The Giant Magellan Telescope ( GMT Statement )
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1 The Giant Magellan Telescope ( GMT Statement ) Yes We Can! Wendy Freedman Carnegie Observatories Chair, GMT Board Science with Giant Telescopes: Public Participation in TMT and GMT, Chicago June 16, 2008
2 Why, Which, Where, What, When? 1. Why build these large optical telescopes? 2. Which telescope(s) should be built? 3. Where will they be built? 4. What are the next steps? 5. When will they be built?
3 GMT Institutions Australian Astronomy Lim. Australian National Univ. Carnegie Observatories Harvard University Smithsonian Astrophysical Observatory Texas A&M University University of Arizona University of Texas, Austin Korea Astronomy & Space Science Institute *NEW* Looking to the Future: National Science Foundation
4 Telescope Concept Alt-az mount Seven x 1.1m segmented secondary mirror (3.2 m Φ) Seven x 8.4 m segmented borosilicate primary mirror Laser housing Pier Telescope stats Height: 38.7 meters 1,125 metric tons Lowest Mode: 4.5 Hz (4.3 Hz with pier)
5 Project SWG GMT Project Science WG Steve Shectman Carnegie Observatories Pat McCarthy, Wendy Freedman (Chair) Carnegie Observatories Roger Angel Roger Angel, Peter Strittmatter U. Arizona Warrick Couch U. Arizona Dan Fabricant Australia Bob Kirshner, Charles Alcock Harvard/Smithsonian CfA Xiaohui Fan Harvard/Smithsonian CfA Phillip MacQueen Arizona David Lambert, Mary Ann Rankin U. Texas at Austin Karl Gebhardt U. Texas at Austin Matt Johns Texas Ed Fry, Nick Suntzeff Carnegie Observatories Gary Hill Texas A&M Charles Jenkins Australia Texas John Huchra Penny Sackett, Matthew Colless Australia David Sprayberry Harvard NOAO Scott Kenyon Alycia Weinberger Smithsonian Carnegie/DTM Pat McCarthy (chair) Carnegie Michael Meyer Arizona David Sprayberry NOAO Megan Donahue Michigan State GMT Board
6 GMT, NSF, AURA and the community Letter to AURA and NSF GMT interest in working with NSF, AURA and community The GMT Board believes that substantial benefits would accrue to both the public and private institutions by forming a strong partnership based on the common goals and aspirations of the scientific community
7 GMT Key Milestones 2005: Casting of GMT1 mirror 2006: Positive External CoDR 2006: NSF funding for technology development 2006: Australia joins the GMT project 2007: GMTO Corporation formed 2007 : Design Development Phase 2007: GMT Board completes Founders Agreement 2008: Generation of GMT1 front surface completed 2008: Korea announces intention to join GMT 2008: GMT1 Testing and Polishing Phase to Begin
8 The GMT on Las Campanas Peak
9 GMT SCIENCE: CONTEXT & SYNERGY Broad Synergy Across Wavelength, Spatial and Time Domains Physical Diagnostics Deep/Wide Surveys High-resolution imaging High SNR & Res. Spectroscopy JWST ALMA LSST SKA Magellan
10 Advantages to Two US ELTs Competitive position for GSMT in next decadal survey Increase science for whole astronomical community Opportunity to optimize instrumentation Increase number of instruments on sky at given time 50% share by NSF in one telescope not current option 25% of one does not provide much access to US community Potential collaborative technologies Most of the funding is coming from outside of NSF This is win-win for the community and the projects
11 ELT Context 2001 Decadal Survey GSMT (30-m class) optical telescope #1 priority for ground-based astronomy public-private partnership This decade: -- Giant Magellan Telescope (GMT) -- Thirty-Meter Telescope (TMT) -- European Extremely Large Telescope (E-ELT) 2010 Decadal Survey beginning fall 2008 GSMT will be re-ranked relative to LSST, SKA, ATST NSF budget still constrained; no construction funding until after 2012
12 Why, Which, Where, What, When? 1. Why build these large optical telescopes? Exciting Science / Synergy with Next-Generation Great Observatories / Optical Window Unique 2. Which telescope(s) should be built? GMT, TMT, E-ELT Note: Keck(2), Magellan(2), Gemini(2), VLT(4), Subaru, HET (2) 3. Where will they be built? Chile, Hawaii (?) 4. What are the next steps? Optical Community Consensus / White papers for Decadal Survey / Funding 5. When will they be built? < 2018!!! [Synergy with JWST]
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