Gemini Planet Imager First Light!http://www.gemini.edu/node/12113
Out of this world first light images emerge from Gemini Planet Imagerhttps://www.llnl.gov/news/newsreleases/2014/Jan/NR-14-01-01.html#.Usw_Z2RDtlM
STScI Astronomers Help Develop and Operate World's Most Powerful Planet Finderhttp://hubblesite.org/newscenter/archive/releases/2014/08/full/
World’s Most Powerful Planet Finder Turns its Eye to the Sky http://www.seti.org/seti-institute/press-release/worlds-most-powerful-planet-finder-gemini-planet-imager-first-light-images
L'imageur d'exoplanètes le plus puissant au monde entame sa missionhttp://www.nouvelles.umontreal.ca/recherche/sciences-technologies/20140107-limageur-dexoplanetes-le-plus-puissant-au-monde-entame-sa-mission.html
Museum-Built Device Helping Astronomers Search for Exoplanetshttp://www.amnh.org/explore/news-blogs/research-posts/museum-built-device-helping-astronomers-search-for-exoplanets
ASU professor, students part of Gemini Planet Imager teamhttps://asunews.asu.edu/20140107-gemini-planet-imager?utm_source=twitterfeed&utm_medium=twitter
El Espectrógrafo y Captador de Imágenes más poderoso del Mundo mira al cielo: la Primera Luz del Captador de Imágenes de Planetas de Geminihttp://www.seti.org/seti-institute/press-release/el-espectr%C3%B3grafo-y-captador-de-im%C3%A1genes-m%C3%A1s-poderoso-del-mundo-mira-al
World's most powerful exoplanet camera looks skywardhttp://news.ucsc.edu/2014/01/planet-imager.html
Powerful Planet Finder Turns Its Eye to the Skyhttp://www.jpl.nasa.gov/news/news.php?release=2014-008
The Gemini Planet Imager is the next generation adaptive optics instrument being built for the Gemini Telescope. The goal is to image extrasolar planets orbiting nearby stars. In 2011, the GPI Exoplanet Survey team was selected to carry out an 890-hour survey campaign from 2014 to 2016 to search and characterize exoplanets around ~600 stars.
WHO: GPI has been built by a consortium of U.S. and Canadian institutions, funded by the Gemini Observatory, which is an international partnership comprising the U.S.A., U.K., Canada, Australia, Argentina, Brazil & Chile. The GPIES campaign is partially funded by NSF, NASA, the University of California and the Laboratory Directed Research and Development funding at the Lawrence LIvermore National Laboratory.
WHEN: After more than 5 years of development (preliminary design review in May 2007 and critical design review (CDR) in May 2008, delta CDR in March, 2009, procurement and fabrication phase until 2011), one year of integration at UCSC LAO in 2013, the instrument was shipped to Chile in August 2013. The first light of the instrument was conducted in November 2013 and Science Operation will start in 2014.
WHERE: Initial deployment at Gemini South, a telescope with an 8-meter diameter mirror located on Cerro Pachon (Chilean Andes) at an altitude of 2,715 meters (9,000 feet). Later, GPI may also be used at the twin facility Gemini North, which is located on Mauna Kea, Hawaii.
WHY: GPI will detect DIRECTLY the light from an extrasolar planet to determine its mass and composition, with an ultimate goal of determining the nature of our own planetary system. Almost 1,000 extrasolar planets are known today, but mostly through indirect Doppler techniques that indicate the planet's mass and orbit or transit events that measure the planet's size and orbit. If we can directly pick out a planet from the star's glare, we can use spectroscopy to measure the planet's size, temperature, gravity, and even the composition of its atmosphere. By targeting many stars we will understand how common or unusual our own planetary system may be.
HOW: The GPI consortium built an advanced adaptive optics using silicon microchip deformable mirrors to remove atmospheric turbulence, and coronagraphic masks to block the diffracted light from the parent star.
WHAT: GPI will provide diffraction limited images between 0.9 and 2.4 microns. Bright natural guide stars (I<9.5 mag) are required for optimal performance of the GPI adaptive optics system. The system will be able to see objects ten million times fainter than their parent star at separations of 0.2-1 arcsecond in a 1-2 hour exposure. The science instrument will provide spectroscopy of any object observed. This allows us to detect warm planets (up to one billion years in age) through their infrared light. We can also measure the polarization of light to see faint disks of dust from other solar systems' comet and asteroid belts.
SO WHAT: GPI will produce the first comprehensive survey of giant exoplanets in the region where giant planets exist in our solar system - from 5 to 40 astronomical units radius. Dozens of these exoplanets will be bright enough for high signal-to-noise ratio spectroscopy, moving our studies of extrasolar planets into the realm of detailed astrophysics.
Beta Pictoris b is a giant planet – several times larger than Jupiter – and is approximately ten million years old. These near-infrared images (1.5-1.8 microns) show the planet glowing in infrared light from the heat released in its formation. The bright star Beta Pictoris is hidden behind a mask in the center of the images; a few scattered starlight artifacts, called ‘speckles,’ are also visible, but vastly fewer than in previous images. Beta Pictoris b is a giant planet – several times larger than Jupiter – and is approximately ten million years old. These near-infrared images (1.5-1.8 microns) show the planet glowing in infrared light from the heat released in its formation. The bright star Beta Pictoris is hidden behind a mask in the center of the images; a few scattered starlight artifacts, called ‘speckles,’ are also visible, but vastly fewer than in previous images. GPI image credit: Image processing by Christian Marois, NRC Canada.
Comparison of Europa observed with Gemini Planet Imager in K1 band on the right and visible albedo visualization based on a composite map made from Galileo SSI and Voyager 1 and 2 data (from USGS) on the left. While GPI is not designed for ‘extended’ objects like this, its observations could help in following surface alterations on icy satellites of Jupiter or atmospheric phenomena (e.g. clouds, haze) on Saturn’s moon Titan. The GPI near-infrared color image is a combination of 3 wavelength channels. Image credit: Processing by Marshall Perrin, Space Telescope, Science Institute and Franck Marchis, SETI Institute
Gemini Planet Imager’s first light image of the light scattered by a disk of dust orbiting the young star HR4796A. This narrow ring is thought to be dust from asteroids or comets left behind by planet formation; some scientists have theorized that the sharp edge of the ring is defined by an unseen planet. The left image (1.9-2.1 microns) shows normal light, including both the dust ring and the residual light from the central star scattered by turbulence in the Earth’s atmosphere. The right image shows only polarized light. Leftover starlight is unpolarized and hence removed from this image. The light from the front edge of the disk is strongly polarized as it scatters towards us. Image credit: Processing by Marshall Perrin, Space Telescope Science Institute
Simulation of the final image produced by GPI. A bright star is observed, but the light is greatly diminished due to the adaptive optics system and coronagraph. A faint point of light (circled) simulates the existence of a planet near the star.
Click for an animation of a simulated data cube. Each frame represents a small step in wavelength. Note how one planet (lower left of the star) winks in and out of the animation, while the other (above the star) gets brighter very slowly. This is how GPI will deliver near-infrared spectra of exoplanets.
GPI: A scientific partnership between institutions from the U.S.A., Canada, Australia, Argentina, Brazil and Chile.