RECON: TNO occultation with 03LD9

Event between 03LD9 and star GA0700:26878922 with event index number of 1664204

Geocentric closest approach at 2025/08/16 21:03:52 UTC

J2000 position of star is 18:35:27.4 -18:25:40
Equinox of date position of star is 18:36:51.3 -18:24:25
Stellar brightness G=16.8, use SENSEUP=128 with the MallinCam and and exposure time of 2 seconds with the QHY174 camera.
Star is 143 degrees from the moon. Moon is 43% illuminated.
Apparent brightness V=23.1

Object is 43.5 AU from the Sun and 42.8 AU from the Earth.
Apparent velocity is 15.9 km/sec on the sky relative to the star, or, 1.8 arcsec/hr.
The 1-sigma error in the time of the event is 1346 seconds.
The 1-sigma cross-track error in the shadow position is 4575 km.

The object has an absolute magnitude Hv=6.6
Diameter=295.1 km assuming a 5% albedo -- 18.6 sec chord
Diameter=120.5 km assuming a 30% albedo -- 7.6 sec chord
Dynamical classification is SCATNEAR
 
 
 
 
 
 
 
 

Star training set for 03LD9, (2025/08/16 21:04UT)
Object            RA         Dec     mag  sep  mel
Antares        16:30:59.0 -26:29:12  0.9 30.12 173
Nunki          18:56:51.1 -26:15:45  2.0  9.10 141
PPM 234652     18:32:56.4 -18:22:58  5.0  0.95 144
PPM 234757     18:37:06.9 -18:31:41  7.6  0.13 143
03LD9          18:36:57.5 -18:24:19 16.8       143
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 03LD9, (2025/08/16 21:04UT)
Object            RA         Dec     mag  sep  mel
Antares        16:29:24.4 -26:25:56  0.9 30.12 173
Nunki          18:55:15.9 -26:17:49  2.0  9.10 141
PPM 234652     18:31:26.3 -18:24:10  5.0  0.95 144
PPM 234757     18:35:36.8 -18:33:02  7.6  0.13 143
03LD9          18:35:27.4 -18:25:40 16.8       143
Positions are for J2000

Event circumstances last updated at 2023/11/13 03:59:48 UT

Marc W. Buie, Southwest Research Institute

RECON