RECON: TNO occultation with 523955

Event between (523955) 98UU43 and star GA1060:01134183 with event index number of 2352733

Geocentric closest approach at 2028/01/27 23:44:17 UTC

J2000 position of star is 05:39:09.8 +17:43:27
Equinox of date position of star is 05:40:34.4 +17:44:09
Stellar brightness G=16.5, use SENSEUP=128 with the MallinCam and and exposure time of 2 seconds with the QHY174 camera.
Star is 123 degrees from the moon. Moon is 2% illuminated.
Apparent brightness V=22.6

Object is 33.9 AU from the Sun and 33.2 AU from the Earth.
Apparent velocity is 17.4 km/sec on the sky relative to the star, or, 2.6 arcsec/hr.
The 1-sigma error in the time of the event is 413 seconds.
The 1-sigma cross-track error in the shadow position is 1947 km.

The object has an absolute magnitude Hv=7.2
Diameter=199.5 km assuming a 5% albedo -- 12.4 sec chord
Diameter=81.5 km assuming a 30% albedo -- 5.1 sec chord
Dynamical classification is 4:3E
 
 
 
 
 
 
 
 

Star training set for 523955, (2028/01/27 23:44UT)
Object            RA         Dec     mag  sep  mel
Betelgeuse     05:56:41.6 +07:24:36  0.4 11.03 126
Alnath         05:28:04.1 +28:37:43  1.6 11.28 120
122 Tau        05:38:41.6 +17:03:18  5.7  0.85 122
PPM 121237     05:41:41.6 +17:41:23  8.4  0.22 123
523955         05:40:48.1 +17:44:16 16.5       123
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 523955, (2028/01/27 23:44UT)
Object            RA         Dec     mag  sep  mel
Betelgeuse     05:55:10.3 +07:24:26  0.4 11.03 126
Alnath         05:26:17.6 +28:36:23  1.6 11.28 120
122 Tau        05:37:03.8 +17:02:24  5.7  0.85 122
PPM 121237     05:40:03.4 +17:40:36  8.4  0.22 123
523955         05:39:09.8 +17:43:27 16.5       123
Positions are for J2000

Event circumstances last updated at 2024/03/06 04:36:32 UT

Marc W. Buie, Southwest Research Institute

RECON