RECON: TNO occultation with 15VW169

Event between 15VW169 and star GA1060:00386722 with event index number of 1021191

Geocentric closest approach at 2019/12/09 18:28:54 UTC

J2000 position of star is 03:39:45.2 +17:52:51
Equinox of date position of star is 03:40:50.6 +17:56:30
Stellar brightness G=16.7, use SENSEUP=128
Star is 9 degrees from the moon. Moon is 94% illuminated.
TNO apparent brightness V=24.2

TNO is 49.2 AU from the Sun and 48.3 AU from the Earth.
The TNO is moving 24.5 km/sec on the sky relative to the star, or, 2.5 arcsec/hr.
The 1-sigma error in the time of the event is 974 seconds.
The 1-sigma cross-track error in the shadow position is 3010 km.

The TNO has an absolute magnitude Hv=7.3
Diameter=205.1 km assuming a 5% albedo -- 8.4 sec chord
Diameter=83.7 km assuming a 30% albedo -- 3.4 sec chord
Dynamical classification is SCATEXTD
 
 
 
 
 
 
 
 

Star training set for 15VW169, (2019/12/09 18:29UT)
Object            RA         Dec     mag  sep  mel
Aldebaran      04:37:04.0 +16:32:52  0.8 13.48  22
44Zet Per      03:55:23.4 +31:56:28  2.8 14.37  21
PPM 119253     03:40:33.6 +16:36:01  6.2  1.35   8
PPM 119223     03:38:10.8 +18:25:44  8.3  0.81   9
PPM 119252     03:40:32.6 +17:57:08  9.9  0.08   9
15VW169        03:40:53.5 +17:56:40 16.7         9
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 15VW169, (2019/12/09 18:29UT)
Object            RA         Dec     mag  sep  mel
Aldebaran      04:35:55.3 +16:30:30  0.8 13.48  22
44Zet Per      03:54:07.9 +31:53:01  2.8 14.37  21
PPM 119253     03:39:25.8 +16:32:11  6.2  1.35   8
PPM 119223     03:37:02.3 +18:21:51  8.3  0.81   9
PPM 119252     03:39:24.3 +17:53:19  9.9  0.08   9
15VW169        03:39:45.2 +17:52:51 16.7         9
Positions are for J2000

Event circumstances last updated at 2019/01/30 20:41:11 UT

Marc W. Buie, Southwest Research Institute

RECON