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Timeline of solar astronomy

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Timeline of solar astronomy

Contents

9th century

  • 850 — Ahmad ibn Muhammad ibn Kathīr al-Farghānī (Alfraganus) gives values for the obliquity of the ecliptic, the precessional movement of the apogees of the Sun

    • 10th century

  • 900–929 — Muhammad ibn Jābir al-Harrānī al-Battānī (Albatenius) discovers that the direction of the Sun's eccentricity is changing
  • 950–1000 — Ibn Yunus observes more than 10,000 entries for the Sun's position for many years using a large astrolabe with a diameter of nearly 1.4 metres

    • 11th century

  • 1031 — Abū al-Rayhān al-Bīrūnī calculates the distance between the Earth and the Sun in his Canon Mas’udicus

    • 17th century

  • 1613 — Galileo Galilei uses sunspot observations to demonstrate the rotation of the Sun
  • 1619 — Johannes Kepler postulates a solar wind to explain the direction of comet tails

    • 19th century

  • 1802 — William Hyde Wollaston observes dark lines in the solar spectrum
  • 1814 — Joseph Fraunhofer systematically studies the dark lines in the solar spectrum
  • 1834 — Hermann Helmholtz proposes gravitational contraction as the energy source for the Sun
  • 1843 — Heinrich Schwabe announces his discovery of the sunspot cycle and estimates its period to be about a decade
  • 1852 — Edward Sabine shows that sunspot number is correlated with geomagnetic field variations
  • 1859 — Richard Carrington discovers solar flares
  • 1860 — Gustav Kirchhoff and Robert Bunsen discover that each chemical element has its own distinct set of spectral lines
  • 1861 — Gustav Spörer discovers the variation of sun-spot latitudes during a solar cycle, explained by Spörer's law
  • 1863 — Richard Carrington discovers the differential nature of solar rotation
  • 1868 — Pierre Janssen and Norman Lockyer discover an unidentified yellow line in solar prominence spectra and suggest it comes from a new element which they name "helium"
  • 1893 — Edward Maunder discovers the 1645-1715 Maunder sunspot minimum

    • 20th century

  • 1904 — Edward Maunder plots the first sunspot "butterfly diagram"
  • 1906 — Karl Schwarzschild explains solar limb darkening
  • 1908 — George Hale discovers the Zeeman splitting of spectral lines from sunspots
  • 1925 — Cecilia Payne proposes hydrogen is the dominant element of the sun, not iron
  • 1929 — Bernard Lyot invents the coronagraph and observes the corona with an "artificial eclipse"
  • 1942 — J.S. Hey detects solar radio waves
  • 1949 — Herbert Friedman detects solar X-rays
  • 1960 — Robert B. Leighton, Robert Noyes, and George Simon discover solar five-minute oscillations by observing the Doppler shifts of solar dark lines
  • 1961 — Horace W. Babcock proposes the magnetic coiling sunspot theory
  • 1970 — Roger Ulrich, John Leibacher, and Robert F. Stein deduce from theoretical solar models that the interior of the Sun could act as a resonant acoustic cavity
  • 1975 — Franz-Ludwig Deubner makes the first accurate measurements of the period and horizontal wavelength of the five-minute solar oscillations
  • 1981 — NASA retrieves data from 1978 that shows a comet crashing into the Sun

    • 21st century

  • 2004 — largest solar flare ever recorded occurs

    • References

    Timeline of solar astronomy Wikipedia
    (Text) CC BY-SA


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