RECON: TNO occultation with 14JU80

Event between 14JU80 and star GA0760:08090037 with event index number of 1045546

Geocentric closest approach at 2020/02/22 21:13:00 UTC

J2000 position of star is 17:35:54.1 -12:15:55
Equinox of date position of star is 17:36:59.5 -12:16:35
Stellar brightness G=14.6, use SENSEUP=128
Star is 63 degrees from the moon. Moon is 1% illuminated.
TNO apparent brightness V=22.3

TNO is 42.9 AU from the Sun and 43.2 AU from the Earth.
The TNO is moving 16.5 km/sec on the sky relative to the star, or, 1.9 arcsec/hr.
The 1-sigma error in the time of the event is 612 seconds.
The 1-sigma cross-track error in the shadow position is 3452 km.

The TNO has an absolute magnitude Hv=5.8
Diameter=416.9 km assuming a 5% albedo -- 25.2 sec chord
Diameter=170.2 km assuming a 30% albedo -- 10.3 sec chord
Dynamical classification is SCATNEAR
 
 
 
 
 
 
 
 

Star training set for 14JU80, (2020/02/22 21:13UT)
Object            RA         Dec     mag  sep  mel
Antares        16:30:38.7 -26:28:30  0.9 21.09  75
35Eta Oph      17:11:32.1 -15:44:55  2.6  7.09  68
PPM 233365     17:39:16.6 -10:56:12  5.7  1.45  62
PPM 233283     17:36:24.5 -12:21:35  8.2  0.17  63
PPM 233304     17:37:11.6 -12:18:23  9.6  0.05  63
14JU80         17:37:01.9 -12:16:36 14.6        62
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 14JU80, (2020/02/22 21:13UT)
Object            RA         Dec     mag  sep  mel
Antares        16:29:24.4 -26:25:56  0.9 21.09  75
35Eta Oph      17:10:22.7 -15:43:29  2.6  7.09  68
PPM 233365     17:38:09.5 -10:55:35  5.7  1.45  62
PPM 233283     17:35:16.7 -12:20:52  8.2  0.17  63
PPM 233304     17:36:03.9 -12:17:42  9.6  0.05  63
14JU80         17:35:54.1 -12:15:55 14.6        63
Positions are for J2000

Event circumstances last updated at 2019/06/07 23:18:00 UT

Marc W. Buie, Southwest Research Institute

RECON