RECON: TNO occultation with 469505

Event between (469505) 03FE128 and star GA0700:07502553 with event index number of 1666745

Geocentric closest approach at 2027/02/13 00:02:36 UTC

J2000 position of star is 17:00:26.3 -19:22:30
Equinox of date position of star is 17:01:52.6 -19:24:34
Stellar brightness G=16.6, use SENSEUP=128 with the MallinCam and and exposure time of 2 seconds with the QHY174 camera.
Star is 141 degrees from the moon. Moon is 36% illuminated.
Apparent brightness V=22.2

Object is 36.9 AU from the Sun and 37.3 AU from the Earth.
Apparent velocity is 17.2 km/sec on the sky relative to the star, or, 2.3 arcsec/hr.
The 1-sigma error in the time of the event is 177 seconds.
The 1-sigma cross-track error in the shadow position is 1444 km.

The object has an absolute magnitude Hv=6.3
Diameter=322.1 km assuming a 5% albedo -- 19.1 sec chord
Diameter=131.5 km assuming a 30% albedo -- 7.8 sec chord
Dynamical classification is 2:1E
 
 
 
 
 
 
 
 

Star training set for 469505, (2027/02/13 00:02UT)
Object            RA         Dec     mag  sep  mel
Antares        16:31:04.5 -26:29:23  0.9 10.04 148
35Eta Oph      17:11:56.1 -15:45:24  2.6  4.35 138
29 Oph         17:03:26.6 -18:55:23  5.9  0.59 140
PPM 232457     17:01:54.5 -19:12:24  8.3  0.21 141
469505         17:02:02.0 -19:24:48 16.6       140
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 469505, (2027/02/13 00:02UT)
Object            RA         Dec     mag  sep  mel
Antares        16:29:24.4 -26:25:56  0.9 10.04 148
35Eta Oph      17:10:22.7 -15:43:29  2.6  4.35 138
29 Oph         17:01:51.2 -18:53:08  5.9  0.59 140
PPM 232457     17:00:18.9 -19:10:06  8.3  0.21 141
469505         17:00:26.3 -19:22:30 16.6       141
Positions are for J2000

Event circumstances last updated at 2024/06/21 21:26:52 UT

Marc W. Buie, Southwest Research Institute

RECON