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  2. Education
  3. Solar Physics Historical Timeline

Solar Physics Historical Timeline

1223 BC - 200 BC

1223 BC
The oldest eclipse record
800 BC
The first plausible recorded sunspot observation
350 BC
Sun circling under a sheltering sky
200 BC
The distance to the Sun

0 - AD 1599

AD 968
The first mention of the solar corona
1128
The first sunspot drawing
1185
The first description of solar prominences
1543
The Sun moves to center stage

1600 - 1799

1609
The Sun in focus
1610
First telescopic observations of sunspots
1644
The Sun as a star
1645-1715
Sunspots vanish
1687
The mass of the Sun
1774-1801
The physical nature of sunspots
1796
The nebular hypothesis

1800 - 1999

1800
The Sun's invisible radiation
1802
Black lines in the Sun
1817
Solar spectroscopy is born
1838
The solar constant
1843
The sunspot cycle
1845
The first solar photograph
1848
The sunspot number
1852
Sunspot cycle linked to geomagnetic activity
1858
The solar differential rotation
1859
First observation of a solar flare
1859
The chemical composition of the Sun
1860
First observations of a coronal mass ejection
1881
The solar constant, again
1908
The magnetic nature of sunspots
1919
The Sun's magnetic cycle
1931
The coronagraph

2000 - present

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Education

  • The Sun: A Pictorial Introduction
  • Questions and Answers About the Sun
  • Solar Physics Historical Timeline
  • Famous Solar-Stellar Scientists
  • Solar Astronomy in the Prehistoric Southwest
  • Suggested Reading
  • Additional Educational Resources
  • Solar Physics Historical Timeline (1223 BC - 200 BC)
  • Solar Physics Historical Timeline (0 - 1599)
  • Solar Physics Historical Timeline (1600 - 1799)
  • Solar Physics Historical Timeline (1800-1999)
  • Solar Physics Historical Timeline (2000-present)

Book traversal links for Solar Physics Historical Timeline

  • Solar Physics Historical Timeline (1223 BC - 200 BC) ›

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This material is based upon work supported by the NSF National Center for Atmospheric Research, a major facility sponsored by the U.S. National Science Foundation and managed by the University Corporation for Atmospheric Research. Any opinions, findings and conclusions or recommendations expressed in this material do not necessarily reflect the views of the U.S. National Science Foundation.