RECON: TNO occultation with 16AN278

Event between 16AN278 and star GA1020:03075094 with event index number of 1950232

Geocentric closest approach at 2021/11/30 14:40:39 UTC

J2000 position of star is 08:03:14.6 +13:34:06
Equinox of date position of star is 08:04:27.6 +13:30:22
Stellar brightness G=15.8, use SENSEUP=128 with the MallinCam and and exposure time of 2 seconds with the QHY174 camera.
Star is 78 degrees from the moon. Moon is 19% illuminated.
TNO apparent brightness V=22.7

TNO is 37.1 AU from the Sun and 36.5 AU from the Earth.
The TNO is moving 13.8 km/sec on the sky relative to the star, or, 1.9 arcsec/hr.
The 1-sigma error in the time of the event is 226 seconds.
The 1-sigma cross-track error in the shadow position is 1515 km.

The TNO has an absolute magnitude Hv=6.9
Diameter=248.9 km assuming a 5% albedo -- 17.8 sec chord
Diameter=101.6 km assuming a 30% albedo -- 7.3 sec chord
Dynamical classification is SCATNEAR
 
 
 
 
 
 
 
 

Star training set for 16AN278, (2021/11/30 14:41UT)
Object            RA         Dec     mag  sep  mel
Pollux         07:46:39.3 +27:58:17  1.1 15.05  84
8 Cnc          08:06:17.6 +13:03:15  5.1  0.63  77
PPM 124801     08:05:19.3 +13:37:28  7.8  0.24  78
PPM 124783     08:04:38.1 +13:36:22  8.7  0.11  78
16AN278        08:04:28.1 +13:30:20 15.8        77
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 16AN278, (2021/11/30 14:41UT)
Object            RA         Dec     mag  sep  mel
Pollux         07:45:17.9 +28:01:33  1.1 15.05  84
8 Cnc          08:05:04.4 +13:07:04  5.1  0.63  77
PPM 124801     08:04:05.8 +13:41:16  7.8  0.24  78
PPM 124783     08:03:24.6 +13:40:08  8.7  0.11  78
16AN278        08:03:14.6 +13:34:06 15.8        78
Positions are for J2000

Event circumstances last updated at 2021/10/09 01:01:49 UT

Marc W. Buie, Southwest Research Institute

RECON