Exoplanet research has advanced remarkably far in a relatively short time. Barely two decades ago, we couldn’t definitively say if exoplanets even existed. Now, we’re starting to learn about their atmospheres. It seems almost inevitable that we’ll stumble upon an exoplanet that resembles Earth—and if we don’t, that will be an equally intriguing discovery.
According to current timelines, the Giant Magellan Telescope, or GMT, will be the first to come online. One of the GMT’s first instruments will be a high-resolution spectrograph that will examine the masses and chemical compositions of exoplanets. Testing using four of the GMT’s seven mirrors is expected to begin in 2019, initial science operations begin in 2020 and all seven mirrors come online in 2024.
The GMT’s third mirror was recently cast at the University of Arizona’s Steward Observatory Mirror Lab. As I stood there looking over the mirror's giant glass honeycomb, one thought kept coming to my mind: This mirror could find life on another planet. This is not hyperbole; it’s real. The GMT and its other large brethren have a shot at determining whether or not we are alone in the Universe.
I sat down with Dr. Wendy Freedman, the director of observatories for the Carnegie Institution for Science, and Dr. Patrick McCarthy, the Giant Magellan Telescope Organization project director, to talk about the new mirror and how the telescope works. Dr. Freedman is also the chair of the GMT board of directors. Please enjoy this short film about how the GMT will shape the search for life.
The Giant Magellan Telescope will have seven 8.4 meters that give it the resolving power of a 24.5 meter telescope. It is being built at the Las Campanas Observatory in Chile, on an 8,500 foot peak in the Andes Mountains. Testing using four of the seven mirrors is expected to begin in 2019, initial science operations begin in 2020 and all seven mirrors come online in 2024.
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