RECON: TNO occultation with 31824

Event between (31824) Elatus and star GA0840:04320189 with event index number of 2195479

Geocentric closest approach at 2021/12/18 06:09:54 UTC

J2000 position of star is 13:43:21.0 -05:47:01
Equinox of date position of star is 13:44:29.3 -05:53:33
Stellar brightness G=15.2, use SENSEUP=128 with the MallinCam and and exposure time of 2 seconds with the QHY174 camera.
Star is 129 degrees from the moon. Moon is 99% illuminated.
TNO apparent brightness V=22.5

TNO is 16.0 AU from the Sun and 16.5 AU from the Earth.
The TNO is moving 20.9 km/sec on the sky relative to the star, or, 6.3 arcsec/hr.
The 1-sigma error in the time of the event is 59 seconds.
The 1-sigma cross-track error in the shadow position is 850 km.

The TNO has an absolute magnitude Hv=10.1
Diameter=56.5 km assuming a 5% albedo -- 2.7 sec chord
Diameter=23.1 km assuming a 30% albedo -- 1.1 sec chord
Dynamical classification is CENTAURR
 
 
 
 
 
 
 
 

Star training set for 31824, (2021/12/18 06:10UT)
Object            RA         Dec     mag  sep  mel
Spica          13:26:21.2 -11:16:31  1.0  7.00 127
80 Vir         13:36:40.0 -05:30:27  5.7  1.99 127
PPM 196818     13:45:03.0 -05:36:32  7.1  0.32 129
PPM 196810     13:44:49.0 -05:42:36  9.3  0.20 129
31824          13:44:29.9 -05:53:36 15.2       130
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 31824, (2021/12/18 06:10UT)
Object            RA         Dec     mag  sep  mel
Spica          13:25:11.5 -11:09:41  1.0  7.00 127
80 Vir         13:35:31.3 -05:23:44  5.7  1.99 127
PPM 196818     13:43:54.2 -05:29:57  7.1  0.32 129
PPM 196810     13:43:40.2 -05:36:01  9.3  0.20 129
31824          13:43:21.0 -05:47:01 15.2       129
Positions are for J2000

Event circumstances last updated at 2021/10/10 01:01:12 UT

Marc W. Buie, Southwest Research Institute

RECON