RECON: TNO occultation with 408832

Event between (408832) 01QJ298 and star UC4-423-141005 with event index number of 81868

Geocentric closest approach at 2017/08/28 01:19:57 UTC

J2000 position of star is 23:09:30.6 -05:32:52
Equinox of date position of star is 23:10:24.5 -05:27:12
Stellar brightness R=16.3, use SENSEUP=128
Star is 115 degrees from the moon. Moon is 38% illuminated.
TNO apparent brightness V=22.7

TNO is 44.7 AU from the Sun and 43.7 AU from the Earth.
The TNO is moving 24.6 km/sec on the sky relative to the star, or, 2.8 arcsec/hr.
The 1-sigma error in the time of the event is 372 seconds.
The 1-sigma cross-track error in the shadow position is 4412 km.

The TNO has an absolute magnitude Hv=6.2
Diameter=346.7 km assuming a 5% albedo -- 14.1 sec chord
Diameter=141.6 km assuming a 30% albedo -- 5.8 sec chord
Dynamical classification is CLASSICAL
 
 
 
 
 
 
 
 

Star training set for 408832, (2017/08/28 01:20UT)
Object            RA         Dec     mag  sep  mel
Fomalhaut      22:58:37.4 -29:31:42  1.2 24.24 104
Markab         23:05:38.5 +15:18:02  2.5 20.79 119
82 Aqr         23:03:27.5 -06:28:44  6.0  2.01 113
PPM 207234     23:11:34.5 -05:51:52  7.3  0.50 116
PPM 207224     23:10:42.4 -05:29:09  9.6  0.08 115
408832         23:10:25.4 -05:27:07 16.3       116
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 408832, (2017/08/28 01:20UT)
Object            RA         Dec     mag  sep  mel
Fomalhaut      22:57:39.5 -29:37:23  1.2 24.24 104
Markab         23:04:45.7 +15:12:18  2.5 20.79 119
82 Aqr         23:02:32.5 -06:34:27  6.0  2.01 113
PPM 207234     23:10:39.6 -05:57:37  7.3  0.50 116
PPM 207224     23:09:47.6 -05:34:54  9.6  0.08 115
408832         23:09:30.6 -05:32:52 16.3       115
Positions are for J2000

Event circumstances last updated at 2017/05/16 18:32:16 UT

Marc W. Buie, Southwest Research Institute

RECON