This artist’s view shows the hot Jupiter exoplanet 51 Pegasi b, which orbits a star about 50 light-years from Earth. In 1995, 51 Pegasi b became the first exoplanet to be found around a sunlike star; now, it is the first alien world to be be directly detected spectroscopically in visible light.

Astronomers have detected an exoplanet's visible-light spectrum directly for the first time ever, a milestone that could help bring many other alien worlds into clearer focus down the road.

The scientists used the HARPS instrument on the European Southern Observatory's 3.6-meter telescope at the La Silla Observatory in Chile to study the spectrum of visible light reflected off the exoplanet 51 Pegasi b, which lies about 50 light-years from Earth in the constellation Pegasus. You can see a new video of 51 Pegasi b and its environs here on Space.com.

51 Pegasi b, a "hot Jupiter" gas giant that orbits close to its parent star, was spotted in 1995, when it became the first alien world ever discovered around a sunlike star. (The first exoplanets of any type were found in 1992 around a superdense, rotating stellar corpse called a pulsar.) [Gallery: The Strangest Alien Planets]

Researchers most often study exoplanet atmospheres by analyzing the starlight that passes through them when worlds cross their stars' faces from Earth's perspective. This method, known as transit spectroscopy, is restricted to use on systems in which the stars and planets align.

This chart shows the large northern constellation of Pegasus. The faint star 51 Pegasi, which is circled in red and can be dimly seen with the naked eye, is orbited by 51 Pegasi b, the first exoplanet ever discovered around a normal star. (Image credit: ESO, IAU and Sky & Telescope)

The new strategy used with 51 Pegasi b, on the other hand, does not depend on planetary transits and could thus find broader applicability, researchers said.

The technique offers other scientific advantages as well.

“This type of detection technique is of great scientific importance, as it allows us to measure the planet’s real mass and orbital inclination, which is essential to more fully understand the system," study lead author Jorge Martins, of the Instituto de Astrofísica e Ciências do Espaço (IA) and the Universidade do Porto in Portugal, said in a statement.

"It also allows us to estimate the planet’s reflectivity, or albedo, which can be used to infer the composition of both the planet’s surface and atmosphere," Martins added.

The new data suggest that 51 Pegasi b is highly reflective, a bit larger in diameter than Jupiter and about half as massive as our solar system's biggest planet, researchers said.

Image showing the sky around the star 51 Pegasi in the northern constellation of Pegasus. This image was created from photographic material forming part of the Digitized Sky Survey 2. (Image credit: ESO/Digitized Sky Survey 2)

The new observations by HARPS (which is short for High Accuracy Radial velocity Planet Searcher) provide a vital proof of concept for the new technique, which could really come into its own when employed with instruments on bigger telescopes, such as the European Southern Observatory's Very Large Telescope (VLT), researchers said.

"We are now eagerly awaiting first light of the ESPRESSO spectrograph on the VLT so that we can do more detailed studies of this and other planetary systems,” said co-author Nuno Santos, also of the IA and Universidade do Porto.

The new study was published today (April 22) in the journal Astronomy & Astrophysics.

Follow Mike Wall on Twitter @michaeldwall and Google+. Follow us @Spacedotcom, Facebook or Google+. Originally published on Space.com.