RECON: TNO occultation with 10BK118

Event between 10BK118 and star GA0360:18182239 with event index number of 1089964

Geocentric closest approach at 2021/04/09 08:02:09 UTC

J2000 position of star is 15:14:04.9 -53:46:22
Equinox of date position of star is 15:15:39.4 -53:51:03
Stellar brightness G=16.7, use SENSEUP=128 with the MallinCam and and exposure time of 2 seconds with the QHY174 camera.
Star is 101 degrees from the moon. Moon is 7% illuminated.
TNO apparent brightness V=23.3

TNO is 19.7 AU from the Sun and 19.1 AU from the Earth.
The TNO is moving 28.8 km/sec on the sky relative to the star, or, 7.5 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 960 km.

The TNO has an absolute magnitude Hv=10.2
Diameter=55.2 km assuming a 5% albedo -- 1.9 sec chord
Diameter=22.5 km assuming a 30% albedo -- 0.8 sec chord
Dynamical classification is CENTAURR
 
 
 
 
 
 
 
 

Star training set for 10BK118, (2021/04/09 08:02UT)
Object            RA         Dec     mag  sep  mel
PPM 360911     14:41:03.6 -60:55:19  0.0  8.45 100
Alp Lup        14:43:21.3 -47:28:41  2.3  8.16 109
PPM 343490     15:12:52.0 -55:25:31  5.5  1.63 100
PPM 343508     15:13:53.8 -53:44:13  8.5  0.28 101
10BK118        15:15:39.4 -53:51:03 16.7       101
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 10BK118, (2021/04/09 08:02UT)
Object            RA         Dec     mag  sep  mel
PPM 360911     14:39:25.4 -60:49:53  0.0  8.45 100
Alp Lup        14:41:55.7 -47:23:18  2.3  8.16 109
PPM 343490     15:11:16.0 -55:20:46  5.5  1.63 100
PPM 343508     15:12:19.5 -53:39:29  8.5  0.28 101
10BK118        15:14:04.9 -53:46:22 16.7       101
Positions are for J2000

Event circumstances last updated at 2021/04/07 23:50:20 UT

Marc W. Buie, Southwest Research Institute

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