RECON: TNO occultation with 555632

Event between (555632) 14BZ57 and star GA0740:04480034 with event index number of 2471122

Geocentric closest approach at 2026/05/15 14:35:56 UTC

J2000 position of star is 10:02:32.1 -14:52:14
Equinox of date position of star is 10:03:42.3 -14:59:17
Stellar brightness G=16.8, 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 2% illuminated.
Apparent brightness V=20.7

Object is 37.0 AU from the Sun and 36.8 AU from the Earth.
Apparent velocity is 11.3 km/sec on the sky relative to the star, or, 1.5 arcsec/hr.
The 1-sigma error in the time of the event is 143 seconds.
The 1-sigma cross-track error in the shadow position is 1762 km.

The object has an absolute magnitude Hv=4.9
Diameter=608.2 km assuming a 5% albedo -- 54.5 sec chord
Diameter=248.3 km assuming a 30% albedo -- 22.3 sec chord
Dynamical classification is SCATEXTD
 
 
 
 
 
 
 
 

Star training set for 555632, (2026/05/15 14:34UT)
Object            RA         Dec     mag  sep  mel
Regulus        10:09:46.5 +11:50:14  1.3 26.88 112
Alphard        09:28:53.0 -08:46:27  2.0 10.57 110
40Ups2Hya      10:06:24.6 -13:11:37  4.6  1.91 120
PPM 222340     10:03:21.5 -15:09:26  8.1  0.19 120
555632         10:03:48.6 -14:59:55 16.8       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 555632, (2026/05/15 14:34UT)
Object            RA         Dec     mag  sep  mel
Regulus        10:08:21.9 +11:58:02  1.3 26.88 112
Alphard        09:27:35.2 -08:39:30  2.0 10.57 110
40Ups2Hya      10:05:07.4 -13:03:52  4.6  1.91 120
PPM 222340     10:02:05.0 -15:01:45  8.1  0.19 120
555632         10:02:32.1 -14:52:14 16.8       120
Positions are for J2000

Event circumstances last updated at 2024/03/19 03:48:14 UT

Marc W. Buie, Southwest Research Institute

RECON