Orders of magnitude (length)

Last updated

Graphical overview of sizes Scales of size.jpg
Graphical overview of sizes

The following are examples of orders of magnitude for different lengths.

Contents

Overview

ScaleRange (m)UnitExample items
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Subatomic 0 Gravitational singularity
10−3610−33 P Fixed value (not a range). Quantum foam, string
10−1810−15 am proton, neutron, pion
Atomic to cellular 10−15 10−12 fm Atomic nucleus
10−12 10−9 pm Wavelength of gamma rays and X-rays, hydrogen atom
10−9 10−6 nm DNA helix, virus, wavelength of optical spectrum, transistors used in CPUs
Cellular to human 10−6 10−3 μm Bacterium, fog water droplet, human hair's diameter [note 1]
10−3 1 mm Mosquito, golf ball, domestic cat, violin, football
Human to astronomical 1103 m Piano, human, automobile, sperm whale, football field, Eiffel Tower
103 106 km Mount Everest, length of Panama Canal and Trans-Siberian Railway, larger asteroid
Astronomical 106 109 Mm The Moon, Earth, one light-second
109 1012 Gm Sun, one light-minute, Earth's orbit
1012 1015 Tm Orbits of outer planets, Solar System
1015 1018 Pm A light-year, the distance to Proxima Centauri
1018 1021 Em Galactic arm
1021 1024 Zm Milky Way, distance to Andromeda Galaxy
1024 1027 Ym Huge-LQG, Hercules–Corona Borealis Great Wall, Observable universe

Detailed list

To help compare different orders of magnitude, the following list describes various lengths between  metres and metres.

Subatomic scale

Factor (m)MultipleValueItem
000 Singularity
10−351 Planck length 0.0000162 qm  Planck length; typical scale of hypothetical loop quantum gravity or size of a hypothetical string and of branes; according to string theory, lengths smaller than this do not make any physical sense. [1] Quantum foam is thought to exist at this scale.
10−24 1 yoctometre (ym)142 ymEffective cross section radius of 1 MeV neutrinos [2]
10−21 1 zeptometre (zm) Preons, hypothetical particles proposed as subcomponents of quarks and leptons; the upper bound for the width of a cosmic string in string theory
7 zmEffective cross section radius of high-energy neutrinos [3]
310 zm De Broglie wavelength of protons at the Large Hadron Collider (4 TeV as of 2012)
10−18 1 attometre (am)Upper limit for the size of quarks and electrons
Sensitivity of the LIGO detector for gravitational waves [4]
Upper bound of the typical size range for "fundamental strings" [1]
10−17 10 am Range of the weak force
10−16 100 am 850 amApproximate proton radius [5]

Atomic to cellular scale

Factor (m)MultipleValueItem
10−15 1 femtometre (fm, fermi)1 fmApproximate limit of the gluon-mediated color force between quarks [6] [7]
1.5 fmEffective cross section radius of an 11 MeV proton [8]
2.81794 fm Classical electron radius [9]
3 fmApproximate limit of the meson-mediated nuclear binding force [6] [7]
1.75 to 15 fmDiameter range of the atomic nucleus [1] [10]
10−12 1 picometre (pm)0.75 to 0.8225 pmLongest wavelength of gamma rays
1 pmDistance between atomic nuclei in a white dwarf
2.4 pm Compton wavelength of electron
5 pmWavelength of shortest X-rays
10−11 10 pm
28 pmRadius of helium atom
53 pm Bohr radius (radius of a hydrogen atom)
10−10 100 pm 100 pm1 ångström (also covalent radius of sulfur atom [11] )
154 pmLength of a typical covalent bond (C–C)
280 pmAverage size of the water molecule (actual lengths may vary)
500 pmWidth of protein α helix
10−9 1 nanometre (nm)1 nmDiameter of a carbon nanotube [12] Diameter of smallest transistor gate (as of 2016) [13]
2 nmDiameter of the DNA helix [14]
2.5 nmSmallest microprocessor transistor gate oxide thickness (as of January 2007)[ citation needed ]
3.4 nmLength of a DNA turn (10 bp) [15]
6–10 nmThickness of cell membrane
10−8 10 nm 10 nmThickness of cell wall in Gram-negative bacteria [ citation needed ]
10 nmAs of 2016, the 10 nanometre was the smallest semiconductor device fabrication node [16]
40 nmExtreme ultraviolet wavelength
50 nm Flying height of the head of a hard disk [17]
10−7 100 nm 121.6 nmWavelength of the Lyman-alpha line [18]
120 nmTypical diameter of the human immunodeficiency virus (HIV) [19]
400–700 nmApproximate wavelength range of visible light [20]

Cellular to human scale

Factor (m)MultipleValueItem
10−6 1 micrometre (μm)

(also called 1 micron)

1–4 μmTypical length of a bacterium [21]
4 μmTypical diameter of spider silk [22]
7 μmTypical size of a red blood cell [23]
10−5 10 μm 10 μmTypical size of a fog, mist, or cloud water droplet
10 μmWidth of transistors in the Intel 4004, the world's first commercial microprocessor
12 μmWidth of acrylic fiber
17-181 μmWidth range of human hair [24]
10−4 100 μm 340 μmSize of a pixel on a 17-inch monitor with a resolution of 1024×768
560 μmThickness of the central area of a human cornea [25]
750 μmMaximum diameter of Thiomargarita namibiensis , the largest bacterium ever discovered (as of 2010)
10−3 1 millimetre (mm)~5 mmLength of an average flea is 1–10 mm (usually <5 mm) [26]
2.54 mmOne-tenth inch; distance between pins in DIP (dual-inline-package) electronic components
5.70 mmDiameter of the projectile in 5.56×45mm NATO ammunition
10−2 1 centimetre (cm)20 mmApproximate width of an adult human finger
54 mm × 86 mmDimensions of a credit card, according to the ISO/IEC 7810 ID-1 standard
73–75 mmDiameter of a baseball, according to Major League Baseball guidelines [27]
10−1 1 decimetre (dm)120 mmDiameter of a compact disc
660 mmLength of the longest pine cones, produced by the sugar pine [28]
900 mmAverage length of a rapier, a fencing sword [29]

Human to astronomical scale

Factor (m)MultipleValueItem
1 (100) 1 metre (m)1 m (exactly)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.
2.72 mHeight of Robert Wadlow, tallest-known human. [30]
8.38 mLength of a London bus (AEC Routemaster)
101 1 decametre (dam)33 mLength of the longest-known blue whale [31]
52 mHeight of the Niagara Falls [32]
93.47 mHeight of the Statue of Liberty
102 1 hectometre (hm)105 mLength of a typical football field
137 m (147 m)Height (present and original) of the Great Pyramid of Giza
300 mHeight of the Eiffel Tower, one of the famous monuments of Paris
979 mHeight of the Salto Angel, the world's highest free-falling waterfall (Venezuela)
103 1 kilometre (km)2.3 kmLength of the Three Gorges Dam, the largest dam in the world [33] [34]
3.1 kmNarrowest width of the Strait of Messina, separating Italy and Sicily
8.848 kmHeight of Mount Everest, the highest mountain on Earth
104 10 km 10.9 kmDepth of the Challenger Deep in the Mariana Trench, the deepest-known point on Earth's surface
27 kmCircumference of the Large Hadron Collider, as of May 2010 the largest and highest energy particle accelerator
42.195 kmLength of a marathon
105 100 km 100 kmThe distance the IAU considers to be the limit to space, called the Karman line
163 kmLength of the Suez Canal, connecting the Mediterranean Sea to the Red Sea
491 kmLength of the Pyrenees, the mountain range separating Spain and France
974.6 kmGreatest diameter of the dwarf planet Ceres. [35]
106 1 megametre (Mm)2.38 MmDiameter of dwarf planet Pluto, formerly the smallest planet category [note 2] in the Solar System
3.48 MmDiameter of the Moon
5.2 MmTypical distance covered by the winner of the 24 Hours of Le Mans automobile endurance race
6.371 MmAverage radius of Earth
6.378 MmEquatorial radius of Earth
6.4 MmLength of the Great Wall of China
6.6 MmApproximate length of the two longest rivers, the Nile and the Amazon
7.821 MmLength of the Trans-Canada Highway
9.288 MmLength of the Trans-Siberian Railway, longest in the world

Astronomical scale

Factor (m)MultipleValueItem
107 10 Mm 12.756 MmEquatorial diameter of Earth
20.004 MmLength of a meridian on Earth (distance between Earth's poles along the surface) [36]
40.075 MmLength of Earth's equator
108 100 Mm 142.984 MmDiameter of Jupiter
299.792 MmDistance traveled by light in vacuum in one second (a light-second, exactly 299,792,458 m by definition of the speed of light)
384.4 Mm Moon's orbital distance from Earth
109 1 gigametre (Gm)1.39 GmDiameter of the Sun
5.15 GmGreatest mileage ever recorded by a car (3.2 million miles by a 1966 Volvo P-1800S) [37]
1010 10 Gm 18 GmApproximately one light-minute
1011 100 Gm 150 Gm1 astronomical unit (au); mean distance between Earth and Sun
1012 1 terametre (Tm)1.3 TmOptical diameter of Betelgeuse
1.4 TmOrbital distance of Saturn from Sun
2 TmEstimated optical diameter of VY Canis Majoris, one of the largest-known stars
5.9 TmOrbital distance of Pluto from the Sun
~ 7.5 TmOuter boundary of the Kuiper belt
1013 10 Tm Diameter of the Solar System as a whole [1]
21.49 TmDistance of the Voyager 1 spacecraft from Sun (as of Oct 2018), the farthest man-made object so far [38]
62.03 TmEstimated radius of the event horizon of the supermassive black hole in NGC 4889, the largest-known black hole to date
1014 100 Tm 180 TmSize of the debris disk around the star 51 Pegasi [39]
200 TmTotal length of DNA molecules in all cells of an adult human body[ citation needed ]
1015 1 petametre (Pm)~7.5 PmSupposed outer boundary of the Oort cloud (~ 50,000 au)
9.461 PmDistance traveled by light in vacuum in one year; at its current speed, Voyager 1 would need 17,500 years to travel this distance
1016 10 Pm 30.857 Pm1 parsec
39.9 PmDistance to nearest star (Proxima Centauri)
41.3 PmAs of March 2013, distance to nearest discovered extrasolar planet (Alpha Centauri Bc)
1017 100 Pm 193 PmAs of October 2010, distance to nearest discovered extrasolar planet with potential to support life as presently defined by science (Gliese 581 d)
615 PmApproximate radius of humanity's radio bubble, caused by high-power TV broadcasts leaking through the atmosphere into outer space
1018 1 exametre (Em)1.9 EmDistance to nearby solar twin (HIP 56948), a star with properties virtually identical to the Sun [40]
1019 10 Em 9.46 EmAverage thickness of Milky Way Galaxy [41] (1,000 to 3,000 ly by 21 cm observations [42] )
1020 100 Em 113.5 EmThickness of Milky Way Galaxy's gaseous disk [43]
1021 1 zettametre (Zm)
1.54 ZmDistance to SN 1987A, the most recent naked eye supernova
1.62 ZmDistance to the Large Magellanic Cloud (a dwarf galaxy orbiting the Milky Way)
1.66 ZmDistance to the Small Magellanic Cloud (another dwarf galaxy orbiting the Milky Way)
1.9 ZmDiameter of galactic disk of Milky Way Galaxy [44] [45] [46] [47]
6.15 ZmDiameter of the low surface brightness disc halo of the giant spiral galaxy Malin 1
1022 10 Zm 13.25 ZmRadius of the diffuse stellar halo of IC 1101, one of the largest-known galaxies
24 ZmDistance to Andromeda Galaxy
30.857 Zm1 megaparsec
50 ZmDiameter of Local Group of galaxies
1023 100 Zm 300–600 ZmDistance to Virgo cluster of galaxies
1024 1 yottametre (Ym)2.19 YmDiameter of the Local Supercluster and the largest voids and filaments
2.8 Ym End of Greatness
~5 YmDiameter of the Horologium Supercluster [48]
9.461 YmDiameter of the Pisces–Cetus Supercluster Complex, the supercluster complex which includes Earth
1025 10 Ym 13 YmLength of the Sloan Great Wall, a giant wall of galaxies (galactic filament) [49]
30.857 Ym1 gigaparsec
37.84 YmLength of the Huge-LQG, a group of 73 quasars
1026 100 Ym 95 YmEstimated light travel distance to certain quasars. Length of the Hercules–Corona Borealis Great Wall, a colossal wall of galaxies, the largest and the most massive structure in the observable universe as of 2014
127 YmEstimated light travel distance to GN-z11, the most distant object ever observed
870 YmApproximate diameter (comoving distance) of the visible universe [1]
1027 1 Rm 1.2 RmLower 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 [50] It equivalently implies that there are at minimum 21 particle horizon-sized volumes in the universe.
[note 3] m mAccording 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. [51] [52]
m mMinimal size of universe after cosmological inflation, implied by one resolution of the No-Boundary Proposal [53]

1 quectometre and less

The quectometre (SI symbol: qm) is a unit of length in the metric system equal to 1030  metres . To help compare different orders of magnitude, this section lists lengths shorter than 10−30 m (1 qm).

1 rontometre

The rontometre (SI symbol: rm) is a unit of length in the metric system equal to 1027  metres .

10 rontometres

1 yoctometre

The yoctometre (SI symbol: ym) is a unit of length in the metric system equal to 1024  metres .

1 zeptometre

The zeptometre (SI symbol: zm) is a unit of length in the metric system equal to 1021  metres . To help compare different orders of magnitude, this section lists lengths between 10−21 m and 10−20 m (1 zm and 10 zm).

10 zeptometres

To help compare different orders of magnitude, this section lists lengths between 10−20 m and 10−19 m (10 zm and 100 zm).

100 zeptometres

To help compare different orders of magnitude, this section lists lengths between 10−19 m and 10−18 m (100 zm and 1 am).

1 attometre

The attometre (SI symbol: am) is a unit of length in the metric system equal to 1018  metres . To help compare different orders of magnitude, this section lists lengths between 10−18 m and 10−17 m (1 am and 10 am).

10 attometres

To help compare different orders of magnitude, this section lists lengths between 10−17 m and 10−16 m (10 am and 100 am).

100 attometres

To help compare different orders of magnitude, this section lists lengths between 10−16 m and 10−15 m (100 am and 1 fm).

1 femtometre (or 1 fermi)

The femtometre (SI symbol: fm) is a unit of length in the metric system equal to 1015  metres . 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 10−15 metres and 10−14 metres (1 femtometre and 10 fm).

10 femtometres

To help compare different orders of magnitude, this section lists lengths between 10−14 m and 10−13 m (10 fm and 100 fm).

100 femtometres

To help compare different orders of magnitude, this section lists lengths between 10−13 m and 10−12 m (100 fm and 1 pm).

1 picometre

The picometre (SI symbol: pm) is a unit of length in the metric system equal to 1012  metres (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).

10 picometres

To help compare different orders of magnitude this section lists lengths between 10−11 and 10−10 m (10 pm and 100 pm).

100 picometres

To help compare different orders of magnitude this section lists lengths between 10−10 and 10−9 m (100 pm and 1 nm; 1  Å and 10 Å).

1 nanometre

The nanometre (SI symbol: nm) is a unit of length in the metric system equal to 109  metres (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).

10 nanometres

To help compare different orders of magnitude this section lists lengths between 10−8 and 10−7 m (10 nm and 100 nm).

100 nanometres

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. Comparison semiconductor process nodes.svg
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.

To help compare different orders of magnitude, this section lists lengths between 10−7 and 10−6 m (100 nm and 1  μm).

1 micrometre (or 1 micron)

The silk for a spider's web is 5-7 mm (0.00020-0.00028 in) wide Loxoceles reclusa iconized thread.png
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 106  metres (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).

10 micrometres

Fog particles are around 10-50 mm (0.00039-0.00197 in) long. FogParticlesHighSpeed.jpg
Fog particles are around 10–50 μm (0.00039–0.00197 in) long.

To help compare different orders of magnitude, this section lists lengths between 10−5 m and 10−4 m (10 μm and 100 μm).

100 micrometres

A paramecium is around 300 mm (0.012 in) long. Paramecium.jpg
A paramecium is around 300 μm (0.012 in) long.

To help compare different orders of magnitude, this section lists lengths between 10−4 m 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) [79] is deprecated; the decimal metric prefix myrio- [80] is obsolete [81] [82] [83] and was not included among the prefixes when the International System of Units was introduced in 1960.

1 millimetre

An average red ant is about 5 mm (0.20 in) long. Fire ants 01.jpg
An average red ant is about 5 mm (0.20 in) long.

The millimetre (SI symbol: mm) is a unit of length in the metric system equal to 103  metres (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).

1 centimetre

An average human fingernail is 1 cm (0.39 in) wide Fingernail label (enwiki).jpg
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 102  metres (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).

1 decimetre

An adult human foot is about 28 cm (11 in) long. Foot on white background.jpg
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 101  metres (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:

Wavelengths

Human-defined scales and structures

Nature

Astronomical

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 Da Vinci Vitruve Luc Viatour.jpg
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 1299,792,458, or 3.3356409519815E-9 of a second.

Conversions

1 metre is:

Human-defined scales and structures

Sports

Nature

Astronomical

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. Image-Blue Whale and Hector Dolphine Colored.jpg
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:

Human-defined scales and structures

Sports

Nature

Astronomical

1 hectometre

The Great Pyramid of Giza is 138.8 m (455 ft) high. Cheops pyramid 01.jpg
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. M27 DLS.JPG
British driver location sign and location marker post on the M27 in Hampshire. The location marker posts are installed at 100-metre intervals.

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:

Human-defined scales and structures

Sports

Nature

Astronomical

1 kilometre

Mount Fuji is 3.776 kilometres (2.346 mi) high. Fuji Kawaguchi 357.JPG
Mount Fuji is 3.776 kilometres (2.346 mi) high.

The kilometre (SI symbol: km) is a unit of length in the metric system equal to 1000  metres (103 m). To help compare different orders of magnitude, this section lists lengths between 1 kilometre and 10  kilometres (103 and 104 metres).

Conversions

1 kilometre (unit symbol km) is equal to:

Human-defined scales and structures

Geographical

Astronomical

10 kilometres

The Strait of Gibraltar is 13 km (8.1 mi) wide. Strait of Gibraltar 5.53940W 35.97279N.jpg
The Strait of Gibraltar is 13 km (8.1 mi) wide.

To help compare different orders of magnitude, this section lists lengths between 10 and 100 kilometres (104 to 105 metres). The myriametre [125] (sometimes also spelled myriometre; 10,000 metres) is a deprecated unit name; the decimal metric prefix myria- [80] (sometimes also written as myrio- [126] [127] [128] ) is obsolete [81] [82] [83] 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. Myriameterstein36RudesheimRhein.JPG
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.

Sports

Human-defined scales and structures

Geographical

Astronomical

100 kilometres

The Suez Canal is 163 km (101 mi) long. Suez canal 30.55N 32.28E.jpg
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 106 metres).

Conversions

A distance of 100 kilometres is equal to about 62 miles (or 62.13711922 miles).

Human-defined scales and structures

Geographical

Astronomical

1 megametre

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. 1e6m comparison Mars Mercury Moon Pluto Haumea - no transparency.png
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 1000000  metres (106 m). To help compare different orders of magnitude, this section lists lengths starting at 106 m (1 Mm or 1,000 km).

Conversions

1 megametre is equal to:

Human-defined scales and structures

Sports

Geographical

Astronomical

10 megametres

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 1e7m comparison Uranus Neptune Sirius B Earth Venus.png
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 107 metres (10 megametres or 10,000 kilometres).

Conversions

10 megametres (10 Mm) is

Human-defined scales and structures

Geographical

Astronomical

100 megametres

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. 1e8m comparison Saturn Jupiter OGLE-TR-122b with Uranus Neptune Sirius B Earth Venus no transparency.png
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. Scale model of Solar System 10 billion to 1.svg
Scale model at megametres of the main Solar System bodies.

To help compare different orders of magnitude, this section lists lengths starting at 108 metres (100 megametres or 100,000 kilometres or 62,150 miles).

1 gigametre

13 things in the gigametre group Gigameter group.png
13 things in the gigametre group
Upper part: Gamma Orionis, Algol B, the Sun (centre), and other objects to scale 1e9m comparison Gamma Orionis, Algol B, the Sun, and smaller - antialiased no transparency.png
Upper 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 1000000000  metres (109 m). To help compare different distances this section lists lengths starting at 109 metres (1 gigametre (Gm) or 1 billion metres).

10 gigametres

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. 1e10m comparison Rigel, Aldebaran, and smaller - antialiased no transparency.png
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.

To help compare different distances this section lists lengths starting at 1010 metres (10 gigametres (Gm) or 10 million kilometres, or 0.07 astronomical units).

100 gigametres

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. 1e11m comparison R Doradus and Betelgeuse, and smaller - antialiased no transparency.png
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 1011 metres (100 gigametre or 100 million kilometres or 0.7 astronomical units).

1 terametre

8 things in the terametre group Terameter group.png
8 things in the terametre group
Comparison 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. 1e12m comparison Kuiper belt and smaller.png
Comparison 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 1000000000000  metres (1012 m). To help compare different distances, this section lists lengths starting at 1012 m (1 Tm or 1 billion km or 6.7 astronomical units).

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. 1e13m comparison Hale Bopp and smaller - HQ no transparency.png
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 1013 m (10 Tm or 10 billion km or 67 astronomical units).

100 terametres

The largest yellow sphere indicates one light month distance from the Sun. Click the image for larger view, more details and links to other scales. 1e14m comparison light day week and month.png
The largest yellow sphere indicates one light month distance from the Sun. Click the image for larger view, more details and links to other scales.

To help compare different distances this section lists lengths starting at 1014 m (100 Tm or 100 billion km or 670 astronomical units).

1 petametre

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. 1e15m comparison cat's eye nebula barnard 68 one light year.png
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.

The petametre (SI symbol: Pm) is a unit of length in the metric system equal to 1015  metres. To help compare different distances this section lists lengths starting at 1015 m (1 Pm or 1 trillion km or 6685 astronomical units (AU) or 0.11 light-years).

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 comparison ten light years bubble nebula.png
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 1e16m comparison 10 light years sirius.png
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 1016 m (10 Pm or 66,800 AU, 1.06 light-years).

100 petametres

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). 1e17m comparison 100 light years nebula clusters.png
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 1017 m (100 Pm or 11 light-years) and 1018 m (106 light-years).

1 exametre

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. 1e18m comparison 1000 light years nebula clusters.png
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 1018 metres. To help compare different distances this section lists lengths between 1018  m (1  Em or 105.7 light-years) and 1019 m (10 Em or 1,057 light-years).

10 exametres

To help compare different orders of magnitude, this section lists distances starting at 10 Em (1019 m or 1,100 light-years).

100 exametres

To help compare different orders of magnitude, this section lists distances starting at 100 Em (1020 m or 11,000 light-years).

1 zettametre

The zettametre (SI symbol: Zm) is a unit of length in the metric system equal to 1021 metres. [54] To help compare different orders of magnitude, this section lists distances starting at 1  Zm (1021  m or 110,000 light-years).

10 zettametres

To help compare different orders of magnitude, this section lists distances starting at 10 Zm (1022 m or 1.1 million light-years).

100 zettametres

To help compare different orders of magnitude, this section lists distances starting at 100 Zm (1023 m or 11 million light-years).

1 yottametre

The yottametre (SI symbol: Ym) is a unit of length in the metric system equal to 1024  metres. [54]

To help compare different orders of magnitude, this section lists distances starting at 1 Ym (1024 m or 105.702 million light-years).

10 yottametres

The universe within one billion light-years of Earth Superclusters atlasoftheuniverse.gif
The universe within one billion light-years of Earth

To help compare different orders of magnitude, this section lists distances starting at 10 Ym (1025 m 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.

100 yottametres

To help compare different orders of magnitude, this section lists distances starting at 100 Ym (1026 m 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.

1 ronnametre

The ronnametre (SI symbol: Rm) is a unit of length in the metric system equal to 1027  metres. [54]

To help compare different orders of magnitude, this section lists distances starting at 1 Rm (1027 m 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.

See also

Notes

  1. The diameter of human hair ranges from 17 to 181 μm Ley, Brian (1999). Elert, Glenn (ed.). "Diameter of a human hair". The Physics Factbook. Retrieved 8 December 2018.
  2. 1 2 The 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
  3. 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 googolplex 10 sextillion) zeroes.
  4. 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 Meteorology. 18 (5): 671–6. Bibcode:1961JAtS...18..671E. doi: 10.1175/1520-0469(1961)018<0671:AFFDSD>2.0.CO;2 .

Related Research Articles

<span class="mw-page-title-main">Astronomical unit</span> Mean distance between Earth and the Sun

The astronomical unit is a unit of length defined to be exactly equal to 149,597,870,700 m. Historically, the astronomical unit was originally conceived as the average Earth-Sun distance, before its modern redefinition in 2012.

Length is a measure of distance. In the International System of Quantities, length is a quantity with dimension distance. In most systems of measurement a base unit for length is chosen, from which all other units are derived. In the International System of Units (SI) system the base unit for length is the metre.

<span class="mw-page-title-main">Metre</span> SI unit of length

The metre is the base unit of length in the International System of Units (SI). Since 2019, the metre has been defined as the length of the path travelled by light in vacuum during a time interval of 1/299792458 of a second, where the second is defined by a hyperfine transition frequency of caesium.

<span class="mw-page-title-main">Micrometre</span> Unit of length; one millionth of a metre

The micrometre as used by the International Bureau of Weights and Measures; SI symbol: μm) or micrometer, also commonly known by the non-SI term micron, is a unit of length in the International System of Units (SI) equalling 1×10−6 metre ; that is, one millionth of a metre.

<span class="mw-page-title-main">Wavelength</span> Distance over which a waves shape repeats

In physics and mathematics, wavelength or spatial period of a wave or periodic function is the distance over which the wave's shape repeats. In other words, it is the distance between consecutive corresponding points of the same phase on the wave, such as two adjacent crests, troughs, or zero crossings. Wavelength is a characteristic of both traveling waves and standing waves, as well as other spatial wave patterns. The inverse of the wavelength is called the spatial frequency. Wavelength is commonly designated by the Greek letter lambda (λ). The term "wavelength" is also sometimes applied to modulated waves, and to the sinusoidal envelopes of modulated waves or waves formed by interference of several sinusoids.

<span class="mw-page-title-main">Arago spot</span> Bright point that appears at the center of a circular objects shadow due to Fresnel diffraction.

In optics, the Arago spot, Poisson spot, or Fresnel spot is a bright point that appears at the center of a circular object's shadow due to Fresnel diffraction. This spot played an important role in the discovery of the wave nature of light and is a common way to demonstrate that light behaves as a wave.

<span class="mw-page-title-main">Luminosity</span> Measurement of radiant electromagnetic power emitted by an object

Luminosity is an absolute measure of radiated electromagnetic energy (light) per unit time, and is synonymous with the radiant power emitted by a light-emitting object. In astronomy, luminosity is the total amount of electromagnetic energy emitted per unit of time by a star, galaxy, or other astronomical objects.

<span class="mw-page-title-main">Gigabit Ethernet</span> Standard for Ethernet networking at a data rate of 1 gigabit per second

In computer networking, Gigabit Ethernet is the term applied to transmitting Ethernet frames at a rate of a gigabit per second. The most popular variant, 1000BASE-T, is defined by the IEEE 802.3ab standard. It came into use in 1999, and has replaced Fast Ethernet in wired local networks due to its considerable speed improvement over Fast Ethernet, as well as its use of cables and equipment that are widely available, economical, and similar to previous standards. The first standard for faster 10 Gigabit Ethernet was approved in 2002.

<i>Clementine</i> (spacecraft) American space project

Clementine was a joint space project between the Ballistic Missile Defense Organization and NASA, launched on January 25, 1994. Its objective was to test sensors and spacecraft components in long-term exposure to space and to make scientific observations of both the Moon and the near-Earth asteroid 1620 Geographos.

<span class="mw-page-title-main">Angular resolution</span> Ability of any image-forming device to distinguish small details of an object

Angular resolution describes the ability of any image-forming device such as an optical or radio telescope, a microscope, a camera, or an eye, to distinguish small details of an object, thereby making it a major determinant of image resolution. It is used in optics applied to light waves, in antenna theory applied to radio waves, and in acoustics applied to sound waves. The colloquial use of the term "resolution" sometimes causes confusion; when an optical system is said to have a high resolution or high angular resolution, it means that the perceived distance, or actual angular distance, between resolved neighboring objects is small. The value that quantifies this property, θ, which is given by the Rayleigh criterion, is low for a system with a high resolution. The closely related term spatial resolution refers to the precision of a measurement with respect to space, which is directly connected to angular resolution in imaging instruments. The Rayleigh criterion shows that the minimum angular spread that can be resolved by an image forming system is limited by diffraction to the ratio of the wavelength of the waves to the aperture width. For this reason, high resolution imaging systems such as astronomical telescopes, long distance telephoto camera lenses and radio telescopes have large apertures.

<span class="mw-page-title-main">Unit of length</span> Reference value of length

A unit of length refers to any arbitrarily chosen and accepted reference standard for measurement of length. The most common units in modern use are the metric units, used in every country globally. In the United States the U.S. customary units are also in use. British Imperial units are still used for some purposes in the United Kingdom and some other countries. The metric system is sub-divided into SI and non-SI units.

In optics, the Fraunhofer diffraction equation is used to model the diffraction of waves when plane waves are incident on a diffracting object, and the diffraction pattern is viewed at a sufficiently long distance from the object, and also when it is viewed at the focal plane of an imaging lens. In contrast, the diffraction pattern created near the diffracting object and is given by the Fresnel diffraction equation.

A diode-pumped solid-state laser (DPSSL) is a solid-state laser made by pumping a solid gain medium, for example, a ruby or a neodymium-doped YAG crystal, with a laser diode.

In meteorology, visibility is the measure of the distance at which an object or light can be clearly discerned. It depends on the transparency of the surrounding air and as such, it is unchanging no matter the ambient light level or time of day. It is reported within surface weather observations and METAR code either in meters or statute miles, depending upon the country. Visibility affects all forms of traffic: roads, railways, sailing and aviation.

<span class="mw-page-title-main">Lapping</span> Process of removing material from two workpieces

Lapping is a machining process in which two surfaces are rubbed together with an abrasive between them, by hand movement or using a machine.

<span class="mw-page-title-main">Multi-mode optical fiber</span> Type of optical fiber mostly used for communication over short distances

Multi-mode optical fiber is a type of optical fiber mostly used for communication over short distances, such as within a building or on a campus. Multi-mode links can be used for data rates up to 800 Gbit/s. Multi-mode fiber has a fairly large core diameter that enables multiple light modes to be propagated and limits the maximum length of a transmission link because of modal dispersion. The standard G.651.1 defines the most widely used forms of multi-mode optical fiber.

<span class="mw-page-title-main">Electromagnetic absorption by water</span>

The absorption of electromagnetic radiation by water depends on the state of the water.

<span class="mw-page-title-main">Laser beam profiler</span> Measurement device

A laser beam profiler captures, displays, and records the spatial intensity profile of a laser beam at a particular plane transverse to the beam propagation path. Since there are many types of lasers—ultraviolet, visible, infrared, continuous wave, pulsed, high-power, low-power—there is an assortment of instrumentation for measuring laser beam profiles. No single laser beam profiler can handle every power level, pulse duration, repetition rate, wavelength, and beam size.

The angstrom or ångström is a metric unit of length equal to 10−10 m; that is, one ten-billionth (US) of a metre, a hundred-millionth of a centimetre, 0.1 nanometre, or 100 picometres. Its symbol is Å, a letter of the Swedish alphabet. The unit is named after the Swedish physicist Anders Jonas Ångström (1814–1874).

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