- Orders of magnitude (length)
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Contents
Section Range (m) Unit Example Items ≥ < Subatomic 0 10−15 am electron, quark, string, Planck length Atomic to cellular 10−15 10−12 fm proton, neutron 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 Human scale 10−6 10−3 µm bacterium, fog water droplet, human hair[1] 10−3 100 mm mosquito, golf ball, football (soccer ball) 100 103 m human being, football (soccer) field, Eiffel Tower 103 106 km Mount Everest, length of Panama Canal, 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 one light-year; distance to Proxima Centauri 1018 1021 Em galactic arm 1021 1024 Zm Milky Way, distance to Andromeda Galaxy 1024 ∞ Ym visible universe Detailed list
To help compare different orders of magnitude, the following list describes various lengths between 1.6×10−35 m and 1.3×1026 m.
Subatomic
Factor (m) Multiple Value Item 10−35 0.000000000016 ym (1.6×10−35 m) Planck length; size of a hypothetical string and of branes; according to string theory lengths smaller than this do not make any physical sense.[2] Quantum foam is thought to exist at this level.
10−24 1 yoctometre (ym) 20 ym (2 × 10−23 metres) effective cross section radius of 1 MeV neutrinos[3] 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 zm (7 × 10−21 metres) effective cross section radius of high energy neutrinos[4] 354 zm (3.54 × 10−19 metres) de Broglie wavelength of protons at the Large Hadron Collider (3.5 TeV as of 2011) 10−18 1 attometre (am) upper limit for the size of quarks and electrons sensitivity of the LIGO detector for gravitational waves upper bound of the typical size range for "fundamental strings"[2] 10−17 10 am range of the weak force 10−16 100 am According to Craig Hogan, a scientist from Fermilab, the predicted scale of resolution of space-time if the universe is assumed to satisfy the holographic principle, a prediction that according to preliminary reports is in agreement with observations at the GEO 600 detector.[5] Atomic to cellular
Clickable image. The thumbnails range left to right from 1e-15m to 1e-7m. (Image description)Factor (m) Multiple Value Item 10−15 1 femtometre (fm) 1.5 fm size of an 11 MeV proton[6] 2.81794 fm classical electron radius[7] scale of the atomic nucleus[2][8] 10−14 10 fm 10−13 100 fm 10−12 1 picometre (pm) ... longest wavelength of gamma rays 2.4 pm Compton wavelength of electron 5 pm wavelength of shortest X-rays 10−11 10 pm 25 pm radius of hydrogen atom 31 pm radius of helium atom 53 pm Bohr radius 10−10 100 pm 100 pm (0.1 nm) 1 Ångström (also covalent radius of sulfur atom[9]) 154 pm (0.154 nm) length of a typical covalent bond (C–C). 500 pm (0.50 nm) width of protein α helix 10−9 1 nanometre (nm) 1 nm diameter of a carbon nanotube[10] 2.5 nm Smallest transistor gate oxide thickness microprocessors (as of Jan 2007) 6–10 nm thickness of cell membrane 10−8 10 nm 10 nm thickness of cell wall in gram-negative bacteria[citation needed] 40 nm extreme ultraviolet wavelength 90 nm Human immunodeficiency virus (HIV) (generally, viruses range in size from 20 nm to 450 nm) 10−7 100 nm 121.6 nm wavelength of the lyman-alpha line[11] 380–435 nm wavelength of violet light—see color and optical spectrum[12] 625–740 nm wavelength of red light[12] Human scale
Click on the thumbnail image to jump to the desired order of length magnitude article: top-left is 1E-6m (10−6), lower-right is 1E5m (105). (Image description)Factor (m) Multiple Value Item 10−6 1 micrometre (µm) 1 µm also called one micron 1–3 µm particle size that a surgical mask removes at 80–95% efficiency[citation needed] 6-8 µm diameter of a red blood cell[13] 10−5 10 µm 10 µm typical size of a fog, mist or cloud water droplet. Chip 10 µm process in 1971. 12 µm width of acrylic fibre 25.4 µm 1/1000 inch, commonly referred to as one mil 10−4 100 µm 100 µm width of a strand of human hair[14] 200 µm typical length of Paramecium caudatum, a ciliate protist 750 µm maximum diameter of Thiomargarita namibiensis, the largest bacterium ever discovered 10−3 1 millimetre (mm) 2.54 mm 1/10th inch; distance between pins in DIP (dual-inline-package) electronic components 5 mm length of average red ant 7.62 mm common military ammunition size 10−2 1 centimetre (cm) 1.5 cm length of a large mosquito 2.54 cm 1 inch 4.267 cm diameter of a golf ball 10−1 1 decimetre (dm) 10 cm wavelength of the highest UHF radio frequency, 3 GHz 30.48 cm 1 foot 91 cm 1 yard 100 1 metre 1 m wavelength of the lowest UHF and highest VHF radio frequency, 300 MHz 1.7 m (5 feet 7 inches) average height of a human 8.38 m The length of a London Bus (Routemaster) 101 1 decametre (dam) 10 m wavelength of the lowest VHF and highest shortwave radio frequency, 30 MHz 33 m length of longest blue whale measured, the largest animal[15] 93.47 m height of the Statue of Liberty (foundation of pedestal to torch) 102 1 hectometre (hm) 100 m wavelength of the lowest shortwave radio frequency and highest medium wave radio frequency, 3 MHz 137 m (147 m) height (present and original) of the Great Pyramid of Giza 979 m height of the Salto Angel, the world's highest free-falling waterfall (Venezuela) 103 1 kilometre (km) 1 km wavelength of the lowest medium wave radio frequency, 300 kHz 1609 m 1 international mile 8848 m height of the highest mountain on earth, Mount Everest 104 10 km 10.911 km depth of deepest part of the ocean, Mariana Trench 13 km narrowest width of the Strait of Gibraltar, separating Europe and Africa 90 km width of the Bering Strait 105 100 km 111 km distance covered by one degree of latitude on Earth's surface 163 km length of the Suez Canal 974.6 km greatest diameter[16] of the dwarf planet,[note 1] Ceres Astronomical
An illustration of the sizes of planets and stars
Click on the thumbnail image to jump to the desired order of length magnitude: top-left is 1e6m, lower-right is 1e17m. (Image description)Factor (m) Multiple Value Item 106 1,000 km = 1 megametre (Mm) 2,390 km diameter of dwarf planet Pluto, formerly the smallest planet category[note 1] of our solar system 3,480 km diameter of the Moon 5,200 km typical distance covered by the winner of the 24 hours of Le Mans automobile endurance race 6,400 km length of the Great Wall of China 6,600 km approximate length of the two longest rivers, the Nile and the Amazon 7,821 km length of the Trans-Canada Highway 9,288 km length of the Trans-Siberian Railway, longest in the world 107 10,000 km 12,756 km equatorial diameter of the Earth 40,075 km length of the Earth's equator 108 100,000 km 142,984 km diameter of Jupiter 299,792.458 km distance travelled by light in one second 384,000 km = 384 Mm Moon's orbital distance from Earth 109 1 million km = 1 gigametre (Gm) 1,390,000 km = 1.39 Gm diameter of the Sun 4,200,000 km = 4.2 Gm greatest mileage ever recorded by a car (A 1966 Volvo P-1800S, still driving) 1010 10 million km 18 million km approximately one light-minute 1011 100 million km 150 million km = 150 Gm 1 astronomical unit (AU); mean distance between Earth and Sun ~ 900 Gm optical diameter of Betelgeuse (~600 × Sun) 1012 1000 million km = 1 terametre (Tm) 1.4 ×109 km orbital distance of Saturn from Sun ~ 3 ×109 km estimated optical diameter of VY Canis Majoris, as of 2007 the largest known star (~2000 × Sun) 5.9 ×109 km = 5.9 Tm orbital distance of Pluto from Sun ~ 7.5 ×109 km = 7.5 Tm outer boundary of the Kuiper belt, inner boundary of the Oort cloud (~ 50 AU) 1013 10 Tm diameter of our Solar System as a whole[2] 16.25×109 km = 16.25 Tm distance of the Voyager 1 spacecraft from Sun (as of Feb 2009[update]), the farthest man-made object so far[17] 1014 100 Tm 1.8×1011 km = 180 Tm size of the debris disk around the star 51 Pegasi [18] 1015 1 petametre (Pm) ~ 7.5 ×1012 km = 7.5 Pm supposed outer boundary of the Oort cloud (~ 50,000 AU) 9.46×1012 km = 9.46 Pm
= 1 light yeardistance travelled by light in one year; at its current speed, Voyager 1 would need 17,500 years to travel this distance 1016 10 Pm 3.2616 light-years
(3.08568×1016 m = 30.8568 Pm)1 parsec 4.22 light-years = 39.9 Pm distance to nearest star (Proxima Centauri) 10.4 light-years = 98.4 Pm as of September 2007, distance to nearest discovered extrasolar planet (Epsilon Eridani b) 1017 100 Pm 20.4 light-years = 193 Pm as of October 2010, distance to nearest discovered extrasolar planet with potential to support life as we know it (Gliese 581 d) 65 light-years = 6.15×1017 m = 615 Pm approximate radius of humanity's radio bubble, caused by high-power TV broadcasts leaking through the atmosphere into outer space 1018 1 exametre (Em) 200 light-years = 1.9 Em distance to nearby solar twin (HIP 56948), a star with properties virtually identical to our Sun [19] 1019 10 Em 1,000 light-years = 9.46 Em or 9.46 × 1015 km average thickness of Milky Way Galaxy[20] (1000 to 3000 ly by 21 cm observations[21]) 1020 100 Em 12,000 light-years = 113.5 Em or 1.135 × 1017 km thickness of Milky Way Galaxy's gaseous disk[22] 1021 1 zettametre (Zm) 100,000 light-years diameter of galactic disk of Milky Way Galaxy[2] 50 kiloparsecs distance to SN 1987A, the most recent naked eye supernova 52 kiloparsecs = 1.6×1021 m = 1.6 Zm distance to the Large Magellanic Cloud (a dwarf galaxy orbiting the Milky Way) 54 kiloparsecs = 1.66 Zm distance to the Small Magellanic Cloud (another dwarf galaxy orbiting the Milky Way) 1022 10 Zm 22.3 Zm = 2.36 million light-years
= 725 kiloparsecsdistance to Andromeda Galaxy 50 Zm (1.6 Mpc) diameter of Local Group of galaxies 1023 100 Zm 300–600 Zm = 10–20 megaparsecs distance to Virgo cluster of galaxies 1024 1 yottametre (Ym) 200 million light-years
= 2 Ym = 60 megaparsecsdiameter of the Local Supercluster and the largest voids and filaments. 550 million light-years
~170 megaparsecs ~5 Ymdiameter of the enormous Horologium Supercluster [23] 1025 10 Ym 1.37 billion light years
= 1.3×1025 m = 13 YmLength of the Sloan Great Wall, a giant wall of galaxies (galactic filament.[24] 1026 100 Ym 1×1010 light-years
= 1026 m = 100 Ymestimated light travel distance to certain quasars 92×109 light years
= 9.2×1026 m = 920 Ymapprox. diameter (comoving distance) of the visible universe[2] 1027 1000 Ym ~250 billion light years
= 2.4×1027 m = 2400 YmAccording to one estimate using the WMAP data,[25] it can be said with 95% confidence that there is a lower limit of 21 particle horizon size patches in the universe. 
Ym megaparsecs
= m
=Ymsize of universe after cosmological inflation, implied by one resolution of the No-Boundary Proposal[26] See also
- Earth's location in the universe
- Powers of Ten, a 1977 short documentary film which depicts the relative scale of the Universe in factors of ten.
Notes
- ^ a b 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
References
- ^ According to The Physics Factbook, the diameter of human hair ranges from 17 to 181 µm. Ley, Brian (1999). "Width of a Human Hair". The Physics Factbook. http://hypertextbook.com/facts/1999/BrianLey.shtml.
- ^ a b c d e f Cliff Burgess; Fernando Quevedo (November 2007). "The Great Cosmic Roller-Coaster Ride" (print). Scientific American (Scientific American, Inc.): p. 55.
- ^ Carl R. Nave. "Cowan and Reines Neutrino Experiment". http://hyperphysics.phy-astr.gsu.edu/hbase/particles/cowan.html#c1. Retrieved 2008-12-04. (6.3 × 10−44 cm2, which gives an effective radius of about 2 × 10−23 m)
- ^ New Scientist – Our world may be a giant hologram
- ^ NIST. CODATA Value: classical electron radius. Retrieved 2009-02-10
- ^ H. E. Smith. "The Scale of the Universe". UCSD. http://cass.ucsd.edu/public/tutorial/scale.html. Retrieved 2009-02-10. "~10-13cm"
- ^ Mark Winter (2008). "WebElements Periodic Table of the Elements / Sulfur / Radii". http://www.webelements.com/sulfur/atom_sizes.html. Retrieved 2008-12-06.
- ^ Flahaut, E.; Bacsa R, Peigney A, Laurent C. (2003). "Gram-Scale CCVD Synthesis of Double-Walled Carbon Nanotubes". Chemical Communications 12 (12): 1442–1443. doi:10.1039/b301514a. PMID 12841282. http://www.rsc.org/Publishing/Journals/CC/article.asp?doi=b301514a. Retrieved 2008-11-14.
- ^ Cohn, J. University of California, Berkeley Lyman alpha systems and cosmology. Retrieved 2009-02-21
- ^ a b Color
- ^ "Through the Microscope: Blood Cells - Life's Blood". Wadsworth Center, New York State Department of Health. http://www.wadsworth.org/chemheme/heme/microscope/rbc.htm. Retrieved 2011-09-13.
- ^ DNA From The Beginning, Classical Genetics, section 6: Genes are real things., "Animation" section, final slide
- ^ "Animal Records". Smithsonian National Zoological Park. http://nationalzoo.si.edu/Animals/AnimalRecords/. Retrieved 2007-05-29.
- ^ Thomas, P. C.; Parker, J. Wm.; McFadden, L. A.; et al. (2005). "Differentiation of the asteroid Ceres as revealed by its shape". Nature 437 (7056): 224–226. Bibcode 2005Natur.437..224T. doi:10.1038/nature03938. PMID 16148926.
- ^ Spacecraft escaping the Solar System
- ^ http://esciencenews.com/articles/2009/09/24/twin.keck.telescopes.probe.dual.dust.disks
- ^ Shiga, David. "Sun's 'twin' an ideal hunting ground for alien life". New Scientist. http://space.newscientist.com/article/dn12725-suns-twin-an-ideal-hunting-ground-for-alien-life.html. Retrieved 2007-10-03.
- ^ Christian, Eric; Samar, Safi-Harb. "How large is the Milky Way?". http://imagine.gsfc.nasa.gov/docs/ask_astro/answers/980317b.html. Retrieved 2008-11-14.
- ^ Duncan, Martin (2008). "Physics 216 – Introduction to Astrophysics". http://www.physics.queensu.ca/~phys216/ch16B.pdf. Retrieved 2008-11-14.
- ^ "Milky Way fatter than first thought". The Sydney Morning Herald. Australian Associated Press. 2008-02-20. http://news.smh.com.au/milky-way-fatter-than-first-thought/20080220-1tbv.html. Retrieved 2008-11-14.
- ^ http://www.atlasoftheuniverse.com/superc/hor.html The Horologium Supercluster
- ^ J. R. Gott III et al., Astrophys. J., 624, 463 (2005). Figure 8 – "Logarithmic Maps of the Universe" – is available as a poster from the homepage of Mario Juric.
- ^ http://arxiv.org/abs/astro-ph/0605709v2 How Many Universes Do There Need To Be?
- ^ http://arxiv.org/abs/hep-th/0610199 "Susskind's Challenge to the Hartle-Hawking No-Boundary Proposal and Possible Resolutions "
External links
- How Big Are Things? displays orders of magnitude in successively larger rooms
- Powers of Ten Travel across the Universe. Altering perspective by changing scale by just a few powers of ten (interactive)
- Cosmos – an Illustrated Dimensional Journey from microcosmos to macrocosmos – from Digital Nature Agency
Orders of magnitude for length in E notation shorter than one metre: <−24 −24 −23 −22 −21 −20 −19 −18 −17 −16 −15 −14 −13 −12 −11 −10 −9 −8 −7 −6 −5 −4 −3 −2 −1 0 longer than 1 metre: 1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20 21 22 23 24 25 26 Orders of magnitude Quantity acceleration · angular velocity · area · charge · computing · currency · data · density · energy · entropy · force · frequency · length · luminous flux · magnetic field · mass · numbers · power · pressure · radiation · resistance · specific energy density · specific heat capacity · speed · temperature · time · voltage · volumeSee also Units of length used in Astronomy Astronomical system of unitsEarth radius (
or RE) · Light-second (ls) · Solar radius (
) · gigametre (Gm) · Astronomical unit (AU) · light-year (ly) · parsec (pc) · kiloparsec (kpc) · megaparsec (Mpc) · gigaparsec (Gpc)Categories:- Length
- Orders of magnitude
- Orders of magnitude (length)
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