RECON: TNO occultation with 530930

Event between (530930) 11WG157 and star GA1340:02088530 with event index number of 2444014

Geocentric closest approach at 2026/01/22 21:02:36 UTC

J2000 position of star is 04:26:11.6 +44:31:21
Equinox of date position of star is 04:27:47.0 +44:34:18
Stellar brightness G=16.5, use SENSEUP=128 with the MallinCam and and exposure time of 2 seconds with the QHY174 camera.
Star is 82 degrees from the moon. Moon is 17% illuminated.
TNO apparent brightness V=22.3

TNO is 30.6 AU from the Sun and 30.0 AU from the Earth.
The TNO is moving 16.5 km/sec on the sky relative to the star, or, 2.7 arcsec/hr.
The 1-sigma error in the time of the event is 170 seconds.
The 1-sigma cross-track error in the shadow position is 2132 km.

The TNO has an absolute magnitude Hv=7.3
Diameter=211.8 km assuming a 5% albedo -- 12.9 sec chord
Diameter=86.5 km assuming a 30% albedo -- 5.3 sec chord
Dynamical classification is 1:1
 
 
 
 
 
 
 
 

Star training set for 530930, (2026/01/22 21:03UT)
Object            RA         Dec     mag  sep  mel
Aldebaran      04:37:25.1 +16:33:35  0.8 28.09  79
Mirphak        03:26:11.8 +49:57:06  1.8 11.76  73
53 Per         04:23:26.7 +46:33:32  4.7  2.14  81
PPM 047072     04:28:08.8 +44:48:36  8.1  0.23  82
530930         04:28:03.2 +44:34:47 16.5        82
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 530930, (2026/01/22 21:03UT)
Object            RA         Dec     mag  sep  mel
Aldebaran      04:35:55.3 +16:30:29  0.8 28.09  79
Mirphak        03:24:19.4 +49:51:40  1.8 11.76  73
53 Per         04:21:33.1 +46:29:56  4.7  2.14  81
PPM 047072     04:26:16.9 +44:45:10  8.1  0.23  82
530930         04:26:11.6 +44:31:21 16.5        82
Positions are for J2000

Event circumstances last updated at 2022/04/13 23:07:35 UT

Marc W. Buie, Southwest Research Institute

RECON