Orbit of comet 1911 VI /Quenisset

Orbit of comet 1911 VI /Quenisset

The orbital elements by Kuhne (1914) have been improved by the use of 205 observations covering the interval from Sept. 24, 1911, to Jan. 24, 1912. Perturbations by all nine planets were taken into account. The 'original' and 'future' values of the reciprocal semimajor axis are f...

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Veröffentlicht in:The Astronomical journal 1974-12, Vol.79, p.1455
Hauptverfasser: van Biesbroeck, G., Vesely, C. D., Marsden, B. G.
Format: Artikel
Sprache:eng
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Zusammenfassung:The orbital elements by Kuhne (1914) have been improved by the use of 205 observations covering the interval from Sept. 24, 1911, to Jan. 24, 1912. Perturbations by all nine planets were taken into account. The 'original' and 'future' values of the reciprocal semimajor axis are found to be plus 0.002494 and plus 0.002764 (plus or minus 0.000016 m.e.) per AU, respectively.
ISSN:0004-6256
DOI:10.1086/111700