RECON: TNO occultation with 548141

Event between (548141) 10CD270 and star GA1000:03710135 with event index number of 2399748

Geocentric closest approach at 2028/08/07 15:12:49 UTC

J2000 position of star is 13:35:15.5 +10:14:43
Equinox of date position of star is 13:36:28.0 +10:07:17
Stellar brightness G=15.9, use SENSEUP=128 with the MallinCam and and exposure time of 2 seconds with the QHY174 camera.
Star is 137 degrees from the moon. Moon is 95% illuminated.
Apparent brightness V=22.2

Object is 25.0 AU from the Sun and 25.4 AU from the Earth.
Apparent velocity is 21.3 km/sec on the sky relative to the star, or, 4.2 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 1640 km.

The object has an absolute magnitude Hv=8.0
Diameter=145.2 km assuming a 5% albedo -- 7.0 sec chord
Diameter=59.3 km assuming a 30% albedo -- 2.9 sec chord
Dynamical classification is CENTAURR
 
 
 
 
 
 
 
 

Star training set for 548141, (2028/08/07 15:13UT)
Object            RA         Dec     mag  sep  mel
Arcturus       14:16:58.4 +19:02:15  0.0 13.22 126
Vindemiatrix   13:03:36.1 +10:48:22  2.8  8.16 145
PPM 129981     13:40:59.3 +10:36:07  5.8  1.17 136
PPM 129931     13:36:58.8 +10:03:33  7.7  0.08 137
548141         13:36:40.6 +10:05:59 15.9       137
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 548141, (2028/08/07 15:13UT)
Object            RA         Dec     mag  sep  mel
Arcturus       14:15:37.9 +19:10:10  0.0 13.22 126
Vindemiatrix   13:02:10.2 +10:57:33  2.8  8.16 145
PPM 129981     13:39:34.4 +10:44:46  5.8  1.17 136
PPM 129931     13:35:33.6 +10:12:17  7.7  0.08 137
548141         13:35:15.5 +10:14:43 15.9       137
Positions are for J2000

Event circumstances last updated at 2024/05/05 03:42:08 UT

Marc W. Buie, Southwest Research Institute

RECON