RECON: TNO occultation with 5145

Event between (5145) Pholus and star UC4-397-075147 with event index number of 198104

Geocentric closest approach at 2019/06/25 00:25:09 UTC

J2000 position of star is 18:03:41.6 -10:40:25
Equinox of date position of star is 18:04:39.8 -10:40:19
Stellar brightness R=13.0, use SENSEUP=32
Star is 89 degrees from the moon. Moon is 54% illuminated.
TNO apparent brightness V=21.6

TNO is 28.3 AU from the Sun and 27.3 AU from the Earth.
The TNO is moving 25.7 km/sec on the sky relative to the star, or, 4.7 arcsec/hr.
The 1-sigma error in the time of the event is 164 seconds.
The 1-sigma cross-track error in the shadow position is 2045 km.

The TNO has an absolute magnitude Hv=7.1
Diameter=229.1 km assuming a 5% albedo -- 8.9 sec chord
Diameter=93.5 km assuming a 30% albedo -- 3.6 sec chord
Dynamical classification is CENTAURR
 
 
 
 
 
 
 
 

Star training set for 5145, (2019/06/25 00:25UT)
Object            RA         Dec     mag  sep  mel
Antares        16:30:36.3 -26:28:25  0.9 27.25 109
35Eta Oph      17:11:29.8 -15:44:52  2.6 13.92 101
64Nu Oph       18:00:06.0 -09:46:28  3.3  1.46  90
PPM 234011     18:06:36.3 -11:01:02  7.7  0.57  89
PPM 233958     18:04:19.7 -10:51:37  9.0  0.22  89
5145           18:04:46.4 -10:40:18 13.0        89
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 5145, (2019/06/25 00:25UT)
Object            RA         Dec     mag  sep  mel
Antares        16:29:24.4 -26:25:56  0.9 27.25 109
35Eta Oph      17:10:22.7 -15:43:29  2.6 13.92 101
64Nu Oph       17:59:01.6 -09:46:27  3.3  1.46  90
PPM 234011     18:05:31.3 -11:01:13  7.7  0.57  89
PPM 233958     18:03:14.8 -10:51:43  9.0  0.22  89
5145           18:03:41.6 -10:40:25 13.0        89
Positions are for J2000

Event circumstances last updated at 2017/07/01 17:48:22 UT

Marc W. Buie, Southwest Research Institute

RECON