RECON: TNO occultation with 472235

Event between (472235) Zhulong and star GA0740:05170505 with event index number of 2309974

Geocentric closest approach at 2023/05/23 13:58:53 UTC

J2000 position of star is 14:21:14.8 -14:55:58
Equinox of date position of star is 14:22:31.5 -15:02:20
Stellar brightness G=14.0, use SENSEUP=64 with the MallinCam and and exposure time of 1 seconds with the QHY174 camera.
Star is 110 degrees from the moon. Moon is 15% illuminated.
Apparent brightness V=21.7

Object is 33.0 AU from the Sun and 32.1 AU from the Earth.
Apparent velocity is 20.9 km/sec on the sky relative to the star, or, 3.2 arcsec/hr.
The 1-sigma error in the time of the event is 68 seconds.
The 1-sigma cross-track error in the shadow position is 1244 km.

The object has an absolute magnitude Hv=6.5
Diameter=295.1 km assuming a 5% albedo -- 14.4 sec chord
Diameter=120.5 km assuming a 30% albedo -- 5.9 sec chord
Dynamical classification is 5:2EEE
 
 
 
 
 
 
 
 

Star training set for 472235, (2023/05/23 13:58UT)
Object            RA         Dec     mag  sep  mel
Spica          13:26:25.7 -11:16:58  1.0 14.16  96
PPM 228402     14:12:07.4 -16:24:41  4.2  2.85 109
PPM 228613     14:20:21.5 -14:38:10  8.5  0.66 110
PPM 228666     14:22:46.9 -14:59:10  9.5  0.08 110
472235         14:22:31.6 -15:02:20 14.0       111
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 472235, (2023/05/23 13:58UT)
Object            RA         Dec     mag  sep  mel
Spica          13:25:11.5 -11:09:41  1.0 14.16  96
PPM 228402     14:10:50.5 -16:18:08  4.2  2.85 109
PPM 228613     14:19:05.0 -14:31:46  8.5  0.66 110
PPM 228666     14:21:30.2 -14:52:48  9.5  0.08 110
472235         14:21:14.8 -14:55:58 14.0       110
Positions are for J2000

Event circumstances last updated at 2023/05/17 03:32:22 UT

Marc W. Buie, Southwest Research Institute

RECON