MIT planetary scientists Julien de Wit and Sara Seager just devised a method that enables them to weigh an exoplanet by measuring the starlight that shines through its atmosphere. It’s so simple, it’s genius. See, when an exoplanet passes in front of its star, it causes a blip in the amount of light that shines toward Earth. This is actually how we’re able to discover exoplanets in the first place.
Not all of the starlight zooms past the exoplanet, though. Some is actually filtered through the atmosphere, and by measuring the spectrum of that light, the MIT scientists are able to learn all kinds of things about the planet, such as atmospheric pressure, temperature, and gravitational pull. With that information, they’ve come up with a new method for calculating not just atmospheric chemistry but a planet’s weight and mass.
via Gizmodo
