Gemini Planet Imager (GPI): New imaging technique reveal planets near bright stars

The GPI is mounted on mounted on a side port of the instrument support structure of the Gemini South telescope. 

Credit: Gemini Planet Observatory

The Gemini Planet Imager (GPI) was built for one purpose: imaging extrasolar planets.

In the seven months since it came online, GPI is proving to be an order-of-magnitude improvement-so much so that it may rewrite the rules of planet-hunting.

Planet-hunting bears some similarity to tracking a rare species through the jungle.

There are a variety of ways to know that it's there, most of which are indirect: The leaves rustling. The undergrowth is trampled. The animal's shadow appears for a fleeting moment before it fades away again.

It is much the same with planets. We can detect them moving their parent planets ever-so-slightly via Doppler shift.

GPI functioning testbed system

We can see the light from that star dim as an exoplanet-or the planet's shadow-passes in front of it.

Once in a while, a young star's dust disk will have a gap in it, from which we infer the presence of a formed or forming planet.

These detection methods have allowed us to catalog over 1700 exoplanets since 1994.

Naturally, ultimate achievement in observation is to see the species or the planet with our own eyes.

That's what the Gemini Planet Imager (GPI) does best: direct detection of exoplanets.

Technically, direct detection means spatially resolving the light of a planet from the light of its parent star: taking a picture of the planet itself.

Before GPI, there were serious limitations to our ability to photograph an exoplanet.

Optical design of the GPI science camera.

The photographic exposure had to be long and the contrast between the star and the exoplanet had to be high. With GPI, what used to be a one-hour photo has become a one-minute photo.

The contrast can be three orders of magnitude lower - the planet can be 1000 times dimmer - and the photo will still turn out.

Micro-Electro-Mechanical Systems (MEMS) mirrors

This remarkable improvement in exoplanet imaging is achieved with a variety of new technologies: for example, deformable silicon Micro-Electro-Mechanical Systems (MEMS) mirrors.

The mirrors can bend and flex in ways that counters atmospheric distortion.

GPI also has a diffraction-suppressing coronagraph, which blocks the light from the parent star so that the planet can be seen more clearly, and an integral field spectrograph, which allows spectra to be taken over an entire two-dimensional field of the sky.

By combining these and other related technologies, images like the now-famous photo of Beta Pictoris b are produced.

They reveal planets many dozens of light years away glowing with residual radiation from their formations millions of years ago.

The bright white dot is the planet Beta Pictoris b, glowing in the infrared light from the heat released when it was formed 10 million years ago. 

The bright star Beta Pictoris b is hidden behind a mask at the center of the image. 

Credit: GPI

GPI can also supply information about the exoplanet's atmospheric composition and interactions with nearby objects such as asteroid belts.

GPI was deployed on the 8-m Gemini South telescope in Chile. Its first image or "first light" took place in November 2013.

Since then, GPI has done an unprecedented job of capturing Jupiter-sized objects around stars similar to our Sun.