J/AJ/149/22     Astrometry of Pluto from 1930-1951 observations    (Buie+, 2015)

Astrometry of Pluto from 1930-1951 observations: the Lampland plate collection. Buie M.W., Folkner W.M. <Astron. J., 149, 22 (2015)> =2015AJ....149...22B 2015AJ....149...22B
ADC_Keywords: Minor planets ; Positional data Keywords: astrometry - ephemerides - Kuiper belt objects: individual: Pluto - planets and satellites: individual: Pluto Abstract: We present a new analysis of 843 photographic plates of Pluto taken by Carl Lampland at Lowell Observatory from 1930-1951. This large collection of plates contains useful astrometric information that improves our knowledge of Pluto's orbit. This improvement provides critical support to the impending flyby of Pluto by New Horizons. New Horizons can do inbound navigation of the system to improve its targeting. This navigation is capable of nearly eliminating the sky-plane errors but can do little to constrain the time of closest approach. Thus the focus on this work was to better determine Pluto's heliocentric distance and to determine the uncertainty on that distance with a particular eye to eliminating systematic errors that might have been previously unrecognized. This work adds 596 new astrometric measurements based on the USNO CCD Astrograph Catalog 4. With the addition of these data the uncertainty of the estimated heliocentric position of Pluto in Developmental Ephemerides 432 (DE432) is at the level of 1000km. This new analysis gives us more confidence that these estimations are accurate and are sufficient to support a successful flyby of Pluto by New Horizons. Description: We present a new analysis of 843 photographic plates of Pluto taken by Carl Lampland at Lowell Observatory from 1930-1951. All of the Lampland plates were taken with the Lowell Observatory 40inch reflector. This facility was located on the main observatory grounds in Flagstaff. The telescope was an f/6 reflector with a Newtonian optical design. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 97 596 Pluto astrometry -------------------------------------------------------------------------------- See also: VI/88 : Ephemerides of Pluto (PLUTO95) (Chapront+ 1995) I/322 : UCAC4 Catalogue (Zacharias+, 2012) J/A+A/570/A86 : Pluto astrometry from 19yrs observations (Benedetti-Rossi+, 2014) J/A+A/553/A14 : Pluto's observations between 1997 and 2010 (Beauvalet+, 2013) J/A+A/515/A32 : Pluto, Charon, Nix, Hydra occultations 2008-15 (Assafin+ 2010) J/A+A/486/613 : Observation of Pluto (Veiga+, 2008) J/A+A/383/1054 : Astrometry of Pluto and Saturn in 1995-2001 (Rapaport+, 2002) J/A+AS/118/105 : Pluto 1991-1994 observations (Ryl'kov+, 1996) http://www.lowell.edu/ : Lowell Observatory Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 12 A12 --- File File name of the archived scan image at Lowell Observatory (1) 14- 23 A10 "Y:M:D" Obs.date UTC date of the middle of the exposure 25- 32 A8 "h:m:s" Obs.time UTC time of the middle of the exposure 34- 35 I2 h RAh Hour of Right Ascension (J2000) (2) 37- 38 I2 min RAm Minute of Right Ascension (J2000) (2) 40- 45 F6.3 s RAs Second of Right Ascension (J2000) (2) 47- 51 F5.3 s e_RAs 1σ uncertainty in RAs (Pluto only) (3) 53 A1 --- DE- Sign of the Declination (J2000) (2) 54- 55 I2 deg DEd Degree of Declination (J2000) (2) 57- 58 I2 arcmin DEm Arcminute of Declination (J2000) (2) 60- 64 F5.2 arcsec DEs Arcsecond of Declination (J2000) (2) 66- 69 F4.2 arcsec e_DEs 1σ uncertainty in DEs (Pluto only) (3) 71- 75 F5.3 --- xchi2 Unweighted χ2 of ξ fit (4) 77- 81 F5.3 --- echi2 Unweighted χ2 of η fit (4) 83- 87 F5.3 arcsec x0Err 1σ uncertainty of ξ zero-point (5) 89- 93 F5.3 arcsec e0Err 1σ uncertainty of η zero-point (5) 95- 97 I3 --- Nstars [32/458] Number of catalog sources used in the local fit in the region of interest around Pluto -------------------------------------------------------------------------------- Note (1): Named for the UT date of the night of observation, followed by the plate number during the night. Note that the first pass processing had not yet discovered the date confusion in some of the nights and had used the date listed in the log book for each of plate identification. Most of the time this leads to a date that is one day earlier. This point is mentioned since both epochs of scans are saved in the archives at Lowell Observatory. Note (2): All measurements are topocentric positions based on UCAC4 catalog (Zacharias et al. 2012, cat. I/322) positions corrected for proper motion to the epoch of each plate. The observatory location was on the main Lowell Observatory campus. The position of the observatory was measured in the center on top of the dome to be N 35° 12.182', W 111°39.988', 2225m on the WGS84 datum. Note (3): These uncertainties estimate the errors in the measured position of Pluto and do not include any contribution from errors in the plate solution or the underlying catalog errors. Note (4): The unweighted χ2 for the fit in each tangent plane axis divided by the number of stars (provide the relative quality of the astrometric fit). These values are also equivalent to the rms of the post-fit residuals in arcseconds. Note (5): Formal uncertainty on the constant term of the ξ and η fits. -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Greg Schwarz [AAS], Sylvain Guehenneux [CDS] 30-Jan-2015
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line