RECON: TNO occultation with 8405

Event between (8405) Asbolus and star UC4-651-024258 with event index number of 178094

Geocentric closest approach at 2019/01/16 13:19:45 UTC

J2000 position of star is 04:54:42.2 +40:11:00
Equinox of date position of star is 04:55:55.4 +40:12:38
Stellar brightness R=15.4, use SENSEUP=128
Star is 32 degrees from the moon. Moon is 73% illuminated.
TNO apparent brightness V=22.6

TNO is 22.0 AU from the Sun and 21.2 AU from the Earth.
The TNO is moving 19.8 km/sec on the sky relative to the star, or, 4.6 arcsec/hr.
The 1-sigma error in the time of the event is 143 seconds.
The 1-sigma cross-track error in the shadow position is 1698 km.

The TNO has an absolute magnitude Hv=9.1
Diameter=91.2 km assuming a 5% albedo -- 4.6 sec chord
Diameter=37.2 km assuming a 30% albedo -- 1.9 sec chord
Dynamical classification is CENTAURR
 
 
 
 
 
 
 
 

Star training set for 8405, (2019/01/16 13:20UT)
Object            RA         Dec     mag  sep  mel
Aldebaran      04:37:00.9 +16:32:46  0.8 24.02  16
3Iot Aur       04:58:14.2 +33:11:40  2.7  7.03  28
5 Aur          05:01:37.1 +39:25:19  6.4  1.33  32
PPM 047520     04:57:50.6 +40:11:52  8.0  0.35  32
PPM 047462     04:55:15.2 +40:02:09  9.7  0.23  32
8405           04:56:01.4 +40:12:46 15.4        32
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 8405, (2019/01/16 13:20UT)
Object            RA         Dec     mag  sep  mel
Aldebaran      04:35:55.3 +16:30:30  0.8 24.02  16
3Iot Aur       04:56:59.6 +33:09:58  2.7  7.03  28
5 Aur          05:00:18.3 +39:23:41  6.4  1.33  32
PPM 047520     04:56:31.4 +40:10:09  8.0  0.35  32
PPM 047462     04:53:56.1 +40:00:22  9.7  0.23  32
8405           04:54:42.2 +40:11:00 15.4        32
Positions are for J2000

Event circumstances last updated at 2017/08/04 18:04:03 UT

Marc W. Buie, Southwest Research Institute

RECON