RECON: TNO occultation with 15VB166

Event between 15VB166 and star GA1100:00576563 with event index number of 2571797

Geocentric closest approach at 2021/11/01 23:58:28 UTC

J2000 position of star is 04:20:31.2 +20:48:00
Equinox of date position of star is 04:21:48.1 +20:51:03
Stellar brightness G=17.0, use SENSEUP=128 with the MallinCam and and exposure time of 2 seconds with the QHY174 camera.
Star is 114 degrees from the moon. Moon is 11% illuminated.
TNO apparent brightness V=23.8

TNO is 32.1 AU from the Sun and 31.2 AU from the Earth.
The TNO is moving 20.8 km/sec on the sky relative to the star, or, 3.3 arcsec/hr.
The 1-sigma error in the time of the event is 115 seconds.
The 1-sigma cross-track error in the shadow position is 1211 km.

The TNO has an absolute magnitude Hv=8.7
Diameter=105.2 km assuming a 5% albedo -- 5.3 sec chord
Diameter=42.9 km assuming a 30% albedo -- 2.2 sec chord
Dynamical classification is 2:1E
 
 
 
 
 
 
 
 

Star training set for 15VB166, (2021/11/01 23:58UT)
Object            RA         Dec     mag  sep  mel
Aldebaran      04:37:10.6 +16:33:05  0.8  5.63 111
44Zet Per      03:55:30.6 +31:56:48  2.8 12.55 116
PPM 093481     04:24:49.8 +21:01:52  5.9  0.73 113
PPM 093442     04:22:49.2 +21:05:24  7.7  0.34 113
15VB166        04:21:48.4 +20:51:03 17.0       113
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 15VB166, (2021/11/01 23:58UT)
Object            RA         Dec     mag  sep  mel
Aldebaran      04:35:55.3 +16:30:29  0.8  5.63 111
44Zet Per      03:54:07.9 +31:53:01  2.8 12.55 116
PPM 093481     04:23:32.4 +20:58:54  5.9  0.73 113
PPM 093442     04:21:31.8 +21:02:23  7.7  0.34 113
15VB166        04:20:31.2 +20:48:00 17.0       114
Positions are for J2000

Event circumstances last updated at 2021/10/08 00:57:11 UT

Marc W. Buie, Southwest Research Institute

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