RECON: TNO occultation with 612083

Event between (612083) 98WX31 and star GA1140:03009751 with event index number of 2805283

Geocentric closest approach at 2027/12/05 16:31:25 UTC

J2000 position of star is 07:32:58.5 +24:38:59
Equinox of date position of star is 07:34:22.8 +24:35:55
Stellar brightness G=15.5, use SENSEUP=128 with the MallinCam and and exposure time of 2 seconds with the QHY174 camera.
Star is 133 degrees from the moon. Moon is 45% illuminated.
Apparent brightness V=22.9

Object is 41.1 AU from the Sun and 40.4 AU from the Earth.
Apparent velocity is 19.1 km/sec on the sky relative to the star, or, 2.3 arcsec/hr.
The 1-sigma error in the time of the event is 882 seconds.
The 1-sigma cross-track error in the shadow position is 4036 km.

The object has an absolute magnitude Hv=6.7
Diameter=270.4 km assuming a 5% albedo -- 14.2 sec chord
Diameter=110.4 km assuming a 30% albedo -- 5.8 sec chord
Dynamical classification is CLASSICAL
 
 
 
 
 
 
 
 

Star training set for 612083, (2027/12/05 16:20UT)
Object            RA         Dec     mag  sep  mel
Pollux         07:47:01.5 +27:57:23  1.1  4.36 135
PPM 097796     07:40:53.0 +24:09:24  6.0  1.48 135
PPM 097701     07:36:32.3 +24:53:21  8.2  0.52 134
PPM 097626     07:33:30.0 +24:28:27 10.0  0.29 133
612083         07:34:40.1 +24:35:17 15.5       134
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 612083, (2027/12/05 16:20UT)
Object            RA         Dec     mag  sep  mel
Pollux         07:45:17.9 +28:01:33  1.1  4.36 135
PPM 097796     07:39:12.0 +24:13:21  6.0  1.48 135
PPM 097701     07:34:50.6 +24:57:08  8.2  0.52 134
PPM 097626     07:31:48.5 +24:32:07 10.0  0.29 133
612083         07:32:58.5 +24:38:59 15.5       133
Positions are for J2000

Event circumstances last updated at 2023/03/04 04:19:28 UT

Marc W. Buie, Southwest Research Institute

RECON