RECON: TNO occultation with 14TX85

Event between 14TX85 and star GA0960:00300329 with event index number of 219376

Geocentric closest approach at 2019/10/23 16:10:21 UTC

J2000 position of star is 03:30:13.5 +07:01:41
Equinox of date position of star is 03:31:15.8 +07:05:37
Stellar brightness G=16.6, use SENSEUP=128
Star is 97 degrees from the moon. Moon is 27% illuminated.
TNO apparent brightness V=22.5

TNO is 36.3 AU from the Sun and 35.4 AU from the Earth.
The TNO is moving 23.3 km/sec on the sky relative to the star, or, 3.3 arcsec/hr.
The 1-sigma error in the time of the event is 142 seconds.
The 1-sigma cross-track error in the shadow position is 1916 km.

The TNO has an absolute magnitude Hv=6.9
Diameter=254.7 km assuming a 5% albedo -- 10.9 sec chord
Diameter=104.0 km assuming a 30% albedo -- 4.5 sec chord
Dynamical classification is SCATEXTD
 
 
 
 
 
 
 
 

Star training set for 14TX85, (2019/10/23 16:10UT)
Object            RA         Dec     mag  sep  mel
Aldebaran      04:37:03.6 +16:32:51  0.8 18.65  79
Menkar         03:03:19.0 +04:09:59  2.5  7.55 104
1Omi Tau       03:25:52.9 +09:05:50  3.6  2.41  97
PPM 146592     03:29:16.6 +07:22:10  8.5  0.57  97
PPM 146634     03:32:05.0 +07:15:53  8.6  0.26  96
14TX85         03:31:17.0 +07:05:42 16.6        96
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 14TX85, (2019/10/23 16:10UT)
Object            RA         Dec     mag  sep  mel
Aldebaran      04:35:55.3 +16:30:30  0.8 18.65  79
Menkar         03:02:16.8 +04:05:21  2.5  7.55 104
1Omi Tau       03:24:48.7 +09:01:42  3.6  2.41  97
PPM 146592     03:28:13.0 +07:18:06  8.5  0.57  97
PPM 146634     03:31:01.4 +07:11:54  8.6  0.26  96
14TX85         03:30:13.5 +07:01:41 16.6        97
Positions are for J2000

Event circumstances last updated at 2019/06/07 22:48:16 UT

Marc W. Buie, Southwest Research Institute

RECON