RECON: TNO occultation with 554102

Event between (554102) 12KW51 and star GA0820:04785896 with event index number of 2227929

Geocentric closest approach at 2023/05/23 22:03:56 UTC

J2000 position of star is 15:35:55.1 -07:37:25
Equinox of date position of star is 15:37:05.2 -07:41:41
Stellar brightness G=17.0, use SENSEUP=128 with the MallinCam and and exposure time of 2 seconds with the QHY174 camera.
Star is 120 degrees from the moon. Moon is 18% illuminated.
TNO apparent brightness V=22.3

TNO is 39.2 AU from the Sun and 38.2 AU from the Earth.
The TNO is moving 24.1 km/sec on the sky relative to the star, or, 3.1 arcsec/hr.
The 1-sigma error in the time of the event is 110 seconds.
The 1-sigma cross-track error in the shadow position is 1482 km.

The TNO has an absolute magnitude Hv=6.4
Diameter=309.0 km assuming a 5% albedo -- 12.8 sec chord
Diameter=126.2 km assuming a 30% albedo -- 5.2 sec chord
Dynamical classification is 2:1E
 
 
 
 
 
 
 
 

Star training set for 554102, (2023/05/23 22:04UT)
Object            RA         Dec     mag  sep  mel
Antares        16:30:50.7 -26:28:55  0.9 22.70 138
27Bet Lib      15:18:16.2 -09:28:04  2.6  5.00 116
PPM 198725     15:35:42.5 -09:15:38  5.6  1.60 120
PPM 198755     15:37:19.1 -07:42:30  8.2  0.04 120
554102         15:37:10.4 -07:42:00 17.0       120
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 554102, (2023/05/23 22:04UT)
Object            RA         Dec     mag  sep  mel
Antares        16:29:24.4 -26:25:56  0.9 22.70 138
27Bet Lib      15:17:00.3 -09:22:59  2.6  5.00 116
PPM 198725     15:34:26.4 -09:11:01  5.6  1.60 120
PPM 198755     15:36:03.7 -07:37:56  8.2  0.04 120
554102         15:35:55.1 -07:37:25 17.0       120
Positions are for J2000

Event circumstances last updated at 2021/10/17 01:16:02 UT

Marc W. Buie, Southwest Research Institute

RECON