Event between (523719) 14LM28 and star GA1520:05036922 with event index number of 2292689
Geocentric closest approach at 2025/09/21 18:43:32 UTC
J2000 position of star is 18:12:12.6 +63:14:10
Equinox of date position of star is 18:12:23.1 +63:14:36
Stellar brightness G=14.4,
use SENSEUP=64 with the MallinCam and and exposure
time of 1 seconds with the QHY174 camera.
Star is 92 degrees from the moon.
Moon is 0% illuminated.
Apparent brightness V=23.2
Object is 20.3 AU from the Sun
and 20.3 AU from the Earth.
Apparent velocity is 22.2
km/sec on the sky relative to the star, or,
5.4 arcsec/hr.
The 1-sigma error in the time of the event is 255 seconds.
The 1-sigma cross-track error in the shadow position is
4314 km.
The object has an absolute magnitude Hv=9.9
Diameter=63.1 km assuming a 5% albedo -- 2.8 sec chord
Diameter=25.8 km assuming a 30% albedo -- 1.1 sec chord
Dynamical classification is CENTAURR
Star training set for 523719, (2025/09/21 18:44UT) Object RA Dec mag sep mel Vega 18:37:48.5 +38:48:31 0.0 24.73 99 Etamin 17:57:12.3 +51:29:13 2.2 11.93 91 36 Dra 18:14:02.5 +64:24:22 5.0 1.18 92 PPM 020837 18:16:23.0 +64:04:55 8.2 0.95 93 PPM 020807 18:13:13.4 +63:21:10 9.0 0.14 92 PPM 020799 18:12:10.8 +63:19:13 10.6 0.08 92 523719 18:12:23.7 +63:14:37 14.4 92 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 523719, (2025/09/21 18:44UT) Object RA Dec mag sep mel Vega 18:36:56.7 +38:47:07 0.0 24.73 99 Etamin 17:56:36.3 +51:29:20 2.2 11.93 91 36 Dra 18:13:55.0 +64:23:51 5.0 1.18 92 PPM 020837 18:16:14.4 +64:04:18 8.2 0.95 93 PPM 020807 18:13:02.6 +63:20:40 9.0 0.14 92 PPM 020799 18:12:00.0 +63:18:46 10.6 0.08 92 523719 18:12:12.6 +63:14:10 14.4 92 Positions are for J2000
Event circumstances last updated at 2024/06/18 02:54:11 UT
Marc W. Buie, Southwest Research Institute