RECON: TNO occultation with 04MW8

Event between 04MW8 and star GA0840:19855165 with event index number of 2577064

Geocentric closest approach at 2022/09/24 18:03:07 UTC

J2000 position of star is 22:01:41.8 -05:59:32
Equinox of date position of star is 22:02:51.6 -05:53:04
Stellar brightness G=11.6, use SENSEUP=8 with the MallinCam and and exposure time of 125 milli-seconds with the QHY174 camera.
Star is 160 degrees from the moon. Moon is 2% illuminated.
TNO apparent brightness V=22.6

TNO is 24.7 AU from the Sun and 23.9 AU from the Earth.
The TNO is moving 18.7 km/sec on the sky relative to the star, or, 3.9 arcsec/hr.
The 1-sigma error in the time of the event is 107 seconds.
The 1-sigma cross-track error in the shadow position is 1411 km.

The TNO has an absolute magnitude Hv=8.6
Diameter=117.5 km assuming a 5% albedo -- 6.3 sec chord
Diameter=48.0 km assuming a 30% albedo -- 2.6 sec chord
Dynamical classification is CENTAURR
 
 
 
 
 
 
 
 

Star training set for 04MW8, (2022/09/24 18:03UT)
Object            RA         Dec     mag  sep  mel
Fomalhaut      22:58:54.1 -29:30:05  1.2 27.06 158
Markab         23:05:53.7 +15:19:41  2.5 26.33 156
30 Aqr         22:04:28.1 -06:24:42  5.5  0.66 160
PPM 205875     22:02:47.0 -06:06:10  8.3  0.22 160
04MW8          22:02:53.2 -05:52:55 11.6       160
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 04MW8, (2022/09/24 18:03UT)
Object            RA         Dec     mag  sep  mel
Fomalhaut      22:57:39.6 -29:37:24  1.2 27.06 158
Markab         23:04:45.8 +15:12:18  2.5 26.33 156
30 Aqr         22:03:16.5 -06:31:21  5.5  0.66 160
PPM 205875     22:01:35.5 -06:12:47  8.3  0.22 160
04MW8          22:01:41.8 -05:59:32 11.6       160
Positions are for J2000

Event circumstances last updated at 2022/03/13 02:16:29 UT

Marc W. Buie, Southwest Research Institute

RECON