RECON: TNO occultation with 470309

Event between (470309) 07JK43 and star GA1040:06693875 with event index number of 2229184

Geocentric closest approach at 2025/05/19 12:02:32 UTC

J2000 position of star is 18:46:32.9 +14:54:25
Equinox of date position of star is 18:47:39.5 +14:56:05
Stellar brightness G=14.1, use SENSEUP=64 with the MallinCam and and exposure time of 1 seconds with the QHY174 camera.
Star is 51 degrees from the moon. Moon is 61% illuminated.
Apparent brightness V=21.7

Object is 26.4 AU from the Sun and 25.8 AU from the Earth.
Apparent velocity is 21.5 km/sec on the sky relative to the star, or, 4.1 arcsec/hr.
The 1-sigma error in the time of the event is 62 seconds.
The 1-sigma cross-track error in the shadow position is 1258 km.

The object has an absolute magnitude Hv=7.3
Diameter=209.9 km assuming a 5% albedo -- 9.8 sec chord
Diameter=85.7 km assuming a 30% albedo -- 4.0 sec chord
Dynamical classification is CENTAURS
 
 
 
 
 
 
 
 

Star training set for 470309, (2025/05/19 12:03UT)
Object            RA         Dec     mag  sep  mel
Vega           18:37:47.8 +38:48:30  0.0 23.97  69
Tarazed        19:47:28.0 +10:40:36  2.7 15.17  37
PPM 135257     18:49:31.6 +15:25:27  6.5  0.66  51
PPM 135235     18:48:39.8 +14:54:00  9.4  0.24  50
470309         18:47:42.1 +14:56:09 14.1        50
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 470309, (2025/05/19 12:03UT)
Object            RA         Dec     mag  sep  mel
Vega           18:36:56.7 +38:47:07  0.0 23.97  69
Tarazed        19:46:15.6 +10:36:48  2.7 15.17  37
PPM 135257     18:48:22.7 +15:23:39  6.5  0.66  51
PPM 135235     18:47:30.6 +14:52:14  9.4  0.24  50
470309         18:46:32.9 +14:54:25 14.1        51
Positions are for J2000

Event circumstances last updated at 2024/06/13 03:50:24 UT

Marc W. Buie, Southwest Research Institute

RECON