RECON: TNO occultation with 29981

Event between (29981) 99TD10 and star GA1060:02535591 with event index number of 257220

Geocentric closest approach at 2020/04/28 18:48:58 UTC

J2000 position of star is 06:58:38.0 +16:56:56
Equinox of date position of star is 06:59:48.1 +16:55:12
Stellar brightness G=16.5, use SENSEUP=128
Star is 7 degrees from the moon. Moon is 29% illuminated.
TNO apparent brightness V=25.2

TNO is 31.8 AU from the Sun and 32.2 AU from the Earth.
The TNO is moving 16.8 km/sec on the sky relative to the star, or, 2.6 arcsec/hr.
The 1-sigma error in the time of the event is 602 seconds.
The 1-sigma cross-track error in the shadow position is 1828 km.

The TNO has an absolute magnitude Hv=10.0
Diameter=109.7 km assuming a 5% albedo -- 3.6 sec chord
Diameter=44.8 km assuming a 30% albedo -- 1.5 sec chord
Dynamical classification is CENTAURR
 
 
 
 
 
 
 
 

Star training set for 29981, (2020/04/28 18:49UT)
Object            RA         Dec     mag  sep  mel
Pollux         07:46:33.4 +27:58:32  1.1 15.44  11
Alhena         06:38:53.2 +16:22:49  1.9  5.04   9
PPM 123373     07:01:27.9 +15:30:19  6.4  1.47   8
PPM 123383     07:01:49.6 +16:55:45  6.7  0.48   7
PPM 123316     06:59:00.4 +16:32:57  8.9  0.42   7
29981          06:59:48.5 +16:55:12 16.5         7
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 29981, (2020/04/28 18:49UT)
Object            RA         Dec     mag  sep  mel
Pollux         07:45:18.0 +28:01:33  1.1 15.44  11
Alhena         06:37:42.8 +16:23:57  1.9  5.04   9
PPM 123373     07:00:18.1 +15:32:06  6.4  1.47   8
PPM 123383     07:00:39.2 +16:57:33  6.7  0.48   7
PPM 123316     06:57:50.1 +16:34:39  8.9  0.42   7
29981          06:58:38.0 +16:56:56 16.5         7
Positions are for J2000

Event circumstances last updated at 2020/03/16 21:27:24 UT

Marc W. Buie, Southwest Research Institute

RECON