RECON: TNO occultation with 14VB41

Event between 14VB41 and star GA0920:00125018 with event index number of 1949586

Geocentric closest approach at 2022/12/12 09:34:47 UTC

J2000 position of star is 01:26:03.1 +02:42:41
Equinox of date position of star is 01:27:10.5 +02:49:26
Stellar brightness G=15.7, use SENSEUP=128 with the MallinCam and and exposure time of 2 seconds with the QHY174 camera.
Star is 106 degrees from the moon. Moon is 84% illuminated.
TNO apparent brightness V=23.1

TNO is 37.4 AU from the Sun and 36.9 AU from the Earth.
The TNO is moving 10.9 km/sec on the sky relative to the star, or, 1.5 arcsec/hr.
The 1-sigma error in the time of the event is 256 seconds.
The 1-sigma cross-track error in the shadow position is 2375 km.

The TNO has an absolute magnitude Hv=7.3
Diameter=174.6 km assuming a 5% albedo -- 19.2 sec chord
Diameter=71.3 km assuming a 30% albedo -- 7.8 sec chord
Dynamical classification is SCATNEAR
 
 
 
 
 
 
 
 

Star training set for 14VB41, (2022/12/12 09:31UT)
Object            RA         Dec     mag  sep  mel
Fomalhaut      22:58:54.8 -29:30:00  1.2 47.99 149
68Omi Cet      02:20:30.4 -02:52:28  2.0 14.48  96
PPM 144619     01:28:04.9 +03:39:13  6.5  0.85 106
PPM 144598     01:26:51.9 +03:05:27  7.4  0.28 106
14VB41         01:27:14.2 +02:49:48 15.7       106
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 14VB41, (2022/12/12 09:31UT)
Object            RA         Dec     mag  sep  mel
Fomalhaut      22:57:39.6 -29:37:24  1.2 47.99 149
68Omi Cet      02:19:20.8 -02:58:45  2.0 14.48  96
PPM 144619     01:26:53.6 +03:32:06  6.5  0.85 106
PPM 144598     01:25:40.7 +02:58:19  7.4  0.28 106
14VB41         01:26:03.1 +02:42:41 15.7       106
Positions are for J2000

Event circumstances last updated at 2021/10/07 00:36:31 UT

Marc W. Buie, Southwest Research Institute

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