RECON: TNO occultation with 523700

Event between (523700) 14GM54 and star GA1120:10204123 with event index number of 324512

Geocentric closest approach at 2020/05/28 21:58:21 UTC

J2000 position of star is 19:36:59.9 +22:18:09
Equinox of date position of star is 19:37:50.9 +22:20:53
Stellar brightness G=14.7, use SENSEUP=128
Star is 129 degrees from the moon. Moon is 36% illuminated.
TNO apparent brightness V=21.6

TNO is 27.0 AU from the Sun and 26.6 AU from the Earth.
The TNO is moving 17.3 km/sec on the sky relative to the star, or, 3.2 arcsec/hr.
The 1-sigma error in the time of the event is 105 seconds.
The 1-sigma cross-track error in the shadow position is 1748 km.

The TNO has an absolute magnitude Hv=7.1
Diameter=229.1 km assuming a 5% albedo -- 13.2 sec chord
Diameter=93.5 km assuming a 30% albedo -- 5.4 sec chord
Dynamical classification is 3:2E+6:4II
 
 
 
 
 
 
 
 

Star training set for 523700, (2020/05/28 21:58UT)
Object            RA         Dec     mag  sep  mel
Vega           18:37:37.8 +38:48:13  0.0 20.89 108
Tarazed        19:47:13.8 +10:39:51  2.7 11.90 139
PPM 109310     19:37:00.7 +22:37:55  6.1  0.35 129
PPM 109351     19:37:59.4 +22:03:10  7.2  0.30 129
PPM 109369     19:38:27.4 +22:15:41  8.7  0.16 129
523700         19:37:52.5 +22:20:58 14.7       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 523700, (2020/05/28 21:58UT)
Object            RA         Dec     mag  sep  mel
Vega           18:36:56.7 +38:47:07  0.0 20.89 108
Tarazed        19:46:15.6 +10:36:48  2.7 11.90 139
PPM 109310     19:36:08.3 +22:35:08  6.1  0.35 129
PPM 109351     19:37:06.7 +22:00:21  7.2  0.30 129
PPM 109369     19:37:34.8 +22:12:52  8.7  0.16 129
523700         19:36:59.9 +22:18:09 14.7       129
Positions are for J2000

Event circumstances last updated at 2019/10/15 22:22:24 UT

Marc W. Buie, Southwest Research Institute

RECON