ᱥᱤᱧ ᱪᱟᱸᱫᱚ ᱢᱟᱱᱰᱮᱨ: ᱨᱮᱱᱟᱜ ᱫᱚᱦᱲᱟᱭᱮᱱ ᱛᱟᱞᱟᱨᱮᱭᱟᱜ ᱯᱷᱟᱨᱟᱠ ᱠᱚ

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{{Infobox planetary system
| title = Solar System
| image = Planets2013.svg
| image_alt = A representative image of the Solar System with sizes, but not distances, to scale
| image_size = 340px
| caption = {{longitem|The [[Sun]] and [[Planets of the solar system|planets]]<br />''(distances not to scale)''|style=padding:8px 0 10px 0;}}
| age = 4.568&nbsp;billion years
| location = {{longitem|{{ublist|class=nowrap |[[Local Interstellar Cloud]], [[Local Bubble]], |[[Orion–Cygnus Arm]], [[Milky Way]]}}}}
| system_mass = 1.0014 [[Solar mass]]es
| neareststar = {{longitem|{{ublist|class=nowrap |[[Proxima Centauri]]{{nbsp|2}}{{smaller|(4.25 [[Light-year|ly]])}} |[[Alpha Centauri]] {{smaller|(4.37 ly)}}}}}}
| nearestplanetary = {{nowrap|[[Proxima Centauri]] system{{nbsp|2}}{{smaller|(4.25 ly)}}}}
| semimajoraxis = {{nowrap|30.10 [[Astronomical unit|AU]]{{nbsp|2}}{{smaller|(4.503&nbsp;billion km)}}}}
| Kuiper_cliff = 50 AU
| noknown_stars = yes
| stars = 1{{nbsp|2}}{{smaller|([[Sun]])}}
| planets = {{longitem|{{hlist|style=font-size:90%|8&nbsp;([[Mercury (planet)|Mercury]]|[[Venus]]|[[Earth]]|[[Mars]]|<br />[[Jupiter]]|[[Saturn]]|[[Uranus]]|[[Neptune]])}}}}
| outerplanetname = [[Neptune]]
| dwarfplanets = {{longitem|Three universally accepted{{hlist|style=font-size:90%|([[Ceres (dwarf planet)|Ceres]]|[[Pluto]]|[[Eris (dwarf planet)|Eris]])}} two named by the [[International Astronomical Union|IAU]] under the expectation they will prove to be{{hlist|style=font-size:90%|([[Haumea]]|[[Makemake]])}}}}
| satellites = {{longitem|575 {{hlist|{{smaller|(185 planetary<ref name="JPLbodies">{{cite web|title=How Many Solar System Bodies |publisher=NASA/JPL Solar System Dynamics |url=http://ssd.jpl.nasa.gov/?body_count |accessdate=20 April 2018}}</ref>}} |{{smaller|390 [[minor planet]]ary<ref name="MPMJohnston">{{cite web|date=15 September 2019|title=Asteroids with Satellites |publisher=Johnston's Archive |author=Wm. Robert Johnston |url=http://www.johnstonsarchive.net/astro/asteroidmoons.html |accessdate=28 September 2019}}</ref>)}}}}}}
| minorplanets = 796,354{{nbsp|2}}{{smaller|(as of 2019-08-27)<ref name=MPCSummary/>}}
| comets = 4,143{{nbsp|2}}{{smaller|(as of 2019-08-27)<ref name=MPCSummary>{{cite web|url=https://minorplanetcenter.net/mpc/summary|title=Latest Published Data|website=The International Astronomical Union Minor Planet Center|accessdate=28 September 2019}}</ref>}}
| roundsat = 19 (5 or 6 likely to be in [[hydrostatic equilibrium]])
| roundsatlink = Planetary-mass moon
| inclination = 60.19°{{nbsp|2}}{{smaller|(ecliptic)}}<!---If anyone can find a cited value for the inclination of the Solar System's invariable plane to the galactic plane, please replace this value--->
| galacticcenter = 27,000&thinsp;±&thinsp;1,000 ly
| orbitalspeed = 220 km/s
| orbitalperiod = 225–250 [[Myr]]
| spectral = [[G-type main-sequence star|G2V]]
| frostline = ≈5 AU<ref name="Mumma">{{Cite journal | last1 = Mumma | first1 = M.J. | last2 = Disanti | first2 = M.A. | last3 = Dello Russo | first3 = N. | last4 = Magee-Sauer | first4 = K. | last5 = Gibb | first5 = E. | last6 = Novak | first6 = R. | doi = 10.1016/S0273-1177(03)00578-7 | title = Remote infrared observations of parent volatiles in comets: A window on the early solar system | journal = Advances in Space Research | volume = 31 | issue = 12 | pages = 2563–2575 | year = 2003 | pmid = | pmc = |bibcode = 2003AdSpR..31.2563M | citeseerx = 10.1.1.575.5091 }}</ref>
| heliopause = ≈120 AU
| hillsphere = ≈1–3 ly
}}
{{Solar System navbox}}
 
''' ᱥᱤᱧ ᱪᱟᱸᱫᱚ ᱢᱟᱱᱰᱮᱨ'''