RECON: TNO occultation with 12JD68

Event between 12JD68 and star GA0940:04597692 with event index number of 1557449

Geocentric closest approach at 2020/02/17 14:17:47 UTC

J2000 position of star is 16:57:25.6 +04:03:55
Equinox of date position of star is 16:58:23.8 +04:02:10
Stellar brightness G=16.5, use SENSEUP=128
Star is 26 degrees from the moon. Moon is 33% illuminated.
TNO apparent brightness V=22.9

TNO is 28.0 AU from the Sun and 28.2 AU from the Earth.
The TNO is moving 20.0 km/sec on the sky relative to the star, or, 3.5 arcsec/hr.
The 1-sigma error in the time of the event is 147 seconds.
The 1-sigma cross-track error in the shadow position is 2034 km.

The TNO has an absolute magnitude Hv=8.2
Diameter=140.6 km assuming a 5% albedo -- 7.0 sec chord
Diameter=57.4 km assuming a 30% albedo -- 2.9 sec chord
Dynamical classification is 3:2E+6:4II
 
 
 
 
 
 
 
 

Star training set for 12JD68, (2020/02/17 14:18UT)
Object            RA         Dec     mag  sep  mel
Antares        16:30:38.7 -26:28:30  0.9 31.24  11
60Bet Oph      17:44:28.1 +04:33:37  2.8 11.49  27
45 Her         16:48:46.0 +05:12:44  5.1  2.68  27
PPM 163499     17:06:23.8 +03:24:45  7.7  2.08  25
PPM 163299     16:58:02.8 +03:53:06  9.8  0.18  26
12JD68         16:58:25.7 +04:02:07 16.5        26
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 12JD68, (2020/02/17 14:18UT)
Object            RA         Dec     mag  sep  mel
Antares        16:29:24.4 -26:25:56  0.9 31.24  11
60Bet Oph      17:43:28.3 +04:34:05  2.8 11.49  27
45 Her         16:47:46.4 +05:14:48  5.1  2.68  27
PPM 163499     17:05:23.5 +03:26:19  7.7  2.08  25
PPM 163299     16:57:02.7 +03:54:55  9.8  0.18  26
12JD68         16:57:25.6 +04:03:55 16.5        26
Positions are for J2000

Event circumstances last updated at 2019/07/02 02:29:40 UT

Marc W. Buie, Southwest Research Institute

RECON