RECON: TNO occultation with 04KV18

Event between 04KV18 and star UC4-366-086908 with event index number of 123767

Geocentric closest approach at 2017/07/05 16:02:04 UTC

J2000 position of star is 17:23:19.6 -16:50:14
Equinox of date position of star is 17:24:20.0 -16:51:09
Stellar brightness R=15.7, use SENSEUP=128
Star is 16 degrees from the moon. Moon is 89% illuminated.
TNO apparent brightness V=23.7

TNO is 29.4 AU from the Sun and 28.4 AU from the Earth.
The TNO is moving 21.7 km/sec on the sky relative to the star, or, 3.8 arcsec/hr.
The 1-sigma error in the time of the event is 242 seconds.
The 1-sigma cross-track error in the shadow position is 1082 km.

The TNO has an absolute magnitude Hv=9.0
Diameter=95.5 km assuming a 5% albedo -- 4.4 sec chord
Diameter=39.0 km assuming a 30% albedo -- 1.8 sec chord
Dynamical classification is CENTAURR
 
 
 
 
 
 
 
 

Star training set for 04KV18, (2017/07/05 16:02UT)
Object            RA         Dec     mag  sep  mel
Antares        16:30:29.0 -26:28:10  0.9 15.76  11
35Eta Oph      17:11:23.0 -15:44:44  2.6  3.30  13
PPM 232892     17:19:19.9 -16:19:45  5.9  1.31  15
PPM 233060     17:27:13.3 -17:05:44  8.5  0.73  16
PPM 233005     17:24:17.7 -16:41:12  9.7  0.17  16
04KV18         17:24:20.5 -16:51:09 15.7        16
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 04KV18, (2017/07/05 16:02UT)
Object            RA         Dec     mag  sep  mel
Antares        16:29:24.4 -26:25:56  0.9 15.76  11
35Eta Oph      17:10:22.7 -15:43:29  2.6  3.30  13
PPM 232892     17:18:19.3 -16:18:42  5.9  1.31  15
PPM 233060     17:26:12.3 -17:04:54  8.5  0.73  16
PPM 233005     17:23:16.9 -16:40:16  9.7  0.17  16
04KV18         17:23:19.6 -16:50:14 15.7        16
Positions are for J2000

Event circumstances last updated at 2017/05/14 18:35:13 UT

Marc W. Buie, Southwest Research Institute

RECON