RECON: TNO occultation with 04TE282

Event between 04TE282 and star GA1240:01621126 with event index number of 169128

Geocentric closest approach at 2018/12/13 23:02:19 UTC

J2000 position of star is 05:09:43.3 +35:14:13
Equinox of date position of star is 05:10:58.4 +35:15:34
Stellar brightness G=14.7, use SENSEUP=128
Star is 105 degrees from the moon. Moon is 36% illuminated.
TNO apparent brightness V=23.1

TNO is 30.2 AU from the Sun and 29.2 AU from the Earth.
The TNO is moving 24.8 km/sec on the sky relative to the star, or, 4.2 arcsec/hr.
The 1-sigma error in the time of the event is 262 seconds.
The 1-sigma cross-track error in the shadow position is 3034 km.

The TNO has an absolute magnitude Hv=8.3
Diameter=130.0 km assuming a 5% albedo -- 5.2 sec chord
Diameter=53.1 km assuming a 30% albedo -- 2.1 sec chord
Dynamical classification is CENTAURR
 
 
 
 
 
 
 
 

Star training set for 04TE282, (2018/12/13 23:02UT)
Object            RA         Dec     mag  sep  mel
Aldebaran      04:37:00.6 +16:32:45  0.8 20.19  94
3Iot Aur       04:58:13.8 +33:11:40  2.7  3.35 102
PPM 070048     05:14:34.4 +37:21:28  6.5  2.22 106
PPM 070014     05:12:26.8 +35:22:46  8.1  0.32 105
PPM 069981     05:11:00.9 +35:15:30 10.0  0.01 105
04TE282        05:10:59.0 +35:15:34 14.7       105
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 04TE282, (2018/12/13 23:02UT)
Object            RA         Dec     mag  sep  mel
Aldebaran      04:35:55.3 +16:30:30  0.8 20.19  94
3Iot Aur       04:56:59.6 +33:09:58  2.7  3.35 102
PPM 070048     05:13:17.2 +37:20:12  6.5  2.22 106
PPM 070014     05:11:10.9 +35:21:27  8.1  0.32 105
PPM 069981     05:09:45.1 +35:14:09 10.0  0.01 105
04TE282        05:09:43.3 +35:14:13 14.7       105
Positions are for J2000

Event circumstances last updated at 2018/10/22 18:23:18 UT

Marc W. Buie, Southwest Research Institute

RECON