RECON: TNO occultation with 54598

Event between (54598) Bienor and star GA1280:03439450 with event index number of 1387614

Geocentric closest approach at 2024/12/04 14:18:20 UTC

J2000 position of star is 07:38:17.0 +39:06:22
Equinox of date position of star is 07:39:56.3 +39:02:57
Stellar brightness G=16.1, use SENSEUP=128 with the MallinCam and and exposure time of 2 seconds with the QHY174 camera.
Star is 167 degrees from the moon. Moon is 12% illuminated.
Apparent brightness V=18.8

Object is 13.4 AU from the Sun and 12.6 AU from the Earth.
Apparent velocity is 16.0 km/sec on the sky relative to the star, or, 6.3 arcsec/hr.
The 1-sigma error in the time of the event is 35 seconds.
The 1-sigma cross-track error in the shadow position is 489 km.

The object has an absolute magnitude Hv=7.4
Diameter=195.0 km assuming a 5% albedo -- 12.2 sec chord
Diameter=79.6 km assuming a 30% albedo -- 5.0 sec chord
Dynamical classification is CENTAURR
 
 
 
 
 
 
 
 

Star training set for 54598, (2024/12/04 14:18UT)
Object            RA         Dec     mag  sep  mel
Pollux         07:46:50.4 +27:57:50  1.1 11.18 178
PPM 072880     07:33:36.8 +38:50:27  6.5  1.25 167
PPM 073023     07:42:54.4 +39:09:06  7.9  0.58 167
PPM 072978     07:38:51.2 +39:02:21 10.0  0.22 167
54598          07:39:58.2 +39:02:53 16.1       167
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, (2024/12/04 14:18UT)
Object            RA         Dec     mag  sep  mel
Pollux         07:45:17.9 +28:01:33  1.1 11.18 178
PPM 072880     07:31:55.5 +38:53:44  6.5  1.25 167
PPM 073023     07:41:13.3 +39:12:41  7.9  0.58 167
PPM 072978     07:37:09.9 +39:05:48 10.0  0.22 167
54598          07:38:17.0 +39:06:22 16.1       167
Positions are for J2000

Event circumstances last updated at 2024/06/12 03:41:00 UT

Marc W. Buie, Southwest Research Institute

RECON