RECON: TNO occultation with 14UT114

Event between 14UT114 and star GA1260:01306867 with event index number of 242163

Geocentric closest approach at 2020/01/16 12:41:10 UTC

J2000 position of star is 04:36:13.8 +36:37:26
Equinox of date position of star is 04:37:27.6 +36:39:38
Stellar brightness G=13.3, use SENSEUP=32
Star is 117 degrees from the moon. Moon is 62% illuminated.
TNO apparent brightness V=21.0

TNO is 15.9 AU from the Sun and 15.2 AU from the Earth.
The TNO is moving 14.6 km/sec on the sky relative to the star, or, 4.8 arcsec/hr.
The 1-sigma error in the time of the event is 216 seconds.
The 1-sigma cross-track error in the shadow position is 2116 km.

The TNO has an absolute magnitude Hv=8.8
Diameter=104.7 km assuming a 5% albedo -- 7.2 sec chord
Diameter=42.8 km assuming a 30% albedo -- 2.9 sec chord
Dynamical classification is CENTAURR
 
 
 
 
 
 
 
 

Star training set for 14UT114, (2020/01/16 12:41UT)
Object            RA         Dec     mag  sep  mel
Aldebaran      04:37:04.4 +16:32:53  0.8 20.12 123
3Iot Aur       04:58:18.1 +33:11:46  2.7  5.48 114
PPM 069587     04:43:12.2 +38:19:00  6.2  2.00 115
PPM 069536     04:37:58.3 +36:59:30  7.6  0.34 117
PPM 069528     04:37:23.6 +36:42:25  9.6  0.06 117
14UT114        04:37:34.0 +36:39:49 13.3       117
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 14UT114, (2020/01/16 12:41UT)
Object            RA         Dec     mag  sep  mel
Aldebaran      04:35:55.3 +16:30:30  0.8 20.12 123
3Iot Aur       04:56:59.6 +33:09:58  2.7  5.48 114
PPM 069587     04:41:50.6 +38:16:47  6.2  2.00 115
PPM 069536     04:36:37.9 +36:57:08  7.6  0.34 117
PPM 069528     04:36:03.4 +36:40:03  9.6  0.06 117
14UT114        04:36:13.8 +36:37:26 13.3       117
Positions are for J2000

Event circumstances last updated at 2018/06/12 19:50:55 UT

Marc W. Buie, Southwest Research Institute

RECON