RECON: TNO occultation with 470308

Event between (470308) 07JH43 and star GA0620:11514833 with event index number of 2219196

Geocentric closest approach at 2023/03/23 23:20:01 UTC

J2000 position of star is 16:59:55.0 -26:12:29
Equinox of date position of star is 17:01:20.5 -26:14:27
Stellar brightness G=16.2, use SENSEUP=128 with the MallinCam and and exposure time of 2 seconds with the QHY174 camera.
Star is 136 degrees from the moon. Moon is 7% illuminated.
Apparent brightness V=21.0

Object is 40.5 AU from the Sun and 40.2 AU from the Earth.
Apparent velocity is 4.7 km/sec on the sky relative to the star, or, 0.6 arcsec/hr.
The 1-sigma error in the time of the event is 387 seconds.
The 1-sigma cross-track error in the shadow position is 2218 km.

The object has an absolute magnitude Hv=4.8
Diameter=758.6 km assuming a 5% albedo -- 139.1 sec chord
Diameter=309.7 km assuming a 30% albedo -- 56.8 sec chord
Dynamical classification is SCATNEAR
 
 
 
 
 
 
 
 

Star training set for 470308, (2023/03/23 23:20UT)
Object            RA         Dec     mag  sep  mel
Antares        16:30:50.1 -26:28:53  0.9  6.84 143
23Tau Sco      16:37:19.9 -28:15:44  2.8  5.71 141
26 Oph         17:01:35.0 -25:01:21  5.8  1.22 136
PPM 266235     17:00:53.8 -26:24:23  8.5  0.19 136
470308         17:01:21.2 -26:14:28 16.2       136
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 470308, (2023/03/23 23:20UT)
Object            RA         Dec     mag  sep  mel
Antares        16:29:24.4 -26:25:56  0.9  6.84 143
23Tau Sco      16:35:52.9 -28:12:58  2.8  5.71 141
26 Oph         17:00:09.6 -24:59:22  5.8  1.22 136
PPM 266235     16:59:27.5 -26:22:23  8.5  0.19 136
470308         16:59:55.0 -26:12:29 16.2       136
Positions are for J2000

Event circumstances last updated at 2023/01/09 03:35:07 UT

Marc W. Buie, Southwest Research Institute

RECON