RECON: TNO occultation with 12LB27

Event between 12LB27 and star GA0980:17318440 with event index number of 1793853

Geocentric closest approach at 2021/06/16 17:09:57 UTC

J2000 position of star is 20:30:24.7 +08:29:26
Equinox of date position of star is 20:31:26.8 +08:33:47
Stellar brightness G=16.8, use SENSEUP=128 with the MallinCam and and exposure time of 2 seconds with the QHY174 camera.
Star is 140 degrees from the moon. Moon is 35% illuminated.
TNO apparent brightness V=21.8

TNO is 15.7 AU from the Sun and 15.0 AU from the Earth.
The TNO is moving 14.6 km/sec on the sky relative to the star, or, 4.8 arcsec/hr.
The 1-sigma error in the time of the event is 122 seconds.
The 1-sigma cross-track error in the shadow position is 1010 km.

The TNO has an absolute magnitude Hv=9.7
Diameter=70.5 km assuming a 5% albedo -- 4.8 sec chord
Diameter=28.8 km assuming a 30% albedo -- 2.0 sec chord
Dynamical classification is CENTAURR
 
 
 
 
 
 
 
 

Star training set for 12LB27, (2021/06/16 17:10UT)
Object            RA         Dec     mag  sep  mel
Vega           18:37:39.9 +38:48:17  0.0 39.57 102
Tarazed        19:47:16.8 +10:40:01  2.7 11.09 129
PPM 170088     20:29:10.2 +08:30:35  6.3  0.57 139
PPM 170156     20:31:38.3 +08:44:35  8.6  0.19 140
12LB27         20:31:27.3 +08:33:49 16.8       140
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 12LB27, (2021/06/16 17:10UT)
Object            RA         Dec     mag  sep  mel
Vega           18:36:56.7 +38:47:07  0.0 39.57 102
Tarazed        19:46:15.6 +10:36:48  2.7 11.09 129
PPM 170088     20:28:07.6 +08:26:15  6.3  0.57 139
PPM 170156     20:30:35.8 +08:40:11  8.6  0.19 140
12LB27         20:30:24.7 +08:29:26 16.8       140
Positions are for J2000

Event circumstances last updated at 2021/04/21 22:32:43 UT

Marc W. Buie, Southwest Research Institute

RECON