RECON: TNO occultation with 118698

Event between (118698) 00OY51 and star GA0840:19842153 with event index number of 2111459

Geocentric closest approach at 2023/06/19 23:43:02 UTC

J2000 position of star is 21:57:20.8 -04:04:59
Equinox of date position of star is 21:58:28.9 -03:58:43
Stellar brightness G=16.3, use SENSEUP=128 with the MallinCam and and exposure time of 2 seconds with the QHY174 camera.
Star is 137 degrees from the moon. Moon is 3% illuminated.
TNO apparent brightness V=23.8

TNO is 34.9 AU from the Sun and 34.4 AU from the Earth.
The TNO is moving 9.3 km/sec on the sky relative to the star, or, 1.3 arcsec/hr.
The 1-sigma error in the time of the event is 727 seconds.
The 1-sigma cross-track error in the shadow position is 4658 km.

The TNO has an absolute magnitude Hv=8.2
Diameter=138.0 km assuming a 5% albedo -- 14.8 sec chord
Diameter=56.4 km assuming a 30% albedo -- 6.1 sec chord
Dynamical classification is 7:4EEE
 
 
 
 
 
 
 
 

Star training set for 118698, (2023/06/19 23:30UT)
Object            RA         Dec     mag  sep  mel
Fomalhaut      22:58:56.5 -29:29:50  1.2 29.26 133
Markab         23:05:55.9 +15:19:55  2.5 25.51 112
PPM 205831     22:00:08.3 -04:15:42  6.2  0.49 137
PPM 205801     21:58:31.1 -03:46:50  8.7  0.19 137
118698         21:58:34.0 -03:58:14 16.3       136
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 118698, (2023/06/19 23:30UT)
Object            RA         Dec     mag  sep  mel
Fomalhaut      22:57:39.6 -29:37:24  1.2 29.26 133
Markab         23:04:45.8 +15:12:18  2.5 25.51 112
PPM 205831     21:58:55.0 -04:22:29  6.2  0.49 137
PPM 205801     21:57:17.8 -03:53:35  8.7  0.19 137
118698         21:57:20.8 -04:04:59 16.3       137
Positions are for J2000

Event circumstances last updated at 2021/10/25 23:33:32 UT

Marc W. Buie, Southwest Research Institute

RECON