RECON: TNO occultation with 14WP510

Event between 14WP510 and star GA1120:00770096 with event index number of 1038955

Geocentric closest approach at 2019/11/13 21:44:03 UTC

J2000 position of star is 04:45:03.4 +22:02:30
Equinox of date position of star is 04:46:11.9 +22:04:32
Stellar brightness G=15.1, use SENSEUP=128
Star is 6 degrees from the moon. Moon is 98% illuminated.
TNO apparent brightness V=22.8

TNO is 35.0 AU from the Sun and 34.0 AU from the Earth.
The TNO is moving 22.9 km/sec on the sky relative to the star, or, 3.3 arcsec/hr.
The 1-sigma error in the time of the event is 95 seconds.
The 1-sigma cross-track error in the shadow position is 1342 km.

The TNO has an absolute magnitude Hv=7.3
Diameter=230.2 km assuming a 5% albedo -- 9.1 sec chord
Diameter=94.0 km assuming a 30% albedo -- 3.7 sec chord
Dynamical classification is 3:2E
 
 
 
 
 
 
 
 

Star training set for 14WP510, (2019/11/13 21:44UT)
Object            RA         Dec     mag  sep  mel
Aldebaran      04:37:03.8 +16:32:52  0.8  5.94   4
Alnath         05:27:33.0 +28:37:21  1.6 11.39  18
PPM 093742     04:46:54.6 +23:39:47  6.1  1.59   7
PPM 093732     04:45:33.8 +21:41:35  8.4  0.42   6
PPM 093725     04:44:55.8 +21:50:59 11.1  0.38   6
14WP510        04:46:14.7 +22:04:37 15.1         7
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 14WP510, (2019/11/13 21:44UT)
Object            RA         Dec     mag  sep  mel
Aldebaran      04:35:55.3 +16:30:30  0.8  5.94   4
Alnath         05:26:17.5 +28:36:23  1.6 11.39  18
PPM 093742     04:45:42.5 +23:37:41  6.1  1.59   7
PPM 093732     04:44:22.7 +21:39:27  8.4  0.42   6
PPM 093725     04:43:44.6 +21:48:50 11.1  0.38   6
14WP510        04:45:03.4 +22:02:30 15.1         6
Positions are for J2000

Event circumstances last updated at 2019/01/29 21:45:14 UT

Marc W. Buie, Southwest Research Institute

RECON