Gemini South shines first sodium laser "constellation"
GeMS, the next-generation adaptive optics system, allows relatively wide-field imaging at extremely high resolution over an exceptionally large portion of the sky.
January 27, 2011
In the early morning of January 22, 2011, a new era in high-resolution astronomy began with the successful propagation of a 5-star sodium laser guide star "constellation" in the skies over Cerro Pachon in Chile.
The Gemini South laser guide star “constellation” (upper left) is captured in this image. The image shows the 50-watt laser beam as it shines upward toward the atmospheric sodium layer about 55 miles (90 kilometers) above earth’s surface to create a pattern of five artificial guide stars used to sample atmospheric turbulence for the Gemini Observatory’s GeMS adaptive optics system. The yellow-orange beam is caused by scattering of the laser's light by Earth's lower atmosphere. The 30-second exposure was obtained January 21-22, 2011, using a 500mm f/5.6 Celestron telescope with a Canon Rebel XT camera at an ISO setting of 1600. Gemini Observatory/AURA
The event, captured by a series of remarkable images, includes one that clearly shows the five laser-produced stars shining in the sky. This first propagation of the Gemini South telescope laser system marks the beginning of on-sky commissioning for the next-generation adaptive optics system called GeMS, or the Gemini Multi-Conjugate Adaptive Optics (MCAO) System. GeMS will allow relatively wide-field imaging at extremely high resolution over an exceptionally large portion of the sky.
Maxime Boccas, who heads the Gemini Observatory's Optical Systems Group, captured the event using a digital camera and 500mm lens as the 50-watt laser, split into five beams, caused sodium atoms about 55 miles (90 kilometers) overhead to glow. The resulting image shows a distinctive 5-point grouping that resembles the pattern on a single die or domino. "The Gemini team has been working very hard for a very long time to get to this point, and when I saw those 5 stars shining on the sky through my viewfinder, it gave me goose bumps," said Boccas. The laser guide stars are not visible to the naked eye and require a telescope or good binoculars to spot in the sky, though scattering from the beam in the lower atmosphere is easily visible.
"This amazing picture illustrates the culmination of a laser development program that started about 10 years ago," said Celine d'Orgeville from the Gemini Observatory who has overseen the laser's development. "Our Gemini team and its partners, including the laser manufacturer, Lockheed Martin Coherent Technologies, have worked extremely hard over the years to reach this milestone," d'Orgeville said. "We can now truthfully say that Gemini is one observatory, two telescopes, and six laser guide stars!" Gemini North has a lower power 14-watt single laser guide star system that saw first light in 2005 and is a key capability for the Gemini telescope on Mauna Kea, Hawaii.
The entire GeMS system will be integrated and commissioned throughout this year and into next. In 2012, the system should begin providing remarkably sharp images for the study of a wide range of topics ranging from the birth and evolution of stars to the dynamics of distant galaxies. GeMS will "feed" a variety of instruments that work in the near-infrared part of the spectrum and produce images and spectra of objects previously unobservable at this level of clarity due to blurring of light caused by turbulence in Earth's atmosphere.
MCAO is a revolutionary approach to astronomical adaptive optics. The technique samples the turbulence structure in the atmosphere at several levels and then uses a technique similar to medical tomography to reconstruct a 3-D snapshot of how the atmosphere is distorting starlight. This is then used to shape a series of deformable mirrors to cancel out this distortion. All of this happens about 1,000 times per second.
The Gemini system is expected to set the stage for the next generation of large ground-based telescopes, which will have mirrors 30 meters in diameter or larger. These telescopes will require the latest adaptive optics technologies to produce images of sufficient resolution given the wide column of air they will observe through.