RECON: TNO occultation with 250112

Event between (250112) 02KY14 and star GA0980:02579009 with event index number of 356226

Geocentric closest approach at 2019/12/06 02:36:39 UTC

J2000 position of star is 07:01:44.6 +09:30:25
Equinox of date position of star is 07:02:48.5 +09:28:41
Stellar brightness G=15.4, use SENSEUP=128
Star is 101 degrees from the moon. Moon is 67% illuminated.
TNO apparent brightness V=21.1

TNO is 13.4 AU from the Sun and 12.6 AU from the Earth.
The TNO is moving 19.4 km/sec on the sky relative to the star, or, 7.6 arcsec/hr.
The 1-sigma error in the time of the event is 91 seconds.
The 1-sigma cross-track error in the shadow position is 828 km.

The TNO has an absolute magnitude Hv=9.7
Diameter=69.2 km assuming a 5% albedo -- 3.6 sec chord
Diameter=28.2 km assuming a 30% albedo -- 1.5 sec chord
Dynamical classification is CENTAURR
 
 
 
 
 
 
 
 

Star training set for 250112, (2019/12/06 02:37UT)
Object            RA         Dec     mag  sep  mel
Betelgeuse     05:56:15.1 +07:24:33  0.4 16.59  84
Alhena         06:38:51.8 +16:22:50  1.9  9.04  95
PPM 151820     07:04:23.3 +09:06:28  6.0  0.53 101
PPM 151767     07:02:45.3 +09:41:02  8.9  0.21 101
PPM 151785     07:03:13.9 +09:31:49 10.4  0.11 101
250112         07:02:50.2 +09:28:38 15.4       101
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 250112, (2019/12/06 02:37UT)
Object            RA         Dec     mag  sep  mel
Betelgeuse     05:55:10.3 +07:24:26  0.4 16.59  84
Alhena         06:37:42.8 +16:23:57  1.9  9.04  95
PPM 151820     07:03:17.9 +09:08:18  6.0  0.53 101
PPM 151767     07:01:39.6 +09:42:49  8.9  0.21 101
PPM 151785     07:02:08.3 +09:33:37 10.4  0.11 101
250112         07:01:44.6 +09:30:25 15.4       101
Positions are for J2000

Event circumstances last updated at 2019/06/07 22:57:16 UT

Marc W. Buie, Southwest Research Institute

RECON