RECON: TNO occultation with 32929

Event between (32929) 95QY9 and star GA1140:00538081 with event index number of 2530727

Geocentric closest approach at 2028/12/08 23:07:38 UTC

J2000 position of star is 03:50:58.5 +25:08:48
Equinox of date position of star is 03:52:26.8 +25:13:09
Stellar brightness G=15.5, use SENSEUP=128 with the MallinCam and and exposure time of 2 seconds with the QHY174 camera.
Star is 103 degrees from the moon. Moon is 53% illuminated.
Apparent brightness V=23.7

Object is 32.0 AU from the Sun and 31.0 AU from the Earth.
Apparent velocity is 23.4 km/sec on the sky relative to the star, or, 3.7 arcsec/hr.
The 1-sigma error in the time of the event is 462 seconds.
The 1-sigma cross-track error in the shadow position is 3659 km.

The object has an absolute magnitude Hv=8.7
Diameter=125.9 km assuming a 5% albedo -- 4.8 sec chord
Diameter=51.4 km assuming a 30% albedo -- 2.0 sec chord
Dynamical classification is 3:2E
 
 
 
 
 
 
 
 

Star training set for 32929, (2028/12/08 23:08UT)
Object            RA         Dec     mag  sep  mel
Aldebaran      04:37:35.1 +16:33:55  0.8 13.59  94
44Zet Per      03:55:57.5 +31:58:02  2.8  6.77 101
PPM 092967     03:52:03.7 +25:39:52  5.5  0.46 103
PPM 092987     03:53:09.7 +25:14:53  6.9  0.10 103
32929          03:52:42.9 +25:13:56 15.5       103
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 32929, (2028/12/08 23:08UT)
Object            RA         Dec     mag  sep  mel
Aldebaran      04:35:55.3 +16:30:29  0.8 13.59  94
44Zet Per      03:54:07.9 +31:53:01  2.8  6.77 101
PPM 092967     03:50:19.0 +25:34:43  5.5  0.46 103
PPM 092987     03:51:25.3 +25:09:46  6.9  0.10 103
32929          03:50:58.5 +25:08:48 15.5       103
Positions are for J2000

Event circumstances last updated at 2024/06/25 21:30:35 UT

Marc W. Buie, Southwest Research Institute

RECON