RECON: TNO occultation with 501546

Event between (501546) 14JJ80 and star GA0940:16720321 with event index number of 1009855

Geocentric closest approach at 2020/12/05 05:53:11 UTC

J2000 position of star is 21:37:43.5 +04:11:51
Equinox of date position of star is 21:38:46.7 +04:17:33
Stellar brightness G=15.0, use SENSEUP=128
Star is 152 degrees from the moon. Moon is 78% illuminated.
TNO apparent brightness V=21.1

TNO is 32.1 AU from the Sun and 32.3 AU from the Earth.
The TNO is moving 16.0 km/sec on the sky relative to the star, or, 2.5 arcsec/hr.
The 1-sigma error in the time of the event is 80 seconds.
The 1-sigma cross-track error in the shadow position is 1201 km.

The TNO has an absolute magnitude Hv=5.8
Diameter=418.8 km assuming a 5% albedo -- 26.2 sec chord
Diameter=171.0 km assuming a 30% albedo -- 10.7 sec chord
Dynamical classification is CENTAURS
 
 
 
 
 
 
 
 

Star training set for 501546, (2020/12/05 05:53UT)
Object            RA         Dec     mag  sep  mel
Fomalhaut      22:58:48.2 -29:30:39  1.2 38.87 150
Markab         23:05:48.3 +15:19:06  2.5 24.07 131
4 Peg          21:39:34.8 +05:52:01  5.9  1.59 150
PPM 172017     21:38:32.1 +04:46:38  6.9  0.49 151
PPM 172037     21:39:09.2 +04:13:48  9.5  0.11 152
501546         21:38:46.7 +04:17:33 15.0       151
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 501546, (2020/12/05 05:53UT)
Object            RA         Dec     mag  sep  mel
Fomalhaut      22:57:39.6 -29:37:24  1.2 38.87 150
Markab         23:04:45.8 +15:12:18  2.5 24.07 131
4 Peg          21:38:32.1 +05:46:19  5.9  1.59 150
PPM 172017     21:37:29.1 +04:40:57  6.9  0.49 151
PPM 172037     21:38:06.0 +04:08:06  9.5  0.11 152
501546         21:37:43.5 +04:11:51 15.0       152
Positions are for J2000

Event circumstances last updated at 2020/12/04 01:10:22 UT

Marc W. Buie, Southwest Research Institute

RECON