RECON: TNO occultation with 04MW8

Event between 04MW8 and star GA0820:22245393 with event index number of 1078400

Geocentric closest approach at 2021/08/12 01:02:38 UTC

J2000 position of star is 21:54:45.7 -07:01:19
Equinox of date position of star is 21:55:53.0 -06:55:14
Stellar brightness G=14.2, use SENSEUP=64 with the MallinCam and and exposure time of 1 seconds with the QHY174 camera.
Star is 144 degrees from the moon. Moon is 14% illuminated.
TNO apparent brightness V=22.6

TNO is 25.1 AU from the Sun and 24.1 AU from the Earth.
The TNO is moving 22.6 km/sec on the sky relative to the star, or, 4.7 arcsec/hr.
The 1-sigma error in the time of the event is 79 seconds.
The 1-sigma cross-track error in the shadow position is 1275 km.

The TNO has an absolute magnitude Hv=8.6
Diameter=117.5 km assuming a 5% albedo -- 5.2 sec chord
Diameter=48.0 km assuming a 30% albedo -- 2.1 sec chord
Dynamical classification is CENTAURR
 
 
 
 
 
 
 
 

Star training set for 04MW8, (2021/08/12 01:01UT)
Object            RA         Dec     mag  sep  mel
Fomalhaut      22:58:50.4 -29:30:26  1.2 27.01 147
PPM 205611     21:48:46.4 -05:48:57  6.3  2.09 143
PPM 205781     21:57:22.1 -06:52:36  8.0  0.37 145
PPM 205727     21:54:48.6 -07:02:08  9.6  0.29 144
04MW8          21:55:54.0 -06:55:08 14.2       145
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 04MW8, (2021/08/12 01:01UT)
Object            RA         Dec     mag  sep  mel
Fomalhaut      22:57:39.6 -29:37:24  1.2 27.01 147
PPM 205611     21:47:38.3 -05:55:00  6.3  2.09 143
PPM 205781     21:56:13.9 -06:58:48  8.0  0.37 145
PPM 205727     21:53:40.2 -07:08:18  9.6  0.29 144
04MW8          21:54:45.7 -07:01:19 14.2       144
Positions are for J2000

Event circumstances last updated at 2021/04/19 23:04:19 UT

Marc W. Buie, Southwest Research Institute

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