Event between (547375) 10PC88 and star GA0900:00315574 with event index number of 2136714
Geocentric closest approach at 2026/10/12 00:15:37 UTC
J2000 position of star is 03:41:13.2 +00:48:37
Equinox of date position of star is 03:42:27.5 +00:53:10
Stellar brightness G=15.5,
use SENSEUP=128 with the MallinCam and and exposure
time of 2 seconds with the QHY174 camera.
Star is 151 degrees from the moon.
Moon is 2% illuminated.
Apparent brightness V=22.2
Object is 26.8 AU from the Sun
and 26.0 AU from the Earth.
Apparent velocity is 19.8
km/sec on the sky relative to the star, or,
3.8 arcsec/hr.
The 1-sigma error in the time of the event is 106 seconds.
The 1-sigma cross-track error in the shadow position is
1319 km.
The object has an absolute magnitude Hv=7.8
Diameter=162.9 km assuming a 5% albedo -- 8.5 sec chord
Diameter=66.5 km assuming a 30% albedo -- 3.5 sec chord
Dynamical classification is CENTAURS
Star training set for 547375, (2026/10/12 00:16UT) Object RA Dec mag sep mel Aldebaran 04:37:27.6 +16:33:40 0.8 20.69 144 Menkar 03:03:41.0 +04:11:36 2.5 10.26 160 10 Tau 03:38:14.6 +00:29:08 4.3 1.16 151 PPM 146746 03:39:12.8 +00:13:38 7.6 1.08 151 PPM 146766 03:40:21.6 +00:52:55 9.1 0.56 151 PPM 146824 03:43:00.0 +01:11:47 10.9 0.32 151 547375 03:42:36.0 +00:53:42 15.5 150 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 547375, (2026/10/12 00:16UT) Object RA Dec mag sep mel Aldebaran 04:35:55.3 +16:30:29 0.8 20.69 144 Menkar 03:02:16.8 +04:05:21 2.5 10.26 160 10 Tau 03:36:52.0 +00:23:56 4.3 1.16 151 PPM 146746 03:37:50.4 +00:08:27 7.6 1.08 151 PPM 146766 03:38:58.8 +00:47:46 9.1 0.56 151 PPM 146824 03:41:37.0 +01:06:43 10.9 0.32 151 547375 03:41:13.2 +00:48:37 15.5 151 Positions are for J2000
Event circumstances last updated at 2024/01/09 04:30:07 UT
Marc W. Buie, Southwest Research Institute