- Henry Draper Catalogue
The Henry Draper Catalogue (HD) is an
astronomical star cataloguepublished between 1918 and 1924, giving spectroscopicclassifications for 225,300 stars; it was later expanded by the Henry Draper Extension (HDE), published between 1925 and 1936, which gave classifications for 46,850 more stars, and by the Henry Draper Extension Charts (HDEC), published from 1937 to 1949 in the form of charts, which gave classifications for 86,933 more stars. In all, 359,083 stars were classified. [The Henry Draper Extension Charts: A catalogue of accurate positions, proper motions, magnitudes and spectral types of 86933 stars, V. V. Nesterov, A. V. Kuzmin, N. T. Ashimbaeva, A. A. Volchkov, S. Röser, and U. Bastian, "Astronomy and Astrophysics Supplement Series" 110 (1995), pp. 367–370, bibcode|1995A&AS..110..367N.] The original HD catalogue covers the entire sky almost completely down to an apparent photographic magnitudeof about 9; the extensions added fainter stars in certain areas of the sky. [http://www.willbell.com/software/hypersky/hd.htm HENRY DRAPER star catalog, edition 1985] , HyperSky documentation, Willmann-Bell, Inc., 1996.] The construction of the Henry Draper Catalogue was part of a pioneering effort to classify stellar spectra, and its catalogue numbers are commonly used as a way of identifying stars.
The origin of the Henry Draper Catalogue goes back to the earliest photographic studies of stellar spectra.
Henry Drapermade the first photograph of a star's spectrumshowing distinct spectral lineswhen he photographed Vegain 1872. He took over a hundred more photographs of stellar spectra before his death in 1882. In 1885, Edward Pickeringbegan to supervise photographic spectroscopy at Harvard College Observatory, using the objective prismmethod. In 1886, Draper's widow, Mary Anne Palmer Draper, became interested in Pickering's research and agreed to fund it under the name "Henry Draper Memorial". [On the Henry Draper Memorial Photographs of Stellar Spectra, George F. Barker, [http://books.google.com/books?id=KcAAAAAAYAAJ "Proceedings of the American Philosophical Society" 24 (1887)] , pp. 166–172.] [p. 75, "Women in Science: Antiquity Through the Nineteenth Century: a Biographical Dictionary with Annotated Bibliography", Marilyn Bailey Ogilvie, MIT Press, 1986, ISBN 026265038X.] Pickering and his coworkers then began to take an objective-prism survey of the sky and to classify the resulting spectra. [The Henry Draper Memorial, Annie J. Cannon, "Journal of the Royal Astronomical Society of Canada" 9, #5 (May-June 1915), pp. 203–215, bibcode|1915JRASC...9..203C.]
A first result of this work was the "Draper Catalogue of Stellar Spectra", published in 1890. This catalogue contained spectroscopic classifications for 10,351 stars, mostly north of declination −25°. Most of the classification was done by
Williamina Fleming. [The Draper Catalogue of stellar spectra photographed with the 8-inch Bache telescope as a part of the Henry Draper memorial, Edward C. Pickering, "Annals of Harvard College Observatory" 27 (1890), bibcode|1890AnHar..27....1P. See in particular pp. 1–2.] The classification scheme used was to subdivide the previously used Secchi classes(I to IV) into more specific classes, given letters from A to N. Also, the letter O was used for stars whose spectra consisted mainly of bright lines, the letter P for planetary nebulae, and the letter Q for spectra not fitting into any of the classes A through P. No star of type N appeared in the catalogue, and the only star of type O was the Wolf-Rayet star HR 2583. Antonia Mauryand Pickering published a more detailed study of the spectra of bright stars in the northern hemisphere in 1897. [Spectra of bright stars photographed with the 11-inch Draper Telescope as part of the Henry Draper Memorial, Antonia C. Maury and Edward C. Pickering, "Annals of Harvard College Observatory" 28, part 1 (1897), pp. 1–128, bibcode|1897AnHar..28....1M.] Maury used classifications numbered from I to XXII; groups I to XX corresponded to subdivisions of the Draper Catalogue types B, A, F, G, K, and M, while XXI and XXII corresponded to the Draper Catalogue types N and O. [Table I, Maury and Pickering 1897.] She was the first to place B stars in their current position, prior to A stars, in the spectral classification. [p. 112, Hearnshaw 1986.]
In 1890, the Harvard College Observatory constructed an observation station in
Arequipa, Peruin order to study the sky in the Southern Hemisphere, and a study of bright stars in the southern hemisphere was published by Annie Jump Cannonand Pickering in 1901. [Spectra of bright southern stars photographed with the 13-inch Boyden telescope as part of the Henry Draper Memorial, Annie J. Cannon and Edward C. Pickering, "Annals of Harvard College Observatory" 28, part 2 (1901), pp. 129–263, bibcode|1901AnHar..28..129C.] [pp. 110–111, 117–118, Hearnshaw 1986.] Cannon used the lettered types of the "Draper Catalogue of Stellar Spectra", but dropped all letters except O, B, A, F, G, K, and M, used in that order, as well as P for planetary nebulae and Q for some peculiar spectra. She also used types such as B5A for stars halfway between types B and A, F2G for stars one-fifth of the way from F to G, and so forth. [pp. 117–119, Hearnshaw 1986.]
Between 1910 and 1915, new discoveries increased interest in stellar classification, and work on the "Henry Draper Catalogue" itself started in 1911. From 1912 to 1915, Cannon and her coworkers classified spectra at the rate of approximately 5,000 per month. [pp. 214–215, Cannon 1915.] The catalogue was published in 9 volumes of the "Annals of Harvard College Observatory" between 1918 and 1924. It contains rough positions, magnitudes, spectral classifications, and, where possible, cross-references to the
Durchmusterungcatalogs for 225,300 stars. [The Henry Draper Catalogue, Annie J. Cannon and Edward C. Pickering, "Annals of Harvard College Observatory";
hours 0 to 3, 91 (1918), bibcode|1918AnHar..91....1C;
hours 4 to 6, 92 (1918), bibcode|1918AnHar..92....1C;
hours 7 to 8, 93 (1919), bibcode|1919AnHar..93....1C;
hours 9 to 11, 94 (1919), bibcode|1919AnHar..94....1C;
hours 12 to 14, 95 (1920), bibcode|1920AnHar..95....1C;
hours 15 to 16, 96 (1921), bibcode|1921AnHar..96....1C;
hours 17 to 18, 97 (1922), bibcode|1922AnHar..97....1C;
hours 19 to 20, 98 (1923), bibcode|1923AnHar..98....1C;
hours 21 to 23, 99 (1924), bibcode|1924AnHar..99....1C.] The classification scheme used was similar to that used in Cannon's 1901 work, except that types such as B, A, B5A, F2G, and so on, had been changed to B0, A0, B5, F2, and so on. As well as the classes O through M, P was used for nebulae and R and N for
carbon stars. [pp. 121–122, 128, 133–134, Hearnshaw 1986; also see pp. 5–11 of the first volume of the Henry Draper Catalogue (Cannon & Pickering 1918.)]
Pickering died on
February 3, 1919, leaving 6 volumes to be overseen by Cannon. [p. 135, "The Analysis of Starlight: One Hundred and Fifty Years of Astronomical Spectroscopy", J. B. Hearnshaw, Cambridge, UK: Cambridge University Press, 1986, ISBN 0-521-25548-1.] Cannon found spectral classifications for 46,850 fainter stars in selected regions of the sky in the "Henry Draper Extension", published in six parts between 1925 and 1936.The Henry Draper extension, Annie J. Cannon, "Annals of Harvard College Observatory" 100 (1925–1936), bibcode|1936AnHar.100....1C.] [p. 1, The Henry Draper charts of stellar spectra, Annie J. Cannon and Harlow Shapley, "Annals of Harvard College Observatory" 105, #1 (1937), pp. 1–19, bibcode|1937AnHar.105....1C.] She continued classifying stars until her death in 1941. Most of these classifications were published in 1949 in the "Henry Draper Extension Charts" (the first portion of these charts was published in 1937.) These charts also contained some classifications by Margaret Walton Mayall, who supervised the work after Cannon's death. [Cannon and Shapley 1937; also see p. 138, Hearnshaw 1986.] [The Henry Draper extension. II, Annie J. Cannon and Margaret Walton Mayall, "Annals of Harvard College Observatory" 112 (1949), bibcode|1949AnHar.112....1C.]
The catalogue and its extensions were the first large-scale attempt to catalogue
spectral types of stars,p. 4, "Galaxies in the Universe: An Introduction", Linda S. Sparke, John S. Gallagher, III, Cambridge, UK: Cambridge University Press, 2nd ed., 2007, ISBN 0521855934.] and its construction led to the Harvard classificationscheme of stellar spectra which is still used today. [p. 13, "From Dust to Stars: Studies of the Formation and Early Evolution of Stars", Norbert S. Schulz, Berlin, New York: Springer, 2005, ISBN 3540237119.]
Availability and usage
Stars contained in the main portion of the catalogue are of medium magnitude, down to about 9m (about 1/15 as bright as the faintest stars visible with the naked eye). The extensions contain stars as faint as the 11th magnitude selected from certain regions of the sky. [ [http://www.britannica.com/EBchecked/topic/92776/Annie-Jump-Cannon Annie Jump Cannon] , article, "Encyclopædia Britannica Online", accessed
September 12, 2008.] Stars in the original catalogue are numbered from 1 to 225300 (prefix "HD") and are numbered in order of increasing right ascensionfor the epoch 1900.0. Stars in the first extension are numbered from 225301 to 272150 (prefix "HDE"), and stars from the extension charts are numbered from 272151 to 359083 (prefix "HDEC"). However, as the numbering is continuous throughout the catalog and its extensions, the prefix "HD" may be used regardless as its use produces no ambiguity. [See p. 2, Cannon and Shapley 1937 and p. 369, Nesterov et al. 1995.] Many stars are customarily identified by their HD numbers.p. 327, "Measuring the Universe: The Cosmological Distance Ladder", Stephen Webb, London, New York: Springer, 1999, ISBN 1852331062.]
The Henry Draper Catalogue and the Extension were available from the
NASA Astronomical Data Centeras part of their third CD-ROMof astronomical catalogues. [ [http://adc.gsfc.nasa.gov/adc/adccdrom3_doc.html Astronomical Data Center CD-ROM: Selected Astronomical Catalogs, Volume 3] , Astronomical Data Center, NASA. Accessed on line September 11, 2008.] Currently, the Catalogue and Extension are available from the VizieRservice of the Centre de Données astronomiques at Strasbourgas catalogue number III/135A. [Henry Draper Catalogue and Extension, A. J. Cannon and E. C. Pickering, CDS ID [http://cdsarc.u-strasbg.fr/viz-bin/Cat?III/135A III/135A] .] Because of their format, putting the Henry Draper Extension Charts into a machine-readable format was more difficult, but this task was eventually completed by 1995 by Nesterov, Röser and their coworkers, and the Charts are now available at VizieRas catalogue number III/182. [Nesterov et al. 1995.] [The Henry Draper Extension Charts: A catalogue of accurate positions, proper motions, magnitudes and spectral types of 86933 stars, V. V. Nesterov, A. V. Kuzmin, N. T. Ashimbaeva, A. A. Volchkov, S. Roeser, and U. Bastian, CDS ID [http://cdsarc.u-strasbg.fr/viz-bin/Cat?III/182 III/182] .]
The Henry Draper Catalogue and its extensions are available on line free of charge at the
VizieRservice of the Centre de Données astronomiques de Strasbourg:
* Henry Draper Catalogue and Extension, A. J. Cannon and E. C. Pickering, CDS ID [http://cdsarc.u-strasbg.fr/viz-bin/Cat?III/135A III/135A] .
* The Henry Draper Extension Charts: A catalogue of accurate positions, proper motions, magnitudes and spectral types of 86933 stars, V. V. Nesterov, A. V. Kuzmin, N. T. Ashimbaeva, A. A. Volchkov, S. Roeser, and U. Bastian, CDS ID [http://cdsarc.u-strasbg.fr/viz-bin/Cat?III/182 III/182] .
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