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If you ’ve ever gazed at a   model of thesolar organisation , you ’ve likely noticed that the sun , planets , synodic month and asteroids pose more or less on the same woodworking plane . But why is that ?

To do this question , we have to travel to the very beginning of the solar organization , about 4.5 billion years ago .

Life’s Little Mysteries

Artwork showing the planets orbiting the sun (from inner to outer): Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus and Neptune.

Back then , thesolar systemwas just a massive , spinning swarm of debris and gas , Nader Haghighipour , an uranologist at the University of Hawaii at Mānoa , severalize Live Science . That massive swarm measured 12,000 astronomical units ( AU ) across ; 1 AU is the average distance betweenEarthand the sunshine , or about 93 million miles ( 150 million kilometers ) . That swarm became so big , that even though it was just filled with dust and gun molecules , the cloud itself started to founder and shrink under its own mass , Haghighipour said .

Related : Why are galaxies different shape ?

As the spinning cloud of detritus and petrol started to collapse , it also flattened . Imagine a pizza pie Almighty throw a spinning slab of dough into the breeze . As it spin , the dough expands but becomes progressively thin and flat . That ’s what happen to the very early solar organization .

Artwork showing the planets orbiting the sun (from inner to outer): Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus and Neptune.

Artwork showing the planets orbiting the sun (from inner to outer): Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus and Neptune.

Meanwhile , in the plaza of this ever - flatten cloud , all those gas molecules got compress together so much , they fire up up , Haghighipour say . Under the vast heat and pressure , hydrogenandheliumatoms fuse and flush - startle a billions - of - years - long nuclear chemical reaction in the form of a baby sensation : the sun . Over the next 50 million age , the Lord’s Day continued to grow , gather up gas and detritus from its surroundings and belch out waves of vivid oestrus and irradiation . slow , the grow sunlight cleared out a halo of empty space around it .

As the sun grew , the cloud continued to collapse , form " a disk around the star [ that ] becomes categorical and flatter and expand and expands with the sun at the centerfield , " Haghighipour enunciate .

finally , the swarm became a prostrate bodily structure called a protoplanetary disk , orbiting the untested star . The disk extend century of AU across and was just one - one-tenth of that aloofness thick , Haghighipour sound out .

A diagram of the solar system

For tens of millions of twelvemonth thereafter , the junk mote in the protoplanetary disk softly swirl around , occasionally knocking into each other . Some even stuck together . And over those millions of yr , those molecule became millimeter - long grains , and those grains became centimeter - long pebble , and the pebble continued to collide and stick together .

— How long is a astronomical year ?

— How massive is the Milky Way ?

an image of the stars with many red dots on it and one large yellow dot

— Do other planets have solar eclipses ?

Eventually , most of the textile in the protoplanetary disk stuck together to form huge objects . Some of those object grew so big that gravity regulate them into spherical planet , dwarf planets andmoons . Other objects became on an irregular basis mould , like asteroid , comet and some small moons .

Despite these object ' unlike sizes , they stick around more or less on the same plane , where their building materials develop . That ’s why , even today , the solar system ’s eight planets and other celestial bodies orb on about the same level .

A composite image of the rings on Saturn, Uranus and Jupiter

earlier published on Live Science .

Multiple blue disks against a dark background.

The composite image shows seven of the solar system�s planets from Earth, after sundown on Feb. 22.

an image of Mercury

An image comparing the relative sizes of our solar system�s known dwarf planets, including the newly discovered 2017 OF201

an illustration showing a large disk of material around a star

An illustration of Jupiter showing its magnetic field

a photo of Venus� fiery surface

selfie taken by a mars rover, showing bits of its hardware in the foreground and rover tracks extending across a barren reddish-sand landscape in the background

images showing auroras on Jupiter

a person holds a GLP-1 injector

A man with light skin and dark hair and beard leans back in a wooden boat, rowing with oars into the sea

an MRI scan of a brain

A photograph of two of Colossal�s genetically engineered wolves as pups.

An illustration of an asteroid in outer space