RECON: TNO occultation with 19255

Event between (19255) 94VK8 and star GA1120:02001658 with event index number of 224265

Geocentric closest approach at 2019/11/06 14:15:24 UTC

J2000 position of star is 06:18:30.9 +23:54:30
Equinox of date position of star is 06:19:42.1 +23:53:58
Stellar brightness G=15.3, use SENSEUP=128
Star is 117 degrees from the moon. Moon is 70% illuminated.
TNO apparent brightness V=23.4

TNO is 42.9 AU from the Sun and 42.2 AU from the Earth.
The TNO is moving 14.9 km/sec on the sky relative to the star, or, 1.7 arcsec/hr.
The 1-sigma error in the time of the event is 1940 seconds.
The 1-sigma cross-track error in the shadow position is 1919 km.

The TNO has an absolute magnitude Hv=7.0
Diameter=239.9 km assuming a 5% albedo -- 16.1 sec chord
Diameter=97.9 km assuming a 30% albedo -- 6.6 sec chord
Dynamical classification is CLASSICAL
 
 
 
 
 
 
 
 

Star training set for 19255, (2019/11/06 14:15UT)
Object            RA         Dec     mag  sep  mel
Betelgeuse     05:56:14.8 +07:24:33  0.4 17.42 109
Alhena         06:38:51.5 +16:22:50  1.9  8.75 121
9 Gem          06:18:11.4 +23:43:57  6.1  0.39 116
PPM 095754     06:20:07.0 +23:35:38  7.8  0.32 117
PPM 095738     06:19:35.1 +23:48:25  9.6  0.10 117
19255          06:19:43.6 +23:53:57 15.3       117
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 19255, (2019/11/06 14:15UT)
Object            RA         Dec     mag  sep  mel
Betelgeuse     05:55:10.3 +07:24:26  0.4 17.42 109
Alhena         06:37:42.8 +16:23:57  1.9  8.75 121
9 Gem          06:16:58.7 +23:44:27  6.1  0.39 116
PPM 095754     06:18:54.4 +23:36:12  7.8  0.32 117
PPM 095738     06:18:22.4 +23:48:57  9.6  0.10 117
19255          06:18:30.9 +23:54:30 15.3       117
Positions are for J2000

Event circumstances last updated at 2019/06/07 22:51:34 UT

Marc W. Buie, Southwest Research Institute

RECON