RECON: TNO occultation with 12UC178

Event between 12UC178 and star GA1080:00511741 with event index number of 1048189

Geocentric closest approach at 2019/10/12 20:39:06 UTC

J2000 position of star is 04:12:13.5 +18:49:14
Equinox of date position of star is 04:13:20.0 +18:52:07
Stellar brightness G=15.1, use SENSEUP=128
Star is 57 degrees from the moon. Moon is 99% illuminated.
TNO apparent brightness V=22.8

TNO is 39.4 AU from the Sun and 38.7 AU from the Earth.
The TNO is moving 16.4 km/sec on the sky relative to the star, or, 2.1 arcsec/hr.
The 1-sigma error in the time of the event is 127 seconds.
The 1-sigma cross-track error in the shadow position is 1560 km.

The TNO has an absolute magnitude Hv=6.8
Diameter=266.7 km assuming a 5% albedo -- 16.2 sec chord
Diameter=108.9 km assuming a 30% albedo -- 6.6 sec chord
Dynamical classification is 5:3EE
 
 
 
 
 
 
 
 

Star training set for 12UC178, (2019/10/12 20:39UT)
Object            RA         Dec     mag  sep  mel
Aldebaran      04:37:03.5 +16:32:51  0.8  6.10  62
44Zet Per      03:55:22.8 +31:56:27  2.8 13.68  57
43Ome1Tau      04:10:19.3 +19:39:36  5.5  1.07  56
PPM 119720     04:15:23.9 +18:56:34  8.1  0.48  57
PPM 119707     04:14:11.4 +18:54:19 10.8  0.20  57
12UC178        04:13:22.4 +18:52:13 15.1        57
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 12UC178, (2019/10/12 20:39UT)
Object            RA         Dec     mag  sep  mel
Aldebaran      04:35:55.3 +16:30:30  0.8  6.10  62
44Zet Per      03:54:07.9 +31:53:01  2.8 13.68  57
43Ome1Tau      04:09:10.1 +19:36:33  5.5  1.07  56
PPM 119720     04:14:15.0 +18:53:38  8.1  0.48  57
PPM 119707     04:13:02.5 +18:51:21 10.8  0.20  57
12UC178        04:12:13.5 +18:49:14 15.1        57
Positions are for J2000

Event circumstances last updated at 2019/02/01 22:22:37 UT

Marc W. Buie, Southwest Research Institute

RECON