RECON: TNO occultation with 26308

Event between (26308) 98SM165 and star GA0960:00256138 with event index number of 212557

Geocentric closest approach at 2019/09/30 21:58:59 UTC

J2000 position of star is 03:00:45.7 +07:35:29
Equinox of date position of star is 03:01:48.0 +07:40:03
Stellar brightness G=15.7, use SENSEUP=128
Star is 171 degrees from the moon. Moon is 7% illuminated.
TNO apparent brightness V=21.9

TNO is 41.3 AU from the Sun and 40.5 AU from the Earth.
The TNO is moving 19.6 km/sec on the sky relative to the star, or, 2.4 arcsec/hr.
The 1-sigma error in the time of the event is 256 seconds.
The 1-sigma cross-track error in the shadow position is 2230 km.

The TNO has an absolute magnitude Hv=5.7
Diameter=436.5 km assuming a 5% albedo -- 22.2 sec chord
Diameter=178.2 km assuming a 30% albedo -- 9.1 sec chord
Dynamical classification is 2:1E+6:3EII
 
 
 
 
 
 
 
 

Star training set for 26308, (2019/09/30 21:59UT)
Object            RA         Dec     mag  sep  mel
Aldebaran      04:37:03.4 +16:32:51  0.8 24.88 148
Menkar         03:03:18.8 +04:09:58  2.5  3.52 170
91Lam Cet      03:00:46.6 +08:59:06  4.7  1.34 172
PPM 146197     03:05:00.8 +07:21:28  7.9  0.85 170
PPM 146128     03:00:54.2 +07:36:15  9.2  0.24 172
26308          03:01:49.0 +07:40:08 15.7       171
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 26308, (2019/09/30 21:59UT)
Object            RA         Dec     mag  sep  mel
Aldebaran      04:35:55.3 +16:30:30  0.8 24.88 148
Menkar         03:02:16.8 +04:05:21  2.5  3.52 170
91Lam Cet      02:59:42.9 +08:54:26  4.7  1.34 172
PPM 146197     03:03:57.6 +07:16:54  7.9  0.85 170
PPM 146128     02:59:51.0 +07:31:36  9.2  0.24 172
26308          03:00:45.7 +07:35:29 15.7       171
Positions are for J2000

Event circumstances last updated at 2019/06/07 22:42:05 UT

Marc W. Buie, Southwest Research Institute

RECON