Grootteordes (lengte): Verskil tussen weergawes
Content deleted Content added
Lyn 380:
<div id="1E6"/>
|-
|rowspan=7|[[1
|rowspan=7|1,000 km = 1 [[
|2,390 km
|diameter van [[Pluto]]
|-
|3,480 km
|diameter
|-
|5,200 km
|
|-
|6,400 km
|
|-
|6,600 km
|
|-
|7,821 km
|
|-
|9,288 km
|
<div id="1E7"/>
|-
|rowspan=2|[[10
|rowspan=2|10,000 km
|12,756 km
|ekwatoriale deursnee van die aarde
|-
|40,075 km
|
<div id="1E8"/>
|-
|rowspan=3|[[100
|rowspan=3|100,000 km
|142,984 km
|diameter
|-
|299,792.458 km
|
|-
|384,000 km = 384 Mm
|[[Maan]] se orbitale afstand van die Aarde
<div id="1E9"/>
|-
|rowspan=2|[[1
|rowspan=2|1 million km = 1 [[
|1,390,000 km = 1.39 Gm
|diameter
|-
|4,200,000 km = 4.2 Gm
|
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|-
| [[10
| 10
|18
|ongeveer een [[ligminuut|ligsekonde]]
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|-
| rowspan=2 | [[100
| rowspan=2 | 100
|150
|1 [[
|-
|~ 900 Gm
|
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|-
|rowspan=4|[[1
|rowspan=4|1000
|1.4 {{E|9}} km
|[[Saturnus]] se orbitale afstand van die Son
|-
|~ 3 {{E|9}} km
|
|-
|5.9 {{E|9}} km = 5.9 Tm
|[[Pluto]] se orbitale afstand van die Son
|-
|~ 7.5 {{E|9}} km = 7.5 Tm
|
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|-
|rowspan=2|[[10
|rowspan=2|10 Tm
|
|diameter
|-
|16.25{{E|9}} km = 16.25 Tm
|
<div id="1E14"/>
|-
|[[100
|100 Tm
|1.8{{E|11}} km = 180 Tm
|
|-
|rowspan=2|[[1
|rowspan=2|1 [[
|~ 7.5 {{E|12}} km = 7.5 Pm
|
|-
|9.46{{E|12}} km = 9.46 Pm<br>= 1 [[
|
<div id="1E16"/>
|-
|rowspan=3|[[10
|rowspan=3|10 Pm
|3.2616
|1 [[parsec]]
|-
|4.22
|
|-
|10.4
|
<div id="1E17"/>
|-
|rowspan=2|[[100
|rowspan=2|100 Pm
|20.4
|
|-
|65
|approximate radius of humanity's radio bubble, caused by high-power TV broadcasts leaking through the atmosphere into outer space
<div id="1E18"/>
|-
|rowspan=1|[[1
|rowspan=1|1 [[
|200
|distance to nearby [[solar twin]] ([[HIP 56948]]), a star with properties virtually identical to our Sun <ref>{{cite web | last = Shiga | first = David | url = http://space.newscientist.com/article/dn12725-suns-twin-an-ideal-hunting-ground-for-alien-life.html | title = Sun's 'twin' an ideal hunting ground for alien life | publisher = New Scientist | accessdate = 2007-10-03 }}</ref>
<div id="1E19"/>
|-
|[[10
|10 Em
|1,000
|average thickness of [[Milky Way Galaxy]]<ref>{{cite web |last=Christian |first=Eric |last2=Samar |first2=Safi-Harb |title=How large is the Milky Way? |url=http://imagine.gsfc.nasa.gov/docs/ask_astro/answers/980317b.html |accessdate=2008-11-14}}</ref> (1000 to 3000 ly by [[Hydrogen line|21 cm observations]]<ref>{{cite web |last=Duncan |first=Martin |title=Physics 216 – Introduction to Astrophysics |chapter=16 |url=http://www.physics.queensu.ca/~phys216/ch16B.pdf |year=2008 |accessdate=2008-11-14}}</ref>)
<div id="1E20"/>
|-
|[[100
|100 Em
|12,000
|thickness of [[Milky Way Galaxy]]'s gaseous disk<ref>{{cite web|url=http://news.smh.com.au/milky-way-fatter-than-first-thought/20080220-1tbv.html |title=Milky Way fatter than first thought |accessdate=2008-11-14 |date=2008-02-20 |work=[[The Sydney Morning Herald]] |publisher=[[Australian Associated Press]]}}</ref>
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|-
|rowspan=4|[[1
|rowspan=4|1 [[
|100,000
|diameter of galactic disk of [[Milky Way Galaxy]]<ref name="Burgess_and_Quevedo"/>
|-
Lyn 541:
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|-
|rowspan=2|[[10
|rowspan=2|10 Zm
| 22.3 Zm = 2.36
|distance to [[Andromeda Galaxy]]
|-
Lyn 550:
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|-
|[[100
|100 Zm
|300–600 Zm = 10–20 [[megaparsecs]]
Lyn 556:
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|-
|rowspan=2|[[1
|rowspan=2|1 [[
|200
|diameter of the [[Local Supercluster]] and the largest voids and filaments.
|-
|550
|diameter of the enormous [[Horologium Supercluster]] <ref>http://www.atlasoftheuniverse.com/superc/hor.html The Horologium Supercluster</ref>
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|-
|[[10
|10 Ym
|1.37
|Length of the [[Sloan Great Wall]], a giant wall of galaxies ([[galactic filament]].<ref>[http://arxiv.org/abs/astro-ph/0310571 J. R. Gott III ''et al.'', ''Astrophys. J.'', '''624''', 463 (2005).] Figure 8 – "Logarithmic Maps of the Universe" – is available as a poster from [http://www.astro.princeton.edu/~mjuric/universe/ the homepage of Mario Juric.]</ref>
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|-
|rowspan=2|[[100
|rowspan=2|100 Ym
|1{{E|10}}
|estimated [[Distance measures (cosmology)|light travel distance]] to certain [[quasars]]
|-
|92{{E|9}}
|approx. diameter ([[comoving distance]]) of the [[visible universe]]<ref name="Burgess_and_Quevedo"/>
|-
|10<sup>27</sup>
|1000 Ym
|~250
|According to one estimate using the [[WMAP]] data,<ref>http://arxiv.org/abs/astro-ph/0605709v2 How Many Universes Do There Need To Be?</ref> it can be said with 95% confidence that there is a lower limit of 21 [[particle horizon]] size patches in the universe.
|-
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