Gérard de Vaucouleurs explained

Gérard de Vaucouleurs
Birth Name:Gérard Henri de Vaucouleurs
Birth Date:25 April 1918
Birth Place:Paris, France
Death Place:Austin, Texas
Field:Astronomy
Work Institutions:Yale University Observatory
Lowell Observatory
Harvard College Observatory
University of Texas at Austin
Alma Mater:Lycee Charlemagne (BSc, 1936)[1]
Sorbonne (PhD, 1949)
Known For:De Vaucouleurs's law
Prizes:Henry Norris Russell Lectureship (1988)
Prix Jules Janssen (1988)

Gérard Henri de Vaucouleurs (25 April 1918  - 7 October 1995)[2] was a French astronomer best known for his studies of galaxies.[3]

Life and career

Gerard de Vaucouleurs was born on April 25, 1918 in Paris, he took the maiden name of his mother as his last name.[4] He had an early interest in amateur astronomy and received his undergraduate degree in 1939 at the Sorbonne in that city.

After military service in World War II, he resumed his pursuit of astronomy. He was married to fellow astronomer Antoinette de Vaucouleurs on October 31, 1944, and the couple would frequently collaborate on astronomical research.[5]

He was fluent in English and spent 1949-51 in England and 1951 - 57 in Australia at Mount Stromlo Observatory. He was at Lowell Observatory in Arizona from 1957-1958 and at Harvard from 1958-60.

In 1960 he was appointed to the University of Texas at Austin, where he spent the rest of his career. He was one of the first five faculty in the newly formed astronomy department there. His wife Antoinette died in 1987. In 1995 he died of a heart attack in his home in Austin at the age of 77. At the time of his death he had a second wife named Elysabeth.

Research

His earliest work had concerned the planet Mars and while at Harvard he used telescope observations from 1909 to 1958 to study the areographic coordinates of features on the surface of Mars.[6] His later work focused on the study of galaxies and he co-authored the Third Reference Catalogue of Bright Galaxies with his wife Antoinette (1921-1987), a fellow UT Austin astronomer and lifelong collaborator.[5]

His specialty included reanalyzing Hubble and Sandage's galaxy atlas and recomputing the distance measurements utilizing a method of averaging many different kinds of metrics such as luminosity, the diameters of ring galaxies, brightest star clusters, etc., in a method he called "spreading the risks." During the 1950s he promoted the idea that galactic clusters are grouped into superclusters.

The de Vaucouleurs modified Hubble sequence is a widely used variant of the standard Hubble sequence.

De Vaucouleurs was awarded the Henry Norris Russell Lectureship by the American Astronomical Society in 1988. He was awarded the Prix Jules Janssen of the Société astronomique de France (Astronomical Society of France) in the same year. He and his wife and longtime collaborator, Antoinette, together produced 400 research and technical papers, 20 books and 100 articles for laymen.

See also

External links

Other resources

Notes and References

  1. Web site: Gerard Henri de Vaucouleurs (1918 - 1995). American Astronomical Society. 29 June 2017. 14 January 2018. https://web.archive.org/web/20180114073711/https://aas.org/obituaries/gerard-henri-de-vaucouleurs-1918-1995. dead.
  2. Burbidge . E. Margaret . 2002 . GÉRARD DE VAUCOULEURS 1918–1995 . Biographical Memoirs . National Academy of Sciences . 82 . National Academy of Sciences Online.
  3. Web site: Gerard de Vaucouleurs McDonald Observatory . 2023-06-17 . mcdonaldobservatory.org.
  4. Burbidge . Geoffrey . 30 November 1995 . Gérard de Vaucouleurs (1918-95) . Nature . 378 . 6556 . 440. 10.1038/378440a0 . 1995Natur.378..440B . 46470185 .
  5. Web site: In Memoriam: Antoinette de Vaucouleurs, 1921-1987 . October 13, 2008 . The University of Texas at Austin .
  6. Book: de Vaucouleurs, Gerard . 1963 . La Physique des Planetes; Communications Presentees au Onzieme Colloque International d'Astrophysique tenu a Liège, les 9, 10 et 11 Juillet 1962. . Liège International Astrophysical Colloquia . 11 . Precision Mapping of Mars . 369–385 . 1963LIACo..11..369D .