RECON: TNO occultation with 02GW31

Event between 02GW31 and star GA0800:04324450 with event index number of 1070681

Geocentric closest approach at 2022/03/06 14:51:08 UTC

J2000 position of star is 13:06:50.9 -08:31:43
Equinox of date position of star is 13:07:59.0 -08:38:40
Stellar brightness G=15.7, use SENSEUP=128 with the MallinCam and and exposure time of 2 seconds with the QHY174 camera.
Star is 165 degrees from the moon. Moon is 16% illuminated.
TNO apparent brightness V=23.6

TNO is 44.3 AU from the Sun and 43.5 AU from the Earth.
The TNO is moving 20.9 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 463 seconds.
The 1-sigma cross-track error in the shadow position is 4141 km.

The TNO has an absolute magnitude Hv=7.1
Diameter=227.0 km assuming a 5% albedo -- 10.9 sec chord
Diameter=92.7 km assuming a 30% albedo -- 4.4 sec chord
Dynamical classification is 3:2E
 
 
 
 
 
 
 
 

Star training set for 02GW31, (2022/03/06 14:49UT)
Object            RA         Dec     mag  sep  mel
Spica          13:26:21.9 -11:16:35  1.0  5.23 170
PPM 196204     13:09:42.0 -09:06:10  5.5  0.62 165
PPM 196140     13:05:56.4 -08:41:23  8.0  0.51 164
PPM 196170     13:07:41.9 -08:35:38  9.2  0.09 165
02GW31         13:08:00.4 -08:38:48 15.7       165
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 02GW31, (2022/03/06 14:49UT)
Object            RA         Dec     mag  sep  mel
Spica          13:25:11.5 -11:09:41  1.0  5.23 170
PPM 196204     13:08:32.4 -08:59:05  5.5  0.62 165
PPM 196140     13:04:47.0 -08:34:16  8.0  0.51 164
PPM 196170     13:06:32.4 -08:28:32  9.2  0.09 165
02GW31         13:06:50.9 -08:31:43 15.7       165
Positions are for J2000

Event circumstances last updated at 2021/10/02 02:47:25 UT

Marc W. Buie, Southwest Research Institute

RECON