RECON: TNO occultation with 04VM131

Event between 04VM131 and star GA1020:01321746 with event index number of 283993

Geocentric closest approach at 2020/08/28 05:32:31 UTC

J2000 position of star is 06:01:29.0 +13:54:17
Equinox of date position of star is 06:02:37.7 +13:54:13
Stellar brightness G=15.1, use SENSEUP=128
Star is 168 degrees from the moon. Moon is 76% illuminated.
TNO apparent brightness V=25.4

TNO is 33.4 AU from the Sun and 33.8 AU from the Earth.
The TNO is moving 18.1 km/sec on the sky relative to the star, or, 2.7 arcsec/hr.
The 1-sigma error in the time of the event is 648 seconds.
The 1-sigma cross-track error in the shadow position is 3955 km.

The TNO has an absolute magnitude Hv=10.0
Diameter=115.3 km assuming a 5% albedo -- 3.3 sec chord
Diameter=47.1 km assuming a 30% albedo -- 1.4 sec chord
Dynamical classification is CENTAURR
 
 
 
 
 
 
 
 

Star training set for 04VM131, (2020/08/28 05:33UT)
Object            RA         Dec     mag  sep  mel
Betelgeuse     05:56:17.5 +07:24:33  0.4  6.68 161
Alhena         06:38:54.3 +16:22:48  1.9  9.09 172
137 Tau        05:53:32.7 +14:10:31  5.5  2.23 167
PPM 121707     06:00:32.7 +13:44:06  7.9  0.54 167
PPM 121780     06:02:51.7 +13:32:04  8.7  0.37 168
04VM131        06:02:39.3 +13:54:13 15.1       168
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 04VM131, (2020/08/28 05:33UT)
Object            RA         Dec     mag  sep  mel
Betelgeuse     05:55:10.3 +07:24:26  0.4  6.68 161
Alhena         06:37:42.8 +16:23:57  1.9  9.09 172
137 Tau        05:52:22.2 +14:10:18  5.5  2.23 167
PPM 121707     05:59:22.5 +13:44:06  7.9  0.54 167
PPM 121780     06:01:41.5 +13:32:09  8.7  0.37 168
04VM131        06:01:29.0 +13:54:17 15.1       168
Positions are for J2000

Event circumstances last updated at 2020/03/08 20:44:47 UT

Marc W. Buie, Southwest Research Institute

RECON