The study came at the heels of a previous study led by Durham University in the U.K., which posited that enormous impacts during the late stages of a planet’s formation could have wide-ranging effects on a young planet’s atmosphere. That study’s researchers said that the impactor’s mass, size, speed and angle upon impact are key considerations when calculating collision outcomes. For the latest research, the team adjusted for those four variables, besides the impactor’s density and whether it was made of iron, rock or both.
“We ran hundreds of different scenarios for many different colliding planets, showing the varying impacts and effects on a planet’s atmosphere depending upon a number of factors,” said lead author Jacob Kegerreis, a professor at the Institute for Computational Cosmology at Durham University.
Previous research suggested that the moon likely formed following a collision between young Earth and a giant impactor estimated to be the size of Mars around 4.5 billion years ago. The simulations showed that Earth might have had lost anywhere between 10 to 60 percent of its atmosphere due to that collision.
But it could also go the other way: A collision with a giant impactor that had a thick atmosphere and traveled at a slower rate could add a lot of atmosphere to a planet.
“This major suite of planetary simulations also sheds light on the role of impacts in the evolution of Earth-like exoplanets,” said co-author Luis Teodoro, a professor at the School of Physics and Astronomy at the University of Glasgow.While the study couldn’t directly explain how the moon was created, the simulations could provide crucial insights into the origin of Earth's closest celestial neighbor, added Kegerreis.
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