RECON: TNO occultation with 12WD37

Event between 12WD37 and star GA1220:03377832 with event index number of 1558826

Geocentric closest approach at 2020/03/21 17:50:06 UTC

J2000 position of star is 09:01:31.3 +33:22:03
Equinox of date position of star is 09:02:45.8 +33:17:14
Stellar brightness G=16.8, use SENSEUP=128
Star is 153 degrees from the moon. Moon is 6% illuminated.
TNO apparent brightness V=25.7

TNO is 36.0 AU from the Sun and 35.4 AU from the Earth.
The TNO is moving 14.2 km/sec on the sky relative to the star, or, 2.0 arcsec/hr.
The 1-sigma error in the time of the event is 236 seconds.
The 1-sigma cross-track error in the shadow position is 1384 km.

The TNO has an absolute magnitude Hv=10.0
Diameter=261.8 km assuming a 5% albedo -- 4.2 sec chord
Diameter=106.9 km assuming a 30% albedo -- 1.7 sec chord
Dynamical classification is SCATEXTD
 
 
 
 
 
 
 
 

Star training set for 12WD37, (2020/03/21 17:50UT)
Object            RA         Dec     mag  sep  mel
Pollux         07:46:33.0 +27:58:33  1.1 17.20 141
66 Cnc         09:02:38.2 +32:10:20  5.9  1.12 154
PPM 074199     09:04:29.4 +32:48:02  7.7  0.61 154
PPM 074142     09:00:21.0 +33:34:18  9.5  0.58 153
PPM 074184     09:03:01.8 +33:16:33 10.9  0.06 153
12WD37         09:02:45.9 +33:17:14 16.8       154
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 12WD37, (2020/03/21 17:50UT)
Object            RA         Dec     mag  sep  mel
Pollux         07:45:18.0 +28:01:33  1.1 17.20 141
66 Cnc         09:01:24.1 +32:15:09  5.9  1.12 154
PPM 074199     09:03:15.1 +32:52:53  7.7  0.61 154
PPM 074142     08:59:06.1 +33:39:04  9.5  0.58 153
PPM 074184     09:01:47.2 +33:21:23 10.9  0.06 153
12WD37         09:01:31.3 +33:22:03 16.8       153
Positions are for J2000

Event circumstances last updated at 2020/03/10 21:11:07 UT

Marc W. Buie, Southwest Research Institute

RECON