GPI

Eric Nielsen, formerly a post-doc at the SETI Institute and now a researcher at Stanford University, led a study of the planet beta Pictoris b that combined direct observation of the planet recorded with the Gemini Planet Imager with additional data from space and ground-based observations. The team estimated the mass of this distant planet to be eight to sixteen times that of Jupiter and found that it likely has an elliptical orbit. A video shows the motion of the planet around its star, something that was inconceivable fifteen years ago. Since it was installed on the Gemini-South telescope in 2013,... read more ❯

A team of astronomers led by Bin Ren (The Johns Hopkins University) imaged the debris disk system around star HD 191089 using the GPI instrument, located at 160 light-year away from us. The structure of the debris disk around this younger sibling of our Sun is strikingly similar to our own Kuiper Belt. New technology available maybe in 2030s, like the giant space telescopes (HabEx & LUVOIR) could one day tell if there is also an Earth 2.0 with the Belt delivering water right now, or is there an exotic world that we have never seen or imagined, or maybe... read more ❯

In November 2014 we set out to observe 600 young, nearby stars with the Gemini Planet Imager (GPI) and the Gemini South telescope. Three years later, the survey has achieved a milestone with more than 400 targets observed. Each frame in this movie shows an image from GPI. The star itself is partially blocked by a mask known as a coronagraph. Together with adaptive optics correcting for turbulence in the Earth’s atmosphere, and advanced image processing, we can  see the stellar neighborhood where Jupiter-like exoplanets, brown dwarfs, and circumstellar disks could be present. 406 stars observed with GPI from Franck Marchis on... read more ❯

Sarah Blunt, REU student class of 2015, is today a full member of the Gemini Planet Imager Exoplanet Survey. Together with SETI researcher Eric Nielsen and Franck Marchis, she has developed an innovative method to fit the orbits of directly imaged exoplanets. She has published her work in Astronomical Journal and is a recipient of an NSF Graduate Research Fellowship that will fund her graduate school. Here her story. Every year the SETI Institute hosts several interns who work with our researchers through a Research Experience for Undergraduates (or REU) program funded by the National Science Foundation. We often wonder what... read more ❯

GPI is here at the SPIE Astronomical Telescopes and Instrumentation conference in Edinburgh, Scotland to talk exoplanets and engineering with our colleagues around the world. We have had talks and posters by GPIES team members on topics from AO and instruments to computing and pipelines. This week has also been a great opportunity to meet face-to-face and discuss some of the finer points of GPI technical challenges and plans going forward. Here are some pictures from the week: Bruce gave a great talk on the GPI instrument and GPIES campaign in the instruments session: [caption id="attachment_690" align="alignnone"... read more ❯

Hello GPI fans! We are just wrapping up our cloudy, snowy May 2016 GPIES observing run. While the weather wasn't the best, we accomplished what we could in between the clouds. We also enjoyed the fact that this was the first all-woman run that any of the 5 of us had ever been on. It was a celebration of women in astronomy! EDIT: To clarify, for myself, I often spend 4-6 weeks at a time at the telescope, and I am often the ONLY woman there. So it was quite a novel experience for me! Winter in Chile means snow in... read more ❯

Announcement from the AAS The American Astronomical Society (AAS) will convene an online press conference on Tuesday, 1 December, featuring exciting new results on exoplanets from Extreme Solar Systems III, a conference taking place from 29 November through 4 December 2015 at the Waikoloa Beach Marriott Resort & Spa on Hawaii Island. ExSS III is the third in a series of conferences that began with Extreme Solar Systems in 2007 in Santorini, Greece, and was followed by Extreme Solar Systems II in 2011 in Jackson Hole, Wyoming. Next week’s conference, like the previous two, will cover all aspects of research on exoplanets.... read more ❯

In a major breakthrough for exoplanet discovery and exploration, the Gemini Planet Imager (GPI) is proving to be one of most powerful and effective instruments ever invented for directly imaging planets in orbit around other stars. An artistic conception of the Jupiter-like exoplanet, 51 Eri b, seen in the near-infrared light that shows the hot layers deep in its atmosphere glowing through clouds. Because of its young age, this young cousin of our own Jupiter is still hot and carries information on the way it was formed 20 million years ago. credits: Danielle Futselaar & Franck Marchis,... read more ❯

Understanding how planets form in the Universe is one of the main motivations for GPI. Thanks to its advanced design, GPI specializes in finding and studying giant planets that are similar to Jupiter in our solar system. These are the kind of planets whose origin we hope to understand much better after our survey is complete. We know that planets form within protoplanetary disks that orbit young stars, and gas giants need to be fully formed within 3-10 million years... read more ❯

I sometimes compare the challenge of directly detecting a Jupiter orbiting a nearby star to finding a glowing needle in a haystack.  Oh, and by the way, the haystack is on fire. It's about as hard as seeing a candle a foot away from a spotlight (1 million candlepower) at a distance of 100 miles. Why is doing this so difficult?  There are three primary reasons: 1.  We observe through atmospheric turbulence, which blurs our view of the star-planet system and scatters starlight, obscuring the faint planet beneath. 2.  Light obeys a wave property called diffraction, which scatters light from a planet's host star throughout the image, obscuring the planet.  This effect... read more ❯