RECON: TNO occultation with 126155

Event between (126155) 01YJ140 and star GA1100:03091524 with event index number of 2142813

Geocentric closest approach at 2021/10/06 00:22:28 UTC

J2000 position of star is 08:37:39.7 +20:03:42
Equinox of date position of star is 08:38:54.8 +19:59:05
Stellar brightness G=15.7, use SENSEUP=128 with the MallinCam and and exposure time of 2 seconds with the QHY174 camera.
Star is 60 degrees from the moon. Moon is 0% illuminated.
TNO apparent brightness V=22.4

TNO is 29.1 AU from the Sun and 29.5 AU from the Earth.
The TNO is moving 17.7 km/sec on the sky relative to the star, or, 3.0 arcsec/hr.
The 1-sigma error in the time of the event is 106 seconds.
The 1-sigma cross-track error in the shadow position is 1405 km.

The TNO has an absolute magnitude Hv=7.5
Diameter=187.9 km assuming a 5% albedo -- 10.6 sec chord
Diameter=76.7 km assuming a 30% albedo -- 4.3 sec chord
Dynamical classification is 3:2E
 
 
 
 
 
 
 
 

Star training set for 126155, (2021/10/06 00:22UT)
Object            RA         Dec     mag  sep  mel
Pollux         07:46:38.7 +27:58:19  1.1 14.35  73
33Eta Cnc      08:33:57.8 +20:21:57  5.3  1.22  62
PPM 098891     08:39:38.3 +20:07:47  8.3  0.22  60
PPM 098877     08:38:48.8 +19:56:11  8.9  0.05  60
126155         08:38:54.8 +19:59:05 15.7        60
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 126155, (2021/10/06 00:22UT)
Object            RA         Dec     mag  sep  mel
Pollux         07:45:17.9 +28:01:33  1.1 14.35  73
33Eta Cnc      08:32:42.4 +20:26:27  5.3  1.22  62
PPM 098891     08:38:23.1 +20:12:26  8.3  0.22  60
PPM 098877     08:37:33.7 +20:00:49  8.9  0.05  60
126155         08:37:39.7 +20:03:42 15.7        60
Positions are for J2000

Event circumstances last updated at 2021/10/04 01:47:29 UT

Marc W. Buie, Southwest Research Institute

RECON