Image credit: NASA/JPL/STScI
Scientists have always wondered how Uranus got tilted so much that it
spins on its side, and now research on the planet’s early formation
gives us new insight. Four billion years ago, scientists believe a young
proto-planet of rock and ice collided with Uranus, causing its extreme
tilt. Instead of rotating like a top spinning nearly upright, as Earth
does, the planet “rolls” on its side as it circles the sun.
The research team, led by Durham University, UK, in collaboration
with scientists at NASA's Ames Research Center in Silicon Valley, used
advanced computing techniques to create the most detailed simulation to
date of the suspected impact.
A simulation of the most likely Uranus-impact
scenario that caused today’s tilted orbit, according to new, highly
detailed simulations. Light gray represents ice materials from Uranus,
while dark gray represents rock materials from Uranus. Purple represents
ice materials from the impactor, while brown represents rock from the
impactor. Light blue represents Uranus’ atmosphere. Credits: Jacob Kegerreis / Durham University
Through more than 50 simulations of impact scenarios using a supercomputer, this research group determined that an object at least twice the mass of Earth likely impacted the young planet with a grazing blow. The collision was so strong it reshaped the entire planet and pushed it onto its side. But, the collision was likely not strong enough to blast the planet’s atmosphere off into space or significantly change its orbit around the Sun. This research was the first of its type to take the planet’s atmosphere into account in its simulations of the impact. This helped the scientists better define what that event might have looked like.
The impact might have left molten ice and lopsided lumps of rock
within the planet, perhaps explaining its tilted and off-center magnetic
field, too. Rock and ice thrown into orbit would have then clumped
together to form the rings and moons around Uranus, now in its newly
established rotation.
But this discovery goes beyond explaining how Uranus became what it
is today. It helps us on our search to understand other planets outside
our solar system – exoplanets. Uranus is a medium-size, gaseous planet
with a rocky and icy core. Based on findings from the Kepler space
telescope, the more common type of exoplanet is very similar to Uranus.
Learning about this impact helps us understand how similar collisions
lead to the formation of other planets, and what this means for their
ability to support life.
The findings, published in The Astrophysical Journal,
paint a riveting picture of Uranus’ early tumultuous years, and gives
us the tools to understand planets like it throughout the cosmos.
Author: Frank Tavares
Members of the news media interested in learning more about this research should refer to the NASA Ames Media Contacts page to get in touch.
Editor: Abigail Tabor
