ESO ELT M5 unit: design and manufacturing status

The ELT is a project led by the European Southern Observatory (ESO) for a 40-m class optical, near- and mid-infrared, ground-based telescope. When it will enter into operation, the ESO ELT will be the largest and most powerful optical telescope ever built. It will not only offer unrivalled light collecting power, but also exceedingly sharp images, thanks to its ability to compensate for the adverse effect of atmospheric turbulence on image sharpness. The basic optical solution for the ESO ELT is a folded three-mirror anastigmat, using a 39-m segmented primary mirror (M1), a 4-m convex secondary mirror (M2), and a 4-m concave tertiary mirror (M3), all active. Folding is provided by two additional flat mirrors sending the beams to either Nasmyth foci along the elevation axis of the telescope. The folding arrangement (flat M4 and M5 mirrors) is conceived to provide conveniently located flat surfaces for an adaptive shell (M4) and field stabilization (M5). The M5 Mirror and M5 Cell contracts started in 2019. Both sub-units are currently designed by the selected contractors. While the cell is still in an early design phase, the mirror design is in the final phase and the manufacturing of the blank has already started. With the focus on the M5 mirror, we flow down the key requirements to the cell and the mirror and highlight the main characteristics of the current design, discussing the challenges of mirror manufacturing. Finally, we conclude with the current status and an overview of the coming milestones.

[1]  M. Bougoin,et al.  A new technological step for sic mirrors preparing OTOS , 2017, International Conference on Space Optics.

[2]  M. Müller,et al.  E-ELT M5 field stabilisation unit scale 1 demonstrator design and performances evaluation , 2010, Astronomical Telescopes + Instrumentation.

[3]  Ralf Jedamzik,et al.  Design and fabrication of a 3m class light weighted mirror blank for the E-ELT M5 , 2011, Optical Engineering + Applications.

[4]  Marc Cayrel,et al.  E-ELT optomechanics: overview , 2012, Other Conferences.

[5]  Martin Dimmler,et al.  Status of E-ELT M5 scale-one demonstrator , 2014, Astronomical Telescopes and Instrumentation.

[6]  Michel Bougoin,et al.  The SiC primary mirror of the EUCLID telescope , 2017, International Conference on Space Optics.

[7]  Martin Dimmler,et al.  Active damping strategies for control of the E-ELT field stabilization mirror , 2012, Other Conferences.

[8]  Steve Williams,et al.  Evaluation of segmented and brazed mirror assemblies , 2005, SPIE Optics + Photonics.

[9]  Mary J. Edwards,et al.  ULE design considerations for a 3m class light weighted mirror blank for E-ELT M5 , 2016, Astronomical Telescopes + Instrumentation.