RECON: TNO occultation with 14SJ349

Event between 14SJ349 and star GA1000:00313042 with event index number of 249640

Geocentric closest approach at 2018/12/08 16:50:42 UTC

J2000 position of star is 03:32:17.9 +10:14:53
Equinox of date position of star is 03:33:19.4 +10:18:39
Stellar brightness G=15.8, use SENSEUP=128
Star is 141 degrees from the moon. Moon is 2% illuminated.
TNO apparent brightness V=22.4

TNO is 35.4 AU from the Sun and 34.5 AU from the Earth.
The TNO is moving 22.5 km/sec on the sky relative to the star, or, 3.2 arcsec/hr.
The 1-sigma error in the time of the event is 374 seconds.
The 1-sigma cross-track error in the shadow position is 4357 km.

The TNO has an absolute magnitude Hv=6.9
Diameter=252.4 km assuming a 5% albedo -- 11.2 sec chord
Diameter=103.0 km assuming a 30% albedo -- 4.6 sec chord
Dynamical classification is 5:3EE
 
 
 
 
 
 
 
 

Star training set for 14SJ349, (2018/12/08 16:51UT)
Object            RA         Dec     mag  sep  mel
Aldebaran      04:37:00.6 +16:32:45  0.8 16.68 157
Menkar         03:03:16.3 +04:09:47  2.5  9.66 131
6 Tau          03:33:37.5 +09:26:10  5.6  0.88 140
PPM 119160     03:33:29.3 +10:48:06  8.4  0.49 141
PPM 119181     03:34:50.8 +10:17:46 10.1  0.37 141
14SJ349        03:33:19.8 +10:18:40 15.8       141
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 14SJ349, (2018/12/08 16:51UT)
Object            RA         Dec     mag  sep  mel
Aldebaran      04:35:55.3 +16:30:30  0.8 16.68 157
Menkar         03:02:16.8 +04:05:21  2.5  9.66 131
6 Tau          03:32:35.9 +09:22:23  5.6  0.88 140
PPM 119160     03:32:27.2 +10:44:19  8.4  0.49 141
PPM 119181     03:33:48.9 +10:14:01 10.1  0.37 141
14SJ349        03:32:17.9 +10:14:53 15.8       140
Positions are for J2000

Event circumstances last updated at 2018/10/19 22:09:28 UT

Marc W. Buie, Southwest Research Institute

RECON