RECON: TNO occultation with 04VY130

Event between 04VY130 and star UC4-535-010509 with event index number of 238034

Geocentric closest approach at 2018/03/07 01:34:43 UTC

J2000 position of star is 04:56:18.4 +16:48:45
Equinox of date position of star is 04:57:20.9 +16:50:24
Stellar brightness R=15.8, use SENSEUP=128
Star is 155 degrees from the moon. Moon is 73% illuminated.
TNO apparent brightness V=23.0

TNO is 29.6 AU from the Sun and 29.6 AU from the Earth.
The TNO is moving 6.7 km/sec on the sky relative to the star, or, 1.1 arcsec/hr.
The 1-sigma error in the time of the event is 473 seconds.
The 1-sigma cross-track error in the shadow position is 2190 km.

The TNO has an absolute magnitude Hv=8.1
Diameter=144.5 km assuming a 5% albedo -- 21.6 sec chord
Diameter=59.0 km assuming a 30% albedo -- 8.8 sec chord
Dynamical classification is 3:2E
 
 
 
 
 
 
 
 

Star training set for 04VY130, (2018/03/07 01:35UT)
Object            RA         Dec     mag  sep  mel
Aldebaran      04:36:58.0 +16:32:40  0.8  4.89 160
Bellatrix      05:26:06.4 +06:21:53  1.6 12.62 147
PPM 120426     04:58:25.4 +17:10:49  6.3  0.43 155
PPM 120395     04:56:22.4 +16:38:53  7.5  0.30 155
PPM 120409     04:57:18.0 +16:35:48 10.6  0.24 155
04VY130        04:57:21.3 +16:50:24 15.8       155
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 04VY130, (2018/03/07 01:35UT)
Object            RA         Dec     mag  sep  mel
Aldebaran      04:35:55.3 +16:30:30  0.8  4.89 160
Bellatrix      05:25:07.8 +06:20:58  1.6 12.62 147
PPM 120426     04:57:22.2 +17:09:12  6.3  0.43 155
PPM 120395     04:55:19.6 +16:37:12  7.5  0.30 155
PPM 120409     04:56:15.2 +16:34:09 10.6  0.24 155
04VY130        04:56:18.4 +16:48:45 15.8       155
Positions are for J2000

Event circumstances last updated at 2018/01/16 17:03:18 UT

Marc W. Buie, Southwest Research Institute

RECON