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Are planets in the solar system that are closer to the Sun older than the ones further away? – Gavriel, age 10, Paducah, Kentucky
A cloud of collapsing gas created our Sun, the first thing to form in our solar system. This happened about 4½ billion years ago.Then the planets began to emerge, as the billions of particles of gas and dust left over from the Sun’s formation became a flattened disk.
Known as a protoplanetary disk, it was enormous and surrounded the Sun for billions of miles. Within the disk, the gas and dust particles started to collide, solidify and stick together, like snowflakes clumping together to form snowballs.
As the particles clung together, the microscopic grains became pebble-size objects and then grew and grew. Some became rocks the size of baseballs, others the size of a house, and a few as big as a planet.
This process, called accretion, is how everything in the solar system – planets, moons, comets and asteroids – came into being.
The ice line
By studying computer models and observing the creation of other star systems, astronomers like us have learned a lot about the early days of our solar system.
When the Sun was still forming and the protoplanetary disk was making planets, there was a distance from the Sun where it was cold enough for ice to gather. That place, the ice line – sometimes called the snow line – was in what’s now the asteroid belt, which is between Mars and Jupiter.
Today, of course, ice is found on almost every planet, even on Mercury. But back then, only the young protoplanets beyond the ice line were cold enough to have it. The ice, gas and dust, slamming into each other for millions of years, accumulated into enormous bodies that ultimately became giant planets – Jupiter, Saturn, Uranus and Neptune.
While all this was happening, the smaller planets inside the ice line were forming too. But with less raw material to work with, Mercury, Venus, Earth and Mars took much longer.
Today, it’s believed that Jupiter and Saturn, the largest planets, were the first to fully form, both within a few million years. Uranus and Neptune were next, within 10 million years. The inner planets, including Earth, took at least 100 million years, maybe more.
To put it another way, the four planets closest to the Sun are the youngest; the two planets farthest out, the next youngest; and the two in between, the oldest. The difference in age between the youngest and oldest planets is perhaps 90 million years.
That sounds like an enormous age difference, but in space, 90 million years isn’t really that long – less than 1% of the total time the universe has been around. One way to consider it: Think of Earth as a little sister with a big brother, Jupiter, who’s 2 or 3 years older.
Location, location, location
Soon after formation the giant worlds began to migrate, moving inward toward the Sun or outward away from the Sun, before finally settling into their final orbits.
For instance, Neptune migrated outward, switching places with Uranus, and pushed a lot of the small, icy bodies into the Kuiper Belt, a place in the outer solar system that’s home to dwarf planets Pluto, Eris and Makemake and millions of comets.
Meanwhile, Jupiter moved inward, and its massive gravity forced some forming planets into the Sun, where they disintegrated. Along the way, Jupiter flung some smaller rocks out of the solar system altogether; the rest went to the asteroid belt.
But most critically, as Jupiter settled into its own orbit, it moved all of the forming objects and likely finalized the location of the remaining inner planets, including Earth.
All of Jupiter’s tugging helped put our planet in the so-called “Goldilocks zone,” a place just the right distance from the Sun, where Earth could have liquid water on its surface and the right temperature for life to evolve. If Jupiter hadn’t formed the way it did, it’s entirely possible life would not have ignited on Earth – and we would not be here today.
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Christopher Palma, Teaching Professor of Astronomy & Astrophysics, Penn State and Lucas Brefka, Ph.D. Student in Astronomy & Astrophysics, Penn State
This article is republished from The Conversation under a Creative Commons license. Read the original article.
