- Minute of arc
A minute of arc, arcminute, or minute of angle (MOA), is a unit of angular measurement equal to one sixtieth (1⁄60) of one degree. In turn, a second of arc or arcsecond is one sixtieth (1⁄60) of one minute of arc. Since one degree is defined as one three hundred and sixtieth (1⁄360) of a rotation, 1 minute of arc is 1⁄21,600 of the same. It is used in those fields which require a unit for the expression of small angles, such as astronomy, navigation and marksmanship.
The number of square arcminutes in a complete sphere is
or approximately 148,510,660.498 square arcminutes.
Symbols and abbreviations
The standard symbol for marking the arcminute is the prime (′) (U+2032), though a single quote (') (U+0027) is commonly used where only ASCII characters are permitted. One arcminute is thus written 1′. It is also abbreviated as arcmin or amin or, less commonly, the prime with a circumflex over it ().
The standard symbol for the arcsecond is the double prime (″) (U+2033), though a double quote (") (U+0022) is commonly used where only ASCII characters are permitted. One arcsecond is thus written 1″. It is also abbreviated as arcsec or asec.
The sexagesimal system of angular measurement Unit Value Symbol Abbreviations In radians (approx.) Degree 1⁄360 circle ° deg 17.4532925 mrad Arcminute 1⁄60 degree ′ (prime) arcmin, amin, am, , MOA 290.8882087 µrad Arcsecond 1⁄60 arcminute ″ (double prime) arcsec, asec, as 4.8481368 µrad Milliarcsecond 1⁄1,000 arcsecond mas 4.8481368 nrad Microarcsecond 1 × 10−6 arcsecond μas 4.8481368 prad
In celestial navigation, seconds of arc are rarely used in calculations, the preference usually being for degrees, minutes and decimals of a minute, written for example as 42° 25′.32 or 42° 25′.322. This notation has been carried over into marine GPS receivers, which normally display latitude and longitude in the latter format by default.
The arcminute is commonly found in the firearms industry and literature, particularly concerning the accuracy of rifles, though the industry tends to refer to it as minute of angle. It is popular because 1 MOA subtends approximately one inch at 100 yards, a traditional distance on target ranges. A shooter can easily readjust their rifle scope by measuring the distance in inches the bullet hole is from the desired impact point and adjusting the scope that many MOA in the same direction. Most target scopes designed for long distances are adjustable in quarter (1⁄4) or eighth (1⁄8) MOA increments or clicks. One eighth MOA is equal to approximately an eighth of an inch at 100 yards or one inch at 800 yards.
Calculating the physical equivalent group size equal to one minute of arc can be done using the equation: equivalent group size = tan(MOA⁄60) × distance. In the example previously given and substituting 3,600 inches for 100 yards, 3,600 tan(1 MOA⁄60) inches = 1.047 inches.
In metric units 1 MOA at 100 meters = 2.908 centimeters.
Sometimes, a firearm's accuracy will be measured in MOA. This simply means that under ideal conditions, the gun with certain ammunition is capable of producing a group of shots whose center points (center-to-center) fit into a circle, the average diameter of circles in several groups can be subtended by that amount of arc. For example, a 1 MOA rifle should be capable, under ideal conditions, of shooting an average 1-inch groups at 100 yards. Some manufacturers such as Weatherby and Cooper offer actual guarantees of real-world MOA performance.
Rifle manufacturers and gun magazines often refer to this capability as sub-MOA, meaning it shoots under 1 MOA. This is typically a single group of 3 to 5 shots at 100 yards, or the average of several groups. If larger samples are taken (i.e., more shots per group) then group size typically increases.
For example mathematical statistical calculation yields the following accuracy for exactly the same rifle and ammunition combination (standard deviations of every shot from center is 1 MOA):
No of shots Size (′/MOA) 2 1.77 3 2.41 5 3.07 10 3.81 20 4.45 100 5.69
Minutes of angle (and its subunit, seconds of angle or SOA—equal to a sixtieth of a MOA) are also used in cartography and navigation. At sea level, one minute of angle (around the equator or a meridian) equals about 1.86 kilometres / 1.16 miles), approximately one nautical mile (approximately, because the Earth is slightly oblate); a second of angle is one sixtieth of this amount: about 30 meters or 100 feet.
Traditionally positions are given using degrees, minutes, and seconds of angles in two measurements: one for latitude, the angle north or south of the equator; and one for longitude, the angle east or west of the Prime Meridian. Using this method, any position on or above the Earth's reference ellipsoid can be precisely given. However, because of the somewhat clumsy base-60 nature of MOA and SOA, many people now prefer to give positions using degrees only, expressed in decimal form to an equal amount of precision. Degrees, given to three decimal places (1⁄1,000 of a degree), have about 1⁄4 the precision as degrees-minutes-seconds (1⁄3,600 of a degree), and so identify locations within about 120 meters or 400 feet.
Property cadastral surveying
Related to cartography, property boundary surveying using the metes and bounds system relies on fractions of a degree to describe property lines' angles in reference to cardinal directions. A boundary "mete" is described with a beginning reference point, the cardinal direction North or South followed by an angle less than 90 degrees and a second cardinal direction, and a linear distance. The boundary runs the specified linear distance from the beginning point, the direction of the distance being determined by rotating the first cardinal direction the specified angle toward the second cardinal direction. For example, North 65° 39′ 18″ West 85.69 feet would describe a line running from the starting point 85.69 feet in a direction 65° 39′ 18″ (or 65.655°) away from north toward the west.
The arcminute and arcsecond are also used in astronomy. Degrees (and therefore arcminutes) are used to measure declination, or angular distance north or south of the celestial equator. The arcsecond is also often used to describe parallax, due to very small parallax angles for stellar parallax, and tiny angular diameters (e.g., Venus varies between 10′′ and 60′′). The parallax, proper motion and angular diameter of a star may also be written in milliarcseconds (mas), or thousandths of an arcsecond. The parsec gets its name from "parallax second", for those arcseconds.
The ESA astrometric space probe Gaia will measure star positions to 20 microarcseconds (µas). There are about 1.3 quadrillion µas in a circle. As seen from Earth, one µas is about the size of a period at the end of a sentence in the Apollo mission manuals left on the moon.
Apart from the sun, the star with the largest angular diameter from Earth is R Doradus, a red supergiant with a diameter of 0.05 arcsecond. Because of the effects of atmospheric seeing, ground-based telescopes will smear the image of a star to an angular diameter of about 0.5 arcsecond; in poor seeing conditions this increases to 1.5 arcseconds or even more. The dwarf planet Pluto has proven difficult to resolve because its angular diameter is about 0.1 arcsecond. This is roughly equivalent to a (40 mm) ping-pong ball viewed at a distance of 50 miles (80 km).
Space telescopes are not affected by the Earth's atmosphere but are diffraction limited. For example, the Hubble space telescope can reach an angular size of stars down to about 0.1″. Techniques exist for improving seeing on the ground. Adaptive optics, for example, can produce images around 0.05 arcsecond on a 10 m class telescope.
For raster graphics, Apple Inc asserts that a display of approximately 300 ppi at a distance of 12 inches (305 mm) from one's eye, or 57 arcseconds per pixel is the maximum amount of detail that the human retina can perceive. Raymond Soneira, president of DisplayMate Technologies, however, stated that the resolution of the human retina is higher than claimed by Apple, working out to 477 ppi at 12 inches (305 mm) or 36 arcseconds per pixel.
The deviation from parallelism between two surfaces, for instance in optical engineering, is usually measured in arcminutes or arcsecond.
- ^ "CELESTIAL NAVIGATION COURSE". International Navigation School. http://www.learntonavigate.com/celestial.htm. Retrieved 4 November 2010. "It is a straight forward method [to obtain a position at sea] and requires no mathematical calculation beyond addition and subtraction of degrees and minutes and decimals of minutes"
- ^ "Astro Navigation Syllabus". http://www.kumquat-data.com/Astro%20Navigation%20Syllabus.htm. Retrieved 4 November 2010. "[Sextant errors] are sometimes [given] in seconds of arc, which will need to be converted to decimal minutes when you include them in your calculation."
- ^ "Shipmate GN30". Norinco. http://norinco.co.in/NCMS/index.php?option=com_content&task=view&id=53&Itemid=81. Retrieved 4 November 2010.
- ^ Wheeler, Robert E.. "Statistical notes on rifle group patterns". http://www.bobwheeler.com/guns/GroupStat.pdf. Retrieved 21 May 2009.
- ^ Bramwell, Denton (January 2009). "Group Therapy The Problem: How accurate is your rifle?". Varmint Hunter 69. http://www.longrangehunting.com/articles/accurate-rifle-groups-1.php. Retrieved 21 May 2009.
- ^ Some studies have shown a larger angular diameter for Betelgeuse. Various studies have produced figures of between 0.042 and 0.069 arcseconds for the star's diameter. The variability of Betelgeuse and difficulties in producing a precise reading for its angular diameter make any definitive figure conjectural.
- ^ NASA.gov Pluto Fact Sheet
- ^ Brandrick, Chris (June 8, 2010"iPhone 4's Retina Display Explained". PC World. http://www.pcworld.com/article/198201/iphone_4s_retina_display_explained.html. Retrieved June 18, 2010.).
- ^ Hachman, Mark (June 9, 2010"Analyst Challenges Apple's iPhone 4 'Retina Display' Claims". PC Magazine. http://www.pcmag.com/article2/0,2817,2364871,00.asp. Retrieved June 23, 2010.).
SI units Base units Derived units Accepted for use
See alsoBook:International System of Units · Category:SI base units
Wikimedia Foundation. 2010.