RECON: TNO occultation with 15BZ518

Event between 15BZ518 and star GA0680:06219272 with event index number of 265962

Geocentric closest approach at 2020/05/08 19:41:49 UTC

J2000 position of star is 15:20:22.9 -20:16:42
Equinox of date position of star is 15:21:32.7 -20:21:01
Stellar brightness G=15.0, use SENSEUP=128
Star is 15 degrees from the moon. Moon is 97% illuminated.
TNO apparent brightness V=26.8

TNO is 48.4 AU from the Sun and 47.4 AU from the Earth.
The TNO is moving 25.3 km/sec on the sky relative to the star, or, 2.6 arcsec/hr.
The 1-sigma error in the time of the event is 131 seconds.
The 1-sigma cross-track error in the shadow position is 2245 km.

The TNO has an absolute magnitude Hv=10.0
Diameter=660.7 km assuming a 5% albedo -- 2.4 sec chord
Diameter=269.7 km assuming a 30% albedo -- 1.0 sec chord
Dynamical classification is SCATEXTD
 
 
 
 
 
 
 
 

Star training set for 15BZ518, (2020/05/08 19:42UT)
Object            RA         Dec     mag  sep  mel
Antares        16:30:39.5 -26:28:32  0.9 16.98   7
7Del Sco       16:01:32.4 -22:40:41  2.3  9.58   6
28 Lib         15:22:03.1 -18:13:52  6.4  2.12  15
PPM 264102     15:20:58.6 -20:56:41  8.5  0.61  15
PPM 264117     15:21:38.4 -20:35:19 10.0  0.24  15
15BZ518        15:21:33.2 -20:21:03 15.0        15
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 15BZ518, (2020/05/08 19:42UT)
Object            RA         Dec     mag  sep  mel
Antares        16:29:24.4 -26:25:56  0.9 16.98   7
7Del Sco       16:00:20.0 -22:37:18  2.3  9.58   6
28 Lib         15:20:53.7 -18:09:32  6.4  2.12  15
PPM 264102     15:19:48.1 -20:52:19  8.5  0.61  15
PPM 264117     15:20:28.0 -20:30:59 10.0  0.24  15
15BZ518        15:20:22.9 -20:16:42 15.0        15
Positions are for J2000

Event circumstances last updated at 2020/03/12 20:24:47 UT

Marc W. Buie, Southwest Research Institute

RECON