Is the Giant Magellan Telescope set to revolutionize ground-based astronomy?

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Discussion Overview

The discussion centers around the Giant Magellan Telescope (GMT) and its potential impact on ground-based astronomy. Participants explore various aspects of its design, efficiency, and capabilities, including the implications of its large mirror and segmented structure.

Discussion Character

  • Exploratory, Technical explanation, Debate/contested

Main Points Raised

  • Some participants express excitement about the GMT's capabilities and its status as the largest ground-based telescope mirror.
  • One participant questions the efficiency of smaller mirror segments, suggesting that collimation issues could be addressed with modern technology.
  • Another participant argues that the design of the GMT allows for easier alignment compared to other telescopes like Keck, potentially reducing costs associated with support hardware and control systems.
  • Concerns are raised about the mid-infrared (MIR) capabilities of the telescope due to background signals from the ground, although it is suggested that the telescope may not primarily focus on MIR observations.
  • A participant with experience on the original Magellan telescope shares insights into the design advantages of the GMT, including cost-effective mirror production and structural benefits.

Areas of Agreement / Disagreement

Participants express a mix of enthusiasm and skepticism regarding the design and efficiency of the GMT. There are differing views on the effectiveness of segmented mirrors and the implications for mid-infrared observations, indicating that the discussion remains unresolved.

Contextual Notes

Limitations include assumptions about the efficiency of mirror segments and the specific applications of the telescope's design. The discussion does not resolve the technical challenges associated with collimation and background signal issues.

Who May Find This Useful

Astronomers, astrophysicists, and individuals interested in advancements in ground-based telescope technology may find this discussion relevant.

jim mcnamara
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Planning is underway for the new super giant Magellan Telescope -- it will be the largest mirror ever on ground based telescopes, according to the link.

http://www.gmto.org/
 
Astronomy news on Phys.org
Looks very interesting!

I wonder just how far it will be able to see!
 
I can't help but wonder is smaller mirror segments would be more efficient. Collimation appears to be the issue with segmented mirrors. Given the power of modern microprocessor, it looks like an opportunity to do something amazing.
 
This is a lot easier to align than something like Keck with a segmented mirror - so the cost of the support hardware and control system is a lot less.
The mirrors should also cost a lot less because they are each a conventional mirror with an identical curvature that can be tested indvidualy. Keck had a hard time making the different off-axis mirror segments.
You can also make the individual primaries much faster - so the telescope is shorter and so the dome and telescope structure is much cheaper

The main drawback of this design is for mid-IR the camera can see through the gaps between the mirrors to the hot ground behind it which gives a larger background signal. But the telescope probably isn't going to be used for MIR.

I worked on the original Magellan (a pair of 6.4m) an I know a lot of the people working on this.
 

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