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Extreme trans-Neptunian objects lead the way to Planet Nine

In the race towards the discovery of Planet Nine, scientists from around the world strive to calculate its orbit using the tracks left by the small bodies that move well beyond Neptune. Now, astronomers from Spain and Cambridge University have confirmed that the orbits of the six extreme trans-Neptunian objects that served as a reference to announce the existence of Planet Nine are not as stable as originally thought.

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Understanding stellar adolescence through T-Tauri stars

A newborn star typically goes through four stages of adolescence. It begins life as a protostar, accreting material and developing a proto-planetary disc. Slowly, stellar winds and radiation blow away the surrounding shell of gas and dust. Next, when the surrounding envelope has cleared, is called the T-Tauri phase. Finally, accretion stops and the source’s radiation comes from the star’s photosphere.

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Cloudy days on exoplanets may hide atmospheric water

Water is a hot topic in the study of exoplanets, including “hot Jupiters” close to their parent stars that can reach a scorching 1,100 °C, meaning any water they host would take the form of vapour. Hot Jupiters have been found with water in their atmospheres, but others appear to have none. NASA scientists wanted to find out what the atmospheres of these giant worlds have in common.

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Universe’s first life might have been born on carbon planets

Our Earth consists of silicate rocks and an iron core with a thin veneer of water and life, but the first potentially habitable worlds to form might have been very different. New research suggests that the early universe might have contained carbon planets consisting of graphite, carbides, and diamond. Astronomers might find these diamond worlds by searching a rare class of stars.