Kadiz: Cudahiya di navbera guhartoyan de

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{{Infobox
| abovestyleawayêser = background:#30D5C8;
| aboveser = Kadiz, Riya Kadizê
| imagewêne = [[Wêne:Milky Way IR Spitzer.jpg|300px]]
| captionsernûçe = Wêneyekî înfraroj ê ku tê de dendika Riya Kadizê diyar e.
| titlestyleawayêsernav = background: #30D5C8;
| headerstyleçînasernivîs = background: #30D5C8;
| belowstyleawayêbin = background: #30D5C8;
| labelstyleawayêetîket = background: inherit;
| header1 sernivîs1 = Observation datadane
| label2etîket2 = [[Galaxy morphological classification|Type]]
| data2dane2 = SBbc ([[barred spiral galaxy]])
| label3etîket3 = Diameter
| data3dane3 = 100,000 light years
| label4etîket4 = Stûrî
| data4dane4 = 12,000 light years (gas)<ref>{{cite web
| title = The Milky Way is twice the size we thought it was
| work = University of Sydney News
| publisher = University of Sydney
| date = 2008-02-20
| url = http://www.usyd.edu.au/news/84.html?newsstoryid=2163
| accessdate = 2008-02-20}}</ref><br />1,000 light years (stars)
| label5etîket5 = Jimara stêrkê
| data5dane5 = 200 to 400 billion
| label6etîket6 = Stêrka herî kevn
| data6dane6 = 13.2 billion years
| label7etîket7 = Giranî
| data7dane7 = 5.8{{e|11}}&nbsp;[[solar mass|M<sub>☉</sub>]]
| label8etîket8 = [[Galactic Center|Sun's distance to galactic center]]
| data8dane8 = 26,000 ± 1400 light-years
| label9etîket9 = [[Sun|Sun's galactic rotation period]]
| data9dane9 = 220 million years (negative rotation)
| label10etîket10 = [[Density wave theory|Spiral pattern rotation period]]
| data10dane10 = 50 million years<ref name = gasdynamics>[http://arxiv.org/abs/astro-ph?papernum=0212516 [astro-ph/0212516&#93; Gas Dynamics in the Milky Way: Second Pattern Speed and Large-Scale Morphology<!-- Bot generated title -->]</ref>
| label11etîket11 = [[Barred spiral galaxy|Bar pattern rotation period]]
| data11dane11 = 15 to 18 million years<ref name=gasdynamics/>
| label12etîket12 = [[Cosmic microwave background|Speed relative to CMB rest frame]]
| data12dane12 = 552 km/s<ref name="dipole">{{cite journal
| author = Kogut, A.; Lineweaver, C.; Smoot, G. F.; Bennett, C. L.; Banday, A.; Boggess, N. W.; Cheng, E. S.; de Amici, G.; Fixsen, D. J.; Hinshaw, G.; Jackson, P. D.; Janssen, M.; Keegstra, P.; Loewenstein, K.; Lubin, P.; Mather, J. C.; Tenorio, L.; Weiss, R.; Wilkinson, D. T.; Wright, E. L.
| title = Dipole Anisotropy in the COBE Differential Microwave Radiometers First-Year Sky Maps
| journal = Astrophysical Journal
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| accessdate = 2007-05-10
| doi = 10.1086/173453 }}</ref>
| belowbin = ''binêre'': [[Galaksî]], [[List of galaxies]]
}}
'''Kadiz''' an '''Kehdiz''' an jî '''Riya Kadizê''' navê galaksiya ku tê de roj ye. Ku meriv şevên sawî (sayî) li ezmên dinêre gewraxîyeke dirêj xuya dibe, ji wê re dibêjin ''Kadiz''. Ew gewraxiya ji komeke stêrkan tê. Di Kadizê de di navbera 200 û 400 milyar stêrkî de hene.