RECON: TNO occultation with 04OP15

Event between 04OP15 and star UC4-389-131024 with event index number of 208117

Geocentric closest approach at 2018/03/31 02:00:26 UTC

J2000 position of star is 20:29:04.0 -12:14:34
Equinox of date position of star is 20:30:03.3 -12:10:56
Stellar brightness R=15.2, use SENSEUP=128
Star is 121 degrees from the moon. Moon is 100% illuminated.
TNO apparent brightness V=23.0

TNO is 38.0 AU from the Sun and 38.4 AU from the Earth.
The TNO is moving 18.9 km/sec on the sky relative to the star, or, 2.4 arcsec/hr.
The 1-sigma error in the time of the event is 365 seconds.
The 1-sigma cross-track error in the shadow position is 4057 km.

The TNO has an absolute magnitude Hv=7.0
Diameter=237.7 km assuming a 5% albedo -- 12.6 sec chord
Diameter=97.0 km assuming a 30% albedo -- 5.1 sec chord
Dynamical classification is SCATEXTD
 
 
 
 
 
 
 
 

Star training set for 04OP15, (2018/03/31 02:00UT)
Object            RA         Dec     mag  sep  mel
Fomalhaut      22:58:39.3 -29:31:31  1.2 38.56 146
Tarazed        19:47:07.6 +10:39:32  2.7 25.21 110
PPM 237602     20:35:12.5 -13:39:26  6.1  1.94 122
PPM 237524     20:31:27.2 -12:10:15  8.2  0.34 121
PPM 237505     20:30:44.6 -12:11:59  9.6  0.17 121
04OP15         20:30:04.3 -12:10:52 15.2       121
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 04OP15, (2018/03/31 02:00UT)
Object            RA         Dec     mag  sep  mel
Fomalhaut      22:57:39.5 -29:37:23  1.2 38.56 146
Tarazed        19:46:15.6 +10:36:48  2.7 25.21 110
PPM 237602     20:34:11.8 -13:43:15  6.1  1.94 122
PPM 237524     20:30:26.9 -12:13:59  8.2  0.34 121
PPM 237505     20:29:44.3 -12:15:42  9.6  0.17 121
04OP15         20:29:04.0 -12:14:34 15.2       121
Positions are for J2000

Event circumstances last updated at 2017/12/02 17:24:09 UT

Marc W. Buie, Southwest Research Institute

RECON