RECON: TNO occultation with 174567

Event between (174567) Varda and star UC4-439-066796 with event index number of 85147

Geocentric closest approach at 2017/10/06 05:19:26 UTC

J2000 position of star is 17:14:44.9 -02:18:17
Equinox of date position of star is 17:15:37.3 -02:19:22
Stellar brightness R=13.2
Star is 121 degrees from the moon. Moon is 100% illuminated.
TNO apparent brightness V=20.2

TNO is 46.8 AU from the Sun and 47.2 AU from the Earth.
The TNO is moving 19.5 km/sec on the sky relative to the star, or, 2.1 arcsec/hr.
The 1-sigma error in the time of the event is 130 seconds.
The 1-sigma cross-track error in the shadow position is 2145 km.

The TNO has an absolute magnitude Hv=3.4
Diameter=1259.0 km assuming a 5% albedo -- 67.7 sec chord
Diameter=514.0 km assuming a 30% albedo -- 27.6 sec chord
Dynamical classification is SCATEXTD
 
 
 
 
 
 
 
 

Star training set for 174567, (2017/10/06 05:19UT)
Object            RA         Dec     mag  sep  mel
Antares        16:30:30.0 -26:28:12  0.9 26.47 128
60Bet Oph      17:44:21.0 +04:33:40  2.8  9.94 113
PPM 180004     17:09:08.7 -01:06:06  6.5  2.04 122
PPM 200547     17:19:46.1 -02:49:42  7.0  1.14 119
PPM 180020     17:15:53.7 -02:31:20  8.8  0.21 120
174567         17:15:40.4 -02:19:26 13.2       120
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 174567, (2017/10/06 05:19UT)
Object            RA         Dec     mag  sep  mel
Antares        16:29:24.4 -26:25:55  0.9 26.47 128
60Bet Oph      17:43:28.3 +04:34:05  2.8  9.94 113
PPM 180004     17:08:13.6 -01:04:47  6.5  2.04 122
PPM 200547     17:18:50.3 -02:48:39  7.0  1.14 119
PPM 180020     17:14:58.0 -02:30:11  8.8  0.21 120
174567         17:14:44.9 -02:18:17 13.2       120
Positions are for J2000

Event circumstances last updated at 2016/10/08 16:38:08 UT

Marc W. Buie, Southwest Research Institute

RECON