RECON: TNO occultation with 385185

Event between (385185) 93RO and star UC4-514-004311 with event index number of 85721

Geocentric closest approach at 2017/10/20 18:43:52 UTC

J2000 position of star is 02:44:32.9 +12:45:44
Equinox of date position of star is 02:45:29.6 +12:50:05
Stellar brightness R=16.5, use SENSEUP=128
Star is 176 degrees from the moon. Moon is 1% illuminated.
TNO apparent brightness V=23.6

TNO is 33.0 AU from the Sun and 32.0 AU from the Earth.
The TNO is moving 23.5 km/sec on the sky relative to the star, or, 3.6 arcsec/hr.
The 1-sigma error in the time of the event is 667 seconds.
The 1-sigma cross-track error in the shadow position is 5834 km.

The TNO has an absolute magnitude Hv=8.4
Diameter=125.9 km assuming a 5% albedo -- 5.4 sec chord
Diameter=51.4 km assuming a 30% albedo -- 2.2 sec chord
Dynamical classification is 3:2E
 
 
 
 
 
 
 
 

Star training set for 385185, (2017/10/20 18:44UT)
Object            RA         Dec     mag  sep  mel
Aldebaran      04:36:56.7 +16:32:37  0.8 27.18 149
Menkar         03:03:12.7 +04:09:31  2.5  9.72 171
38 Ari         02:45:55.9 +12:31:11  5.4  0.33 176
PPM 118469     02:43:15.9 +12:55:16  8.4  0.56 176
PPM 118500     02:45:17.6 +12:39:49 10.0  0.18 176
385185         02:45:31.3 +12:50:12 16.5       176
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 385185, (2017/10/20 18:44UT)
Object            RA         Dec     mag  sep  mel
Aldebaran      04:35:55.3 +16:30:30  0.8 27.18 149
Menkar         03:02:16.8 +04:05:22  2.5  9.72 171
38 Ari         02:44:57.7 +12:26:43  5.4  0.33 176
PPM 118469     02:42:17.6 +12:50:45  8.4  0.56 176
PPM 118500     02:44:19.3 +12:35:20 10.0  0.18 176
385185         02:44:32.9 +12:45:44 16.5       176
Positions are for J2000

Event circumstances last updated at 2017/04/24 16:12:40 UT

Marc W. Buie, Southwest Research Institute

RECON