RECON: TNO occultation with 307982

Event between (307982) 04PG115 and star GA0980:18278311 with event index number of 2185793

Geocentric closest approach at 2025/12/07 17:11:38 UTC

J2000 position of star is 22:57:56.9 +08:46:54
Equinox of date position of star is 22:59:09.9 +08:54:41
Stellar brightness G=16.0, use SENSEUP=128 with the MallinCam and and exposure time of 2 seconds with the QHY174 camera.
Star is 123 degrees from the moon. Moon is 89% illuminated.
Apparent brightness V=21.2

Object is 40.6 AU from the Sun and 40.5 AU from the Earth.
Apparent velocity is 9.0 km/sec on the sky relative to the star, or, 1.1 arcsec/hr.
The 1-sigma error in the time of the event is 168 seconds.
The 1-sigma cross-track error in the shadow position is 1630 km.

The object has an absolute magnitude Hv=5.0
Diameter=611.0 km assuming a 5% albedo -- 67.1 sec chord
Diameter=249.4 km assuming a 30% albedo -- 27.4 sec chord
Dynamical classification is SCATNEAR
 
 
 
 
 
 
 
 

Star training set for 307982, (2025/12/07 17:07UT)
Object            RA         Dec     mag  sep  mel
Markab         23:06:03.3 +15:20:43  2.5  6.64 117
50Rho Peg      22:56:32.0 +08:57:18  4.9  0.67 123
PPM 173605     22:59:48.2 +09:57:53  8.2  1.05 122
PPM 173608     22:59:54.2 +08:56:41  8.6  0.16 122
307982         22:59:15.2 +08:55:15 16.0       122
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 307982, (2025/12/07 17:07UT)
Object            RA         Dec     mag  sep  mel
Markab         23:04:45.8 +15:12:18  2.5  6.64 117
50Rho Peg      22:55:13.8 +08:48:59  4.9  0.67 123
PPM 173605     22:58:30.0 +09:49:32  8.2  1.05 122
PPM 173608     22:58:35.8 +08:48:19  8.6  0.16 122
307982         22:57:56.9 +08:46:54 16.0       123
Positions are for J2000

Event circumstances last updated at 2024/03/03 06:09:41 UT

Marc W. Buie, Southwest Research Institute

RECON