RECON: TNO occultation with 14BD70

Event between 14BD70 and star GA0920:03272942 with event index number of 1555043

Geocentric closest approach at 2020/10/23 01:49:37 UTC

J2000 position of star is 08:50:08.6 +03:11:15
Equinox of date position of star is 08:51:09.6 +03:06:50
Stellar brightness G=11.4, use SENSEUP=8
Star is 154 degrees from the moon. Moon is 45% illuminated.
TNO apparent brightness V=22.1

TNO is 45.9 AU from the Sun and 46.2 AU from the Earth.
The TNO is moving 13.6 km/sec on the sky relative to the star, or, 1.5 arcsec/hr.
The 1-sigma error in the time of the event is 271 seconds.
The 1-sigma cross-track error in the shadow position is 3539 km.

The TNO has an absolute magnitude Hv=5.3
Diameter=517.6 km assuming a 5% albedo -- 37.9 sec chord
Diameter=211.3 km assuming a 30% albedo -- 15.5 sec chord
Dynamical classification is SCATEXTD
 
 
 
 
 
 
 
 

Star training set for 14BD70, (2020/10/23 01:50UT)
Object            RA         Dec     mag  sep  mel
Regulus        10:09:28.7 +11:51:53  1.3 21.26 144
Alphard        09:28:36.6 -08:44:59  2.0 15.08 139
7Eta Hya       08:44:18.8 +03:19:20  4.0  1.74 155
PPM 155044     08:50:17.6 +03:24:25  7.7  0.38 155
PPM 155075     08:51:35.3 +03:27:51  9.2  0.37 154
14BD70         08:51:13.7 +03:06:32 11.4       154
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 14BD70, (2020/10/23 01:50UT)
Object            RA         Dec     mag  sep  mel
Regulus        10:08:22.0 +11:58:02  1.3 21.26 144
Alphard        09:27:35.2 -08:39:31  2.0 15.08 139
7Eta Hya       08:43:13.6 +03:23:53  4.0  1.74 155
PPM 155044     08:49:12.4 +03:29:06  7.7  0.38 155
PPM 155075     08:50:30.1 +03:32:34  9.2  0.37 154
14BD70         08:50:08.6 +03:11:15 11.4       154
Positions are for J2000

Event circumstances last updated at 2019/07/02 21:51:05 UT

Marc W. Buie, Southwest Research Institute

RECON