Format: Short Description (ICOMOS-IAU Case Study format)

Presentation

Geographical position 

• InfoTheme: Astronomy from the Renaissance to the mid-twentieth century
  Entity: 37
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  Status: PUB
  Date: 2011-08-22 11:08:01
  Author(s): Gudrun Wolfschmidt, Clive Ruggles

Mount Wilson, Los Angeles County, State of California, USA.

Location 

• InfoTheme: Astronomy from the Renaissance to the mid-twentieth century
  Entity: 37
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  Date: 2012-04-30 15:53:48
  Author(s): Gudrun Wolfschmidt, Clive Ruggles

Latitude 34° 13′ 28″ N, longitude 118° 3′ 31″ W. Elevation 1740m above mean sea level. This is the location of the 150ft solar tower.

General description 

• InfoTheme: Astronomy from the Renaissance to the mid-twentieth century
  Entity: 37
  Subentity: 1
  Version: 6
  Status: PUB
  Date: 2017-11-10 16:05:47
  Author(s): Gudrun Wolfschmidt, Clive Ruggles

The Mount Wilson Observatory, founded in 1904, is one of a number of observatories built around the turn of the 20th century at mountain locations chosen for the quality of the astronomical seeing. It is one of three great observatories conceived by George Ellery Hale (1868-1938), a pre-eminent figure in the development of the best possible equipment for advancing solar and stellar astrophysics.

Brief inventory 

• InfoTheme: Astronomy from the Renaissance to the mid-twentieth century
  Entity: 37
  Subentity: 1
  Version: 5
  Status: PUB
  Date: 2012-08-01 23:49:33
  Author(s): Gudrun Wolfschmidt, Clive Ruggles

The instruments at Mount Wilson include:

• The horizontal ‘Snow telescope’, built in 1903 by George W. Ritchey (1864-1945) and moved here in 1904.
• The 60 ft solar tower telescope (1904; the dome was not installed until 1914).
• The 150ft solar tower telescope (1910).
• The 60-inch (1.5m) silver-on-glass-mirror reflector, made by George W. Ritchey (1908).
• The Hooker 100-inch (2.5 m) equatorial reflector, also made Ritchey (1917).

History 

• InfoTheme: Astronomy from the Renaissance to the mid-twentieth century
  Entity: 37
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  Version: 2
  Status: PUB
  Date: 2012-05-16 11:06:07
  Author(s): Gudrun Wolfschmidt, Clive Ruggles

Hale, who was director of the Yerkes Observatory at Williams Bay, Wisconsin from 1895 until 1905, obtained a grant to found the Mount Wilson observatory from the Carnegie Institution of Washington (CIW). The mountain site provided near-ideal conditions for the world’s largest telescope, the 60-inch reflector, which went into service in December 1908. The even larger 100-inch reflector went into service in 1917.

Meanwhile, in 1904, the Snow telescope for solar observations was moved to Mount Wilson Observatory. It was not hugely successful, however, because the horizontal solar telescope was affected by air-currents from the warmed-up soil. For this reason, Hale had the idea of building a tower telescope, and the 60 ft solar tower telescope was duly constructed. In 1908 the larger 150 ft tower was built with the help of the Carnegie Foundation.

Further technological progress was made in many areas during the following decades, examples being the photomultiplier tube and the development of the modern magnetograph (using fibre-optics) in order to improve the solar images.

In 1984, the CIW was considering closing the Mount Wilson Observatory, but in 1985 it accepted the wishes of the Division of Astronomy and Astrophysics at the University of California at Los Angeles (UCLA) to use the towers for research in solar seismology, supported by the Mount Wilson Observatory Association (MWOA).

Cultural and symbolic dimension 

• InfoTheme: Astronomy from the Renaissance to the mid-twentieth century
  Entity: 37
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  Version: 1
  Status: PUB
  Date: 2011-08-22 11:08:01
  Author(s): Gudrun Wolfschmidt, Clive Ruggles

The importance of reflectors is directly connected to the rise of astrophysics. The new silvered-glass reflecting telescopes were essential for spectroscopy and photography because they had no chromatic aberration. The two glass reflectors at Mount Wilson (the 60-inch reflector and the Hooker telescope) represent the triumph of such reflectors at the beginning of the 20th century. The Hooker telescope remained the largest telescope in the world until 1949.

Mount Wilson saw the realisation by Harlow Shapley (1885–1972) that our solar system is not at or near the centre of our own galaxy (the Milky Way), arguably a 20th-century equivalent to the ‘Copernican revolution’); the realisation by Edwin Hubble (1889–1953) that globular clusters and spiral nebulae were in fact other galaxies outside the Milky Way; and the distance measurements, also by Hubble, that allowed him to present a linear distance-redshift relation which revealed that the Universe is expanding.

Mount Wilson was also of key importance in the development of solar astronomy. The solar tower, a special new architecture, was invented here, as were various new instruments for studying the solar atmosphere. Using the 60ft tower, Hale discovered in 1908 that sunspots have strong magnetic fields, several thousand times stronger than the Earth’s.

Management and use

Present use 

• InfoTheme: Astronomy from the Renaissance to the mid-twentieth century
  Entity: 37
  Subentity: 1
  Version: 1
  Status: PUB
  Date: 2011-08-22 11:08:01
  Author(s): Gudrun Wolfschmidt, Clive Ruggles

The observatory remains an active scientific institution, with both towers still being used for solar research.

Management, interpretation and outreach 

• InfoTheme: Astronomy from the Renaissance to the mid-twentieth century
  Entity: 37
  Subentity: 1
  Version: 1
  Status: PUB
  Date: 2011-08-22 11:08:01
  Author(s): Gudrun Wolfschmidt, Clive Ruggles

Since 1986, Mount Wilson Observatory has been operated under an agreement with the CIW by the Mount Wilson Institute (MWI), a non-profit corporation whose mission focuses on scientific research, historic preservation, astronomical education and public outreach.

The Friends of Mount Wilson Observatory (FOMWO) offer visits of the observatory to the public. Visitors are given the opportunity to view the Universe through the 60-inch telescope, the largest telescope in the world available exclusively to the public.