RECON: TNO occultation with 471136

Event between (471136) 10EO65 and star UC4-285-093800 with event index number of 146469

Geocentric closest approach at 2018/05/12 21:26:57 UTC

J2000 position of star is 16:32:44.8 -33:08:19
Equinox of date position of star is 16:33:54.5 -33:10:31
Stellar brightness R=15.5, use SENSEUP=128
Star is 125 degrees from the moon. Moon is 9% illuminated.
TNO apparent brightness V=21.1

TNO is 14.4 AU from the Sun and 13.4 AU from the Earth.
The TNO is moving 18.4 km/sec on the sky relative to the star, or, 6.8 arcsec/hr.
The 1-sigma error in the time of the event is 153 seconds.
The 1-sigma cross-track error in the shadow position is 692 km.

The TNO has an absolute magnitude Hv=9.5
Diameter=75.9 km assuming a 5% albedo -- 4.1 sec chord
Diameter=31.0 km assuming a 30% albedo -- 1.7 sec chord
Dynamical classification is CENTAURR
 
 
 
 
 
 
 
 

Star training set for 471136, (2018/05/12 21:27UT)
Object            RA         Dec     mag  sep  mel
Antares        16:30:32.2 -26:28:16  0.9  6.75 128
26Eps Sco      16:51:21.4 -34:19:30  2.3  3.80 121
PPM 295143     16:32:35.1 -34:44:34  4.2  1.59 124
PPM 295160     16:33:19.5 -33:30:43  8.4  0.36 125
PPM 295187     16:34:56.2 -33:23:16  9.5  0.30 124
471136         16:33:56.2 -33:10:34 15.5       124
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 471136, (2018/05/12 21:27UT)
Object            RA         Dec     mag  sep  mel
Antares        16:29:24.4 -26:25:56  0.9  6.75 128
26Eps Sco      16:50:08.9 -34:17:40  2.3  3.80 121
PPM 295143     16:31:22.9 -34:42:16  4.2  1.59 124
PPM 295160     16:32:07.9 -33:28:26  8.4  0.36 125
PPM 295187     16:33:44.7 -33:21:02  9.5  0.30 124
471136         16:32:44.8 -33:08:19 15.5       125
Positions are for J2000

Event circumstances last updated at 2017/12/02 17:31:48 UT

Marc W. Buie, Southwest Research Institute

RECON