RECON: TNO occultation with 281371

Event between (281371) 08FC76 and star UC4-505-022464 with event index number of 318623

Geocentric closest approach at 2019/11/04 02:38:08 UTC

J2000 position of star is 06:14:03.2 +10:58:15
Equinox of date position of star is 06:15:08.0 +10:57:50
Stellar brightness R=16.2, use SENSEUP=128
Star is 143 degrees from the moon. Moon is 47% illuminated.
TNO apparent brightness V=20.2

TNO is 11.8 AU from the Sun and 11.1 AU from the Earth.
The TNO is moving 13.6 km/sec on the sky relative to the star, or, 6.1 arcsec/hr.
The 1-sigma error in the time of the event is 81 seconds.
The 1-sigma cross-track error in the shadow position is 1071 km.

The TNO has an absolute magnitude Hv=9.3
Diameter=83.2 km assuming a 5% albedo -- 6.1 sec chord
Diameter=34.0 km assuming a 30% albedo -- 2.5 sec chord
Dynamical classification is CENTAURR
 
 
 
 
 
 
 
 

Star training set for 281371, (2019/11/04 02:38UT)
Object            RA         Dec     mag  sep  mel
Betelgeuse     05:56:14.8 +07:24:33  0.4  5.87 137
Alhena         06:38:51.5 +16:22:50  1.9  7.90 150
75 Ori         06:18:12.3 +09:56:01  5.4  1.27 143
PPM 122109     06:14:18.6 +10:37:08  7.7  0.40 143
PPM 122125     06:14:56.5 +10:50:10  9.5  0.14 143
281371         06:15:09.3 +10:57:49 16.2       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 281371, (2019/11/04 02:38UT)
Object            RA         Dec     mag  sep  mel
Betelgeuse     05:55:10.3 +07:24:26  0.4  5.87 137
Alhena         06:37:42.8 +16:23:57  1.9  7.90 150
75 Ori         06:17:06.6 +09:56:31  5.4  1.27 143
PPM 122109     06:13:12.6 +10:37:32  7.7  0.40 143
PPM 122125     06:13:50.4 +10:50:35  9.5  0.14 143
281371         06:14:03.2 +10:58:15 16.2       143
Positions are for J2000

Event circumstances last updated at 2019/06/07 22:50:58 UT

Marc W. Buie, Southwest Research Institute

RECON