It’s not easy to capture images of objects in the night sky, as they’re so very far away. So, when astronomers do get good ones, you can be sure that they’ll let everyone know. And, that’s what’s happened this month over at the Universidad Catolica del Norte in Chile.  Using ESO‘s Very Large Telescope Interferometer (VLTI) at the Paranal Observatory in Chile, a team of astronomers led by Keiichi Ohnaka captured the best image that we’ve ever seen of the surface and atmosphere of a star, Antares, other than that of the sun.


Using ESO’s Very Large Telescope Interferometer astronomers have constructed this remarkable image of the red supergiant star Antares. This is the most detailed image ever of this object or any other star apart from the Sun.

The VLTI is rather unique in what it can do as it has the ability to combine light from up to four telescopes in which to create a 200-meter virtual telescope. This allows it to see far more than any other single telescope could. As Ohnaka explains, “The VLTI is the only facility that can directly measure the gas motions in the extended atmosphere of Antares – a crucial step towards clarifying this problem. The next challenge is to identify what’s driving the turbulent motions.”

Using ESO’s Very Large Telescope Interferometer astronomers have constructed this remarkable map of the motions of material on the surface of the red supergiant star Antares. This is the first such velocity map of any star other than the Sun. In red regions, the material is moving away from us and in the blue areas, the material is approaching. The empty region around the star is not a real feature but shows where velocity measurements were not possible.


Antares is a red supergiant with a mass of about 12 times that of the Sun with a diameter about 700 times larger. According to experts, it has shed three solar-masses of material during its lifetime. Armed with the new results, the team created a 2D velocity map of a star’s atmosphere using the VLTI. The data they gathered was used to calculate the difference between the speed of the atmospheric gas various points on the star and the average speed across the whole star. The final result was the first ever map of the relative speed of atmospheric gas across the whole of Antares.

“In the future, this observing technique can be applied to different types of stars to study their surfaces and atmospheres in unprecedented detail,” says Ohnaka. “Our work brings stellar astrophysics to a new dimension and opens an entirely new window to observe stars.”


This chart shows the prominent constellation of Scorpius (The Scorpion). At the heart of this very striking grouping of stars lies the bright red supergiant star Antares.

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