RECON: TNO occultation with 99CY118

Event between 99CY118 and star GA0960:03980637 with event index number of 263579

Geocentric closest approach at 2020/05/08 21:15:56 UTC

J2000 position of star is 14:04:05.7 +07:24:33
Equinox of date position of star is 14:05:00.7 +07:19:17
Stellar brightness G=11.2, use SENSEUP=8
Star is 45 degrees from the moon. Moon is 97% illuminated.
TNO apparent brightness V=24.4

TNO is 36.7 AU from the Sun and 35.8 AU from the Earth.
The TNO is moving 21.7 km/sec on the sky relative to the star, or, 3.0 arcsec/hr.
The 1-sigma error in the time of the event is 510 seconds.
The 1-sigma cross-track error in the shadow position is 4818 km.

The TNO has an absolute magnitude Hv=8.7
Diameter=111.7 km assuming a 5% albedo -- 5.1 sec chord
Diameter=45.6 km assuming a 30% albedo -- 2.1 sec chord
Dynamical classification is SCATNEAR
 
 
 
 
 
 
 
 

Star training set for 99CY118, (2020/05/08 21:16UT)
Object            RA         Dec     mag  sep  mel
Arcturus       14:16:35.6 +19:04:42  0.0 12.09  51
Vindemiatrix   13:03:11.4 +10:51:01  2.8 15.69  59
PPM 160252     14:02:20.9 +08:47:50  5.9  1.63  46
PPM 160315     14:05:42.4 +06:54:06  8.2  0.44  44
PPM 160306     14:04:59.9 +07:17:00 10.5  0.04  45
99CY118        14:05:06.5 +07:18:44 11.2        45
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 99CY118, (2020/05/08 21:16UT)
Object            RA         Dec     mag  sep  mel
Arcturus       14:15:38.3 +19:10:20  0.0 12.09  51
Vindemiatrix   13:02:10.3 +10:57:33  2.8 15.69  59
PPM 160252     14:01:20.5 +08:53:42  5.9  1.63  46
PPM 160315     14:04:41.5 +06:59:54  8.2  0.44  44
PPM 160306     14:03:59.1 +07:22:49 10.5  0.04  45
99CY118        14:04:05.7 +07:24:33 11.2        45
Positions are for J2000

Event circumstances last updated at 2018/05/31 17:26:09 UT

Marc W. Buie, Southwest Research Institute

RECON