RECON: TNO occultation with 29981

Event between (29981) 99TD10 and star GA1040:02929549 with event index number of 1481023

Geocentric closest approach at 2026/01/13 01:45:27 UTC

J2000 position of star is 07:39:26.2 +15:36:57
Equinox of date position of star is 07:40:49.7 +15:33:30
Stellar brightness G=14.6, use SENSEUP=128 with the MallinCam and and exposure time of 2 seconds with the QHY174 camera.
Star is 115 degrees from the moon. Moon is 28% illuminated.
Apparent brightness V=24.5

Object is 37.8 AU from the Sun and 36.8 AU from the Earth.
Apparent velocity is 26.5 km/sec on the sky relative to the star, or, 3.6 arcsec/hr.
The 1-sigma error in the time of the event is 286 seconds.
The 1-sigma cross-track error in the shadow position is 1640 km.

The object has an absolute magnitude Hv=8.8
Diameter=109.7 km assuming a 5% albedo -- 4.0 sec chord
Diameter=44.8 km assuming a 30% albedo -- 1.6 sec chord
Dynamical classification is CENTAURR
 
 
 
 
 
 
 
 

Star training set for 29981, (2026/01/13 01:45UT)
Object            RA         Dec     mag  sep  mel
Pollux         07:46:54.5 +27:57:40  1.1 12.48 116
PPM 124242     07:38:35.3 +16:50:39  6.1  1.41 115
PPM 124241     07:38:29.7 +14:49:44  8.2  0.93 115
PPM 124298     07:41:29.6 +15:33:03  9.1  0.14 114
29981          07:40:55.0 +15:33:16 14.6       114
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 29981, (2026/01/13 01:45UT)
Object            RA         Dec     mag  sep  mel
Pollux         07:45:17.9 +28:01:33  1.1 12.48 116
PPM 124242     07:37:05.7 +16:54:15  6.1  1.41 115
PPM 124241     07:37:01.3 +14:53:19  8.2  0.93 115
PPM 124298     07:40:00.8 +15:36:45  9.1  0.14 114
29981          07:39:26.2 +15:36:57 14.6       114
Positions are for J2000

Event circumstances last updated at 2024/06/18 21:23:56 UT

Marc W. Buie, Southwest Research Institute

RECON