Grootteordes (lengte): Verskil tussen weergawes

in Wikipedia, die vrye ensiklopedie
Content deleted Content added
Lyn 232: Lyn 232:
<div id="1E-6"/>
<div id="1E-6"/>
|-
|-
|rowspan=3|[[1 micrometre|10<sup>−6</sup>]]
|rowspan=3|[[1 mikrometer|10<sup>−6</sup>]]
|rowspan=3|1 [[micrometre]] (µm)
|rowspan=3|1 [[mikrometer]] (µm)
|1&nbsp;µm
|1&nbsp;µm
|also called one [[micron]]
|word ook een [[mikron]] genoem
|-
|-
|1–3&nbsp;µm
|1–3&nbsp;µm
Lyn 243: Lyn 243:
|diameter of a [[red blood cell]]<ref>{{Cite web | url=http://www.wadsworth.org/chemheme/heme/microscope/rbc.htm | title=Through the Microscope: Blood Cells - Life's Blood | publisher=Wadsworth Center, New York State Department of Health | accessdate=2011-09-13 }}</ref>
|diameter of a [[red blood cell]]<ref>{{Cite web | url=http://www.wadsworth.org/chemheme/heme/microscope/rbc.htm | title=Through the Microscope: Blood Cells - Life's Blood | publisher=Wadsworth Center, New York State Department of Health | accessdate=2011-09-13 }}</ref>
|-
|-
|rowspan=3|[[10 micrometres|10<sup>−5</sup>]]
|rowspan=3|[[10 mikrometers|10<sup>−5</sup>]]
|rowspan=3|10&nbsp;µm
|rowspan=3|10&nbsp;µm
|10&nbsp;µm
|10&nbsp;µm
Lyn 254: Lyn 254:
|1/1000&nbsp;inch, commonly referred to as one [[Thou (unit of length)|mil]]
|1/1000&nbsp;inch, commonly referred to as one [[Thou (unit of length)|mil]]
|-
|-
|rowspan=3|[[1 myriometre|10<sup>−4</sup>]]
|rowspan=3|[[100 mikrometers|10<sup>−4</sup>]]
|rowspan=3|100&nbsp;µm
|rowspan=3|100&nbsp;µm
|100&nbsp;µm
|100&nbsp;µm
Lyn 267: Lyn 267:
<div id="1E-3"/>
<div id="1E-3"/>
|-
|-
|rowspan=3|[[1 millimetre|10<sup>−3</sup>]]
|rowspan=3|[[1 millimeter|10<sup>−3</sup>]]
|rowspan=3|1 [[millimetre]] (mm)
|rowspan=3|1 [[millimeter]] (mm)
|2.54&nbsp;mm
|2.54&nbsp;mm
|1/10th inch; distance between pins in [[dual in-line package|DIP]] (dual-inline-package) electronic components
|1/10th inch; distance between pins in [[dual in-line package|DIP]] (dual-inline-package) electronic components
Lyn 278: Lyn 278:
|common military ammunition size
|common military ammunition size
|-
|-
|rowspan=3|[[1 centimetre|10<sup>−2</sup>]]
|rowspan=3|[[1 centimeter|10<sup>−2</sup>]]
|rowspan=3|1 [[centimetre]] (cm)
|rowspan=3|1 [[centimeter]] (cm)
|1.5&nbsp;cm
|1.5&nbsp;cm
|length of a large [[mosquito]]
|length of a large [[mosquito]]
Lyn 289: Lyn 289:
|diameter of a [[golf ball]]
|diameter of a [[golf ball]]
|-
|-
|rowspan=3|[[1 decimetre|10<sup>−1</sup>]]
|rowspan=3|[[1 decimeter|10<sup>−1</sup>]]
|rowspan=3|1 [[decimetre]] (dm)
|rowspan=3|1 [[decimeter]] (dm)
|10&nbsp;cm
|10&nbsp;cm
|wavelength of the highest [[Ultra high frequency|UHF]] radio frequency, 3&nbsp;GHz
|wavelength of the highest [[Ultra high frequency|UHF]] radio frequency, 3&nbsp;GHz
Lyn 301: Lyn 301:
<div id="1E0"/>
<div id="1E0"/>
|-
|-
|rowspan=3|[[1 metre|10<sup>0</sup>]]
|rowspan=3|[[1 meter|10<sup>0</sup>]]
|rowspan=3|1 [[metre]]
|rowspan=3|1 [[meter]]
| 1 m
| 1 m
|wavelength of the lowest [[Ultra high frequency|UHF]] and highest [[Very high frequency|VHF]] radio frequency, 300&nbsp;MHz
|wavelength of the lowest [[Ultra high frequency|UHF]] and highest [[Very high frequency|VHF]] radio frequency, 300&nbsp;MHz
Lyn 312: Lyn 312:
|The length of a London Bus ([[Routemaster]])
|The length of a London Bus ([[Routemaster]])
|-
|-
|rowspan=3|[[1 decametre|10<sup>1</sup>]]
|rowspan=3|[[1 dekameter|10<sup>1</sup>]]
|rowspan=3|1 [[decametre]] (dam)
|rowspan=3|1 [[dekameter]] (dam)
|10 m
|10 m
|wavelength of the lowest [[Very high frequency|VHF]] and highest [[shortwave]] radio frequency, 30&nbsp;MHz
|wavelength of the lowest [[Very high frequency|VHF]] and highest [[shortwave]] radio frequency, 30&nbsp;MHz
Lyn 323: Lyn 323:
|height of the [[Statue of Liberty]] (foundation of pedestal to torch)
|height of the [[Statue of Liberty]] (foundation of pedestal to torch)
|-
|-
|rowspan=3|[[1 hectometre|10<sup>2</sup>]]
|rowspan=3|[[1 hectometer|10<sup>2</sup>]]
|rowspan=3|1 [[hectometre]] (hm)
|rowspan=3|1 [[hectometer]] (hm)
|100 m
|100 m
|wavelength of the lowest [[shortwave]] radio frequency and highest [[medium wave]] radio frequency, 3&nbsp;MHz
|wavelength of the lowest [[shortwave]] radio frequency and highest [[medium wave]] radio frequency, 3&nbsp;MHz
Lyn 335: Lyn 335:
<div id="1E3"/>
<div id="1E3"/>
|-
|-
|rowspan=3|[[1 kilometre|10<sup>3</sup>]]
|rowspan=3|[[1 kilometer|10<sup>3</sup>]]
|rowspan=3|1 [[kilometre]] (km)
|rowspan=3|1 [[kilometer]] (km)
|1&nbsp;km
|1&nbsp;km
|wavelength of the lowest [[medium wave]] radio frequency, 300&nbsp;kHz
|wavelength of the lowest [[medium wave]] radio frequency, 300&nbsp;kHz
Lyn 346: Lyn 346:
|height of the highest mountain on earth, [[Mount Everest]]
|height of the highest mountain on earth, [[Mount Everest]]
|-
|-
|rowspan=3|[[1 myriametre|10<sup>4</sup>]]<!-- Please consider renaming the obsolete term myriametre to [[10 kilometres (order of magnitude)]] -->
|rowspan=3|[[10 kilometers|10<sup>4</sup>]]<!-- Please consider renaming the obsolete term myriametre to [[10 kilometres (order of magnitude)]] -->
|rowspan=3|10&nbsp;km
|rowspan=3|10&nbsp;km
|10.911&nbsp;km
|10.911&nbsp;km
Lyn 357: Lyn 357:
|width of the [[Bering Strait]]
|width of the [[Bering Strait]]
|-
|-
|rowspan=3|[[100 kilometres|10<sup>5</sup>]]
|rowspan=3|[[100 kilometers|10<sup>5</sup>]]
|rowspan=3|100&nbsp;km
|rowspan=3|100&nbsp;km
|111&nbsp;km
|111&nbsp;km

Wysiging soos op 12:27, 2 April 2012

Hierdie artikel of onderafdeling van die artikel is onder ontwikkeling.
As u wil bydra tot die ontwikkeling daarvan, spring gerus in, maar moet dit asseblief nie uitvee nie.
Software Development
Hierdie artikel moet vertaal word.
Indien die artikel nie vertaal of oorgeskryf word binne die volgende twee weke nie, sal dit gelys word vir verwydering.


Afdeling Reeks (m) Eenheid Voorbeeld
<
Subatomies 0 10−15 am elektron, kwark, string, Planck-lengte
Atoom na sellulêre 10−15 10−12 fm proton, neutron
10−12 10−9 pm golflengte van gammastrale en x-strale, waterstof atoom
10−9 10−6 nm DNA heliks, virus, golflengte van sigbare spektrum
Menslike skaal 10−6 10−3 µm bakterie, mis (water druppel), menslike haar[1]
10−3 100 mm muskiet, golfbal, voetbal (sokkerbal)
100 103 m mens, voetbal (sokkerveld), Eiffel-toring
103 106 km Mount Everest, lengte van die Panamakanaal, groter asteroïde
Astronomies 106 109 Mm die Maan, Aarde, een ligsekonde
109 1012 Gm Son, een ligminuut, Aarde se wentelbaan
1012 1015 Tm wentelbane van buitenste planete, Sonnestelsel
1015 1018 Pm een ligjaar; afstand na Proxima Centauri
1018 1021 Em spiraalvormige sterrestelsel
1021 1024 Zm Melkweg, afstand na Andromeda sterrestelsel
1024 Ym waarneembare heelal

Gedetailleerde lys

Om te help verskillende grootteordes te vergelyk, die volgende lys verduidelik die verskeie lengtes tussen 1.6×10−35 m en 1.3×1026 m.

Subatomies

Faktor (m) Meervoudige Waarde Item
10−35 0.000000000016 ym (1.6×10−35 m) Planck-lengte; grootte van 'n hipotetiese string en van membrane; volgens die string theorie lengtes kleiner as dit maak nie wetenskaplik sin nie.[2]

Gedink kwantum skuim bestaan op hierdie vlak.

10−24 1 joktometer (ym) 20 ym (2 × 10−23 meters) effektiewe dwarsdeursnit radius van 1 MeV neutrinos[3]
10−21 1 zeptometer (zm) Preons, hipotetiese deeltjies voorgestel as onderafdelings van quarks en leptonen; die bogrens vir die breedte van 'n kosmiese string in string theorie.
7 zm (7 × 10−21 meters) effektiewe dwarsdeursnit radius van hoë energie neutrinos[4]
354 zm (3.54 × 10−19 meters) de Broglie golflengte van protone by die Large Hadron Collider (3.5 TeV van 2011)
10−18 1 attometer (am) boonste limiet vir die grootte van quarks en elektrone
sensitiwiteit van die LIGO detektor vir gravitasie golwe
bogrens van die tipiese grootte vir "fundamentele stringe"[2]
10−17 10 am omvang van die swak kernkrag
10−16 100 am Volgens Craig Hogan, 'n wetenskaplike van Fermilab, die voorgespelde skaal van resolusie van ruimtetyd, as daar aanvaar word dat die heelal voldoen aan die holografiese beginsel, 'n voorspelling dat volgens voorlopige verslae is in ooreenstemming met waarnemings by die GEO 600 detektor.[5]

Atoom na sellulêre

1 E-15m - Click on the relevant thumbnail image to jump to the desired order of length magnitude: left is 1e-15m, right is 1e-8m. Click on information icon bottom-left for description of image.1 E-14 m1 E-13 m1 E-12 m1 E-11 m1 E-10 m1 E-9 m1 E-8 m1 E-7 m
Clickable image. The thumbnails range left to right from 1e-15m to 1e-7m. (Image description)
Faktor (m) Meervoudige Waarde 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[verwysing benodig]
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]

Menslike skaal

1 E-6 m - Click on the relevant thumbnail image to jump to the desired order of length magnitude: top-left is 1e-6m, bottom-right is 1e5m. Click on information icon bottom-left for description of image.1 E-5 m1 E-4 m1 E-3 m1 E-2 m1 E-1 m1 E0 m1 E1 m1 E2 m1 E3 m1 E4 m1 E5 m
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)
Faktor (m) Meervoudige Waarde Item
10−6 1 mikrometer (µm) 1 µm word ook een mikron genoem
1–3 µm particle size that a surgical mask removes at 80–95% efficiency[verwysing benodig]
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 millimeter (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 centimeter (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 decimeter (dm) 10 cm wavelength of the highest UHF radio frequency, 3 GHz
30.48 cm 1 foot
91 cm 1 yard
100 1 meter 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 dekameter (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 hectometer (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 kilometer (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

Astronomies

An illustration of the sizes of planets and stars

Sjabloon:Orders of magnitude (length) imagemap astronomical-scale

Faktor (m) Meervoudige Waarde 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 (Sjabloon:As of), 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 year
distance 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 kiloparsecs
distance 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 megaparsecs
diameter of the Local Supercluster and the largest voids and filaments.
550 million light-years
~170 megaparsecs ~5 Ym
diameter of the enormous Horologium Supercluster [23]
1025 10 Ym 1.37 billion light years
= 1.3×1025 m = 13 Ym
Length of the Sloan Great Wall, a giant wall of galaxies (galactic filament.[24]
1026 100 Ym 1×1010 light-years
= 1026 m = 100 Ym
estimated light travel distance to certain quasars
92×109 light years
= 9.2×1026 m = 920 Ym
approx. diameter (comoving distance) of the visible universe[2]
1027 1000 Ym ~250 billion light years
= 2.4×1027 m = 2400 Ym
According 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
= Ym
size of universe after cosmological inflation, implied by one resolution of the No-Boundary Proposal[26]

Sien ook

Notas

  1. 1,0 1,1 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

Verwysings

  1. 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.
  2. 2,0 2,1 2,2 2,3 2,4 2,5 Cliff Burgess (November 2007). "The Great Cosmic Roller-Coaster Ride". Scientific American (print). Scientific American, Inc. p. 55. {{cite news}}: |access-date= requires |url= (hulp); |format= requires |url= (hulp); Onbekende parameter |coauthors= geïgnoreer (hulp)
  3. Carl R. Nave. "Cowan and Reines Neutrino Experiment". Besoek op 4 Desember 2008. (6.3 × 10−44 cm2, which gives an effective radius of about 2 × 10−23 m)
  4. Carl R. Nave. "Neutron Absorption Cross-sections". Besoek op 4 Desember 2008. (area for 20 GeV about 10 × 10−42 m2 gives effective radius of about 2 × 10−21 m; for 250 GeV about 150 × 10−42 m2 gives effective radius of about 7 × 10−21 m)
  5. New Scientist – Our world may be a giant hologram
  6. Carl R. Nave. "Scattering Cross Section". Besoek op 10 Februarie 2009. (diameter of the Scattering Cross Section of an 11 MeV proton with a target proton)
  7. NIST. CODATA Value: classical electron radius. Retrieved 2009-02-10
  8. H. E. Smith. "The Scale of the Universe". UCSD. Besoek op 10 Februarie 2009. ~10-13cm
  9. Mark Winter (2008). "WebElements Periodic Table of the Elements / Sulfur / Radii". Besoek op 6 Desember 2008.
  10. Flahaut, E. (2003). "Gram-Scale CCVD Synthesis of Double-Walled Carbon Nanotubes". Chemical Communications. 12 (12): 1442–1443. doi:10.1039/b301514a. PMID 12841282. Besoek op 14 November 2008. {{cite journal}}: Onbekende parameter |coauthors= geïgnoreer (hulp)
  11. Cohn, J. University of California, Berkeley Lyman alpha systems and cosmology. Retrieved 2009-02-21
  12. 12,0 12,1 Color
  13. "Through the Microscope: Blood Cells - Life's Blood". Wadsworth Center, New York State Department of Health. Besoek op 13 September 2011.
  14. DNA From The Beginning, Classical Genetics, section 6: Genes are real things., "Animation" section, final slide
  15. "Animal Records". Smithsonian National Zoological Park. Besoek op 29 Mei 2007.
  16. Thomas, P. C. (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. {{cite journal}}: Onbekende parameter |coauthors= geïgnoreer (hulp)
  17. Spacecraft escaping the Solar System
  18. http://esciencenews.com/articles/2009/09/24/twin.keck.telescopes.probe.dual.dust.disks
  19. Shiga, David. "Sun's 'twin' an ideal hunting ground for alien life". New Scientist. Besoek op 3 Oktober 2007.
  20. Christian, Eric; Samar, Safi-Harb. "How large is the Milky Way?". Besoek op 14 November 2008.
  21. Duncan, Martin (2008). "Physics 216 – Introduction to Astrophysics" (PDF). Besoek op 14 November 2008. {{cite web}}: |chapter= ignored (hulp)
  22. "Milky Way fatter than first thought". The Sydney Morning Herald. Australian Associated Press. 20 Februarie 2008. Besoek op 14 November 2008.
  23. http://www.atlasoftheuniverse.com/superc/hor.html The Horologium Supercluster
  24. 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.
  25. http://arxiv.org/abs/astro-ph/0605709v2 How Many Universes Do There Need To Be?
  26. http://arxiv.org/abs/hep-th/0610199 "Susskind's Challenge to the Hartle-Hawking No-Boundary Proposal and Possible Resolutions "

External links