RECON: TNO occultation with 69990

Event between (69990) 98WU31 and star GA1080:01368378 with event index number of 352342

Geocentric closest approach at 2019/01/30 10:52:04 UTC

J2000 position of star is 05:48:21.3 +19:55:24
Equinox of date position of star is 05:49:28.7 +19:55:42
Stellar brightness G=16.8, use SENSEUP=128
Star is 163 degrees from the moon. Moon is 25% illuminated.
TNO apparent brightness V=23.7

TNO is 35.6 AU from the Sun and 34.8 AU from the Earth.
The TNO is moving 17.3 km/sec on the sky relative to the star, or, 2.5 arcsec/hr.
The 1-sigma error in the time of the event is 214 seconds.
The 1-sigma cross-track error in the shadow position is 1322 km.

The TNO has an absolute magnitude Hv=8.1
Diameter=144.5 km assuming a 5% albedo -- 8.4 sec chord
Diameter=59.0 km assuming a 30% albedo -- 3.4 sec chord
Dynamical classification is 3:2E
 
 
 
 
 
 
 
 

Star training set for 69990, (2019/01/30 10:52UT)
Object            RA         Dec     mag  sep  mel
Betelgeuse     05:56:12.3 +07:24:33  0.4 12.62 158
Alnath         05:27:30.0 +28:37:18  1.6 10.03 165
PPM 121513     05:53:31.3 +19:52:16  6.4  0.95 162
PPM 121502     05:52:59.8 +19:31:29  7.1  0.92 163
PPM 121423     05:49:58.3 +19:55:49  8.8  0.11 163
69990          05:49:29.2 +19:55:43 16.8       163
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 69990, (2019/01/30 10:52UT)
Object            RA         Dec     mag  sep  mel
Betelgeuse     05:55:10.3 +07:24:26  0.4 12.62 158
Alnath         05:26:17.5 +28:36:23  1.6 10.03 165
PPM 121513     05:52:23.4 +19:52:04  6.4  0.95 162
PPM 121502     05:51:52.1 +19:31:17  7.1  0.92 163
PPM 121423     05:48:50.4 +19:55:32  8.8  0.11 163
69990          05:48:21.3 +19:55:24 16.8       163
Positions are for J2000

Event circumstances last updated at 2018/12/04 05:12:51 UT

Marc W. Buie, Southwest Research Institute

RECON