How are planets formed?

January 30, 2015 by Elizabeth Howell, Universe Today
This artist’s conception shows a newly formed star surrounded by a swirling protoplanetary disk of dust and gas. Credit: University of Copenhagen/Lars Buchhave

How did the Solar System's planets come to be? The leading theory is something known as the "protoplanet hypothesis", which essentially says that very small objects stuck to each other and grew bigger and bigger—big enough to even form the gas giants, such as Jupiter.

But how the heck did that happen? More details below.

Birthing the Sun

About 4.6 billion years ago, as the goes, the location of today's Solar System was nothing more than a loose collection of gas and dust—what we call a . (Orion's Nebula is one of the most famous examples you can see in the .)

Then something happened that triggered a pressure change in the center of the cloud, scientists say. Perhaps it was a supernova exploding nearby, or a passing star changing the gravity. Whatever the change, however, the cloud collapsed and created a disc of material, according to NASA.

The center of this disc saw a great increase in pressure that eventually was so powerful that loosely floating in the cloud began to come into contact. Eventually, they fused and produced helium, kickstarting the formation of the Sun.

The Sun was a hungry youngster—it ate up 99% of what was swirling around, NASA says—but this still left 1% of the disc available for other things. And this is where began.

The Orion Nebula. Credit: Vasco Soeiro
Time of chaos

The Solar System was a really messy place at this time, with gas and dust and debris floating around. But planet formation appears to have happened relatively rapidly. Small bits of dust and gas began to clump together. The young Sun pushed much of the gas out to the outer Solar System and its heat evaporated any ice that was nearby.

Over time, this left rockier planets closer to the Sun and gas giants that were further away. But about four billion or so years ago, an event called the "late heavy bombardment" resulted in small bodies pelting the bigger members of the Solar System. We almost lost the Earth when a Mars-sized object crashed into it, as the theory goes.

What caused this is still under investigation, but some scientists believe it was because the were moving around and perturbing smaller bodies at the fringe of the Solar System. At any rate, in simple terms, the clumping together of protoplanets (planets in formation) eventually formed the planets.

We can still see leftovers of this process everywhere in the Solar System. There is an asteroid belt between Mars and Jupiter that perhaps would have coalesced into a planet had Jupiter's gravity not been so strong. And we also have comets and asteroids that are sometimes considered referred to as "building blocks" of our Solar System.

We've described in detail what happened in our own Solar System, but the important takeaway is that many of these processes are at work in other places. So when we speak about exoplanet systems—planets beyond our Solar System—it is believed that a similar sequence of events took place. But how similar is still being learned.

These images are some of the first to be taken during Spitzer’s warm mission — a new phase that began after the telescope, which operated for more than five-and-a-half years, ran out of liquid coolant. They show a star formation region (DR22 in Cygnus),DR22, in the constellation Cygnus the Swan. Credit: NASA / JPL-Caltech
Making the case

One major challenge to this theory, of course, is no one (that we know of!) was recording the early history of the Solar System. That's because the Earth wasn't even formed yet, so it was impossible for any life—let alone intelligent life—to keep track of what was happening to the planets around us.

There are two major ways astronomers get around this problem. The first is simple observation. Using powerful telescopes such as the Atacama Large Millimeter/submillimeter Array (ALMA), astronomers can actually observe dusty discs around young planets. So we have numerous examples of stars with planets being born around them.

Artist’s impression of a Mars-sized object crashing into the Earth, starting the process that eventually created our Moon. Credit: Joe Tucciarone

The second is using modelling. To test their observational hypotheses, astronomers run computer modelling to see if (mathematically speaking) the ideas work out. Often they will try to use different conditions during the simulation, such as perhaps a passing star triggering changes in the dust cloud. If the model holds after many runs and under several conditions, it's more likely to be true.

That said, there still are some complications. We can't use modelling yet to exactly predict how the planets of the Solar System ended up where they were. Also, in fine detail our Solar System is kind of a messy place, with phenomena such as asteroids with moons.

And we need to have a better understanding of external factors that could affect planet formation, such as supernovae (explosions of old, massive stars.) But the protoplanet hypothesis is the best we've got—at least for now.

Artist’s impression of the Solar Nebula. Credit: NASA
How are planets formed?
This animation, created from individual radar images, clearly show the rough outline of 2004 BL86 and its newly-discovered moon. Credit: NASA/JPL-Caltech

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antialias_physorg
5 / 5 (7) Feb 02, 2015
Only in a world of math could Jupiter have moons which would supposedly form by this process also...apparently unimpeded by Jupiters gravity,

What says they formed there?

Also the mechanism is different. Its moons are in orbit around it. Stuff can coalesce when it's in orbit around other stuff (e.g. planets in our solar system). But when you have massive stuff moving PAST other massive stuff (e.g. a planet like Jupiter moving past a ring of gas/rubble) things look different. Such an action tends to smear out the mass along the the orbit relative to their common center of orbit (i.e. the sun).
cjn
5 / 5 (5) Feb 02, 2015
Such an action tends to smear out the mass along the the orbit relative to their common center of orbit (i.e. the sun).


Yep, you see with Ceres and Vesta that the accretion can occur in the Asteroid belt, but that there is/was an external factor great enough to prohibit coalescence of the belt matter into a "planet". I think physics/math and reason would point to Jupiter as the influence, as it is both large enough and "close" enough to impact planet formation. I'm not sure what alternative reset is proposing, but planetary gravity in Jovian orbit > solar gravity for moon creation -no conundrum here.
cjn
5 / 5 (5) Feb 02, 2015
reset:
"I think physics/math and reason would point to Jupiter" - Nope...just math.


Alright, propose an alternative. Enlighten us on your model of the universe.
viko_mx
1 / 5 (2) Feb 02, 2015


The main theory for the formation of star systems are so imperfect that no longer be accepted in kindergarten. Within a radius of a few light years around the solar system there are no remnants of protocloud or super novae that may be caused compression (or blowing apart) of proto cloud. What caused the rotation of the sun, the planets and the moons in the solar system? How have emerged so different in chemical composition and physical structure solid satellites orbiting gas giants and why are exactly on this location?

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