RECON: TNO occultation with 05EZ300

Event between 05EZ300 and star GA0740:05036740 with event index number of 1190653

Geocentric closest approach at 2023/01/27 16:02:01 UTC

J2000 position of star is 13:39:35.9 -15:57:11
Equinox of date position of star is 13:40:47.8 -16:03:54
Stellar brightness G=16.3, use SENSEUP=128 with the MallinCam and and exposure time of 2 seconds with the QHY174 camera.
Star is 173 degrees from the moon. Moon is 40% illuminated.
TNO apparent brightness V=22.8

TNO is 31.7 AU from the Sun and 31.5 AU from the Earth.
The TNO is moving 3.9 km/sec on the sky relative to the star, or, 0.6 arcsec/hr.
The 1-sigma error in the time of the event is 693 seconds.
The 1-sigma cross-track error in the shadow position is 3837 km.

The TNO has an absolute magnitude Hv=7.6
Diameter=182.8 km assuming a 5% albedo -- 46.7 sec chord
Diameter=74.6 km assuming a 30% albedo -- 19.0 sec chord
Dynamical classification is 3:2E
 
 
 
 
 
 
 
 

Star training set for 05EZ300, (2023/01/27 16:02UT)
Object            RA         Dec     mag  sep  mel
Spica          13:26:24.7 -11:16:52  1.0  5.93 176
83 Vir         13:45:44.8 -16:17:39  5.6  1.20 173
PPM 227645     13:41:13.4 -16:33:47  6.6  0.50 172
PPM 227636     13:40:49.4 -15:59:13  9.8  0.08 173
05EZ300        13:40:50.6 -16:04:10 16.3       173
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 05EZ300, (2023/01/27 16:02UT)
Object            RA         Dec     mag  sep  mel
Spica          13:25:11.5 -11:09:41  1.0  5.93 176
83 Vir         13:44:29.9 -16:10:45  5.6  1.20 173
PPM 227645     13:39:58.5 -16:26:48  6.6  0.50 172
PPM 227636     13:39:34.7 -15:52:14  9.8  0.08 173
05EZ300        13:39:35.9 -15:57:11 16.3       173
Positions are for J2000

Event circumstances last updated at 2022/03/18 00:56:22 UT

Marc W. Buie, Southwest Research Institute

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