RECON: TNO occultation with 447178

Event between (447178) 05RO43 and star GA0740:03965779 with event index number of 2291007

Geocentric closest approach at 2026/10/06 20:43:23 UTC

J2000 position of star is 08:28:13.5 -14:31:38
Equinox of date position of star is 08:29:21.5 -14:36:32
Stellar brightness G=16.2, use SENSEUP=128 with the MallinCam and and exposure time of 2 seconds with the QHY174 camera.
Star is 35 degrees from the moon. Moon is 16% illuminated.
Apparent brightness V=19.3

Object is 15.0 AU from the Sun and 15.4 AU from the Earth.
Apparent velocity is 26.4 km/sec on the sky relative to the star, or, 8.5 arcsec/hr.
The 1-sigma error in the time of the event is 58 seconds.
The 1-sigma cross-track error in the shadow position is 1595 km.

The object has an absolute magnitude Hv=7.2
Diameter=208.9 km assuming a 5% albedo -- 8.5 sec chord
Diameter=85.3 km assuming a 30% albedo -- 3.5 sec chord
Dynamical classification is CENTAURR
 
 
 
 
 
 
 
 

Star training set for 447178, (2026/10/06 20:41UT)
Object            RA         Dec     mag  sep  mel
Sirius         06:46:19.8 -16:45:12 -1.5 24.90  55
15Rho Pup      08:08:41.1 -24:22:59  2.8 10.92  46
PPM 220100     08:27:10.2 -15:01:06  6.0  0.69  36
PPM 220155     08:29:31.6 -14:40:45  8.5  0.06  35
447178         08:29:28.4 -14:37:02 16.2        35
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 447178, (2026/10/06 20:41UT)
Object            RA         Dec     mag  sep  mel
Sirius         06:45:08.0 -16:43:26 -1.5 24.90  55
15Rho Pup      08:07:32.5 -24:18:14  2.8 10.92  46
PPM 220100     08:25:55.6 -14:55:46  6.0  0.69  36
PPM 220155     08:28:16.7 -14:35:21  8.5  0.06  35
447178         08:28:13.5 -14:31:38 16.2        35
Positions are for J2000

Event circumstances last updated at 2024/04/18 03:44:44 UT

Marc W. Buie, Southwest Research Institute

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