The north slope of Mount Wilson as seen from Angeles Crest Highway
|Elevation||5,713 ft (1,741 m) NAVD 88|
|Prominence||150 ft (50 m) |
|Parent range||San Gabriel Mountains|
|Topo map||USGS Mount Wilson|
Mount Wilson is a peak in the San Gabriel Mountains, located within the San Gabriel Mountains National Monument and Angeles National Forest in Los Angeles County, California. With only minor topographical prominence the peak is not naturally noticeable from a distance, although it is easily identifiable due to the large number of antennas near its summit. It is a subsidiary peak of nearby San Gabriel Peak.
It is the location of the Mount Wilson Observatory, which is an important astronomical facility in Southern California with historic 60-inch (1,524 mm) and 100-inch (2,540 mm) telescopes, and 60-foot (18.3 m) and 150-foot (45.7 m) solar towers. The newer CHARA Array, run by Georgia State University, is also sited there and does important interferometric stellar research.
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 south of the summit are far shorter leading to unobstructed views across the Los Angeles Basin, Orange County, the Inland Empire, and out to Ventura County, San Diego County and the Pacific Ocean. On most days Santa Catalina Island, California, some 65 miles south, is visible. On clear days, other Channel Islands visible include San Clemente Island at 95 miles, Santa Barbara Island at 76 miles, San Nicolas Island at 107 miles, Santa Cruz Island at 98 miles and San Miguel Island at 133 miles. At an elevation of 5,710 feet, the horizon on the ocean extends 92 miles.
Mount Wilson is also heavily utilized for relay broadcasting of radio and television for the Greater Los Angeles Area. The FM broadcasters include but are not limited to KRRL-FM 92.3, KCBS-FM 93.1, KTWV 94.7, KKLQ-FM 100.3, KIIS-FM 102.7, KOST-FM 103.5, and KBIG-FM 104.3.
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 lens grinder Alvan Clark, prepared an experiment with 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, 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," now the Mount Wilson Toll Road. Passage fare was 25¢ round trip for hikers (equivalent to $7 in 2018) and 50¢ for horseback.
In 1892, 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 and was impressed by the perfect conditions for which to set up the observatory, which would become the Mount Wilson Solar Observatory in 1904. In 1905 40 acres (160,000 m2) were leased for 99 years by the Carnegie Institution for Science in order to construct telescopes and construction began on a new Mt. Wilson Hotel. In 1908 a 60-inch (1524 mm) telescope was completed at the summit, and in 1910 the 150-foot (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. This concept is the basis of the Big Bang theory of cosmology.
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.
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 these, according to the FCC database, is the guyed mast built for KCBS-TV, now owned by Richland Towers, which stands at a height of 972 feet (296.3 m), built in 1986.
The following television stations transmit from Mount Wilson:
|Callsign||Virtual Channel||Transmit Channel||Affiliation|
In 1984 the Carnegie Institution for Science 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 was the largest optical interferometric array at the time. Ground was broken for the telescopes in 1999 and the facility became operational in 2001.