Since 2019, defined as the length of the path travelled by light in a vacuum during a time interval of 1/299,792,458 of a second, where the second is defined by a hyperfine transition frequency of caesium.
Approximate diameter (comoving distance) of the visible universe[4]
1027
1 Rm
1.2 Rm
Lower bound of the (possibly infinite) radius of the universe, if it is a 3-sphere, according to one estimate using the WMAP data at 95% confidence[48] It equivalently implies that there are at minimum 21 particle horizon-sized volumes in the universe.
According to the laws of probability, the distance one must travel until one encounters a volume of space identical to our observable universe with conditions identical to our own.[49][50]
The quectometre (SI symbol: qm) is a unit of length in the metric system equal to 10−30metres.
To help compare different orders of magnitude, this section lists lengths shorter than 10−30m (1 qm).
1.6 × 10−5 quectometres (1.6 × 10−35 metres) – the Planck length (Measures of distance shorter than this do not make physical sense, according to current theories of physics.)
1 qm – 1 quectometre, the smallest named subdivision of the metre in the SI base unit of length, one nonillionth of a metre.[52]
The zeptometre (SI symbol: zm) is a unit of length in the metric system equal to 10−21metres.
To help compare different orders of magnitude, this section lists lengths between 10−21m and 10−20 m (1 zm and 10 zm).
The attometre (SI symbol: am) is a unit of length in the metric system equal to 10−18metres.
To help compare different orders of magnitude, this section lists lengths between 10−18m and 10−17 m (1 am and 10 am).
The femtometre (SI symbol: fm) is a unit of length in the metric system equal to 10−15metres.
In particle physics, this unit is sometimes called a fermi, also with abbreviation "fm". To help compare different orders of magnitude, this section lists lengths between 10−15metres and 10−14 metres (1 femtometre and 10 fm).
To help compare different orders of magnitude, this section lists lengths between 10−13m and 10−12 m (100 fm and 1 pm).
570 fm – typical distance from the atomic nucleus of the two innermost electrons (electrons in the 1s shell) in the uranium atom, the heaviest naturally-occurring atom
1 picometre
The picometre (SI symbol: pm) is a unit of length in the metric system equal to 10−12metres (1/1000000000000 m = 0.000000000001 m).
To help compare different orders of magnitude this section lists lengths between 10−12 and 10−11 m (1 pm and 10 pm).
The nanometre (SI symbol: nm) is a unit of length in the metric system equal to 10−9metres (1/1000000000 m = 0.000000001 m).
To help compare different orders of magnitude, this section lists lengths between 10−9 and 10−8 m (1 nm and 10 nm).
Comparison of sizes of semiconductor manufacturing process nodes with some microscopic objects and visible light wavelengths. At this scale, the width of a human hair is about 10 times that of the image.[62]
To help compare different orders of magnitude, this section lists lengths between 10−7 and 10−6m (100 nm and 1 μm).
100 nm – greatest particle size that can fit through a surgical mask[63]
300 nm – greatest particle size that can fit through a HEPA (high efficiency particulate air) filter (N100 removes up to 99.97% at 0.3 micrometres, N95 removes up to 95% at 0.3 micrometres)[citation needed]
700–1.4 μm – wavelength of near-infrared radiation
1 micrometre (or 1 micron)
The silk for a spider's web is 5–7 μm (0.00020–0.00028 in) wide
The micrometre (SI symbol: μm) is a unit of length in the metric system equal to 10−6metres (1/1000000 m = 0.000001 m).
To help compare different orders of magnitude, this section lists some items with lengths between 10−6 and 10−5 m (between 1 and 10 micrometres, or μm).
To help compare different orders of magnitude, this section lists lengths between 10−4m and 10−3 m (100 μm and 1 mm). The term myriometre (abbr. mom, equivalent to 100 micrometres; frequently confused with the myriametre, 10 kilometres)[77] is deprecated; the decimal metric prefix myrio-[78] is obsolete[79][80][81] and was not included among the prefixes when the International System of Units was introduced in 1960.
100 μm – 1/10 of a millimetre
100 μm – 0.00394 inches
100 μm – smallest distance that can be seen with the naked eye
100 μm – average diameter of a strand of human hair[24]
The millimetre (SI symbol: mm) is a unit of length in the metric system equal to 10−3metres (1/1000 m = 0.001 m).
To help compare different orders of magnitude, this section lists lengths between 10−3 m and 10−2 m (1 mm and 1 cm).
An average human fingernail is 1 cm (0.39 in) wide
The centimetre (SI symbol: cm) is a unit of length in the metric system equal to 10−2metres (1/100 m = 0.01 m).
To help compare different orders of magnitude, this section lists lengths between 10−2 m and 10−1 m (1 cm and 1 dm).
8.6 cm × 5.4 cm – dimensions of a standard credit card[citation needed]
9 cm – length of a speckled padloper, the smallest-known turtle
1 decimetre
An adult human foot is about 28 cm (11 in) long.
The decimetre (SI symbol: dm) is a unit of length in the metric system equal to 10−1metres (1/10 m = 0.1 m).
To help compare different orders of magnitude, this section lists lengths between 10 centimetres and 100 centimetres (10−1 metre and 1 metre).
Conversions
10 centimetres (abbreviated to 10 cm) is equal to:
1 decimetre (dm), a term not in common use (1 L = 1 dm3.)
10 cm = 1 dm – diameter of the human cervix upon entering the second stage of labour
11 cm = 1.1 dm – diameter of an average potato in the US
13 cm = 1.3 dm – body length of a Goliath birdeater
15 cm = 1.5 dm – approximate size of largest beetle species
19 cm = 1.9 dm – length of a banana
26.3 cm = 2.6 dm – length of average male human foot
29.98 cm = 2.998 dm – distance light in vacuum travels in one nanosecond
30 cm = 3.0 dm – maximum leg length of a Goliath birdeater
31 cm = 3.1 dm – wingspan of largest butterfly species Ornithoptera alexandrae
46 cm = 4.6 dm – length of an average domestic cat
50 to 65 cm = 5–6.5 dm – a coati's tail
66 cm = 6.6 dm – length of the longest pine cones (produced by the sugar pine[93])
Astronomical
84 cm = 8.4 dm – approximate diameter of 2008 TS26, a meteoroid
1 metre
Leonardo da Vinci drew the Vitruvian Man within a square of side 1.83 m (6 ft 0 in) and a circle about 1.2 m (3 ft 11 in) in radius
To help compare different orders of magnitude, this section lists lengths between one metre and ten metres.
Light, in vacuum, travels 1 metre in 1⁄299,792,458, or 3.3356409519815E-9 of a second.
1.63 m – (5 feet 4 inches) (or 64 inches) – height of average U.S. female human as of 2002[update] (source: U.S. Centers for Disease Control and Prevention (CDC))
1.75 m – (5 feet 8 inches) – height of average U.S. male human as of 2002[update] (source: U.S. CDC as per female above)
2.5 m – height of a sunflower
2.72 m – (8 feet 11 inches) – tallest-known human (Robert Wadlow)[30]
3.63 m – the record wingspan for living birds (a wandering albatross)
5.5 m – height of a Baluchitherium, the largest land mammal ever lived
6.5 m – wingspan of Argentavis, the largest flying bird known
7.4 m – wingspan of Pelagornis, the bird with longest wingspan ever.[99]
7.5 m – approximate length of the human gastrointestinal tract
Astronomical
3–6 m – approximate diameter of 2003 SQ222, a meteoroid
4.1 m – diameter of 2008 TC3, a small asteroid that flew into the Earth's atmosphere on 7 October 2008[100]
1 decametre
A blue whale has been measured as 33 m (108 ft) long; this drawing compares its length to that of a human diver and a dolphin.
The decametre (SI symbol: dam) is a unit of length in the metric system equal to 10 metres (101 m).
To help compare different orders of magnitude, this section lists lengths between 10 and 100 metres.
Conversions
10 metres (very rarely termed a decametre which is abbreviated as dam) is equal to:
13 metres – length of a giant squid and colossal squid, the largest living invertebrates
15 metres – approximate distance the tropical circles of latitude are moving towards the equator and the polar circles are moving towards the poles each year due to a natural, gradual decrease in the Earth's axial tilt
18 metres – height of a Sauroposeidon, the tallest-known dinosaur
20 metres – length of a Leedsichthys, the largest-known fish to have lived
21 metres – height of High Force waterfall in England
33 metres – length of a blue whale,[103] the largest animal on earth, living or extinct, in terms of mass
39 metres – length of a Supersaurus, the longest-known dinosaur and longest vertebrate[104]
55 metres – length of a bootlace worm, the longest-known animal[105]
66 metres - highest possible sea level rise due to a complete melting of all ice on Earth
83 metres – height of a Western hemlock
Astronomical
30 metres – diameter of 1998 KY26, a rapidly spinning meteoroid
30.8568 metres – 1 femtoparsec
32 metres – approximate diameter of 2008 HJ, a small meteoroid
1 hectometre
The Great Pyramid of Giza is 138.8 m (455 ft) high.British driver location sign and location marker post on the M27 in Hampshire. The location marker posts are installed at 100-metre intervals.[106]
The hectometre (SI symbol: hm) is a unit of length in the metric system equal to 100 metres (102 m).
To compare different orders of magnitude this section lists lengths between 100 metres and 1,000 metres (1 kilometre).
Conversions
100 metres (sometimes termed a hectometre) is equal to:
328 feet
one side of a 1 hectare square
a fifth of a modern li, a Chinese unit of measurement
the approximate distance travelled by light in 300 nanoseconds
Human-defined scales and structures
100 metres – wavelength of the highest medium wave radio frequency, 3 MHz
100 metres – spacing of location marker posts on British motorways
138.8 metres – height of the Great Pyramid of Giza (Pyramid of Cheops)
139 metres – height of the world's tallest roller coaster, Kingda Ka[107]
169 metres - height of the Washington Monument
187 metres – shortest wavelength of the broadcast radio AM band, 1600 kHz
192 metres - height of the Gateway Arch
202 metres – length of the Széchenyi Chain Bridge connecting Buda and Pest
270 metres - length of the Titanic
318 metres – height of The New York Times Building
318.9 metres – height of the Chrysler Building
328 metres – height of Auckland's Sky Tower, the tallest free-standing structure in the Southern Hemisphere[when?]
330 metres – height of the Eiffel Tower (including antenna)[108]
341 metres – height of the world's tallest bridge, the Millau Viaduct[when?]
390 metres – height of the Empire State Building
400–800 metres – heights of the world's tallest skyscrapers of the past 80 years[when?]
458 metres – length of the Knock Nevis, the world's largest supertanker
The kilometre (SI symbol: km) is a unit of length in the metric system equal to 1000metres (103 m).
To help compare different orders of magnitude, this section lists lengths between 1 kilometre and 10 kilometres (103 and 104metres).
5.072 km – height of Tanggula Mountain Pass, below highest peak in the Tanggula Mountains, highest railway pass in the world as of August 2005[update][118]
To help compare different orders of magnitude, this section lists lengths between 10 and 100 kilometres (104 to 105metres). The myriametre[123] (sometimes also spelled myriometre; 10,000 metres) is a deprecated unit name; the decimal metric prefix myria-[78] (sometimes also written as myrio-[124][125][126]) is obsolete[79][80][81] and was not included among the prefixes when the International System of Units was introduced in 1960.
Conversions
10 kilometres is equal to:
Distance marker on the Rhine: 36 (XXXVI) myriametres from Basel. The stated distance is 360 km (220 mi); the comma is the decimal separator in Germany .
66 km – diameter of Naiad, the innermost of Neptune's moons
100 kilometres
The Suez Canal is 163 km (101 mi) long.
A length of 100 kilometres (about 62 miles), as a rough amount, is relatively common in measurements on Earth and for some astronomical objects.
It is the altitude at which the FAI defines spaceflight to begin.
To help compare orders of magnitude, this section lists lengths between 100 and 1,000 kilometres (105 and 106metres).
Conversions
A distance of 100 kilometres is equal to about 62 miles (or 62.13711922 miles).
Human-defined scales and structures
100 km – the Karman line: the internationally-recognized boundary of outer space
105 km – distance from Giridih to Bokaro
109 km – length of High Speed 1 between London and the Channel Tunnel[135]
Small planets, the Moon and dwarf planets in the Solar System have diameters from one to ten million metres. Top row: Mars (left), Mercury (right); bottom row: Moon (left), Pluto (center), and Haumea (right), to scale.
The megametre (SI symbol: Mm) is a unit of length in the metric system equal to 1000000metres (106 m).
To help compare different orders of magnitude, this section lists lengths starting at 106m (1 Mm or 1,000 km).
Planets from Venus up to Uranus have diameters from ten to one hundred million metres. Top row: Uranus (left), Neptune (right); middle row: Earth (left), Sirius B (center), and Venus (right), to scale
To help compare different orders of magnitude, this section lists lengths starting at 107metres (10 megametres or 10,000 kilometres).
The Earth-Moon orbit, Saturn, OGLE-TR-122b, Jupiter, and other objects, to scale. Click on image for detailed view and links to other length scales.Scale model at megametres of the main Solar System bodies.
To help compare different orders of magnitude, this section lists lengths starting at 108metres (100 megametres or 100,000 kilometres or 62,150 miles).
986 Mm – Diameter of HD 100546 b's surrounding disk
1 gigametre
13 things in the gigametre groupUpper part: Gamma Orionis, Algol B, the Sun (centre), and other objects to scale
; lower part: their darker mirror images (artist's interpretation).
The gigametre (SI symbol: Gm) is a unit of length in the metric system equal to 1000000000metres (109 m).
To help compare different distances this section lists lengths starting at 109metres (1 gigametre (Gm) or 1 billion metres).
5.0 Gm – Closest approach of Comet Halley to Earth, happened on 10 April 837
5.0 Gm – (proposed) Size of the arms of the giant triangle shaped Michelson interferometer of the Laser Interferometer Space Antenna (LISA) planned to start observations sometime in the 2030s.
Rigel and Aldebaran (top left and right) compared to smaller stars, the Sun (very small dot in lower middle, with orbit of Mercury as yellow ellipse) and transparent sphere with radius of one light-minute.
From largest to smallest: Jupiter's orbit, red supergiant star Betelgeuse, Mars' orbit, Earth's orbit, star R Doradus, and orbits of Venus, Mercury. Inside R Doradus's depiction are the blue supergiant star Rigel and red giant star Aldebaran. The faint yellow glow around the Sun represents one light-minute. Click image to see more details and links to their scales.
To help compare distances at different orders of magnitude this section lists lengths starting at 1011metres (100 gigametre or 100 million kilometres or 0.7 astronomical units).
109 Gm (0.7 au) Distance between Venus and the Sun
149.6 Gm (93.0 million mi; 1.0 au) – Distance between the Earth and the Sun – the original definition of the astronomical unit
965 Gm (6.4 au) – Maximum distance between the Earth and Jupiter
1 terametre
8 things in the terametre groupComparison of size of the Kuiper belt (large faint torus) with the star VY Canis Majoris (within Saturn's orbit), Betelgeuse (inside Jupiter's orbit) and R Doradus (small central red sphere) together with the orbits of Neptune and Uranus, to scale. The yellow ellipses represent the orbits of each planet and the dwarf planet Pluto.
The terametre (SI symbol: Tm) is a unit of length in the metric system equal to 1000000000000metres (1012 m).
To help compare different distances, this section lists lengths starting at 1012m (1 Tm or 1 billion km or 6.7 astronomical units).
1.83 Tm – 12.2 au – Diameter of HR 5171 A, the largest-known yellow hypergiant star although the latest research suggests it is a red hypergiant with a diameter about 2.1 Tm (14 au)[161][162]
7.5 Tm – 50.1 au – Outer radius of the Kuiper Belt
10 terametres
Sedna's orbit (left) is longer than 100 Tm, but other lengths are between 10 and 100 Tm: Comet Hale-Bopp's orbit (lower, faint orange); one light-day (yellow spherical shell with yellow Vernal point arrow as radius); the heliosphere's termination shock (blue shell); and other arrows show positions of Voyager 1 (red) and Pioneer 10 (green). Click on image for larger view and links to other scales.
To help compare different distances this section lists lengths starting at 1013m (10 Tm or 10 billion km or 67 astronomical units).
10 Tm – 67 AU – Diameter of a hypothetical quasi-star
11.1 Tm – 74.2 AU – Distance that Voyager 1 began detecting returning particles from termination shock
Largest circle with yellow arrow indicates one light-year from Sun; Cat's Eye Nebula on left and Barnard 68 in middle are depicted in front of Comet 1910 A1's orbit. Click image for larger view, details and links to other scales.
7.5 Pm – 50,000 AU – Possible outer boundary of Oort cloud (other estimates are 75,000 to 125,000 or even 189,000 AU (1.18, 2, and 3 light-years, respectively))
9.5 Pm – 63,241.1 AU – One light-year, the distance traveled by light in one year
9.9 Pm – 66,000 AU – Aphelion distance of the C/1999 F1 (Catalina)
10 petametres
Objects with size order of magnitude 1e16m: Ten light-years (94.6 Pm) radius circle with yellow Vernal Point arrow; Bubble Nebula (NGC 7635), left; Dumbbell Nebula (NGC 6853), right; one light-year shell lower right with the smaller Cat's Eye Nebula (NGC_6543) and Barnard 68 adjacent.1e16m lengths: Ten light-years (94.6 Pm) yellow shell; Sirius below right; BL Ceti below left; Proxima and Alpha Centauri upper right; light-year shell with Comet 1910 A1's orbit inside top right
To help compare different distances this section lists lengths starting at 1016m (10 Pm or 66,800 AU, 1.06 light-years).
15 Pm – 1.59 light-years – Possible outer radius of Oort cloud
Lengths with order of magnitude 1e17m: yellow Vernal Point arrow traces hundred light-year radius circle with smaller ten light-year circle at right; globular cluster Messier 5 in background; 12 light-year radius Orion Nebula middle right; 50-light-year-wide view of the Carina Nebula bottom left; Pleiades cluster and Bubble nebula with similar diameters each around 10 light-years bottom right; grey arrows show distances from Sun to stars Aldebaran (65 light-years) and Vega (25 light-years).
To help compare different distances this section lists lengths between 1017m (100 Pm or 11 light-years) and 1018 m (106 light-years).
260 Pm – 27 light-years – Distance to Chara, a star approximately as bright as the Sun. Its faintness gives an idea how the Sun would appear when viewed from this distance.
Lengths with order of magnitude 1e18m: thousand light-year radius circle with yellow arrow and 100 light-year circle at right with globular cluster Messier 5 within and Carina Nebula in front; globular cluster Omega Centauri to left of both; part of the 1,400-light-year-wide Tarantula Nebula fills the background.
The exametre (SI symbol: Em) is a unit of length in the metric system equal to 1018metres. To help compare different distances this section lists lengths between 1018m (1 Em or 105.7 light-years) and 1019 m (10 Em or 1,057 light-years).
240 Em – 25,000 light-years – Distance to the Canis Major Dwarf Galaxy
260 Em – 28,000 light-years – Distance to the center of the Galaxy
400 Em – 48,000 light years – Diameter of the Fireworks Galaxy
830 Em – 88,000 light-years – Distance to the Sagittarius Dwarf Elliptical Galaxy
1 zettametre
The zettametre (SI symbol: Zm) is a unit of length in the metric system equal to 1021metres.[52]
To help compare different orders of magnitude, this section lists distances starting at 1 Zm (1021m or 110,000 light-years).
9.5 Ym – 996 million light-years – Diameter of the Eridanus Supervoid
10 yottametres
The universe within one billion light-years of Earth
To help compare different orders of magnitude, this section lists distances starting at 10 Ym (1025m or 1.1 billion light-years). At this scale, expansion of the universe becomes significant. Distance of these objects are derived from their measured redshifts, which depends on the cosmological models used.
13 Ym – 1.37 billion light-years – Length of the South Pole Wall
13 Ym – 1.38 billion light-years – Length of the Sloan Great Wall
To help compare different orders of magnitude, this section lists distances starting at 100 Ym (1026m or 11 billion light-years). At this scale, expansion of the universe becomes significant. Distance of these objects are derived from their measured redshifts, which depend on the cosmological models used.
260 Ym – 27.4 billion light-years – Diameter of the observable universe (double LTD)
440 Ym – 46 billion light-years – Radius of the universe measured as a comoving distance
590 Ym – 62 billion light-years – Cosmological event horizon: the largest comoving distance from which light will ever reach us (the observer) at any time in the future
886.48 Ym – 93.7 billion light-years – The diameter of the observable universe (twice the particle horizon); however, there might be unobserved distances that are even greater.
To help compare different orders of magnitude, this section lists distances starting at 1 Rm (1027m or 110 billion light-years). At this scale, expansion of the universe becomes significant. Distance of these objects are derived from their measured redshifts, which depend on the cosmological models used.
>1 Rm - >105.7 billion light-years – Size of universe beyond the cosmic light horizon, depending on its curvature; if the curvature is zero (i.e. the universe is spatially flat), the value can be infinite (see Shape of the universe) as previously mentioned
≈101010120Light-years – the possible size of the universe after cosmological inflation
↑ 2.02.1The exact category (asteroid, dwarf planet, or planet) to which particular Solar System objects belong, has been subject to some revision since the discovery of extrasolar planets and trans-Neptunian objects
↑10115 is 1 followed by 115 zeroes, or a googol multiplied by a quadrillion. 1010115 is 1 followed by a quadrillion googol zeroes. 101010122is 1 followed by 1010122 (a googolplex10 sextillion) zeroes.
↑But not cloud or high-level fog droplets; droplet size increases with altitude. For a contradictory study indicating larger drop sizes even in ground fog, see Eldridge, Ralph G. (October 1961). "A Few Fog Drop-Size Distributions". Journal of Meteorology18 (5): 671–6. doi:10.1175/1520-0469(1961)018<0671:AFFDSD>2.0.CO;2. Bibcode: 1961JAtS...18..671E.
↑Abbott, B. P. (2016). "Observation of Gravitational Waves from a Binary Black Hole Merger". Physical Review Letters116 (6): 061102. doi:10.1103/PhysRevLett.116.061102. PMID26918975. Bibcode: 2016PhRvL.116f1102A. "On 14 September 2015 at 09:50:45 UTC the two detectors of the Laser Interferometer Gravitational-Wave Observatory simultaneously observed a transient gravitational-wave signal. The signal sweeps upwards in frequency from 35 to 250 Hz with a peak gravitational-wave strain of 1.0×10−21.".
↑ 4.04.14.24.3Cite error: Invalid <ref> tag; no text was provided for refs named Burgess_and_Quevedo
↑Langevin, Dominique (2008). "Chapter 10: DNA-Surfactant/Lipid Complexes at Liquid Interfaces". DNA Interactions with Polymers and Surfactants. Hoboken, NJ: John Wiley & Sons, Inc.. p. 265. doi:10.1002/9780470286364.ch10. ISBN978-0-470-25818-7. "DNA has 20 elementary charges per helical turn over the corresponding length of 3.4nm"
↑Page, Don N.; Allende Prieto, C.; Garzon, F.; Wang, H.; Liu, C.; Deng, L. (18 October 2006). "Susskind's challenge to the Hartle Hawking no-boundary proposal and possible resolutions". Journal of Cosmology and Astro-Particle Physics2007 (1): 004. doi:10.1088/1475-7516/2007/01/004. Bibcode: 2007JCAP...01..004P.
↑Annis, Patty J. October 1991. Kansas State University. Fine Particle POLLUTION. Figure 1. (tobacco smoke: 10 to 1000 nm; virus particles: 3 to 50 nm; bacteria: 30 to 30000 nm; cooking oil smoke: 30 to 30000 nm; wood smoke: 7 to 3000 nm)
↑Eninger, Robert M.; Hogan, Christopher J.; Biswas, Pratim; Adhikari, Atin; Reponen, Tiina; Grinshpun, Sergey A. (2009). "Electrospray versus Nebulization for Aerosolization and Filter Testing with Bacteriophage Particles". Aerosol Science and Technology43 (4): 298–304. doi:10.1080/02786820802626355. Bibcode: 2009AerST..43..298E.
↑ 79.079.1Comité International des Poids et Mesures (1935) (in fr), Procès-Verbaux des Séances, 17 (2 ed.), Paris, France: Gauthier-Villars, imprimeur-libraire du Bureau des Longitudes, de l'École Polytechnique, p. 76
↑ 80.080.1Metric System of Weights and Measures – Guidelines for Use. US: Director of the National Bureau of Standards. 1 June 1975. Federal Register FR Doc.75-15798 (18 June 1975). "Accordingly, the following units and terms listed in the table of metric units in section 2 of the act of 28 July 1866, that legalized the metric system of weights and measures in the United States, are no longer accepted for use in the United States: myriameter, stere, millier or tonneau, quintal, myriagram, kilo (for kilogram)."
↑ 81.081.1Barbrow, Louis E., ed (1 October 1976). "Appendix 7". Weights and Measures Standards of the United States, a brief history. Derived from a prior work by Louis A. Fisher (1905). US: US Department of Commerce, National Bureau of Standards. p. 33. NBS Special Publication 447; NIST SP 447; 003-003-01654-3. https://www.nist.gov/pml/wmd/pubs/upload/sp-447-2.pdf. Retrieved 12 October 2015.
↑Akeson, Rachel; Beichman, Charles; Kervella, Pierre; Fomalont, Edward; Benedict, G. Fritz (2021). "Precision Millimeter Astrometry of the α Centauri AB System". The Astronomical Journal162 (1): 14. doi:10.3847/1538-3881/abfaff. Bibcode: 2021AJ....162...14A.
↑Liebert, James; Young, Patrick A.; Arnett, David; Holberg, J. B.; Williams, Kurtis A. (2005). "The Age and Progenitor Mass of Sirius B". The Astrophysical Journal630 (1): L69–L72. doi:10.1086/462419. Bibcode: 2005ApJ...630L..69L.
↑Baines, Ellyn K.; Armstrong, J. Thomas; Schmitt, Henrique R.; Zavala, R. T.; Benson, James A.; Hutter, Donald J.; Tycner, Christopher; Belle, Gerard T. van (2017). "Fundamental Parameters of 87 Stars from the Navy Precision Optical Interferometer". The Astronomical Journal155: 30. doi:10.3847/1538-3881/aa9d8b.
↑Moravveji, Ehsan; Guinan, Edward F; Shultz, Matt; Williamson, Michael H; Moya, Andres (4 January 2012). "Asteroseismology of the Nearby SN-II Progenitor: Rigel Part I. The MOST High Precision Photometry and Radial Velocity Monitoring". Astrophysical Journal747 (2): 2. doi:10.1088/0004-637X/747/2/108. Bibcode: 2012ApJ...747..108M.
↑Richichi, A.; Roccatagliata, V.; Shultz, Matt; Williamson, Michael H.; Moya, Andres (2005). "Aldebaran's angular diameter: How well do we know it?". Astronomy & Astrophysics433 (1): 305–312. doi:10.1051/0004-6361:20041765. Bibcode: 2005A&A...433..305R. They derived an angular diameter of 20.58±0.03 milliarcsec, which given a distance of 65 light-years yields a diameter of 61 million km.
↑Chesneau, O.; Dessart, L.; Mourard, D.; Bério, Ph.; Buil, Ch.; Bonneau, D.; Borges Fernandes, M.; Clausse, J. M. et al. (2010). "Time, spatial, and spectral resolution of the H α line-formation region of Deneb and Rigel with the VEGA/CHARA interferometer". Astronomy and Astrophysics521: A5. doi:10.1051/0004-6361/201014509. Bibcode: 2010A&A...521A...5C.
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↑diameter=sin(65 arcminutes)*1270 light-years=24; where "65.00 × 60.0 (arcmin)" sourced from Revised NGC Data for NGC 1976
↑distance × sin( diameter_angle ), using distance of 5kpc (15.8 ± 1.1 kly) and angle 36.3', = 172 ± 12.5 ly.
↑van de Ven, G.; van den Bosch, R. C. E.; Verolme, E. K.; de Zeeuw, P. T. (2006). "The dynamical distance and intrinsic structure of the globular cluster ω Centauri". Astronomy and Astrophysics445 (2): 513–543. doi:10.1051/0004-6361:20053061. Bibcode: 2006A&A...445..513V. "best-fit dynamical distance D=4.8±0.3 kpc ... consistent with the canonical value 5.0±0.2 kpc obtained by photometric methods".
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