RECON: TNO occultation with 600217

Event between (600217) 11QY100 and star GA0880:01161113 with event index number of 2730107

Geocentric closest approach at 2023/04/13 02:09:28 UTC

J2000 position of star is 06:14:45.6 -01:24:07
Equinox of date position of star is 06:15:52.2 -01:24:36
Stellar brightness G=16.1, use SENSEUP=128 with the MallinCam and and exposure time of 2 seconds with the QHY174 camera.
Star is 147 degrees from the moon. Moon is 53% illuminated.
TNO apparent brightness V=21.5

TNO is 19.8 AU from the Sun and 20.1 AU from the Earth.
The TNO is moving 22.2 km/sec on the sky relative to the star, or, 5.5 arcsec/hr.
The 1-sigma error in the time of the event is 45 seconds.
The 1-sigma cross-track error in the shadow position is 834 km.

The TNO has an absolute magnitude Hv=8.2
Diameter=137.4 km assuming a 5% albedo -- 6.2 sec chord
Diameter=56.1 km assuming a 30% albedo -- 2.5 sec chord
Dynamical classification is CENTAURR
 
 
 
 
 
 
 
 

Star training set for 600217, (2023/04/13 02:09UT)
Object            RA         Dec     mag  sep  mel
Betelgeuse     05:56:26.0 +07:24:34  0.4 10.07 151
Saiph          05:48:51.7 -09:39:47  2.1 10.65 136
PPM 176187     06:16:45.3 -00:31:22  6.2  0.91 148
PPM 176186     06:16:37.6 -01:24:32  8.2  0.17 147
600217         06:15:56.4 -01:24:38 16.1       147
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 600217, (2023/04/13 02:09UT)
Object            RA         Dec     mag  sep  mel
Betelgeuse     05:55:10.3 +07:24:26  0.4 10.07 151
Saiph          05:47:45.4 -09:40:11  2.1 10.65 136
PPM 176187     06:15:34.0 -00:30:49  6.2  0.91 148
PPM 176186     06:15:26.8 -01:24:00  8.2  0.17 147
600217         06:14:45.6 -01:24:07 16.1       147
Positions are for J2000

Event circumstances last updated at 2021/12/02 01:24:25 UT

Marc W. Buie, Southwest Research Institute

RECON