RECON: TNO occultation with 12HW87

Event between 12HW87 and star GA0740:14597892 with event index number of 2157028

Geocentric closest approach at 2024/08/03 12:11:52 UTC

J2000 position of star is 17:59:38.0 -15:09:47
Equinox of date position of star is 18:01:00.0 -15:09:46
Stellar brightness G=16.4, use SENSEUP=128 with the MallinCam and and exposure time of 2 seconds with the QHY174 camera.
Star is 147 degrees from the moon. Moon is 1% illuminated.
Apparent brightness V=23.1

Object is 34.6 AU from the Sun and 33.8 AU from the Earth.
Apparent velocity is 16.2 km/sec on the sky relative to the star, or, 2.4 arcsec/hr.
The 1-sigma error in the time of the event is 646 seconds.
The 1-sigma cross-track error in the shadow position is 3073 km.

The object has an absolute magnitude Hv=7.6
Diameter=184.5 km assuming a 5% albedo -- 11.4 sec chord
Diameter=75.3 km assuming a 30% albedo -- 4.6 sec chord
Dynamical classification is SCATNEAR
 
 
 
 
 
 
 
 

Star training set for 12HW87, (2024/08/03 12:12UT)
Object            RA         Dec     mag  sep  mel
Antares        16:30:55.2 -26:29:04  0.9 23.85 129
35Eta Oph      17:11:47.4 -15:45:13  2.6 11.88 136
PPM 233766     17:57:44.0 -15:48:53  6.1  1.03 146
PPM 233865     18:00:55.8 -15:09:02  7.9  0.03 147
12HW87         18:01:02.5 -15:09:46 16.4       147
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 12HW87, (2024/08/03 12:12UT)
Object            RA         Dec     mag  sep  mel
Antares        16:29:24.4 -26:25:56  0.9 23.85 129
35Eta Oph      17:10:22.7 -15:43:29  2.6 11.88 136
PPM 233766     17:56:19.0 -15:48:47  6.1  1.03 146
PPM 233865     17:59:31.3 -15:09:02  7.9  0.03 147
12HW87         17:59:38.0 -15:09:47 16.4       147
Positions are for J2000

Event circumstances last updated at 2023/11/08 05:25:34 UT

Marc W. Buie, Southwest Research Institute

RECON