RECON: TNO occultation with 491768

Event between (491768) 12VV113 and star GA0900:00258820 with event index number of 236152

Geocentric closest approach at 2019/12/16 22:24:37 UTC

J2000 position of star is 03:05:26.3 +01:41:34
Equinox of date position of star is 03:06:26.7 +01:46:03
Stellar brightness G=12.8, use SENSEUP=32
Star is 101 degrees from the moon. Moon is 75% illuminated.
TNO apparent brightness V=23.6

TNO is 40.8 AU from the Sun and 40.0 AU from the Earth.
The TNO is moving 19.0 km/sec on the sky relative to the star, or, 2.4 arcsec/hr.
The 1-sigma error in the time of the event is 281 seconds.
The 1-sigma cross-track error in the shadow position is 2491 km.

The TNO has an absolute magnitude Hv=7.4
Diameter=199.5 km assuming a 5% albedo -- 10.5 sec chord
Diameter=81.5 km assuming a 30% albedo -- 4.3 sec chord
Dynamical classification is SCATEXTD
 
 
 
 
 
 
 
 

Star training set for 491768, (2019/12/16 22:25UT)
Object            RA         Dec     mag  sep  mel
Aldebaran      04:37:04.1 +16:32:52  0.8 26.74  75
Menkar         03:03:19.5 +04:10:01  2.5  2.52 101
93 Cet         03:03:25.4 +04:25:50  5.4  2.77 101
PPM 146201     03:05:40.1 +01:56:26  7.0  0.26 101
PPM 146212     03:06:06.5 +01:59:10 10.7  0.23 101
491768         03:06:28.3 +01:46:10 12.8       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 491768, (2019/12/16 22:25UT)
Object            RA         Dec     mag  sep  mel
Aldebaran      04:35:55.3 +16:30:30  0.8 26.74  75
Menkar         03:02:16.8 +04:05:21  2.5  2.52 101
93 Cet         03:02:22.5 +04:21:11  5.4  2.77 101
PPM 146201     03:04:38.1 +01:51:49  7.0  0.26 101
PPM 146212     03:05:04.4 +01:54:34 10.7  0.23 101
491768         03:05:26.3 +01:41:34 12.8       101
Positions are for J2000

Event circumstances last updated at 2019/06/07 23:01:44 UT

Marc W. Buie, Southwest Research Institute

RECON