RECON: TNO occultation with 54598

Event between (54598) Bienor and star GA1340:02377096 with event index number of 1003480

Geocentric closest approach at 2020/11/30 22:04:55 UTC

J2000 position of star is 04:46:03.2 +44:35:45
Equinox of date position of star is 04:47:33.6 +44:37:56
Stellar brightness G=16.9, use SENSEUP=128
Star is 23 degrees from the moon. Moon is 100% illuminated.
TNO apparent brightness V=21.6

TNO is 14.2 AU from the Sun and 13.3 AU from the Earth.
The TNO is moving 21.7 km/sec on the sky relative to the star, or, 8.1 arcsec/hr.
The 1-sigma error in the time of the event is 27 seconds.
The 1-sigma cross-track error in the shadow position is 486 km.

The TNO has an absolute magnitude Hv=10.0
Diameter=186.2 km assuming a 5% albedo -- 2.8 sec chord
Diameter=76.0 km assuming a 30% albedo -- 1.1 sec chord
Dynamical classification is CENTAURR
 
 
 
 
 
 
 
 

Star training set for 54598, (2020/11/30 22:05UT)
Object            RA         Dec     mag  sep  mel
Aldebaran      04:37:07.4 +16:32:59  0.8 28.17   7
3Iot Aur       04:58:21.5 +33:11:50  2.7 11.62  11
59 Per         04:44:23.6 +43:24:11  5.2  1.35  21
PPM 047309     04:46:05.6 +44:48:12  7.8  0.31  23
PPM 047319     04:47:03.9 +44:24:25 10.0  0.24  22
54598          04:47:33.7 +44:37:56 16.9        23
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 54598, (2020/11/30 22:05UT)
Object            RA         Dec     mag  sep  mel
Aldebaran      04:35:55.3 +16:30:29  0.8 28.17   7
3Iot Aur       04:56:59.6 +33:09:58  2.7 11.62  11
59 Per         04:42:54.3 +43:21:53  5.2  1.35  21
PPM 047309     04:44:35.0 +44:45:58  7.8  0.31  23
PPM 047319     04:45:33.6 +44:22:13 10.0  0.24  22
54598          04:46:03.2 +44:35:45 16.9        23
Positions are for J2000

Event circumstances last updated at 2020/11/16 22:18:01 UT

Marc W. Buie, Southwest Research Institute

RECON