Mount Wilson (California)
The north slope of Mount Wilson as seen from Angeles Crest Highway
|Elevation||5,713 ft (1,741 m) NAVD 88|
|Prominence||5,260 ft (1,600 m)|
|Los Angeles County, California, U.S.|
|Range||San Gabriel Mountains|
|Topo map||USGS Mount Wilson|
Mount Wilson is one of the better-known peaks in the San Gabriel Mountains, part of the Angeles National Forest in Los Angeles County, California. It is the location of the Mount Wilson Observatory and has become the astronomical center of Southern California with 60-inch (1,524 mm) and 100-inch (2,540 mm) telescopes, and 60-foot-tall (18.3 m) and 150-foot-tall (45.7 m) solar towers. The summit is at 5,710 feet (1,740 m). While not the tallest peak in its vicinity, it is high enough in elevation that snow can sometimes interrupt astronomical activities on the mountain. All of the mountains west of the summit are far shorter leading to unobstructed views all the way to Pacific Ocean. On an extremely clear day Santa Catalina Island, California, some 70 miles southwest, is visible, with the horizon stretching another 30 miles beyond that.
The native inhabitants of the San Gabriels probably belonged to various tribes of the Tongva people who lived in the low-lying valleys. Granite outcroppings along the Angeles Crest show signs of meal preparations with metate pots ground into rock surfaces.
The first recorded exploration of the mountain was performed by Benjamin Davis Wilson also known as "Don Benito". Wilson, who was the grandfather of George S. Patton, was the owner of Rancho San Pascual in about 1852 and ran a winery at his home, "Lake Vineyard", which was in the area of today's San Marino. Wilson hoped to find a suitable wood for his casks but was disappointed by the poor quality of trees on the mountain. He built a trail, following an established Indian route, which became known as the Mount Wilson Trail. In turn Wilson's trail became the predecessor of the Mount Wilson Toll Road. He was surprised to find line shacks at the summit, probably left by Spaniards who were known to track down destructive grizzly bears. He built a three-room cabin along the trail called "Halfway House." Despite Wilson's inability to find adequate wood, the hike became a popular pastime for locals who would make a weekend trip to the summit. These hikers built signal fires on the summit to let people below know that the party had arrived safely.
In 1889 Professor William Pickering of Harvard University along with Alvan P. Clark, famous lens grinder, prepared an experiment with a 4-and-13-inch (102 and 330 mm) telescopes at Mount Wilson. University students would operate the telescopes for nighttime viewing, but more often than not they would log in "bad weather, no visibility" and head to town to relieve their boredom. The small observatory was abandoned with plans to build a larger one at a later date.
In 1891 Prof. Thaddeus S. C. Lowe incorporated the Pasadena & Mount Wilson Railroad with the plan of building a scenic mountain railroad to the summit of Mt. Wilson. At the same time land and easement disputes between camp owners Steils and Strain were going on over the public and private use of the Mount Wilson Trail. The courts ruled that the trail was a public thoroughfare and that any blockading would be illegal. At the foot of the mountain, a local contractor Thomas Banbury built a 10-mile (15 km) roadway to be named "The New Mount Wilson Trail," aka "The Mount Wilson Toll Road." Passage fare was 25¢ round trip for hikers and 50¢ for horseback.
In 1892 Prof. Charles William Eliot, president of Harvard University, planned to have two 40-inch (102 cm) lenses shipped from Alvan Clark & Sons in Corning, New York to the newly named Mount Harvard, directly adjacent to Mt. Wilson. The money was to be put up by Mr. Spence of the University of Southern California. Walter Raymond, of Raymond & Whitcomb Travel Agency, Boston, and owner of the Raymond Hotel, Pasadena, offered to pay for rail from New York. Lowe offered to take the lenses up via his yet-to-be-built Mt. Wilson Railway. Spence died suddenly and left no word of the money for the project. The lenses ended up at Yerkes Observatory in Wisconsin, and Lowe's railway ended up going to Oak Mountain (Mount Lowe).
In 1903 George Ellery Hale visited Mt. Wilson only to become enthused by the perfect conditions for which to set up an observatory, which would become the Mount Wilson Observatory. In 1905 40 acres (160,000 m2) were leased for 99 years by the Carnegie Institute for telescopes, and construction began on a new Mt. Wilson Hotel. In 1908 a 60-inch (1524 mm) telescope was installed at the summit, and in 1910 the 150-foot-tall (46 m) Solar Tower was erected. In 1913 the hotel burned down and was replaced by a second hotel that lasted until its demolition in 1966. The Toll Road opened to automobiles in 1912 and lasted until 1936.
In 1919, American astronomer Edwin Hubble arrived at Mt. Wilson and, throughout the 1920s, made many astronomical discoveries using the Hooker Telescope. Among his contributions are the observational proof that many nebulous objects are actually galaxies beyond our own Milky Way galaxy, the classification of galaxies according to the Hubble sequence, and the development of Hubble's law relating a galaxy's observed red shift to its distance away. These contributions led to an understanding that the universe is not static, but expanding.
In 1926 Albert Abraham Michelson made what was the most precise calculation of the speed of light at the time by measuring the round-trip travel time of light between Mount Wilson and Mount San Antonio 22 miles (35 km) away.
Mount Wilson Electronics Reservation
The first television antenna on Mount Wilson was erected in 1947 for pioneer station KTLA Channel 5. At about the same time, the first FM station broadcast from Mount Wilson, which was the old KFI-FM on 105.9 FM (signed off in 1950). The mountain became so popular as a site for transmitters that, in 1963, the Metromedia company bought 720 acres (2.9 km2) from the Mount Wilson Hotel Company. Metromedia built Skyline Park, which consisted of a pavilion, a children's zoo and landscaped walks. The park closed in 1976 after operating at a loss for almost a decade. The property is now the home of numerous transmitters serving the Los Angeles metropolitan area and includes radio, television and microwave relay facilities. The tallest of which, according to the FCC database, is the guyed mast, formerly home of KCBS-TV, now operated by Richland Towers, which stands at a height of 972 feet (296.3 m), built in 1986.
Television on Mount Wilson
The following television stations transmit from Mount Wilson:
|Callsign||Virtual Channel||Physical Channel||Affiliation|
- Most of the stations in the Los Angeles DMA not listed in the above table transmit from Mt. Harvard, an adjacent peak. These stations are (listed by virtual channel followed by physical channel): KSCI channel 18/18 (Multilingual Ind.), KWHY channel 22/42 (MundoFox), KHTV-CD channel 27/27 (HSN), KPXN channel 30/38 (ION), KVEA channel 52/39 (Telemundo), KRCA channel 62/35 (Estrella TV), KBEH channel 63/24 (CNN Latino), and analog KSFV-CA channel 6 (Spanish Religious).
In 1984 the Carnegie Institute began the process of shutting down the observatories on Mount Wilson, opting to concentrate on newer sites in Chile. In 1986 the Mt. Wilson Institute was formed and plans to reopen the observatories were made so that by 2000 all the telescopes were back in operation.
Construction began in 1996 for six 1-meter telescopes by the Center for High Angular Resolution Astronomy at Georgia State University. This is the largest optical interferometric array ever built. Ground was broken for the telescopes in 1999 and the facility became operational in 2001.
- Sierra Madre, California – at the base of Mt. Wilson, has a trailhead which leads up the mountain.
- "Wilson Peak". NGS data sheet. U.S. National Geodetic Survey. Retrieved 2009-08-17.
- "Mount Wilson, California". Peakbagger.com. Retrieved 2013-02-20.
- "History of Mt. Wilson". oldradio.com. Retrieved 2010-12-04.
- "The Story of Mt. Wilson, California Part 3 – Broadcasters Invade". oldradio.com. Retrieved 2010-12-04.
- "Antenna Structure Registration 1012836". fccinfo.com. Retrieved 2010-12-04.
- "Antenna Structure Registration Search Results Within 15 Kilometers of 34-13-55.0 and 118-04-18.0". fccinfo.com. Retrieved 2010-12-04.
- Center for High Angular Resolution Astronomy Web site (http://www.chara.gsu.edu/CHARA/), Retrieved 8-4-2011.
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