RECON: TNO occultation with 12UB178

Event between 12UB178 and star UC4-514-006770 with event index number of 239590

Geocentric closest approach at 2018/11/10 21:08:22 UTC

J2000 position of star is 04:04:13.3 +12:37:38
Equinox of date position of star is 04:05:14.7 +12:40:36
Stellar brightness R=15.5, use SENSEUP=128
Star is 155 degrees from the moon. Moon is 11% illuminated.
TNO apparent brightness V=22.5

TNO is 47.0 AU from the Sun and 46.0 AU from the Earth.
The TNO is moving 25.3 km/sec on the sky relative to the star, or, 2.7 arcsec/hr.
The 1-sigma error in the time of the event is 609 seconds.
The 1-sigma cross-track error in the shadow position is 4753 km.

The TNO has an absolute magnitude Hv=5.8
Diameter=424.6 km assuming a 5% albedo -- 16.8 sec chord
Diameter=173.4 km assuming a 30% albedo -- 6.9 sec chord
Dynamical classification is CLASSICAL
 
 
 
 
 
 
 
 

Star training set for 12UB178, (2018/11/10 21:08UT)
Object            RA         Dec     mag  sep  mel
Aldebaran      04:37:00.3 +16:32:45  0.8  8.59 163
Menkar         03:03:16.1 +04:09:46  2.5 17.53 137
35Lam Tau      04:01:43.7 +12:32:32  3.5  0.88 154
PPM 119597     04:06:14.4 +13:20:49  8.3  0.71 155
PPM 119590     04:05:21.8 +12:33:29  8.7  0.12 155
12UB178        04:05:16.3 +12:40:41 15.5       155
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 12UB178, (2018/11/10 21:08UT)
Object            RA         Dec     mag  sep  mel
Aldebaran      04:35:55.3 +16:30:30  0.8  8.59 163
Menkar         03:02:16.8 +04:05:21  2.5 17.53 137
35Lam Tau      04:00:40.8 +12:29:25  3.5  0.88 154
PPM 119597     04:05:11.2 +13:17:49  8.3  0.71 155
PPM 119590     04:04:18.8 +12:30:27  8.7  0.12 155
12UB178        04:04:13.3 +12:37:38 15.5       155
Positions are for J2000

Event circumstances last updated at 2018/05/24 01:55:56 UT

Marc W. Buie, Southwest Research Institute

RECON