RECON: TNO occultation with 05RH52

Event between 05RH52 and star GA1100:00015106 with event index number of 268115

Geocentric closest approach at 2020/06/01 12:22:36 UTC

J2000 position of star is 00:07:16.0 +20:36:38
Equinox of date position of star is 00:08:14.2 +20:42:55
Stellar brightness G=16.5, use SENSEUP=128
Star is 157 degrees from the moon. Moon is 76% illuminated.
TNO apparent brightness V=23.9

TNO is 41.7 AU from the Sun and 42.1 AU from the Earth.
The TNO is moving 22.1 km/sec on the sky relative to the star, or, 2.6 arcsec/hr.
The 1-sigma error in the time of the event is 261 seconds.
The 1-sigma cross-track error in the shadow position is 5262 km.

The TNO has an absolute magnitude Hv=7.5
Diameter=191.4 km assuming a 5% albedo -- 8.7 sec chord
Diameter=78.2 km assuming a 30% albedo -- 3.5 sec chord
Dynamical classification is SCATNEAR
 
 
 
 
 
 
 
 

Star training set for 05RH52, (2020/06/01 12:23UT)
Object            RA         Dec     mag  sep  mel
Deneb          20:42:07.7 +45:21:15  1.3 48.66 109
Algenib        00:14:17.4 +15:17:49  2.8  5.61 162
89Chi Peg      00:15:39.7 +20:19:12  4.8  1.77 158
PPM 116174     00:10:07.5 +20:02:18  7.7  0.81 157
PPM 089415     00:07:53.7 +20:40:24  8.8  0.11 157
05RH52         00:08:19.1 +20:43:27 16.5       157
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 05RH52, (2020/06/01 12:23UT)
Object            RA         Dec     mag  sep  mel
Deneb          20:41:25.9 +45:16:49  1.3 48.66 109
Algenib        00:13:14.2 +15:11:01  2.8  5.61 162
89Chi Peg      00:14:36.3 +20:12:24  4.8  1.77 158
PPM 116174     00:09:04.3 +19:55:30  7.7  0.81 157
PPM 089415     00:06:50.6 +20:33:35  8.8  0.11 157
05RH52         00:07:16.0 +20:36:38 16.5       157
Positions are for J2000

Event circumstances last updated at 2018/10/26 21:13:05 UT

Marc W. Buie, Southwest Research Institute

RECON