VN71

Event between 01VN71 and star GA1220:02850712 with event index number of 168610

Geocentric closest approach at 2018/12/12 15:36:25 UTC

J2000 position of star is 06:39:40.2 +32:16:46
Equinox of date position of star is 06:40:53.8 +32:15:40
Stellar brightness G=16.3, use SENSEUP=128
Star is 138 degrees from the moon. Moon is 24% illuminated.
TNO apparent brightness V=23.7

TNO is 30.4 AU from the Sun and 29.5 AU from the Earth.
The TNO is moving 23.3 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 334 seconds.
The 1-sigma cross-track error in the shadow position is 2325 km.

The TNO has an absolute magnitude Hv=8.9
Diameter=102.3 km assuming a 5% albedo -- 4.4 sec chord
Diameter=41.8 km assuming a 30% albedo -- 1.8 sec chord
Dynamical classification is 3:2E
 
 
 
 
 
 
 
 

Star training set for 01VN71, (2018/12/12 15:36UT)
Object            RA         Dec     mag  sep  mel
Pollux         07:46:28.4 +27:58:44  1.1 14.79 153
PPM 071742     06:33:41.3 +32:26:24  6.0  1.53 137
PPM 071904     06:40:19.5 +31:44:53  7.8  0.53 138
PPM 071939     06:42:23.8 +32:23:51  9.5  0.34 139
PPM 071911     06:40:52.1 +31:55:11 10.3  0.34 139
01VN71         06:40:54.2 +32:15:40 16.3       139
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 01VN71, (2018/12/12 15:36UT)
Object            RA         Dec     mag  sep  mel
Pollux         07:45:18.1 +28:01:33  1.1 14.79 153
PPM 071742     06:32:27.2 +32:27:18  6.0  1.53 137
PPM 071904     06:39:05.8 +31:45:58  7.8  0.53 138
PPM 071939     06:41:09.7 +32:25:00  9.5  0.34 139
PPM 071911     06:39:38.3 +31:56:17 10.3  0.34 139
01VN71         06:39:40.2 +32:16:46 16.3       138
Positions are for J2000

Event circumstances last updated at 2018/11/04 22:24:16 UT

Marc W. Buie, Southwest Research Institute

RECON