Calais Observatory | |
Location | Meridian Park, North and Lincoln Streets, Calais, Maine |
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Coordinates | 45°11′5.15″N67°16′50.74″W / 45.1847639°N 67.2807611°W |
Area | 0.5 acres (0.20 ha) |
Built | 1857 |
NRHP reference No. | 12001069 [1] |
Added to NRHP | December 19, 2012 |
The Calais Observatory is a pair of granite fixtures in Meridian Park in Calais, Maine. The two stones were used for mounting scientific equipment used in a variety of astronomical observations, principally for the accurate calculation by the United States Coast Survey of Calais's longitude with respect to meridians in Cambridge, Massachusetts, and Greenwich, England. [2] The site was listed on the National Register of Historic Places in 2012, [1] and is part of the National Oceanic and Atmospheric Administration's Heritage Trail program. [3] At the time of its longitude determination in 1866 with respect to the Greenwich Meridian, it was arguably one of the most precisely located places in the United States. [4]
The Calais Observatory site is located on a granite knob in Meridian Park, on the grounds of the former Calais Academy, at the corner of North and Lincoln Streets. The surviving elements of the observatory are two granite fixtures, along with flat pads chiseled out of the bedrock, and several drill holes. The site was known to be sheltered by a nominally permanent structure in both 1857 and 1866, but had by 1895 lost whatever shelter it had. [4]
The shorter of the two granite fixtures is called the transit stone; it stands about 3 feet 6 inches (1.07 m) tall, 2 feet 7 inches (0.79 m) wide, and 2 feet (0.61 m) deep, and is oriented so that its sides align with the cardinal compass points. The top of the stone is incised with two channels, for aligning an astronomical transit and to accommodate the device's crank. The taller fixture is known as the clock stone, and about 1 foot (0.30 m) square at its base, tapering to 8 inches (0.20 m) at its top 8 feet (2.4 m) off the ground. It is located about 2 feet (0.61 m) west of the transit stone, and has a number of grooves and holes carved into it. The exact function of this stone is not documented, but its features are consistent with the mounting of a Hardy pendulum clock of the type used by the survey crews. The clock would have been removed from its case and mounted on this stone; the transit stone would not have accommodated the clock. In addition to the two stone fixtures, there are rough square pads carved out of the bedrock about 4.5 feet (1.4 m) north and south of the transit stone, and there are two holes drilled into the bedrock, 20 feet (6.1 m) and 36 feet (11 m) west of the transit stone; the function of these features is not known. [4]
The accurate calculation of a location's longitude was long a critical element of maritime navigation. After abortive previous attempts, the United States Coast Survey began work in the 1830s to produce a consistent set of nautical charts for the nation's coastline. The Harvard College Observatory in Cambridge, Massachusetts was chosen in 1847 as the site of the prime reference point for the longitude determinations, and survey work extended from there. The advent of telegraphy made possible the simultaneous exchange of time signals between distant locations to determine the difference in time between observed passage of an object in the sky (often Polaris) at different locations. With sufficiently accurate time pieces, longitude could be determined with significant precision. [4]
On August 31, 1857, a survey crew installed equipment at this site, and at Thomas Hill in Bangor, Maine, and its longitude was established with respect to Cambridge, and to facilitate the determination of longitude at the observatory in Fredericton, New Brunswick. With the advent of transatlantic communications cables (first laid in 1858), the idea of coordinating the longitude with respect to the Greenwich Meridian became feasible. Although the first cable failed soon after operation, a second cable was laid 1866, connecting Foilhommerum on Valentia Island in Ireland with Heart's Content, Newfoundland. The longitudes of the Irish and Newfoundland stations were determined with respect to Greenwich in the summer of 1866, and in December of that year, observations were conducted at Calais to determine its longitude with respect to Greenwich. This allowed the entire United States longitudinal framework to be coordinated with that of Great Britain. The observatory was used once more, in 1895, to determine with greater precision its longitude with respect to Cambridge. [4]
In 1998 the transit stone was found to have been pushed over and set against a nearby tree. The city returned it to its original 1857 location, and a surveyor with the National Geodetic Survey (one of the successors to the U.S. Coast Survey) in 2004 confirmed the stone's location to be within 2 inches (5.1 cm) of its 1866 observed location. [4]
Greenwich Mean Time (GMT) is the local mean time at the Royal Observatory in Greenwich, London, counted from midnight. At different times in the past, it has been calculated in different ways, including being calculated from noon; as a consequence, it cannot be used to specify a particular time unless a context is given. The term GMT is also used as one of the names for the time zone UTC+00:00 and, in UK law, is the basis for civil time in the United Kingdom.
Longitude is a geographic coordinate that specifies the east–west position of a point on the surface of the Earth, or another celestial body. It is an angular measurement, usually expressed in degrees and denoted by the Greek letter lambda (λ). Meridians are imaginary semicircular lines running from pole to pole that connect points with the same longitude. The prime meridian defines 0° longitude; by convention the International Reference Meridian for the Earth passes near the Royal Observatory in Greenwich, south-east London on the island of Great Britain. Positive longitudes are east of the prime meridian, and negative ones are west.
Nevil Maskelyne was the fifth British Astronomer Royal. He held the office from 1765 to 1811. He was the first person to scientifically measure the mass of the planet Earth. He created The Nautical Almanac, in full the British Nautical Almanac and Astronomical Ephemeris for the Meridian of the Royal Observatory at Greenwich using Tobias Mayer's corrections for Euler's Lunar Theory tables.
The United States Naval Observatory (USNO) is a scientific and military facility that produces geopositioning, navigation and timekeeping data for the United States Navy and the United States Department of Defense. Established in 1830 as the Depot of Charts and Instruments, it is one of the oldest scientific agencies in the United States, and remains the country's leading authority for astronomical and timing data for all purposes.
The Royal Observatory, Greenwich is an observatory situated on a hill in Greenwich Park in south east London, overlooking the River Thames to the north. It played a major role in the history of astronomy and navigation, and because the Prime Meridian passed through it, it gave its name to Greenwich Mean Time, the precursor to today's Coordinated Universal Time (UTC). The ROG has the IAU observatory code of 000, the first in the list. ROG, the National Maritime Museum, the Queen's House and the clipper ship Cutty Sark are collectively designated Royal Museums Greenwich.
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A prime meridian is an arbitrarily-chosen meridian in a geographic coordinate system at which longitude is defined to be 0°. Together, a prime meridian and its anti-meridian form a great circle. This great circle divides a spheroid, like Earth, into two hemispheres: the Eastern Hemisphere and the Western Hemisphere. For Earth's prime meridian, various conventions have been used or advocated in different regions throughout history. Earth's current international standard prime meridian is the IERS Reference Meridian. It is derived, but differs slightly, from the Greenwich Meridian, the previous standard.
John Pond FRS was a renowned English astronomer who became the sixth Astronomer Royal, serving from 1811 to 1835.
The historic prime meridian or Greenwich meridian is a geographical reference line that passes through the Royal Observatory, Greenwich, in London, England. The modern IERS Reference Meridian widely used today is based on the Greenwich meridian, but differs slightly from it. This prime meridian was first established by Sir George Airy in 1851, and by 1884, over two-thirds of all ships and tonnage used it as the reference meridian on their charts and maps. In October of that year, at the behest of US President Chester A. Arthur, 41 delegates from 25 nations met in Washington, D.C., United States, for the International Meridian Conference. This conference selected the meridian passing through Greenwich as the world standard prime meridian due to its popularity. However, France abstained from the vote, and French maps continued to use the Paris meridian for several decades. In the 18th century, London lexicographer Malachy Postlethwayt published his African maps showing the "Meridian of London" intersecting the Equator a few degrees west of the later meridian and Accra, Ghana.
In geography and geodesy, a meridian is the locus connecting points of equal longitude, which is the angle east or west of a given prime meridian. In other words, it is a line of longitude. The position of a point along the meridian is given by that longitude and its latitude, measured in angular degrees north or south of the Equator. On a Mercator projection or on a Gall-Peters projection, each meridian is perpendicular to all circles of latitude. A meridian is half of a great circle on Earth's surface. The length of a meridian on a modern ellipsoid model of Earth has been estimated as 20,003.93 km (12,429.87 mi).
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