Pluto Occultation of P131.1

Ron Stone has provided new astrometric measurements of this star from observations at the FASTT at the U.S. Naval Observatory, which were averaged with unpublished UCAC** values for the position to calculate the offsets given below. The offset is relative to the star's published position, as determined by McDonald and Elliot (see AJ 120 2000)***. The Pluto offsets to its ephemeris were estimated from Pluto's recent occultation with P126 in July 2002. Results for Pluto are tabulated as offsets from the unmodified light-time corrected, geocentric JPL Horizon's ephemeris (PLU006 and DE-0406, LE-0406).
Reference Position (2.0)*** RA (J2000) Dec (J2000) R Mag*
P131.1 16 58 49.456 -12 51 31.41 15.65
Offsets from Reference
Body RA (arcsec) Dec (arcsec)  
P131.1 + 0.312+/– 0.103 – 0.428+/– 0.089  
Pluto – 0.02 +/– 0.007 – 0.023 +/– 0.007  

* From Ron Stone's reduction

**Zacharias, UCAC unpublished

*** McDonald 2000 AJ 120 1599

P131.1 Current Prediction

(as of 2002 07 26

1:39 PM EDT)

Date and Time (yyyy mm dd hh:mm:ss) 2002 08 21 06:57:07 UT
Minimum Geocentric Separation (arcsec) 0.02 +/- 0.101
Position Angle (in degrees, clockwise from East) 117
Geocentric Shadow Velocity (km s-1) 6.7
Star Magnitude 15.7 (V)
Solar Angle (deg) 107
East Longitude (deg) -179
Distance (AU) 30.24
Prediction Version p131.1-2.2

Prediction Notes

Archive of past P131.1 occultation predictions.

Pluto Occultation Predictions for Individual Sites

Site East Longitude Latitude Distance* (km) Immersion (UT)

Mid-time (UT)

Emersion (UT)
Anderson Mesa -111 32 12 35 05 48 1854   06:42:37  
Dominion Observatory, Canada -123 25 00 48 31 12 118 06:38 53 06:41:45 06:44:37
Geocentric     414 06:54:25 06:57:07 06:59:50
Guillermo Haro, Mexico -110 23 00 31 03 12 2263   06:43:05  
IRTF -155 28 29 19 49 46 41 06:44:26 06:47:15 06:50:05
Lick -121 38 12 19 49 36 2573   06:44:55  
Lowell -111 39 54 35 12 12 1839   06:42:36  
Mauna Kea -155 28 12 19 49 24 41 06:44:26 06:47:15 06:50:05
Mt Lemmon -110 47 30 32 26 30 2123   06:42:55  
Palomar -116 51 54 33 21 24 1755  

06:42:52

 
WIRO -105 58 36 41 05 54 1513   06:42:02  

 

Last updated by Katie Carbonari (kcarbon@mit.edu) 2002 07 17 1:05 PM EDT

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