RECON: TNO occultation with 14KZ101

Event between 14KZ101 and star UC4-432-066385 with event index number of 138627

Geocentric closest approach at 2017/08/01 18:33:54 UTC

J2000 position of star is 16:59:48.2 -03:41:35
Equinox of date position of star is 17:00:43.1 -03:43:04
Stellar brightness R=13.6, use SENSEUP=64
Star is 17 degrees from the moon. Moon is 70% illuminated.
TNO apparent brightness V=21.8

TNO is 34.0 AU from the Sun and 33.4 AU from the Earth.
The TNO is moving 12.6 km/sec on the sky relative to the star, or, 1.9 arcsec/hr.
The 1-sigma error in the time of the event is 647 seconds.
The 1-sigma cross-track error in the shadow position is 4268 km.

The TNO has an absolute magnitude Hv=6.4
Diameter=317.7 km assuming a 5% albedo -- 25.2 sec chord
Diameter=129.7 km assuming a 30% albedo -- 10.3 sec chord
Dynamical classification is SCATNEAR
 
 
 
 
 
 
 
 

Star training set for 14KZ101, (2017/08/01 18:34UT)
Object            RA         Dec     mag  sep  mel
Antares        16:30:29.3 -26:28:10  0.9 23.88  12
13Zet Oph      16:38:07.7 -10:36:05  2.6  8.88   9
23 Oph         16:55:32.2 -06:10:53  5.3  2.78  15
PPM 200274     17:02:36.5 -03:47:38  8.3  0.47  18
PPM 200236     17:00:12.5 -03:55:27  9.7  0.24  17
14KZ101        17:00:43.8 -03:43:05 13.6        17
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 14KZ101, (2017/08/01 18:34UT)
Object            RA         Dec     mag  sep  mel
Antares        16:29:24.4 -26:25:56  0.9 23.88  12
13Zet Oph      16:37:09.6 -10:34:01  2.6  8.88   9
23 Oph         16:54:35.7 -06:09:15  5.3  2.78  15
PPM 200274     17:01:40.9 -03:46:10  8.3  0.47  18
PPM 200236     16:59:16.9 -03:53:56  9.7  0.24  17
14KZ101        16:59:48.2 -03:41:35 13.6        17
Positions are for J2000

Event circumstances last updated at 2017/05/16 18:30:08 UT

Marc W. Buie, Southwest Research Institute

RECON