E-ELT goes to Chile

As expected, ESO Council have accepted the recommendation to build the European Extremely Large Telescope at Cerro Armazones in the Chilean Andes. The decision was announced yesterday with the customary nice words and some cool accompanying imagery, video and a dedicated ESOCast episode, which you can all see here.

Particularly noteworthy is the nod of thanks ESO give to Spain, who were competing with Chile for the chance to to host the telescope. While many European astronomers, especially the Britons who’ve traditionally had the largest foreign presence on the island, have a great big soft spot for La Palma, I think a collective sigh of relief went through the community on hearing the news. La Palma is undoubtedly an excellent observing site, but it’s just not of the same quality as Paranal or Armazones – it’s more humid, has fewer clear nights and is plagued by Saharan sand in its atmosphere.

With this announcement, all three of the ELT-type telescopes  – E-ELT, GMT and TMT – now have a home. Now all they need is money to start building!

Image: ESO/S. Brunier

Aloha TMT

In a long awaited announcement, America’s largest optical telescope project unveiled the chosen site for its new observatory. After a long and extensive campaign of site testing and comparison, and, more importantly perhaps, much politicking, the Thirty Meter Telescope board have reached an agreement to build their telescope on the Mauna Kea in Hawaii.

The TMT, a collaboration of US, Canadian and Japanese institutes, is one of three projects in the so-called class of extremely large telescopes, or ELTs. In the last year, two potenial sites were studied in a final run-off: the well known Hawaiian mountain Mauna Kea, and Cerro Armazones, an as yet undeveloped site in the Chilean Andes. As both sites are excellent from the astroclimatological perspective, it is rumoured that the Japanese involvement was at least partly responsible for the final choice. All three of the partner countries already have telescopes and infastructure on Mauna Kea.

With the smallest of the ELTs, the 24-m
Giant Magellan Telescope confirmed to be sited at Las Campanas, also in Chile, and ESO’s strong ties with the country, TMT will ensure that an ELT will also be watching the Northern skies. In addition seems sensible to question the sanity of locating three of the world’s most powerful telescopes in a relatively small area – and one with substantial seismic activity at that.

All eyes are now on ESO, whose 42-m ELT project, the imaginatively named European ELT, is the last in the trio to be found a home. While ESO are running an extensive testing campaign at 5 sites around the world, there is much speculation that TMT’s second-choice site, Armazones, could now be in the running for the E-ELT. An announcement from ESO is expected in the next year.

Prime real estate for astronomy

Cordon Macon, a candidate site of the E-ELT

Cordon Macon, a candidate site of the E-ELT

I recently spotted this great image on the ESO website, where it was “ESO Chile Image of the Month” a while ago.  It’s an eastward view over Cordon Macon, located in the Argentinian province of Salta and one of the candidate sites for the European Extremely Large Telescope, or E-ELT. The equipment used for monitoring of the site is just a tiny speck on the ridge, shown enlarged in the inset.

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Moore Foundation funds detector research

Artists impression of the 30-m primary mirror of the Thirthy Meter Telescope (TMT)

Artist's impression of the 30-m primary mirror of the Thirthy Meter Telescope (TMT)

The Gordon and Betty Moore Foundation recently awarded $2.8 million to researchers at the Rochester Institute of Technology for the development of noiseless detectors in the framework of the Thirty Meter Telescope project. This is really good news for astronomers: not only is it a significant amount of money invested in a hugely important area of our science, the Foundation’s high profile helps raise awareness of the value of this work. Personally I’m happy this research is being carried out at a research institution rather than a private company, as corporate strategies are not always compatible with the “niche applications” that astronomy instruments usually are.

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Well played, Australia

Astronomy Professor Penny Sackett, former head of the Astronomy department of the Australian National University (ANU) in Canberra, was appointed as Australia’s next Chief Scientist at the end of September. Although a theoretical physicist by education, Sackett is very well known in astronomy for her work in exoplanet detection and involvement in the US-led Giant Magellan Telescope project.

She was also in charge of rebuilding Mt Stromlo observatory, that was tragically destroyed in a bush fire in 2003.

An astronomer, and she’s a woman to boot. Score! Congratulations to her.