RECON: TNO occultation with 02GV32

Event between 02GV32 and star GA0660:17530355 with event index number of 1037360

Geocentric closest approach at 2020/05/29 14:41:38 UTC

J2000 position of star is 17:42:18.0 -23:59:12
Equinox of date position of star is 17:43:32.0 -23:59:42
Stellar brightness G=16.9, use SENSEUP=128
Star is 114 degrees from the moon. Moon is 44% illuminated.
TNO apparent brightness V=25.1

TNO is 32.1 AU from the Sun and 31.1 AU from the Earth.
The TNO is moving 22.2 km/sec on the sky relative to the star, or, 3.5 arcsec/hr.
The 1-sigma error in the time of the event is 322 seconds.
The 1-sigma cross-track error in the shadow position is 1538 km.

The TNO has an absolute magnitude Hv=10.0
Diameter=204.2 km assuming a 5% albedo -- 2.7 sec chord
Diameter=83.4 km assuming a 30% albedo -- 1.1 sec chord
Dynamical classification is 3:2E
 
 
 
 
 
 
 
 

Star training set for 02GV32, (2020/05/29 14:42UT)
Object            RA         Dec     mag  sep  mel
Antares        16:30:39.7 -26:28:32  0.9 16.65  98
35Eta Oph      17:11:33.0 -15:44:56  2.6 11.16 105
PPM 267309     17:48:59.7 -22:29:01  6.1  1.96 115
PPM 267136     17:42:04.7 -23:50:43  8.2  0.37 114
PPM 267164     17:43:40.0 -23:44:42  9.3  0.25 114
02GV32         17:43:32.8 -23:59:42 16.9       114
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 02GV32, (2020/05/29 14:42UT)
Object            RA         Dec     mag  sep  mel
Antares        16:29:24.4 -26:25:56  0.9 16.65  98
35Eta Oph      17:10:22.7 -15:43:29  2.6 11.16 105
PPM 267309     17:47:45.6 -22:28:40  6.1  1.96 115
PPM 267136     17:40:49.9 -23:50:10  8.2  0.37 114
PPM 267164     17:42:25.3 -23:44:12  9.3  0.25 114
02GV32         17:42:18.0 -23:59:12 16.9       114
Positions are for J2000

Event circumstances last updated at 2020/03/06 21:43:40 UT

Marc W. Buie, Southwest Research Institute

RECON