RECON: TNO occultation with 119473

Event between (119473) 01UO18 and star UC4-553-006927 with event index number of 93906

Geocentric closest approach at 2017/12/08 23:14:10 UTC

J2000 position of star is 03:31:38.7 +20:24:37
Equinox of date position of star is 03:32:38.9 +20:28:05
Stellar brightness R=15.1, use SENSEUP=128
Star is 94 degrees from the moon. Moon is 65% illuminated.
TNO apparent brightness V=22.4

TNO is 29.0 AU from the Sun and 28.1 AU from the Earth.
The TNO is moving 21.9 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 443 seconds.
The 1-sigma cross-track error in the shadow position is 4341 km.

The TNO has an absolute magnitude Hv=7.8
Diameter=166.0 km assuming a 5% albedo -- 7.6 sec chord
Diameter=67.8 km assuming a 30% albedo -- 3.1 sec chord
Dynamical classification is 3:2E
 
 
 
 
 
 
 
 

Star training set for 119473, (2017/12/08 23:14UT)
Object            RA         Dec     mag  sep  mel
Aldebaran      04:36:57.1 +16:32:38  0.8 15.73  80
44Zet Per      03:55:15.8 +31:56:08  2.8 12.53  87
65 Ari         03:25:28.3 +20:51:57  5.9  1.73  96
PPM 092559     03:31:32.8 +20:09:48  8.4  0.41  95
PPM 092591     03:33:29.4 +20:14:07  9.0  0.30  94
119473         03:32:41.0 +20:28:13 15.1        94
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 119473, (2017/12/08 23:14UT)
Object            RA         Dec     mag  sep  mel
Aldebaran      04:35:55.3 +16:30:30  0.8 15.73  80
44Zet Per      03:54:07.9 +31:53:01  2.8 12.53  87
65 Ari         03:24:26.1 +20:48:12  5.9  1.73  96
PPM 092559     03:30:30.6 +20:06:11  8.4  0.41  95
PPM 092591     03:32:27.1 +20:10:32  9.0  0.30  94
119473         03:31:38.7 +20:24:37 15.1        94
Positions are for J2000

Event circumstances last updated at 2017/04/24 16:15:01 UT

Marc W. Buie, Southwest Research Institute

RECON