RECON: TNO occultation with 470309

Event between (470309) 07JK43 and star UC4-479-068749 with event index number of 329932

Geocentric closest approach at 2020/05/20 21:59:51 UTC

J2000 position of star is 17:49:47.9 +05:36:56
Equinox of date position of star is 17:50:45.1 +05:36:39
Stellar brightness R=13.1, use SENSEUP=32
Star is 129 degrees from the moon. Moon is 3% illuminated.
TNO apparent brightness V=21.0

TNO is 24.8 AU from the Sun and 24.0 AU from the Earth.
The TNO is moving 23.0 km/sec on the sky relative to the star, or, 4.8 arcsec/hr.
The 1-sigma error in the time of the event is 67 seconds.
The 1-sigma cross-track error in the shadow position is 1430 km.

The TNO has an absolute magnitude Hv=7.0
Diameter=239.9 km assuming a 5% albedo -- 10.4 sec chord
Diameter=97.9 km assuming a 30% albedo -- 4.3 sec chord
Dynamical classification is CENTAURR
 
 
 
 
 
 
 
 

Star training set for 470309, (2020/05/20 22:00UT)
Object            RA         Dec     mag  sep  mel
Vega           18:37:37.7 +38:48:13  0.0 34.85 105
60Bet Oph      17:44:28.8 +04:33:37  2.8  1.89 131
PPM 164771     17:54:13.8 +06:05:55  5.8  0.98 128
PPM 164620     17:49:43.4 +05:41:45  7.2  0.28 129
PPM 164665     17:51:04.9 +05:41:23  9.6  0.11 129
470309         17:50:47.9 +05:36:38 13.1       129
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 470309, (2020/05/20 22:00UT)
Object            RA         Dec     mag  sep  mel
Vega           18:36:56.7 +38:47:07  0.0 34.85 105
60Bet Oph      17:43:28.3 +04:34:05  2.8  1.89 131
PPM 164771     17:53:14.0 +06:06:06  5.8  0.98 128
PPM 164620     17:48:43.4 +05:42:04  7.2  0.28 129
PPM 164665     17:50:04.9 +05:41:40  9.6  0.11 129
470309         17:49:47.9 +05:36:56 13.1       129
Positions are for J2000

Event circumstances last updated at 2019/06/07 23:40:13 UT

Marc W. Buie, Southwest Research Institute

RECON