RECON: TNO occultation with 600217

Event between (600217) 11QY100 and star GA0860:01600983 with event index number of 2730317

Geocentric closest approach at 2024/01/19 11:15:16 UTC

J2000 position of star is 06:38:55.8 -02:35:24
Equinox of date position of star is 06:40:01.9 -02:36:40
Stellar brightness G=14.2, use SENSEUP=64 with the MallinCam and and exposure time of 1 seconds with the QHY174 camera.
Star is 61 degrees from the moon. Moon is 64% illuminated.
TNO apparent brightness V=21.3

TNO is 20.0 AU from the Sun and 19.1 AU from the Earth.
The TNO is moving 20.6 km/sec on the sky relative to the star, or, 5.4 arcsec/hr.
The 1-sigma error in the time of the event is 57 seconds.
The 1-sigma cross-track error in the shadow position is 832 km.

The TNO has an absolute magnitude Hv=8.2
Diameter=137.4 km assuming a 5% albedo -- 6.7 sec chord
Diameter=56.1 km assuming a 30% albedo -- 2.7 sec chord
Dynamical classification is CENTAURR
 
 
 
 
 
 
 
 

Star training set for 600217, (2024/01/19 11:15UT)
Object            RA         Dec     mag  sep  mel
Sirius         06:46:12.5 -16:45:00 -1.5 14.22  68
Saiph          05:48:53.9 -09:39:46  2.1 14.55  52
PPM 176316     06:34:51.2 -01:14:25  5.1  1.90  59
PPM 176357     06:39:32.9 -02:33:59  7.7  0.15  60
600217         06:40:08.3 -02:36:47 14.2        61
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, (2024/01/19 11:15UT)
Object            RA         Dec     mag  sep  mel
Sirius         06:45:08.0 -16:43:24 -1.5 14.22  68
Saiph          05:47:45.4 -09:40:11  2.1 14.55  52
PPM 176316     06:33:37.9 -01:13:13  5.1  1.90  59
PPM 176357     06:38:20.4 -02:32:38  7.7  0.15  60
600217         06:38:55.8 -02:35:24 14.2        60
Positions are for J2000

Event circumstances last updated at 2021/12/02 01:49:11 UT

Marc W. Buie, Southwest Research Institute

RECON