RECON: TNO occultation with 120132

Event between (120132) 03FY128 and star GA0680:05754095 with event index number of 2428724

Geocentric closest approach at 2022/03/02 05:42:35 UTC

J2000 position of star is 13:53:01.6 -21:34:55
Equinox of date position of star is 13:54:14.0 -21:41:18
Stellar brightness G=12.2, use SENSEUP=16 with the MallinCam and and exposure time of 250 milli-seconds with the QHY174 camera.
Star is 120 degrees from the moon. Moon is 1% illuminated.
TNO apparent brightness V=21.0

TNO is 40.8 AU from the Sun and 40.2 AU from the Earth.
The TNO is moving 13.8 km/sec on the sky relative to the star, or, 1.7 arcsec/hr.
The 1-sigma error in the time of the event is 133 seconds.
The 1-sigma cross-track error in the shadow position is 1597 km.

The TNO has an absolute magnitude Hv=4.8
Diameter=663.8 km assuming a 5% albedo -- 48.1 sec chord
Diameter=271.0 km assuming a 30% albedo -- 19.6 sec chord
Dynamical classification is SCATNEAR
 
 
 
 
 
 
 
 

Star training set for 120132, (2022/03/02 05:43UT)
Object            RA         Dec     mag  sep  mel
Spica          13:26:21.8 -11:16:35  1.0 12.37 131
PPM 262311     13:58:42.1 -23:07:48  5.8  1.77 118
PPM 262217     13:55:03.9 -21:19:37  8.3  0.41 120
PPM 262210     13:54:48.9 -21:35:49  9.6  0.16 120
120132         13:54:15.4 -21:41:25 12.2       119
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 120132, (2022/03/02 05:43UT)
Object            RA         Dec     mag  sep  mel
Spica          13:25:11.5 -11:09:41  1.0 12.37 131
PPM 262311     13:57:27.7 -23:01:21  5.8  1.77 118
PPM 262217     13:53:50.2 -21:13:07  8.3  0.41 120
PPM 262210     13:53:35.1 -21:29:19  9.6  0.16 120
120132         13:53:01.6 -21:34:55 12.2       120
Positions are for J2000

Event circumstances last updated at 2021/10/04 01:50:02 UT

Marc W. Buie, Southwest Research Institute

RECON