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The ‘topsy turvy’ ocean circulation of saline exoplanets

According to new research, the salt levels of oceans on distant Earth-like planets could have a major effect on their climates. Computer models reveal that exoplanets with very saline oceans could have circulation patterns opposite to that on Earth, resulting in dramatic warming of their polar regions, possibly extending their range of habitability.

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Astronomers discover white dwarf with an oxygen atmosphere

Researchers have discovered a white dwarf star with an atmosphere dominated by oxygen — a type of white dwarf that has been theorised to exist but not identified to date. The finding could challenge the textbook wisdom of single stellar evolution, and provide a critical link to some types of supernovae discovered over the past decade.

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Andromeda Galaxy’s first spinning neutron star found

Decades of searching in the Andromeda Galaxy has finally paid off, with the discovery of an elusive breed of stellar corpse — a neutron star, by ESA’s XMM-Newton space telescope. Neutron stars are the small and extraordinarily dense remains of a once-massive star that exploded as a powerful supernova at the end of its natural life.

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Global Astronomy Month begins 1 April

Global Astronomy Month (GAM), organised each April by Astronomers Without Borders, is the world’s largest annual global celebration of astronomy. Each GAM brings new ideas and new opportunities, and GAM 2016 is no exception, once again bringing enthusiasts together worldwide to celebrate Astronomers Without Borders’ motto: One People, One Sky.

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Map of rocky exoplanet reveals a lava world

An international team of astronomers, led by the University of Cambridge, has obtained the most detailed ‘fingerprint’ of a rocky planet outside our solar system to date, and found a planet of two halves: one that is almost completely molten, and the other which is almost completely solid. Exoplanet 55 Cancri e lies 40 light-years from the Sun.

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Trigger for Milky Way’s youngest supernova identified

Astronomers have used data from NASA’s Chandra X-ray Observatory and the VLA to determine the likely trigger for the most recent supernova in the Milky Way. They applied a new technique that could have implications for understanding other Type Ia supernovae, a class of stellar explosions that scientists use to determine the expansion rate of the universe.