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In astronomy, Galactocentrism is the theory that the Milky Way Galaxy, home of Earth's Solar System, is at or near the center of the Universe.[1][2]

Observations by William Herschel in 1785 suggested that the Milky Way was a disk-shaped galaxy with the sun in a central position. Although heliocentric, Herschel's observations were the first attempt at an observational cosmology.[3]

Herschel's heliocentric theory was overthrown by astronomer Harlow Shapley's work on globular clusters in 1918. Shapley's research marked the transition from heliocentrism to galactocentrism, placing the Galactic Center of the Milky Way Galaxy far away from the sun, towards Sagittarius. Heber Doust Curtis and Edwin Hubble further refuted the heliocentric view of the universe by showing that spirals are themselves far-flung galactic systems. By 1925, the galactocentric model was established.[3]

The theory of Galactocentrism was an important step in the development of cosmological models as speculation on the existence of other galaxies, comparable in size and structure to our own, placed the earth in its proper perspective with respect to the rest of the universe. Shifts from heliocentrism to galactocentrism and later acentrism have been compared in significance to the Copernican Revolution.[3]

William Herschel's Heliocentrism[edit]

Thomas Wright and Kant first speculated that fuzzy patches of light called nebulae were actually distant "island universes" consisting of many stellar systems.[4] The shape of our own galaxy was expected to resemble such "islands universes." But "scientific arguments were marshalled against such a possibility," and this view was rejected by almost all scientists until Edwin Hubble's measurements in 1924.[5]

William Herschel's model of the Milky Way, 1785

In 1783, amateur astronomer William Herschel attempted to determine the shape of the galaxy by examining stars through his handmade telescopes. Herschel was the first to propose a model of the galaxy based on observation and measurement.[6] He concluded that it was in the shape of a disk, but incorrectly assumed that the sun was in the center of the disk.[7][3][8][9]

Seeing that the stars belonging to the Milky Way galaxy appeared to encircle the Earth, Herschel carefully counted stars of given apparent magnitudes, and after finding the numbers were the same in all directions, concluded Earth must be close to the center of the galaxy. However, there were two flaws in Herschel's methodology: magnitude is not a reliable index to the distance of stars, and some of the areas that he mistook for empty space were actually dark, obscuring nebulae that blocked his view toward the center of the Milky Way.[10]

The Herschel model remained relatively unchallenged for the next hundred years, with minor refinements. Jacobus Kapteyn introduced motion, density, and luminosity to Herschel's star counts, which still implied a near-central location of the Sun.[7]

Harlow Shapley and Galactocentrism[edit]

In 1918, as Kapteyn was refining his model, Herschel's heliocentric theory was overthrown by astronomer Harlow Shapley's work on globular clusters. Shapley's observational cosmology marked a transition from Heliocentrism to Galactocentrism.[11][7][3]

Shapley had been studying the asymmetrical distribution of globular clusters, estimating the distance and location of individual objects by using variable stars as standard candles. Globular clusters contain many cepheid variable stars, whose precise relationship between luminosity and variability period was established by Henrietta Leavitt in 1908.[7] Using cepheid and RR Lyrae variables to systematically chart the distribution of globular clusters, Shapley discovered that the stars in the Milky Way orbited a common center thousands of light years away from the Sun.[12] The galactic center was determined to be in the direction of the Sagittarius constellation, approximately 50,000 light-years from us.[12]

Sextans A, a member of the local group of galaxies, which includes the Andromeda and Milky Way spirals, Lowell Observatory, 2013

In 1920 Heber Doust Curtis and Harlow Shapley participated in the Great Debate on the nature of nebulae and galaxies, and the size of the universe. Shapley believed that distant nebulae were relatively small and lay within the Milky Way galaxy. Curtis advocated the now-accepted view that nebulae were farther away, and that other galaxies apart from the Milky Way therefore existed.[3] By 1925, Edwin Hubble had confirmed that many objects previously thought to be clouds of dust and gas and classified as "nebulae" were actually galaxies beyond the Milky Way.[13][14][15]

"The realization, only a few decades ago, that our Galaxy is not unique and central in the universe ranks with the acceptance of the Copernican system as one of the great advances in cosmological thought." George O. Abell[3]

When astronomers realized that starlight can be absorbed by clouds of gas and dust, infrared radiation was used to penetrate the dust clouds.[9] Estimates dating after 2000 locate the Solar System within the range 24–28.4 kilolight-years (7.4–8.7 kiloparsecs) from the Galactic Center of the Milky Way galaxy.[16]


  1. ^ "Definition of galactocentric". Merriam-Webster Dictionary. Retrieved 6 June 2018.
  2. ^ "Definition of galactocentric in English". English Oxford Living Dictionaries. Retrieved 6 June 2018.
  3. ^ a b c d e f g Berendzen, Richard (1975). "Geocentric to heliocentric to galactocentric to acentric: the continuing assault to the egocentric". Vistas in Astronomy. 17 (1): 65–83. Bibcode:1975VA.....17...65B. doi:10.1016/0083-6656(75)90049-5.
  4. ^ Harrison, Edward Robert (2000), Cosmology: The Science of the Universe, Cambridge University Press, pp. 67–71, ISBN 978-0-521-66148-5
  5. ^ Berendzen, Richard (1975). "Geocentric to heliocentric to galactocentric to acentric: the continuing assault to the egocentric". Vistas in Astronomy. 17: 65–83. doi:10.1016/0083-6656(75)90049-5. Retrieved 26 August 2020.
  6. ^ Herschel, William (1 January 1785). "XII. On the construction of the heavens". Philosophical Transactions of the Royal Society of London. 75: 213–266. doi:10.1098/rstl.1785.0012. S2CID 186213203.
  7. ^ a b c d van de Kamp, Peter (October 1965), "The Galactocentric Revolution, A Reminiscent Narrative", Publications of the Astronomical Society of the Pacific, 77 (458): 324–328, Bibcode:1965PASP...77..325V, doi:10.1086/128228
  8. ^ "The Shape of the Milky Way from Starcounts". Astro 801. Retrieved 5 June 2018.
  9. ^ a b "Meet the Stargazers". WHYY. Retrieved 6 June 2018.
  10. ^ Ferris, Timothy (2003), Coming of Age in the Milky Way, HarperCollins, pp. 150–159, ISBN 978-0-06-053595-7
  11. ^ Bergh, Sidney van den (2011). "Hubble and Shapley—Two Early Giants of Observational Cosmology". Journal of the Royal Astronomical Society of Canada. 105 (6). arXiv:1110.2445.
  12. ^ a b Kopal, Z. (1972), "'Great Debate:' Obituary of Harlow Shapley", Nature, NASA, 240 (5381): 429–430, Bibcode:1972Natur.240..429., doi:10.1038/240429a0
  13. ^ Roberts, Jacob (2017). "A Giant of Astronomy". Distillations. 3 (3): 6–11. Retrieved May 16, 2018.
  14. ^ Hubble, Edwin (December 1926). "Extragalactic nebulae". Astrophysical Journal. 64 (64): 321–369. Bibcode:1926ApJ....64..321H. doi:10.1086/143018.
  15. ^ Hetherington, Edith W.; Hetherington, Norriss S. (2009). Astronomy and culture. Santa Barbara, Calif.: Greenwood Press/ABC-CLIO. p. 174. ISBN 978-0313345364.
  16. ^ Francis, Charles; Anderson, Erik (June 2014). "Two estimates of the distance to the Galactic Centre". Monthly Notices of the Royal Astronomical Society. 441 (2): 1105–1114. arXiv:1309.2629. Bibcode:2014MNRAS.441.1105F. doi:10.1093/mnras/stu631. S2CID 119235554.