Skip to content
Tech News
← Back to articles

Planet orbits so close to its star that their magnetic fields connect

read original more articles
Why This Matters

The discovery of magnetic field interactions between a star and its closely orbiting exoplanet highlights new complexities in star-planet dynamics, which could influence our understanding of planetary habitability and magnetic protection. This finding emphasizes the importance of studying magnetic interactions in exoplanet systems, especially those with ultra-close orbits, as they may impact atmospheric retention and potential habitability for future exploration. For consumers and the industry, it underscores the evolving landscape of exoplanet research and the need for advanced detection and analysis tools.

Key Takeaways

For most of human history, our view of “close to the Sun” was defined by the orbit of Mercury, with its 88-day orbit and barren, baking surface. But from the moment we started discovering exoplanets, it became very clear that our own Solar System was anything but a guide to the rest of the galaxy. Planets with orbits only a few days long are strikingly common, with the proximity to the star creating things that seem bizarre from our perspective: metal vapor in the atmosphere, or atmospheres puffed out to ridiculously low densities.

Now, we can apparently add an additional oddity: overlapping magnetic fields. Researchers have found a star/planet combo that experiences periodic brightening, which they ascribe to the interactions between the magnetic fields of both bodies.

Looking for repetition

This is one of those cases where theory came before discovery. People had already proposed that a planet orbiting close to its host star could interact with it if its magnetic field were sufficiently strong. And, in a number of cases, researchers have found evidence that this is happening, with one case of an extremely young star emitting flares seemingly in response to the orbit of its innermost planet.

An international team of researchers has created the most comprehensive look at flaring in a star with a close-in planet. The star itself is called GJ 436, a red dwarf half the mass of the Sun that resides about 30 light-years from Earth. It has a single known exoplanet that is about four times as massive as Earth, and it completes an orbit every 2.6 days.