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Asteroseismology reveals magnetic fields deep within stars

Astronomers have for the first time probed the magnetic fields in the mysterious inner regions of stars, finding they are strongly magnetised. Using a technique called asteroseismology, the scientists were able to calculate the magnetic field strengths in the fusion-powered hearts of dozens of red giants, stars that are evolved versions of our Sun.

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VLA reveals spectacular “haloes” of spiral galaxies

An international team of astronomers used the Karl G. Jansky Very Large Array (VLA) to investigate 35 edge-on spiral galaxies at distances from 11 million to 137 million light-years from Earth. The study has revealed that “haloes” of cosmic rays and magnetic fields above and below the galaxies’ discs are much more common than previously thought.

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IRIS and Hinode: a stellar research team

NASA’s Interface Region Imaging Spectrograph satellite, or IRIS, and the Japan Aerospace Exploration Agency’s (JAXA)/NASA’s Hinode solar observatory, have just made a significant step towards understanding why the corona — the outermost, wispy layer of the Sun’s atmosphere — is hundreds of times hotter than the lower photosphere, which is the Sun’s visible surface.

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Sharp-eyed ALMA spots a flare on famous red giant star

Observations with the Atacama Large Millimetre/submillimetre Array (ALMA) have revealed what seems to be a gigantic flare on the surface of Mira, one of the closest and most famous red giant stars in the sky. Activity like this in red giants — similar to what we see in the Sun — comes as a surprise to astronomers.

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The seasons of the Sun

A team of researchers has determined that the Sun undergoes a type of seasonal variability with its activity waxing and waning over the course of nearly two years. This behaviour affects the approximately 11-year solar cycle, sometimes amplifying solar storms that can buffet Earth’s atmosphere.