Event between (523713) 14JX80 and star GA0940:06502089 with event index number of 2377983
Geocentric closest approach at 2028/09/14 22:21:22 UTC
J2000 position of star is 18:14:04.5 +05:13:23
Equinox of date position of star is 18:15:14.3 +05:13:54
Stellar brightness G=16.7,
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 20% illuminated.
Apparent brightness V=22.1
Object is 37.2 AU from the Sun
and 37.0 AU from the Earth.
Apparent velocity is 13.4
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 103 seconds.
The 1-sigma cross-track error in the shadow position is
2555 km.
The object has an absolute magnitude Hv=6.2
Diameter=340.4 km assuming a 5% albedo -- 26.3 sec chord
Diameter=139.0 km assuming a 30% albedo -- 10.7 sec chord
Dynamical classification is 5:2EEE+5:2EII
Star training set for 523713, (2028/09/14 22:22UT) Object RA Dec mag sep mel Vega 18:37:54.6 +38:48:41 0.0 33.96 118 60Bet Oph 17:44:53.5 +04:33:26 2.8 7.65 138 73 Oph 18:10:59.6 +04:00:02 6.0 1.67 143 PPM 165339 18:12:32.4 +05:40:04 8.0 0.85 142 PPM 165385 18:13:57.1 +05:28:28 9.7 0.45 143 PPM 165429 18:15:25.8 +05:18:49 11.4 0.08 143 523713 18:15:29.2 +05:14:00 16.7 143 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 523713, (2028/09/14 22:22UT) Object RA Dec mag sep mel Vega 18:36:56.7 +38:47:07 0.0 33.96 118 60Bet Oph 17:43:28.3 +04:34:06 2.8 7.65 138 73 Oph 18:09:34.0 +03:59:36 6.0 1.67 143 PPM 165339 18:11:07.9 +05:39:35 8.0 0.85 142 PPM 165385 18:12:32.5 +05:27:55 9.7 0.45 143 PPM 165429 18:14:01.0 +05:18:12 11.4 0.08 143 523713 18:14:04.5 +05:13:23 16.7 143 Positions are for J2000
Event circumstances last updated at 2023/08/26 02:51:45 UT
Marc W. Buie, Southwest Research Institute