RECON: TNO occultation with 531017

Event between (531017) 12BA155 and star GA0800:04077256 with event index number of 2439607

Geocentric closest approach at 2027/12/10 20:15:49 UTC

J2000 position of star is 11:14:04.5 -08:16:49
Equinox of date position of star is 11:15:18.8 -08:24:50
Stellar brightness G=16.8, use SENSEUP=128 with the MallinCam and and exposure time of 2 seconds with the QHY174 camera.
Star is 131 degrees from the moon. Moon is 90% illuminated.
Apparent brightness V=21.9

Object is 36.8 AU from the Sun and 36.9 AU from the Earth.
Apparent velocity is 9.6 km/sec on the sky relative to the star, or, 1.3 arcsec/hr.
The 1-sigma error in the time of the event is 237 seconds.
The 1-sigma cross-track error in the shadow position is 1887 km.

The object has an absolute magnitude Hv=6.1
Diameter=354.8 km assuming a 5% albedo -- 38.3 sec chord
Diameter=144.9 km assuming a 30% albedo -- 15.7 sec chord
Dynamical classification is 5:2EEE
 
 
 
 
 
 
 
 

Star training set for 531017, (2027/12/10 20:18UT)
Object            RA         Dec     mag  sep  mel
Regulus        10:09:51.5 +11:49:46  1.3 26.01 108
4Gam Crv       12:17:14.9 -17:41:49  2.6 17.65 148
PPM 194312     11:18:23.2 -07:17:15  6.1  1.35 131
PPM 194258     11:15:37.7 -08:28:50  7.1  0.06 131
531017         11:15:29.3 -08:25:58 16.8       131
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 531017, (2027/12/10 20:18UT)
Object            RA         Dec     mag  sep  mel
Regulus        10:08:21.9 +11:58:02  1.3 26.01 108
4Gam Crv       12:15:48.1 -17:32:30  2.6 17.65 148
PPM 194312     11:16:58.2 -07:08:05  6.1  1.35 131
PPM 194258     11:14:12.9 -08:19:40  7.1  0.06 131
531017         11:14:04.5 -08:16:49 16.8       131
Positions are for J2000

Event circumstances last updated at 2024/06/23 21:27:34 UT

Marc W. Buie, Southwest Research Institute

RECON