RECON: TNO occultation with 50000

Event between (50000) Quaoar and star GA0740:25672621 with event index number of 2328002

Geocentric closest approach at 2028/03/29 04:38:58 UTC

J2000 position of star is 19:01:14.7 -14:42:06
Equinox of date position of star is 19:02:37.2 -14:39:57
Stellar brightness G=17.0, use SENSEUP=128 with the MallinCam and and exposure time of 2 seconds with the QHY174 camera.
Star is 117 degrees from the moon. Moon is 9% illuminated.
Apparent brightness V=18.8

Object is 42.6 AU from the Sun and 42.7 AU from the Earth.
Apparent velocity is 9.3 km/sec on the sky relative to the star, or, 1.1 arcsec/hr.
The 1-sigma error in the time of the event is 361 seconds.
The 1-sigma cross-track error in the shadow position is 1654 km.

The object has an absolute magnitude Hv=2.4
Diameter=1905.5 km assuming a 5% albedo -- 212.8 sec chord
Diameter=777.9 km assuming a 30% albedo -- 86.9 sec chord
Dynamical classification is CLASSICAL
 
 
 
 
 
 
 
 

Star training set for 50000, (2028/03/29 04:40UT)
Object            RA         Dec     mag  sep  mel
Antares        16:31:08.6 -26:29:32  0.9 37.26 153
Nunki          18:57:00.9 -26:15:32  2.0 11.68 121
PPM 235374     19:03:10.3 -15:14:25  6.5  0.59 117
PPM 235371     19:03:04.1 -14:28:34  9.2  0.19 117
50000          19:02:51.1 -14:39:35 17.0       117
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 50000, (2028/03/29 04:40UT)
Object            RA         Dec     mag  sep  mel
Antares        16:29:24.4 -26:25:56  0.9 37.26 153
Nunki          18:55:15.9 -26:17:49  2.0 11.68 121
PPM 235374     19:01:33.5 -15:16:58  6.5  0.59 117
PPM 235371     19:01:27.9 -14:31:06  9.2  0.19 117
50000          19:01:14.7 -14:42:06 17.0       117
Positions are for J2000

Event circumstances last updated at 2024/03/07 04:20:22 UT

Marc W. Buie, Southwest Research Institute

RECON