RECON: TNO occultation with 12DR30

Event between 12DR30 and star UC4-133-026013 with event index number of 153585

Geocentric closest approach at 2018/11/02 06:39:24 UTC

J2000 position of star is 09:44:43.3 -63:31:11
Equinox of date position of star is 09:45:11.2 -63:36:05
Stellar brightness R=13.7, use SENSEUP=64
Star is 77 degrees from the moon. Moon is 32% illuminated.
TNO apparent brightness V=20.2

TNO is 19.0 AU from the Sun and 19.3 AU from the Earth.
The TNO is moving 37.2 km/sec on the sky relative to the star, or, 9.6 arcsec/hr.
The 1-sigma error in the time of the event is 69 seconds.
The 1-sigma cross-track error in the shadow position is 3116 km.

The TNO has an absolute magnitude Hv=7.1
Diameter=227.0 km assuming a 5% albedo -- 6.1 sec chord
Diameter=92.7 km assuming a 30% albedo -- 2.5 sec chord
Dynamical classification is CENTAURS
 
 
 
 
 
 
 
 

Star training set for 12DR30, (2018/11/02 06:39UT)
Object            RA         Dec     mag  sep  mel
Bet Cru        12:48:50.1 -59:47:29  1.3 21.60  80
Iot Car        09:17:35.6 -59:21:17  2.3  5.37  74
PPM 357533     09:45:45.9 -62:35:43  3.4  1.01  76
PPM 357579     09:49:46.1 -63:14:23  8.2  0.63  77
PPM 357531     09:45:38.6 -63:48:18  9.2  0.20  78
12DR30         09:45:13.1 -63:36:25 13.7        77
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 12DR30, (2018/11/02 06:39UT)
Object            RA         Dec     mag  sep  mel
Bet Cru        12:47:43.1 -59:41:20  1.3 21.60  80
Iot Car        09:17:05.4 -59:16:31  2.3  5.37  74
PPM 357533     09:45:14.8 -62:30:28  3.4  1.01  76
PPM 357579     09:49:15.0 -63:09:05  8.2  0.63  77
PPM 357531     09:45:09.0 -63:43:04  9.2  0.20  78
12DR30         09:44:43.3 -63:31:11 13.7        77
Positions are for J2000

Event circumstances last updated at 2017/08/17 16:16:22 UT

Marc W. Buie, Southwest Research Institute

RECON