RECON: TNO occultation with 15VR166

Event between 15VR166 and star GA1060:00349055 with event index number of 1019868

Geocentric closest approach at 2019/02/10 09:50:08 UTC

J2000 position of star is 03:24:17.9 +17:41:57
Equinox of date position of star is 03:25:22.9 +17:45:57
Stellar brightness G=15.9, use SENSEUP=128
Star is 32 degrees from the moon. Moon is 26% illuminated.
TNO apparent brightness V=23.9

TNO is 36.3 AU from the Sun and 36.2 AU from the Earth.
The TNO is moving 3.9 km/sec on the sky relative to the star, or, 0.5 arcsec/hr.
The 1-sigma error in the time of the event is 1850 seconds.
The 1-sigma cross-track error in the shadow position is 2665 km.

The TNO has an absolute magnitude Hv=8.1
Diameter=147.9 km assuming a 5% albedo -- 38.1 sec chord
Diameter=60.4 km assuming a 30% albedo -- 15.6 sec chord
Dynamical classification is 7:4EEE
 
 
 
 
 
 
 
 

Star training set for 15VR166, (2019/02/10 09:50UT)
Object            RA         Dec     mag  sep  mel
Aldebaran      04:37:01.2 +16:32:46  0.8 17.15  48
Menkar         03:03:16.8 +04:09:49  2.5 14.64  23
63Tau2Ari      03:23:51.4 +20:48:33  6.2  3.06  33
PPM 119006     03:21:04.3 +17:34:10  8.2  1.05  31
PPM 119056     03:25:19.7 +17:36:55  9.8  0.15  31
15VR166        03:25:23.0 +17:45:57 15.9        32
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 15VR166, (2019/02/10 09:50UT)
Object            RA         Dec     mag  sep  mel
Aldebaran      04:35:55.3 +16:30:30  0.8 17.15  48
Menkar         03:02:16.8 +04:05:21  2.5 14.64  23
63Tau2Ari      03:22:45.2 +20:44:31  6.2  3.06  33
PPM 119006     03:19:59.3 +17:30:04  8.2  1.05  31
PPM 119056     03:24:14.6 +17:32:55  9.8  0.15  31
15VR166        03:24:17.9 +17:41:57 15.9        32
Positions are for J2000

Event circumstances last updated at 2019/01/31 18:04:33 UT

Marc W. Buie, Southwest Research Institute

RECON