RECON: TNO occultation with 00YV1

Event between 00YV1 and star UC4-559-011435 with event index number of 107629

Geocentric closest approach at 2018/03/29 07:29:13 UTC

J2000 position of star is 04:49:39.7 +21:44:08
Equinox of date position of star is 04:50:41.9 +21:45:53
Stellar brightness R=16.2, use SENSEUP=128
Star is 86 degrees from the moon. Moon is 94% illuminated.
TNO apparent brightness V=23.9

TNO is 44.9 AU from the Sun and 45.3 AU from the Earth.
The TNO is moving 16.4 km/sec on the sky relative to the star, or, 1.8 arcsec/hr.
The 1-sigma error in the time of the event is 746 seconds.
The 1-sigma cross-track error in the shadow position is 4550 km.

The TNO has an absolute magnitude Hv=7.2
Diameter=218.8 km assuming a 5% albedo -- 13.4 sec chord
Diameter=89.3 km assuming a 30% albedo -- 5.5 sec chord
Dynamical classification is CLASSICAL
 
 
 
 
 
 
 
 

Star training set for 00YV1, (2018/03/29 07:29UT)
Object            RA         Dec     mag  sep  mel
Aldebaran      04:36:58.2 +16:32:40  0.8  6.15  90
Alnath         05:27:26.8 +28:37:16  1.6 10.76  77
PPM 093742     04:46:48.7 +23:39:37  6.1  2.10  87
PPM 093789     04:49:49.0 +21:20:47  7.3  0.47  87
PPM 093794     04:50:06.1 +21:49:20 11.8  0.16  86
00YV1          04:50:45.1 +21:45:58 16.2        86
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 00YV1, (2018/03/29 07:29UT)
Object            RA         Dec     mag  sep  mel
Aldebaran      04:35:55.3 +16:30:30  0.8  6.15  90
Alnath         05:26:17.5 +28:36:24  1.6 10.76  77
PPM 093742     04:45:42.5 +23:37:41  6.1  2.10  87
PPM 093789     04:48:43.8 +21:18:56  7.3  0.47  87
PPM 093794     04:49:00.8 +21:47:30 11.8  0.16  86
00YV1          04:49:39.7 +21:44:08 16.2        86
Positions are for J2000

Event circumstances last updated at 2017/05/13 17:34:27 UT

Marc W. Buie, Southwest Research Institute

RECON