Proxima Centauri tagged posts

Proxima Centauri’s no good, very bad day

An artist’s impression of a flare from Proxima Centauri, modeled after the loops of glowing hot gas seen in the largest solar flares. An artist’s impression of the exoplanet Proxima b is shown in the foreground. Proxima b orbits its star 20 times closer than the Earth orbits the Sun. A flare 10 times larger than a major solar flare would blast Proxima b with 4,000 times more radiation than the Earth gets from our Sun’s flares. Credit: Roberto Molar Candanosa / Carnegie Institution for Science, NASA/SDO, NASA/JPL.

An artist’s impression of a flare from Proxima Centauri, modeled after the loops of glowing hot gas seen in the largest solar flares. An artist’s impression of the exoplanet Proxima b is shown in the foreground. Proxima b orbits its star 20 times closer than the Earth orbits the Sun. A flare 10 times larger than a major solar flare would blast Proxima b with 4,000 times more radiation than the Earth gets from our Sun’s flares. Credit: Roberto Molar Candanosa / Carnegie Institution for Science, NASA/SDO, NASA/JPL.

Flare illuminates lack of a dust ring; puts habitability of Proxima b in question. Astronomers have detected a massive stellar flare – an energetic explosion of radiation – from the closest star to our own Sun, Proxima Centauri, which occurred last March...

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Another Close-by Planetary System?

This artist's impression shows how the newly discovered belts of dust around the closest star to the Solar System, Proxima Centauri, may look. ALMA observations revealed the glow coming from cold dust in a region between one to four times as far from Proxima Centauri as the Earth is from the Sun. The data also hint at the presence of an even cooler outer dust belt and indicate the presence of an elaborate planetary system. These structures are similar to the much larger belts in the Solar System and are also expected to be made from particles of rock and ice that failed to form planets. Note that this sketch is not to scale -- to make Proxima b clearly visible it has been shown further from the star and larger than it is in reality. Credit: ESO/M. Kornmesser

This artist’s impression shows how the newly discovered belts of dust around the closest star to the Solar System, Proxima Centauri, may look. ALMA observations revealed the glow coming from cold dust in a region between one to four times as far from Proxima Centauri as the Earth is from the Sun. The data also hint at the presence of an even cooler outer dust belt and indicate the presence of an elaborate planetary system. These structures are similar to the much larger belts in the Solar System and are also expected to be made from particles of rock and ice that failed to form planets. Note that this sketch is not to scale — to make Proxima b clearly visible it has been shown further from the star and larger than it is in reality. Credit: ESO/M. Kornmesser

ALMA discovers cold dust around ...

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Scientists take 1st Tentative Steps to explore Potential Climate of Proxima B

An artist’s impression of the surface of Proxima B. Image courtesy of ESO/M. Kornmesser

An artist’s impression of the surface of Proxima B. Image courtesy of ESO/M. Kornmesser

The quest to discover whether a planet orbiting our closest neighboring star, Proxima Centauri (4.2 light years or 25 trillion miles from Earth), has the potential to support life has taken a new, exhilarating twist. The planet was only discovered in August 2016, and is thought to be of similar size to Earth, creating the possibility that it could have an `Earth-like’ atmosphere. Scientists from the University of Exeter have embarked on their first, tentative steps to explore the potential climate of the exoplanet, known as Proxima B.

Early studies have suggested that the planet is in the habitable zone of its star Proxima Centauri...

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Planets of Red Dwarf Stars may face Oxygen Loss in Habitable zones

In this artist's concept, X-ray and extreme ultraviolet light from a young red dwarf star cause ions to escape from an exoplanet's atmosphere. Scientists have developed a model that estimates the oxygen ion escape rate on planets around red dwarfs, which plays an important role in determining an exoplanet's habitability. (screen shot from video) Credit: NASA Goddard/Conceptual Image Lab; Michael Lentz, animator/Genna Duberstein, producer

In this artist’s concept, X-ray and extreme ultraviolet light from a young red dwarf star cause ions to escape from an exoplanet’s atmosphere. Scientists have developed a model that estimates the oxygen ion escape rate on planets around red dwarfs, which plays an important role in determining an exoplanet’s habitability. (screen shot from video) Credit: NASA Goddard/Conceptual Image Lab; Michael Lentz, animator/Genna Duberstein, producer

The search for life beyond Earth starts in habitable zones could potentially allow liquid water to pool on a planet’s surface. New NASA research suggests some of these zones might not actually be able to support life due to frequent stellar eruptions from young red dwarf stars...

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