For some 20 years, astronomers have been discovering exoplanets, or planets orbiting other stars, in various indirect fashions. These discoveries are just as scientific and valid as a visual observance, if not more so. But once in a while there’s a milestone that’s worth noting for the thrill as much as for the science. The first time we actually saw an exoplanet, i.e. directly imaged, in 2008 was one such example. Now we have the first official detection of an exoplanet’s visible light spectrum, courtesy of the HARPS planet-hunting machine and the ESO’s 3.6-meter telescope at the La Silla Observatory in Chile.
The exoplanet in question orbits the star 51 Pegasi, and is roughly 50 light-years away from Earth in the constellation Pegasus. What also makes this discovery noteworthy is that this exoplanet, 51 Pegasi b, is the first one we ever discovered back in 1995 that orbits a normal star like the Sun. For amateur astronomers, 51 Pegasi itself has an apparent magnitude of 5.49 — meaning you can *just* about see it without binoculars or a telescope if you’re under dark skies. Fortunately, we have much more sophisticated instrumentation available to us than the naked eye: