In a study published this week in the journal Nature Astronomy, scientists described how they used the National Science Foundation’s Karl G. Jansky Very Large Array radio telescope to observe a star called YZ Ceti. It’s located about 12 lightyears from Earth and is classified as a red dwarf. This type of star is dimmer, cooler, and smaller than our own, but the havoc it could cause to a planet’s atmosphere is no less severe.
Its known exoplanet called YZ Ceti is a rocky planet about 70% the size of Earth, but it orbits its star much, much closer, completing a revolution every two days. While scientists were analyzing the radio waves coming from this star, they picked up occasional brighter bursts, and one likely explanation is that the planet has a strong magnetic field.
A planetary magnetic field like this could help an exoplanet to retain an atmosphere, like Earth’s. On planet, scientists observed interactions between the magnetic field and the sun’s radiation in the form of auroras — the aurora borealis in the northern hemisphere and the aurora australis in the southern hemisphere. And if YZ Ceti has its atmosphere, then these magnetic interactions would result in a similar phenomenon on that planet. While this is a first-of-its-kind observation, scientists are hopeful to refine the technique and point telescopes at other stars and planets in the future.