RECON: TNO occultation with 00YE2

Event between 00YE2 and star GA1100:01431754 with event index number of 231263

Geocentric closest approach at 2019/12/28 15:20:00 UTC

J2000 position of star is 05:47:46.6 +20:44:33
Equinox of date position of star is 05:48:56.1 +20:44:53
Stellar brightness G=14.8, use SENSEUP=128
Star is 142 degrees from the moon. Moon is 6% illuminated.
TNO apparent brightness V=24.1

TNO is 38.3 AU from the Sun and 37.3 AU from the Earth.
The TNO is moving 24.6 km/sec on the sky relative to the star, or, 3.3 arcsec/hr.
The 1-sigma error in the time of the event is 930 seconds.
The 1-sigma cross-track error in the shadow position is 3883 km.

The TNO has an absolute magnitude Hv=8.3
Diameter=133.7 km assuming a 5% albedo -- 5.4 sec chord
Diameter=54.6 km assuming a 30% albedo -- 2.2 sec chord
Dynamical classification is 2:1E
 
 
 
 
 
 
 
 

Star training set for 00YE2, (2019/12/28 15:20UT)
Object            RA         Dec     mag  sep  mel
Betelgeuse     05:56:15.3 +07:24:33  0.4 13.45 140
Alnath         05:27:33.4 +28:37:21  1.6  9.25 137
PPM 121513     05:53:34.5 +19:52:17  6.4  1.39 143
PPM 094877     05:48:50.1 +20:56:46  7.9  0.20 142
PPM 094896     05:49:28.1 +20:46:30  8.9  0.12 142
00YE2          05:48:58.1 +20:44:53 14.8       142
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 00YE2, (2019/12/28 15:20UT)
Object            RA         Dec     mag  sep  mel
Betelgeuse     05:55:10.3 +07:24:26  0.4 13.45 140
Alnath         05:26:17.5 +28:36:23  1.6  9.25 137
PPM 121513     05:52:23.4 +19:52:04  6.4  1.39 143
PPM 094877     05:47:38.4 +20:56:26  7.9  0.20 142
PPM 094896     05:48:16.5 +20:46:10  8.9  0.12 142
00YE2          05:47:46.6 +20:44:33 14.8       142
Positions are for J2000

Event circumstances last updated at 2019/06/07 23:05:02 UT

Marc W. Buie, Southwest Research Institute

RECON