RECON: TNO occultation with 471325

Event between (471325) 11KT19 and star GA0980:04212694 with event index number of 256719

Geocentric closest approach at 2020/04/25 20:48:31 UTC

J2000 position of star is 15:51:59.1 +09:00:46
Equinox of date position of star is 15:52:55.4 +08:57:20
Stellar brightness G=12.4, use SENSEUP=16
Star is 151 degrees from the moon. Moon is 7% illuminated.
TNO apparent brightness V=21.7

TNO is 28.1 AU from the Sun and 27.2 AU from the Earth.
The TNO is moving 32.0 km/sec on the sky relative to the star, or, 5.8 arcsec/hr.
The 1-sigma error in the time of the event is 83 seconds.
The 1-sigma cross-track error in the shadow position is 3682 km.

The TNO has an absolute magnitude Hv=7.2
Diameter=218.8 km assuming a 5% albedo -- 6.8 sec chord
Diameter=89.3 km assuming a 30% albedo -- 2.8 sec chord
Dynamical classification is CENTAURR
 
 
 
 
 
 
 
 

Star training set for 471325, (2020/04/25 20:49UT)
Object            RA         Dec     mag  sep  mel
Arcturus       14:16:35.4 +19:04:40  0.0 25.43 131
Unukalhai      15:45:16.2 +06:21:47  2.6  3.22 153
27Lam Ser      15:47:25.9 +07:17:26  5.1  2.15 152
PPM 162053     15:56:20.3 +09:09:54  7.9  0.86 151
PPM 161979     15:52:28.6 +09:10:20  9.6  0.25 150
471325         15:52:57.9 +08:57:11 12.4       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 471325, (2020/04/25 20:49UT)
Object            RA         Dec     mag  sep  mel
Arcturus       14:15:38.2 +19:10:18  0.0 25.43 131
Unukalhai      15:44:16.3 +06:25:33  2.6  3.22 153
27Lam Ser      15:46:26.3 +07:21:09  5.1  2.15 152
PPM 162053     15:55:21.6 +09:13:24  7.9  0.86 151
PPM 161979     15:51:29.9 +09:13:56  9.6  0.25 150
471325         15:51:59.1 +09:00:46 12.4       151
Positions are for J2000

Event circumstances last updated at 2019/06/07 23:31:11 UT

Marc W. Buie, Southwest Research Institute

RECON