RECON: TNO occultation with 03TK58

Event between 03TK58 and star GA1140:02158828 with event index number of 2005144

Geocentric closest approach at 2024/01/05 16:38:42 UTC

J2000 position of star is 06:22:24.1 +24:56:37
Equinox of date position of star is 06:23:52.2 +24:55:49
Stellar brightness G=15.1, use SENSEUP=128 with the MallinCam and and exposure time of 2 seconds with the QHY174 camera.
Star is 117 degrees from the moon. Moon is 35% illuminated.
Apparent brightness V=23.4

Object is 45.9 AU from the Sun and 44.9 AU from the Earth.
Apparent velocity is 25.6 km/sec on the sky relative to the star, or, 2.8 arcsec/hr.
The 1-sigma error in the time of the event is 1055 seconds.
The 1-sigma cross-track error in the shadow position is 3994 km.

The object has an absolute magnitude Hv=6.8
Diameter=259.4 km assuming a 5% albedo -- 10.1 sec chord
Diameter=105.9 km assuming a 30% albedo -- 4.1 sec chord
Dynamical classification is CLASSICAL
 
 
 
 
 
 
 
 

Star training set for 03TK58, (2024/01/05 16:39UT)
Object            RA         Dec     mag  sep  mel
Betelgeuse     05:56:28.4 +07:24:34  0.4 18.70 122
Alhena         06:39:05.9 +16:22:36  1.9  9.26 113
PPM 095919     06:26:12.5 +25:02:02  6.3  0.54 116
PPM 095851     06:23:46.8 +25:04:10  9.7  0.14 117
03TK58         06:23:52.8 +24:55:48 15.1       117
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 03TK58, (2024/01/05 16:39UT)
Object            RA         Dec     mag  sep  mel
Betelgeuse     05:55:10.3 +07:24:26  0.4 18.70 122
Alhena         06:37:42.8 +16:23:57  1.9  9.26 113
PPM 095919     06:24:43.7 +25:02:55  6.3  0.54 116
PPM 095851     06:22:18.0 +25:04:58  9.7  0.14 117
03TK58         06:22:24.1 +24:56:37 15.1       117
Positions are for J2000

Event circumstances last updated at 2023/11/04 04:08:13 UT

Marc W. Buie, Southwest Research Institute

RECON