Event between (78799) 02XW93 and star GA1240:02825523 with event index number of 2436593
Geocentric closest approach at 2025/12/25 16:38:47 UTC
J2000 position of star is 06:39:56.4 +34:42:34
Equinox of date position of star is 06:41:32.8 +34:41:08
Stellar brightness G=15.4,
use SENSEUP=128 with the MallinCam and and exposure
time of 2 seconds with the QHY174 camera.
Star is 119 degrees from the moon.
Moon is 28% illuminated.
Apparent brightness V=21.5
Object is 46.3 AU from the Sun
and 45.3 AU from the Earth.
Apparent velocity is 26.4
km/sec on the sky relative to the star, or,
2.9 arcsec/hr.
The 1-sigma error in the time of the event is 181 seconds.
The 1-sigma cross-track error in the shadow position is
1690 km.
The object has an absolute magnitude Hv=4.9
Diameter=605.4 km assuming a 5% albedo -- 23.9 sec chord
Diameter=247.1 km assuming a 30% albedo -- 9.7 sec chord
Dynamical classification is CENTAURR
Star training set for 78799, (2025/12/25 16:41UT) Object RA Dec mag sep mel Pollux 07:46:54.3 +27:57:41 1.1 15.44 135 34Bet Aur 06:01:26.2 +44:56:50 1.9 12.82 110 PPM 071742 06:34:08.9 +32:26:03 6.0 2.74 118 PPM 071969 06:44:17.2 +34:04:10 7.9 0.82 120 PPM 071944 06:43:17.4 +34:49:58 9.4 0.37 120 PPM 071912 06:41:22.4 +34:47:19 10.1 0.12 119 78799 06:41:40.0 +34:41:02 15.4 120 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 78799, (2025/12/25 16:41UT) Object RA Dec mag sep mel Pollux 07:45:17.9 +28:01:33 1.1 15.44 135 34Bet Aur 05:59:31.6 +44:56:51 1.9 12.82 110 PPM 071742 06:32:27.1 +32:27:18 6.0 2.74 118 PPM 071969 06:42:34.2 +34:05:48 7.9 0.82 120 PPM 071944 06:41:33.8 +34:51:34 9.4 0.37 120 PPM 071912 06:39:38.8 +34:48:51 10.1 0.12 119 78799 06:39:56.4 +34:42:34 15.4 119 Positions are for J2000
Event circumstances last updated at 2024/03/04 05:37:36 UT
Marc W. Buie, Southwest Research Institute