RECON: TNO occultation with 469506

Event between (469506) 03FF128 and star GA0660:09546632 with event index number of 1237572

Geocentric closest approach at 2023/03/02 01:04:35 UTC

J2000 position of star is 17:06:43.6 -22:21:07
Equinox of date position of star is 17:08:05.8 -22:22:50
Stellar brightness G=16.0, use SENSEUP=128 with the MallinCam and and exposure time of 2 seconds with the QHY174 camera.
Star is 156 degrees from the moon. Moon is 75% illuminated.
TNO apparent brightness V=22.0

TNO is 31.0 AU from the Sun and 31.1 AU from the Earth.
The TNO is moving 9.9 km/sec on the sky relative to the star, or, 1.6 arcsec/hr.
The 1-sigma error in the time of the event is 415 seconds.
The 1-sigma cross-track error in the shadow position is 1247 km.

The TNO has an absolute magnitude Hv=6.9
Diameter=254.7 km assuming a 5% albedo -- 25.7 sec chord
Diameter=104.0 km assuming a 30% albedo -- 10.5 sec chord
Dynamical classification is 3:2E
 
 
 
 
 
 
 
 

Star training set for 469506, (2023/03/02 01:05UT)
Object            RA         Dec     mag  sep  mel
Antares        16:30:49.9 -26:28:53  0.9  9.42 149
35Eta Oph      17:11:42.5 -15:45:07  2.6  6.68 154
PPM 266403     17:07:34.9 -21:35:41  6.3  0.80 156
PPM 266431     17:09:10.0 -22:31:28  8.8  0.28 156
469506         17:08:07.3 -22:22:52 16.0       156
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 469506, (2023/03/02 01:05UT)
Object            RA         Dec     mag  sep  mel
Antares        16:29:24.4 -26:25:56  0.9  9.42 149
35Eta Oph      17:10:22.7 -15:43:29  2.6  6.68 154
PPM 266403     17:06:11.8 -21:33:54  6.3  0.80 156
PPM 266431     17:07:46.3 -22:29:44  8.8  0.28 156
469506         17:06:43.6 -22:21:07 16.0       156
Positions are for J2000

Event circumstances last updated at 2022/10/03 04:22:34 UT

Marc W. Buie, Southwest Research Institute

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