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A second of arc, arcsecond (abbreviated as arcsec), or arc second, denoted by the symbol ″, [2] is a unit of angular measurement equal to 1 / 60 of a minute of arc, 1 / 3600 of a degree, [1] 1 / 1 296 000 of a turn, and π / 648 000 (about 1 / 206 264.8 ) of a radian.
It is defined by taking the fixed numerical value of the speed of light in vacuum c to be 299 792 458 when expressed in the unit m s −1, where the second is defined in terms of ∆ν Cs." [1] 1 / 10 000 000 of the distance from the Earth's equator to the North Pole measured on the meridian arc through Paris. L kilogram: kg mass
Evolution of the SI base units [1]: 6 [5] [6]; Unit name Definition [n 1]; second: Prior: (1675) 1 / 86 400 of a day of 24 hours of 60 minutes of 60 seconds. TLB; Interim (1956): 1 / 31 556 925.9747 of the tropical year for 1900 January 0 at 12 hours ephemeris time.
A minute of arc, arcminute (arcmin), arc minute, or minute arc, denoted by the symbol ′, is a unit of angular measurement equal to 1 / 60 of one degree. [1] Since one degree is 1 / 360 of a turn, or complete rotation, one arcminute is 1 / 21 600 of a turn.
0°0′1″ The second of arc (or arcsecond, or just second) is 1 / 60 of a minute of arc and 1 / 3600 of a degree (n = 1,296,000). It is denoted by a double prime ( ″ ). For example, 3° 7′ 30″ is equal to 3 + 7 / 60 + 30 / 3600 degrees, or 3.125 degrees. The arcsecond is the angle used to measure a parsec ...
Angular resolution (arc seconds) Wavelength Type Site Year Global mm-VLBI Array (successor to the Coordinated Millimeter VLBI Array) 0.000012 (12 μas) radio (at 1.3 cm) very long baseline interferometry array of different radio telescopes: a range of locations on Earth and in space [8] 2002 - Very Large Telescope/PIONIER: 0.001 (1 mas)
JuJu Watkins went 4-of-11 on 3-point attempts en route to 30 points, and No. 4-ranked Southern California claimed the regular-season Big Ten Conference championship with an 80-67 defeat of second ...
In practical applications it is often small: for example the triangles of geodetic survey typically have a spherical excess much less than 1' of arc. [14] On the Earth the excess of an equilateral triangle with sides 21.3 km (and area 393 km 2) is approximately 1 arc second. There are many formulae for the excess.