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Mount Wilson Toll Road

Altadena, CaliforniaFormer toll roads in CaliforniaHiking trails in CaliforniaHistory of Los Angeles County, CaliforniaHistory of Pasadena, California
Parks in Los Angeles County, CaliforniaSan Gabriel MountainsSan Gabriel Valley
Mt Wilson Tollhouse
Mt Wilson Tollhouse

The Mount Wilson Toll Road (1891–1936) is a historic roadway which ascended Mount Wilson via a vehicular passable road from the base of the foothills in Altadena. It was accessible from Pasadena via Santa Anita Avenue (nowadays the north-south portion of Altadena Drive) which drove right to the front porch of the toll house. The road is still accessible to non-motorized traffic (hikers, bicyclists, and horses) by way of Eaton Canyon (either from the Nature Center entrance, or an access gate on Pinecrest Drive, just off Altadena Drive in Altadena). Segments of it have been closed at various times due to landslides. A 2005 landslide destroyed 50 yards of the road, but it has since been rebuilt and reopened.Mount Wilson had always been active with human passage starting from the days of the local Native Americans. It was Benjamin Davis Wilson who established a proper trail to the summit of Mt. Wilson from Sierra Madre through the Little Santa Anita Canyon.

Excerpt from the Wikipedia article Mount Wilson Toll Road (License: CC BY-SA 3.0, Authors, Images).

Mount Wilson Toll Road
Mount Wilson Trail,

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Latitude Longitude
N 34.198333333333 ° E -118.05416666667 °
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Mount Wilson Trail

Mount Wilson Trail
91023
California, United States
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Mt Wilson Tollhouse
Mt Wilson Tollhouse
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Mount Wilson (California)
Mount Wilson (California)

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) aperture telescopes, and 60-foot (18.3 m) and 150-foot (45.7 m) tall 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, some 65 mi (105 km) south, is visible. On clear days, other Channel Islands visible include San Clemente Island at 95 mi (153 km), Santa Barbara Island at 76 mi (122 km), San Nicolas Island at 107 mi (172 km), Santa Cruz Island at 98 mi (158 km) and San Miguel Island at 133 mi (214 km). At an elevation of 5,710 ft (1,740 m), the horizon on the ocean extends 92 mi (148 km). Mount Wilson is also heavily utilized for relay broadcasting of radio and television for the Greater Los Angeles Area.

Mount Wilson Observatory
Mount Wilson Observatory

The Mount Wilson Observatory (MWO) is an astronomical observatory in Los Angeles County, California, United States. The MWO is located on Mount Wilson, a 5,710-foot (1,740-meter) peak in the San Gabriel Mountains near Pasadena, northeast of Los Angeles. The observatory contains two historically important telescopes: the 100-inch (2.5 m) Hooker telescope, which was the largest aperture telescope in the world from its completion in 1917 to 1949, and the 60-inch telescope which was the largest operational telescope in the world when it was completed in 1908. It also contains the Snow solar telescope completed in 1905, the 60 foot (18 m) solar tower completed in 1908, the 150 foot (46 m) solar tower completed in 1912, and the CHARA array, built by Georgia State University, which became fully operational in 2004 and was the largest optical interferometer in the world at its completion. Due to the inversion layer that traps warm air and smog over Los Angeles, Mount Wilson has steadier air than any other location in North America, making it ideal for astronomy and in particular for interferometry. The increasing light pollution due to the growth of greater Los Angeles has limited the ability of the observatory to engage in deep space astronomy, but it remains a productive center, with the CHARA array continuing important stellar research. The initial efforts to mount a telescope to Mount Wilson occurred in the 1880s by one of the founders of University of Southern California, Edward Falles Spence, but he died without finishing the funding effort. The observatory was conceived and founded by George Ellery Hale, who had previously built the 1 meter telescope at the Yerkes Observatory, then the world's largest telescope. The Mount Wilson Solar Observatory was first funded by the Carnegie Institution of Washington in 1904, leasing the land from the owners of the Mount Wilson Hotel in 1904. Among the conditions of the lease was that it allow public access.