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A team at the 91±¬ΑΟ and the University of Bern has computationally simulated more than 200,000 hypothetical Earth-like worlds all in orbit of stars like our sun. As they report in a paper accepted to the Planetary Science Journal and submitted Dec. 6 to the preprint site arXiv, on these simulated exoplanets, one common feature of present-day Earth was often lacking: partial ice coverage. About 90% of these potentially habitable hypothetical worlds lacked partial surface ice like polar caps.

Aspects of an otherwise Earthlike planet’s tilt and orbital dynamics can severely affect its potential habitability β€” even triggering abrupt β€œsnowball states” where oceans freeze and surface life is impossible, according to new research from 91±¬ΑΟ astronomers.

The world’s attention is now on Proxima Centauri b, a possibly Earth-like planet about 4.22 light-years away. It’s in its star’s habitable zone — but could it in fact be habitable? If so, the planet evolved very different than Earth, say researchers at the 91±¬ΑΟ-based Virtual Planetary Laboratory.

New research by 91±¬ΑΟ astronomer Rory Barnes and co-authors describes possible planetary systems where a gravitational nudge from one planet with just the right orbital configuration and tilt could have a mild to devastating effect on the orbit and climate of another, possibly habitable world.