RECON: TNO occultation with 535986

Event between (535986) 15BN518 and star GA1100:03087551 with event index number of 1618944

Geocentric closest approach at 2020/12/31 15:56:53 UTC

J2000 position of star is 08:36:00.4 +21:42:33
Equinox of date position of star is 08:37:13.5 +21:38:08
Stellar brightness G=16.4, use SENSEUP=128 with the MallinCam and and exposure time of 2 seconds with the QHY174 camera.
Star is 8 degrees from the moon. Moon is 98% illuminated.
TNO apparent brightness V=22.5

TNO is 37.1 AU from the Sun and 36.2 AU from the Earth.
The TNO is moving 22.4 km/sec on the sky relative to the star, or, 3.1 arcsec/hr.
The 1-sigma error in the time of the event is 59 seconds.
The 1-sigma cross-track error in the shadow position is 1312 km.

The TNO has an absolute magnitude Hv=6.8
Diameter=263.0 km assuming a 5% albedo -- 11.7 sec chord
Diameter=107.4 km assuming a 30% albedo -- 4.8 sec chord
Dynamical classification is SCATEXTD
 
 
 
 
 
 
 
 

Star training set for 535986, (2020/12/31 15:57UT)
Object            RA         Dec     mag  sep  mel
Pollux         07:46:35.9 +27:58:26  1.1 13.11   6
33Eta Cnc      08:33:55.2 +20:22:06  5.3  1.48   7
PPM 098828     08:35:52.3 +21:25:11  8.4  0.38   7
PPM 098845     08:36:55.9 +21:42:33 10.4  0.10   7
535986         08:37:13.6 +21:38:07 16.4         8
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 535986, (2020/12/31 15:57UT)
Object            RA         Dec     mag  sep  mel
Pollux         07:45:18.0 +28:01:33  1.1 13.11   6
33Eta Cnc      08:32:42.4 +20:26:27  5.3  1.48   7
PPM 098828     08:34:39.2 +21:29:35  8.4  0.38   7
PPM 098845     08:35:42.6 +21:46:58 10.4  0.10   7
535986         08:36:00.4 +21:42:33 16.4         7
Positions are for J2000

Event circumstances last updated at 2020/12/23 00:22:33 UT

Marc W. Buie, Southwest Research Institute

RECON