RECON: TNO occultation with 523640

Event between (523640) 10RO64 and star GA0880:00138870 with event index number of 1055415

Geocentric closest approach at 2021/02/08 18:40:36 UTC

J2000 position of star is 01:41:00.7 -00:27:31
Equinox of date position of star is 01:42:05.3 -00:21:10
Stellar brightness G=14.9, use SENSEUP=128 with the MallinCam and and exposure time of 2 seconds with the QHY174 camera.
Star is 100 degrees from the moon. Moon is 11% illuminated.
TNO apparent brightness V=21.5

TNO is 41.2 AU from the Sun and 41.7 AU from the Earth.
The TNO is moving 19.0 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 99 seconds.
The 1-sigma cross-track error in the shadow position is 1824 km.

The TNO has an absolute magnitude Hv=5.2
Diameter=549.6 km assuming a 5% albedo -- 28.9 sec chord
Diameter=224.4 km assuming a 30% albedo -- 11.8 sec chord
Dynamical classification is SCATEXTD
 
 
 
 
 
 
 
 

Star training set for 523640, (2021/02/08 18:42UT)
Object            RA         Dec     mag  sep  mel
Fomalhaut      22:58:48.8 -29:30:36  1.2 48.58  53
68Omi Cet      02:20:24.9 -02:52:58  2.0  9.90 108
PPM 183660     01:38:56.3 -03:20:02  6.5  3.08  98
PPM 174960     01:42:27.0 -00:24:02  8.5  0.10 100
523640         01:42:05.5 -00:21:09 14.9       100
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 523640, (2021/02/08 18:42UT)
Object            RA         Dec     mag  sep  mel
Fomalhaut      22:57:39.6 -29:37:24  1.2 48.58  53
68Omi Cet      02:19:20.8 -02:58:45  2.0  9.90 108
PPM 183660     01:37:52.1 -03:26:27  6.5  3.08  98
PPM 174960     01:41:22.2 -00:30:24  8.5  0.10 100
523640         01:41:00.7 -00:27:31 14.9       100
Positions are for J2000

Event circumstances last updated at 2021/01/22 20:41:53 UT

Marc W. Buie, Southwest Research Institute

RECON