RECON: TNO occultation with 149348

Event between (149348) 02VS130 and star UC4-570-014825 with event index number of 165495

Geocentric closest approach at 2018/11/22 22:20:21 UTC

J2000 position of star is 05:07:25.4 +23:50:10
Equinox of date position of star is 05:08:29.7 +23:51:30
Stellar brightness R=16.6, use SENSEUP=128
Star is 22 degrees from the moon. Moon is 100% illuminated.
TNO apparent brightness V=22.6

TNO is 42.9 AU from the Sun and 41.9 AU from the Earth.
The TNO is moving 24.2 km/sec on the sky relative to the star, or, 2.9 arcsec/hr.
The 1-sigma error in the time of the event is 1526 seconds.
The 1-sigma cross-track error in the shadow position is 3557 km.

The TNO has an absolute magnitude Hv=6.3
Diameter=331.1 km assuming a 5% albedo -- 13.7 sec chord
Diameter=135.2 km assuming a 30% albedo -- 5.6 sec chord
Dynamical classification is CLASSICAL
 
 
 
 
 
 
 
 

Star training set for 149348, (2018/11/22 22:20UT)
Object            RA         Dec     mag  sep  mel
Aldebaran      04:37:00.4 +16:32:45  0.8 10.40  13
Alnath         05:27:29.3 +28:37:18  1.6  6.38  28
103 Tau        05:09:15.8 +24:17:18  5.3  0.46  22
PPM 094048     05:06:20.9 +23:49:25  8.3  0.51  22
PPM 094072     05:08:07.4 +24:03:34  9.6  0.22  22
149348         05:08:34.4 +23:51:35 16.6        22
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 149348, (2018/11/22 22:20UT)
Object            RA         Dec     mag  sep  mel
Aldebaran      04:35:55.3 +16:30:30  0.8 10.40  13
Alnath         05:26:17.5 +28:36:24  1.6  6.38  28
103 Tau        05:08:06.6 +24:15:54  5.3  0.46  22
PPM 094048     05:05:12.0 +23:47:56  8.3  0.51  22
PPM 094072     05:06:58.4 +24:02:09  9.6  0.22  22
149348         05:07:25.4 +23:50:10 16.6        22
Positions are for J2000

Event circumstances last updated at 2017/08/03 16:26:25 UT

Marc W. Buie, Southwest Research Institute

RECON