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#Paranal

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Bundespräsident #Steinmeier besucht diese Woche das #Paranal-Observatorium in #Chile – ein weltweit bedeutender Ort astronomischer Forschung. Doch nebenan soll nun ein Industriepark entstehen – mit schwerwiegenden Folgen für die #Forschung. Sophia Boddenberg berichtet: riffreporter.de/de/internation

RiffReporter · Konflikt in Chile: Wasserstoffproduktion versus astronomische ForschungBy Sophia Boddenberg
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Because of #Chile’s 🇨🇱 near-ideal conditions for astronomy, it has become home to almost 40 percent 📊 of the world’s ground-based astronomy observing 🔭 capacity. Including current projects under construction 🏗️, within the next decade that number will increase 📈 to 60 percent. This makes any threat to the natural celestial purity of this remote region of Chile a threat to the present and future of ground-based astronomy as a whole scientificamerican.com/article

Scientific American · Europe’s Extremely Large Telescope Faces a New Dire ThreatBy Katherine Helen Laliotis
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I edited a couple of my own photos into a size comparison of ESO's Very Large Telescope(s) and Extremely Large Telescope. The top is the VLT photographed from the ELT (in the middle of the day) and the bottom photo is the ELT photographed from the VLT (at sunset). Same distance (20 km), same camera, same lens, so the scale of the two photos should be identical.

The source photos (and more) can be found here: drhotdog.smugmug.com/Astronomy

Edit: I removed the ELT scale bar because of a couple of issues. First, because the photo of the ELT was taken from a lower altitude part of the ELT building is hidden behind the near side of the flattened mountaintop. Second, the ELT dome doors have not yet been installed so the current structure is, I think, less than 80 metres tall.

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I've started to sift through all the photos I took in Chile, picking out and reprocessing the good ones, and uploading them to web galleries here: drhotdog.smugmug.com/Astronomy

Web galleries? Yes, I know, it's very 2010 of me. It's also the only way to share photos in quantity without having all the detail squeezed out of them by heavy re-compression.

Here's an example pic of the VISTA telescope at sunset, as seen from the VLT Platform. The VISTA telescope was built to perform an all sky imaging survey in the near infrared, but with that complete the infrared camera is being replaced with a visible wavelength spectroscopic survey instrument, 4MOST (4most.eu/).

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These are two of the four lasers in question, mounted on the side of VLT Unit Telescope 4. They are the black objects labelled LGSU1 and LGSU4. LGSU2 and LGSU3 are mounted in the corresponding positions on the far side of the telescope. Each of the four laser guide star units emits 22 Watts of continuous wave optical power at 589 nm.

Below the lasers you can see the 8.2 metre diameter primary mirror almost side on, and in the centre of the structure above you can see the small Deformable Secondary Mirror.

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There are two exciting things about today.

1. There is now help-yourself ice cream in the Paranal Observatory canteen.

2. The maintenance on the 4 Laser Guide Star Facility has been completed, so we will all be going up to the Platform after dinner to get photos of the sky lasers from close range. This is just in time, as tonight is our last night here.

First segments of the world's largest telescope mirror shipped to Chile

The construction of the European Southern Observatory’s Extremely Large Telescope (ESO's ELT) has reached an important milestone with the delivery to ESO and shipment to Chile of the first 18 segments of the telescope’s main mirror (M1).

Once they arrive in Chile, the segments will be transported to the ELT Technical Facility, at ESO’s Paranal Observatory in the country’s Atacama Desert, where they will be coated in preparation for their future installation on the telescope main structure.

Unable to be physically made in one piece, M1 will consist of 798 individual segments arranged in a large hexagonal pattern, with an additional 133 being produced to facilitate the recoating of segments.

With a diameter of more than 39 metres, it will be the largest telescope mirror in the world.

The final stage in the production process of M1 segments — polishing — was carried out by world-leading optical systems manufacturer Safran Reosc near Poitiers, central France, at a building completely refurbished to work on this delicate task.

As part of the process, Safran Reosc developed new automation workflows and measurement techniques to ensure that the polishing met the high standards required for ESO's ELT.

The surface irregularities of the mirror are less than 10 nanometres (less than one thousandth of the width of a human hair).

To reach this level of performance, Safran Reosc used a technique called ion-beam figuring, in which a beam of ions sweeps the mirror surface and removes irregularities atom by atom
#elt #astrodon #Paranal #Chile
eso.org/public/news/eso2319/

www.eso.orgFirst segments of the world's largest telescope mirror shipped to ChileThe construction of the European Southern Observatory’s Extremely Large Telescope (ESO's ELT) has reached an important milestone with the delivery to ESO and shipment to Chile of the first 18 segments of the telescope’s main mirror (M1). Once they arrive in Chile, the segments will be transported to the ELT Technical Facility, at ESO’s Paranal Observatory in the country’s Atacama Desert, where they will be coated in preparation for their future installation on the telescope main structure. Unable to be physically made in one piece, M1 will consist of 798 individual segments arranged in a large hexagonal pattern, with an additional 133 being produced to facilitate the recoating of segments. With a diameter of more than 39 metres, it will be the largest telescope mirror in the world.