Occultation of P384.2

The following prediction is the result obtained from the analysis of 14 strip scans obtained at the Lowell Observatory Astrograph by MIT observers in the summer of 2005, compared with an offset to the light-time corrected, geocentric JPL Horizon's ephemeris (PLU013, DE-0412, DE405) determined by comparing the Pluto system barycenter to the measured barycenter from the strips.  The offsets between the measured RA and Dec of P384.2 and its UCAC2 values are also given in the table.

 

Reference star position:
(UCAC2, at epoch of event)
RA (J2000) Dec (J2000) R Mag
P384.2 17 41 12.0743 –15 41 34.575 14.8
Offsets from Reference Position/Ephemeris
Body RA (arcsec) Dec (arcsec) Notes

P384.2

–0.362 ± 0.028 +0.106 ± 0.010 From 14 strip scans
Pluto System Barycenter 0 ± 0 ± From USNO frames
Pluto 0 ± 0 ± From PLU013

 

P384.2 UCAC 2.0 Prediction

(as of: 2005 11 10)

Geocentric Mid-time (yyyy mm dd hh:mm:ss) 2006 6 12 16:20:01 UT
Minimum Geocentric Separation (arcsec) 0.153 ± 0.010
Position Angle (deg) 178.8
Star Magnitude 14.8 R
Prediction Version P384.2-AST-1.0

Prediction Notes

Archive of all P384.2 occultation predictions based on alternate sources of data, including past predictions.

 

P384.2 Occultation Predictions for Individual Sites

Site East Longitude Latitude Distance (km)

Mid-time (UT)

Hobart 147 26 24 –42 48 18 482 16:18:33
Mt. John 170 27 54 –43 59 12 34 16:17:36
Mt. Stromlo 149 00 30 –35 19 12 1202 16:18:17
Siding Spring 149 03 42 –31 16 24 1618 16:18:12
Geocentric ---------- --------- 3560 16:20:01

Please direct all inquiries to Planetary Astronomy Lab (planetary-astronomy@mit.edu)

Last updated by Michael J Person(mjperson@mit.edu) 2006-04-10 15:00

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