RECON: TNO occultation with 523773

Event between (523773) 14XS40 and star GA0840:03691944 with event index number of 347776

Geocentric closest approach at 2018/12/05 02:22:18 UTC

J2000 position of star is 08:57:47.1 -05:36:51
Equinox of date position of star is 08:58:43.2 -05:41:16
Stellar brightness G=15.2, use SENSEUP=128
Star is 90 degrees from the moon. Moon is 5% illuminated.
TNO apparent brightness V=21.2

TNO is 36.9 AU from the Sun and 36.5 AU from the Earth.
The TNO is moving 11.5 km/sec on the sky relative to the star, or, 1.6 arcsec/hr.
The 1-sigma error in the time of the event is 163 seconds.
The 1-sigma cross-track error in the shadow position is 1384 km.

The TNO has an absolute magnitude Hv=5.4
Diameter=501.2 km assuming a 5% albedo -- 43.6 sec chord
Diameter=204.6 km assuming a 30% albedo -- 17.8 sec chord
Dynamical classification is SCATEXTD
 
 
 
 
 
 
 
 

Star training set for 523773, (2018/12/05 02:22UT)
Object            RA         Dec     mag  sep  mel
Regulus        10:09:22.7 +11:52:26  1.3 24.84  77
Alphard        09:28:31.1 -08:44:29  2.0  7.99  82
PPM 191823     08:55:13.9 -05:30:26  6.4  0.89  91
PPM 191884     08:58:55.1 -04:56:01  7.1  0.76  90
PPM 191875     08:58:31.1 -05:45:15  9.2  0.08  90
523773         08:58:43.6 -05:41:17 15.2        90
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 523773, (2018/12/05 02:22UT)
Object            RA         Dec     mag  sep  mel
Regulus        10:08:22.0 +11:58:02  1.3 24.84  77
Alphard        09:27:35.2 -08:39:31  2.0  7.99  82
PPM 191823     08:54:17.4 -05:26:04  6.4  0.89  91
PPM 191884     08:57:58.5 -04:51:35  7.1  0.76  90
PPM 191875     08:57:34.7 -05:40:49  9.2  0.08  90
523773         08:57:47.1 -05:36:51 15.2        90
Positions are for J2000

Event circumstances last updated at 2018/10/24 21:08:15 UT

Marc W. Buie, Southwest Research Institute

RECON