Henry Draper Catalogue

The Henry Draper Catalogue (HD) is an astronomical star catalogue published between 1918 and 1924, giving spectroscopic classifications 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 as of August 2017.[1][2]

The HD catalogue is named after Henry Draper, an amateur astronomer, and covers the entire sky almost completely down to an apparent photographic magnitude of about 9; the extensions added fainter stars in certain areas of the sky.[3] 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.[4][5]

Henry Draper Catalogue
Alternative namesThe Henry Draper Catalogue

History

The origin of the Henry Draper Catalogue dates back to the earliest photographic studies of stellar spectra. Henry Draper made the first photograph of a star's spectrum showing distinct spectral lines when he photographed Vega in 1872. He took over a hundred more photographs of stellar spectra before his death in 1882. In 1885, Edward Pickering began to supervise photographic spectroscopy at Harvard College Observatory, using the objective prism method. 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.[6][7] Pickering and his coworkers then began to take an objective-prism survey of the sky and to classify the resulting spectra.[8]

Classifications in the Draper Catalogue of Stellar Spectra[9]
Secchi Draper Comment
I A, B, C, D Hydrogen lines dominant.
II E, F, G, H, I, K, L
III M
IV N Did not appear in the catalogue.
O Wolf–Rayet spectra with bright lines.
P Planetary nebulae.
Q Other spectra.

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.[10] 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.[9]

Antonia Maury and Pickering published a more detailed study of the spectra of bright stars in the northern hemisphere in 1897.[11] 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.[12] She was the first to place B stars in their current position, prior to A stars, in the spectral classification.[13]

In 1890, the Harvard College Observatory constructed an observation station in Arequipa, Peru in order to study the sky in the Southern Hemisphere, and a study of bright stars in the southern hemisphere was published by Annie Jump Cannon and Pickering in 1901.[14][15] 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.[16]

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.[17] 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 Durchmusterung catalogs for 225,300 stars.[18] 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.[19]

Pickering died on February 3, 1919, leaving 6 volumes to be overseen by Cannon.[20] 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.[2][21] 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.[22][23]

The catalogue and its extensions were the first large-scale attempt to catalogue spectral types of stars,[5] and its construction led to the Harvard classification scheme of stellar spectra which is still used today.[24]

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.[3][25] Stars in the original catalogue are numbered from 1 to 225300 (prefix HD) and are numbered in order of increasing right ascension for 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.[26] Many stars are customarily identified by their HD numbers.[4]

The Henry Draper Catalogue and the Extension were available from the NASA Astronomical Data Center as part of their third CD-ROM of astronomical catalogues.[27] Currently, the Catalogue and Extension are available from the VizieR service of the Centre de Données astronomiques (French for "Astronomical Data Center") at Strasbourg as catalogue number III/135A.[28] 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 VizieR as catalogue number III/182.[1]

References

  1. ^ a b Nesterov, V. V.; Kuzmin, A. V.; Ashimbaeva, N. T.; Volchkov, A. A.; Röser, S.; Bastian, U. (1995). "The Henry Draper Extension Charts: A catalogue of accurate positions, proper motions, magnitudes and spectral types of 86933 stars". Astronomy and Astrophysics Supplement Series. 110: 367. Bibcode:1995A&AS..110..367N. CDS ID III/182.
  2. ^ a b Cannon, Annie. J. (1936). "The Henry Draper extension". Annals of Harvard College Observatory. 100: 1. Bibcode:1936AnHar.100....1C.
  3. ^ a b "HD (S0): HENRY DRAPER star catalog, edition 1985 (19930406)". HyperSky. Willmann-Bell, Inc. 1996. Archived from the original on May 9, 2008.
  4. ^ a b Webb, Stephen (1999). Measuring the Universe: The Cosmological Distance Ladder. Springer. p. 327. ISBN 978-1-85233-106-1.
  5. ^ a b Sparke, Linda S.; Gallagher, John S., III (2007). Galaxies in the Universe: An Introduction (2nd ed.). Cambridge University Press. p. 4. ISBN 978-0-521-85593-8.
  6. ^ Barker, George F. (1887). "On the Henry Draper Memorial Photographs of Stellar Spectra". Proceedings of the American Philosophical Society. 24: 166–172.
  7. ^ Ogilvie, Marilyn Bailey (1986). Women in Science: Antiquity Through the Nineteenth Century: a Biographical Dictionary with Annotated Bibliography. MIT Press. p. 75. ISBN 978-0-262-65038-0.
  8. ^ Cannon, Annie J. (1915). "The Henry Draper Memorial". Journal of the Royal Astronomical Society of Canada. 9: 203. Bibcode:1915JRASC...9..203C.
  9. ^ a b Hearnshaw 1986, p. 108; Pickering 1890, p. 2–4
  10. ^ Pickering, Edward C. (1890). "The Draper Catalogue of stellar spectra photographed with the 8-inch Bache telescope as a part of the Henry Draper memorial". Annals of Harvard College Observatory. 27: 1–388. Bibcode:1890AnHar..27....1P. See in particular pp. 1–2.
  11. ^ Maury, Antonia C.; Pickering, Edward C. (1897). "Spectra of bright stars photographed with the 11-inch Draper Telescope as part of the Henry Draper Memorial". Annals of Harvard College Observatory. 28: 1. Bibcode:1897AnHar..28....1M.
  12. ^ Maury & Pickering 1897, Table I
  13. ^ Hearnshaw 1986, p. 112
  14. ^ Cannon, Annie J.; Pickering, Edward C. (1901). "Spectra of bright southern stars photographed with the 13-inch Boyden telescope as part of the Henry Draper Memorial". Annals of Harvard College Observatory. 28: 129. Bibcode:1901AnHar..28..129C.
  15. ^ Hearnshaw 1986, pp. 110–111, 117–118
  16. ^ Hearnshaw 1986, pp. 117–119
  17. ^ Cannon 1915, pp. 214–215
  18. ^ Cannon, Annie J.; Pickering, Edward C. (1918). "The Henry Draper Catalogue". Annals of Harvard College Observatory.;
    hours 0 to 3, 91 (1918), Bibcode1918AnHar..91....1C;
    hours 4 to 6, 92 (1918), Bibcode1918AnHar..92....1C;
    hours 7 to 8, 93 (1919), Bibcode1919AnHar..93....1C;
    hours 9 to 11, 94 (1919), Bibcode1919AnHar..94....1C;
    hours 12 to 14, 95 (1920), Bibcode1920AnHar..95....1C;
    hours 15 to 16, 96 (1921), Bibcode1921AnHar..96....1C;
    hours 17 to 18, 97 (1922), Bibcode1922AnHar..97....1C;
    hours 19 to 20, 98 (1923), Bibcode1923AnHar..98....1C;
    hours 21 to 23, 99 (1924), Bibcode1924AnHar..99....1C.
  19. ^ Hearnshaw 1986, pp. 121–122, 128, 133–134; also see Cannon & Pickering 1918, vol. 1, pp. 5–11
  20. ^ Hearnshaw, J. B. (1986). The Analysis of Starlight: One Hundred and Fifty Years of Astronomical Spectroscopy. Cambridge University Press. p. 135. ISBN 978-0-521-25548-6.
  21. ^ Cannon, Annie Jump; Shapley, Harlow (1937). "The Henry Draper charts of stellar spectra". Annals of Harvard College Observatory. 105 (1): 1. Bibcode:1937AnHar.105....1C.
  22. ^ Cannon & Shapley 1937; Hearnshaw 1986, p. 138
  23. ^ Cannon, Annie J.; Mayall, Margaret Walton (1949). "The Henry Draper extension. II". Annals of Harvard College Observatory. 112: 1. Bibcode:1949AnHar.112....1C.
  24. ^ Schulz, Norbert S. (2005). From Dust to Stars: Studies of the Formation and Early Evolution of Stars. Springer. p. 13. ISBN 978-3-540-23711-2.
  25. ^ Annie Jump Cannon, article, Encyclopædia Britannica Online, accessed September 12, 2008.
  26. ^ See p. 2, Cannon and Shapley 1937 and p. 369, Nesterov et al. 1995.
  27. ^ Astronomical Data Center CD-ROM: Selected Astronomical Catalogs, Volume 3 Archived 2008-09-16 at the Wayback Machine, Astronomical Data Center, NASA. Accessed on line September 11, 2008.
  28. ^ Henry Draper Catalogue and Extension, A. J. Cannon and E. C. Pickering, CDS ID III/135A.

External links

The Henry Draper Catalogue and its extensions are available on line free of charge at the VizieR service of the Centre de Données astronomiques de Strasbourg:

  • Henry Draper Catalogue and Extension, A. J. Cannon and E. C. Pickering, CDS ID 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 III/182.
26 Boötis

26 Boötis (26 Boo, 26 Bootis) is a star in the constellation Boötes. Its apparent magnitude is 5.91.

32 Boötis

32 Boötis (32 Boo) is a star in the constellation Boötes. Its apparent magnitude is 5.55.

32 Ophiuchi

32 Ophiuchi (32 Oph) is a star in the constellation Hercules. Its apparent magnitude is 5.00.

33 Boötis

33 Boötis (33 Boo) is a star in the constellation Boötes. Its apparent magnitude is 5.39.

38 Aurigae

38 Aurigae is a star in the constellation Auriga. Its apparent magnitude is 6.08. It is approximately 71.84 light years from Earth.

40 Boötis

40 Boötis (40 Boo, 40 Bootis) is a star in the constellation Boötes. Its apparent magnitude is 5.64.

62 Aurigae

62 Aurigae is a star in the constellation Auriga. Its apparent magnitude is 6.02.

64 Aurigae

64 Aurigae (64 Aur) is a star in the constellation Auriga. Its apparent magnitude is 5.87.

68 Aquarii

68 Aquarii (abbreviated 68 Aqr) is a star in the constellation of Aquarius. 68 Aquarii is its Flamsteed designation, though it also bears the Bayer designation of g2 Aquarii. Its apparent magnitude is 5.24.

68 Aquarii is a high proper-motion star. It is designated as HD 215721 in the Henry Draper Catalogue.

HD 101570

HD 101570 is a star in the constellation Centaurus. Its apparent magnitude is 4.92.

HD 121474

HD 121474 is a star in the constellation Centaurus. Its apparent magnitude is 4.71.

HD 123569

HD 123569 is a star in the constellation Centaurus. Its apparent magnitude is 4.75.

HD 125628

HD 125628 is a double star in the constellation Centaurus. Its apparent magnitude is 4.92.

HD 79447

HD 79447, also known as i Carinae (i Car) is a star in the constellation Carina. It is a blue-white B-type giant with an apparent magnitude of +3.96 and is approximately 499 light years from Earth.

HD 81101

HD 81101, also known as k Carinae (k Car), is a star in the constellation Carina.

k Carinae is a yellow G-type giant with an apparent magnitude of +4.79. It is approximately 223 light years from Earth.

HD 83944

HD 83944, also called m Carinae (m Car), is a star in the constellation Carina.

m Carinae is a blue-white B-type subgiant with an apparent magnitude of +4.51. It is approximately 224 light years from Earth.

Nova Sagittarii 1898

Nova Sagittarii 1898 (also called V1059 Sagittarii) was a nova, which lit up in 1898 in the constellation Sagittarius. Nova Sagittarii 1898 reached magnitude 4.5.

V604 Aquilae

V604 Aquilae or Nova Aquilae 1905 was a nova, which occurred in the constellation Aquila in 1905 with a maximum brightness of 7.6 mag.

V849 Ophiuchi

V849 Ophiuchi or Nova Ophiuchi 1919 was a nova that lit up in 1919 in the constellation Ophiuchus and reached a brightness of 7.4 mag.

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