RECON: TNO occultation with 15VR164

Event between 15VR164 and star GA1080:00428855 with event index number of 1019763

Geocentric closest approach at 2019/01/07 12:39:50 UTC

J2000 position of star is 03:47:40.2 +18:51:10
Equinox of date position of star is 03:48:45.6 +18:54:36
Stellar brightness G=16.9, use SENSEUP=128
Star is 116 degrees from the moon. Moon is 2% illuminated.
TNO apparent brightness V=23.1

TNO is 31.2 AU from the Sun and 30.5 AU from the Earth.
The TNO is moving 14.6 km/sec on the sky relative to the star, or, 2.4 arcsec/hr.
The 1-sigma error in the time of the event is 518 seconds.
The 1-sigma cross-track error in the shadow position is 4791 km.

The TNO has an absolute magnitude Hv=8.1
Diameter=143.2 km assuming a 5% albedo -- 9.8 sec chord
Diameter=58.5 km assuming a 30% albedo -- 4.0 sec chord
Dynamical classification is 3:2E
 
 
 
 
 
 
 
 

Star training set for 15VR164, (2019/01/07 12:40UT)
Object            RA         Dec     mag  sep  mel
Aldebaran      04:37:00.9 +16:32:46  0.8 11.73 127
44Zet Per      03:55:19.9 +31:56:19  2.8 13.11 120
13 Tau         03:43:25.0 +19:45:35  5.7  1.52 115
PPM 119423     03:53:24.5 +18:58:24  8.5  1.10 117
PPM 119363     03:48:47.2 +18:57:40  9.6  0.05 116
15VR164        03:48:45.9 +18:54:37 16.9       116
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 15VR164, (2019/01/07 12:40UT)
Object            RA         Dec     mag  sep  mel
Aldebaran      04:35:55.3 +16:30:30  0.8 11.73 127
44Zet Per      03:54:07.9 +31:53:01  2.8 13.11 120
13 Tau         03:42:18.9 +19:42:01  5.7  1.52 115
PPM 119423     03:52:18.6 +18:55:03  8.5  1.10 117
PPM 119363     03:47:41.4 +18:54:13  9.6  0.05 116
15VR164        03:47:40.2 +18:51:10 16.9       116
Positions are for J2000

Event circumstances last updated at 2018/12/04 05:06:49 UT

Marc W. Buie, Southwest Research Institute

RECON