RECON: TNO occultation with 01FK193

Event between 01FK193 and star GA0740:05366141 with event index number of 207702

Geocentric closest approach at 2019/08/29 11:46:48 UTC

J2000 position of star is 15:08:01.9 -15:16:25
Equinox of date position of star is 15:09:07.4 -15:20:52
Stellar brightness G=14.5, use SENSEUP=128
Star is 86 degrees from the moon. Moon is 1% illuminated.
TNO apparent brightness V=23.4

TNO is 43.6 AU from the Sun and 43.9 AU from the Earth.
The TNO is moving 13.5 km/sec on the sky relative to the star, or, 1.5 arcsec/hr.
The 1-sigma error in the time of the event is 456 seconds.
The 1-sigma cross-track error in the shadow position is 2837 km.

The TNO has an absolute magnitude Hv=6.8
Diameter=261.8 km assuming a 5% albedo -- 19.5 sec chord
Diameter=106.9 km assuming a 30% albedo -- 8.0 sec chord
Dynamical classification is CLASSICAL
 
 
 
 
 
 
 
 

Star training set for 01FK193, (2019/08/29 11:47UT)
Object            RA         Dec     mag  sep  mel
Antares        16:30:37.0 -26:28:26  0.9 22.00 108
27Bet Lib      15:18:04.1 -09:27:15  2.6  6.28  87
21Nu Lib       15:07:43.6 -16:19:55  5.2  1.04  86
PPM 229784     15:08:31.9 -15:29:30  8.1  0.20  86
PPM 229792     15:09:01.9 -15:11:11  9.5  0.16  86
01FK193        15:09:07.7 -15:20:53 14.5        87
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 01FK193, (2019/08/29 11:47UT)
Object            RA         Dec     mag  sep  mel
Antares        16:29:24.4 -26:25:56  0.9 22.00 108
27Bet Lib      15:17:00.3 -09:22:59  2.6  6.28  87
21Nu Lib       15:06:37.6 -16:15:25  5.2  1.04  86
PPM 229784     15:07:26.1 -15:25:01  8.1  0.20  86
PPM 229792     15:07:56.2 -15:06:43  9.5  0.16  86
01FK193        15:08:01.9 -15:16:25 14.5        86
Positions are for J2000

Event circumstances last updated at 2019/08/04 22:08:14 UT

Marc W. Buie, Southwest Research Institute

RECON