RECON: TNO occultation with 04HH79

Event between 04HH79 and star GA0700:07919489 with event index number of 2632492

Geocentric closest approach at 2024/02/23 01:31:43 UTC

J2000 position of star is 17:06:08.7 -18:05:21
Equinox of date position of star is 17:07:32.2 -18:07:11
Stellar brightness G=16.4, use SENSEUP=128 with the MallinCam and and exposure time of 2 seconds with the QHY174 camera.
Star is 119 degrees from the moon. Moon is 98% illuminated.
Apparent brightness V=23.3

Object is 42.1 AU from the Sun and 42.3 AU from the Earth.
Apparent velocity is 12.4 km/sec on the sky relative to the star, or, 1.5 arcsec/hr.
The 1-sigma error in the time of the event is 684 seconds.
The 1-sigma cross-track error in the shadow position is 2191 km.

The object has an absolute magnitude Hv=6.9
Diameter=251.2 km assuming a 5% albedo -- 20.2 sec chord
Diameter=102.6 km assuming a 30% albedo -- 8.3 sec chord
Dynamical classification is CLASSICAL
 
 
 
 
 
 
 
 

Star training set for 04HH79, (2024/02/23 01:32UT)
Object            RA         Dec     mag  sep  mel
Antares        16:30:53.5 -26:29:00  0.9 11.90 112
35Eta Oph      17:11:45.9 -15:45:11  2.6  2.57 119
PPM 232651     17:09:39.1 -17:38:20  6.0  0.69 119
PPM 232594     17:07:12.9 -18:08:50  8.1  0.09 118
04HH79         17:07:33.3 -18:07:12 16.4       119
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 04HH79, (2024/02/23 01:32UT)
Object            RA         Dec     mag  sep  mel
Antares        16:29:24.4 -26:25:56  0.9 11.90 112
35Eta Oph      17:10:22.7 -15:43:29  2.6  2.57 119
PPM 232651     17:08:14.9 -17:36:33  6.0  0.69 119
PPM 232594     17:05:48.4 -18:06:58  8.1  0.09 118
04HH79         17:06:08.7 -18:05:21 16.4       119
Positions are for J2000

Event circumstances last updated at 2023/11/04 04:09:41 UT

Marc W. Buie, Southwest Research Institute

RECON