The worlds largest telescope the Extremely Large Telescope (ELT) is under construction in Chile. When it captures its first light, sometime in 2027 or 2028, Irish adaptive optics technology will be there to ensure it sees further and with greater clarity than any telescope in human history.
The opportunity for Irish astronomers to take part in the ELT project arose when the government decided to join the European Southern Observatory (ESO) the top intergovernmental astronomy organisation in Europe in 2018. Membership cost 14.66 million, with an annual fee of 3.5 million.
A team of researchers at NUI Galway, led by Dr Nicholas Devaney, with expertise in adaptive optics are involved in the ELT project as part of a consortium also involving the Grenoble Institute for Planetary Sciences and Astrophysics and the National Institute of Astrophysics (INAF) in Italy.
The consortium will design and manage the construction of an instrument on the ELT, called multi-conjugate adaptive optics relay (MAORY), which corrects image distortion due to atmosphere blurring. The NUIG team were invited to join the MAORY project based on their scientific reputation.
The Galway team is responsible for the device we call the test unit that is needed to pass all the performance on this domain here in Europe and then also when we arrive on the mountains in Chile, says Paolo Ciliegi, an astronomer at INAF; the overall principal investigator of MAORY.
They put on the table their expertise in adaptive optics and also the construction of this test unit, Ciliegi adds.
The construction of the ELT at an altitude of some 10,000 feet on top of a mountain called Cerro Amazones has halted due to the Covid situation in Chile. The site is in the Atacama Desert, a high plateau covering an area slightly bigger than Ireland, and made up mostly of stones, salt and sand.
The altitude puts it above the cloud line, so there is very little precipitation, which can distort telescope images of space. That dryness this is the driest desert on the planet outside the poles make it an ideal location for astronomers to view the heavens. Yet the ELT must still peer up and out through about 480km of atmosphere, with the distortion that this brings.
When you feel the bumpiness in an airplane thats the atmospheric turbulence, says Devaney. The turbulent atmosphere, he says, is made up of bubbles of air with differing temperatures. The speed of light through air varies slightly with the temperature of the air through which it travels.
The net effect of this is to reduce the sharpness of images from space that a ground telescope can gather. That introduces distortions in the light which leads to a blurry image instead of a sharper image, he adds.
Adaptive optics technology works hard to overcome such atmospheric distortion. This task is akin to gathering light that has been bent and scattered in water and rebuilding it into its underformed original form. This is the job that the MAORY instrument will be performing for the ELT.
A limitation of adaptive optics technology up to now has been that it relies on a natural constellation of bright stars to sharpen distorted images from an optical telescope viewing a big area of sky, but such constellations are not always available. In order to get over this issue scientists use guide stars.
The ELT is going to generate six artificial laser-generated guide stars which will act like a natural constellation of six bright stars to facilitate adaptive optics to work wherever the ELT is pointing towards in the sky. It has proved a huge challenge over decades to get the lasers up to sufficient power to produce bright enough guide stars to facilitate adaptive optics.
After much research scientists decided to use a sodium wavelength for producing guide stars. This is because there is a natural layer of charged sodium ions in the Earths atmosphere at an altitude of 90km, which can be excited and energized by a laser so that it looks just like a natural star.
This is perfect for astronomers, says Devaney. Its like the ions were put out there specifically for that purpose. It means that it is possible to make constellations of artificial guide stars using the six lasers on the ELT.
An optical telescope works by gathering light through mirrors. The bigger its mirrors the more light the telescope can gather and the farther it can see. The main mirror of the ELT will be an enormous 39 metres ( 127.9ft), in diameter. Thats roughly equivalent to 21 men, six feet tall, lying head to toe.
The designers knew that technically it wasnt possible to construct the main mirror as one piece. They also knew that it would be difficult to carry large mirror segments to a mountain top. A decision was therefore made to separately make 798 hexagonal-shaped segments; each 1.5 metres wide weighing 250kg, which, when aligned carefully together, would make up the main ELT mirror.
The mirror segments had to be aligned with nano-metre precision, and that alignment has to be maintained as the telescope moves and tracks objects. There are some 9,000 tiny sensors arranged around each segment so that any kind of motion in one segment with respect to another is accounted for.
There are also actuators that bend the mirrors into optimum shape. The biggest optical telescopes today have three mirrors. The ELT will have five.
In return for Devaneys team working on the adaptive optics on the ELT his astronomer colleagues at NUIG are to be offered ELT observation time. One of those scientists hoping to use the ELT to advance his work is physicist Dr Matt Redman, director of the centre of astronomy at NUIG.
Redman is interested in planetary nebulae. These are badly named celestial objects as they have nothing to do with planets. They looked like planets when viewed by the first telescopes so thats how they got the name. They might better be described as the glowing shell of gas ejected from a dying star.
These nebulae are observed in a variety of shapes including butterfly-shaped, elliptical, spherical, ring-shaped, bi-polar, cylindrical and round.
The big mystery is that the Sun is round, spherical and will turn into one of these objects, and these objects are not round and spherical, says Redman. The most likely idea is a companion star, or even a companion planet, disturbing the material as the dying star throws it off, he explains.
I am hoping the MAORY will be able to get right into the centre of these objects and we might even see that shaping mechanism happening, he adds.
There are some who question the economic and scientific logic of building expensive telescopes on the top of Chilean mountains in order to see through atmospheric distortion when it is possible to put a space telescope, like the Hubble telescope, into orbit up where atmospheric distortion is not a factor.
The justification lies in the cost of getting telescopes into orbit against building them on Earth. The Hubble Space Telescope, which had a primary mirror 2.4metres wide, cost 2.5 billion (today equivalent) to get into orbit and operational. The ELT will cost some 1.3 billion; about half the price.
This point of view holds that although they do different things, ground-based telescopes like ELT give more scientific bang for your buck than space telescopes. The James Webb Space Telescope (JWST), set to launch in November, will cost 8.2 billion.
The ELT sees farther, clearer. You are able to collect a lot more, like with a 39-metre mirror, says Devaney. You are able to see further away and see things that are much fainter, such as really faint galaxies. The ELT will be able to see things that are fainter than was possible with the Hubble.
The huge jump in astronomical capability that the ELT will provide is likely to trigger a round of unexpected scientific findings that will change our understanding of the Universe and how it was formed in its earliest days.
Weve seen it before. For example, in 1998 data from the Hubble led scientists to conclude the universe was expanding at an ever accelerating rate. Each time there is a big step forward like this it leads to a huge mushrooming of astronomical activities and discoveries, says Devaney.
More here:
Worlds largest telescope will see better with Irish technology - The Irish Times
- Rotational spectra of isotopic species of methyl cyanide, CH_3CN, in their ground vibrational states up to terahertz frequencies [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Cosmological parameter extraction and biases from type Ia supernova magnitude evolution [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Continuous monitoring of pulse period variations in Hercules X-1 using Swift/BAT [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Constraining the ortho-to-para ratio of H{_2} with anomalous H{_2}CO absorption [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- A photometric and spectroscopic study of the new dwarf spheroidal galaxy in Hercules - Metallicity, velocities, and a clean list of RGB members [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Luminosities and mass-loss rates of SMC and LMC AGB stars and red supergiants [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Electron beam – plasma system with the return current and directivity of its X-ray emission [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- The propagation of the shock wave from a strong explosion in a plane-parallel stratified medium: the Kompaneets approximation [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Analysis of hydrogen-rich magnetic white dwarfs detected in the Sloan Digital Sky Survey [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Letter: Centaurus A as TeV \gamma-ray and possible UHE cosmic-ray source [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Young pre-low-mass X-ray binaries in the propeller phase - Nature of the 6.7-h periodic X-ray source 1E 161348-5055 in RCW 103 [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Radiative rates and electron impact excitation rates for transitions in Cr VIII [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Solar granulation from photosphere to low chromosphere observed in Ba II 4554 Å line [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Does the HD 209458 planetary system pose a challenge to the stellar atmosphere models? [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Effect of asymmetry of the radio source distribution on the apparent proper motion kinematic analysis [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Destriping CMB temperature and polarization maps [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Search for cold debris disks around M-dwarfs. II [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Precise data on Leonid fireballs from all-sky photographic records [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- An X-ray view of 82 LINERs with Chandra and XMM-Newton data [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Radio observations of ZwCl 2341.1+0000: a double radio relic cluster [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Candidate free-floating super-Jupiters in the young \sigma Orionis open cluster [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- The metallicity gradient as a tracer of history and structure: the Magellanic Clouds and M33 galaxies [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- XMMSL1 J060636.2-694933: an XMM-Newton slew discovery and Swift/Magellan follow up of a new classical nova in the LMC [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- The inner rim structures of protoplanetary discs [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- The solar Ba{\sf II} 4554 Å line as a Doppler diagnostic: NLTE analysis in 3D hydrodynamical model [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Magnetic evolution of superactive regions - Complexity and potentially unstable magnetic discontinuities [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Low-mass protostars and dense cores in different evolutionary stages in IRAS 00213+6530 [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- PMAS optical integral field spectroscopy of luminous infrared galaxies - I. The atlas [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- First AGILE catalog of high-confidence gamma-ray sources [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Radiative hydrodynamics simulations of red supergiant stars - I. interpretation of interferometric observations [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Extrasolar planets and brown dwarfs around A–F type stars - VII. \theta Cygni radial velocity variations: planets or stellar phenomenon? [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Cosmic rays and the magnetic field in the nearby starburst galaxy NGC 253 - II. The magnetic field structure [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Physical structure and water line spectrum predictions of the intermediate mass protostar OMC2-FIR4 [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- The bright galaxy population of five medium redshift clusters - II. Quantitative galaxy morphology [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Dust in brown dwarfs and extra-solar planets - II. Cloud formation for cosmologically evolving abundances [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- The quiet Sun magnetic field observed with ZIMPOL on THEMIS - I. The probability density function [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Complexity in the sunspot cycle [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Properties and nature of Be stars - 26. Long-term and orbital changes of \zeta Tauri [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- The massive Wolf-Rayet binary LSS 1964 (=WR 29) - II. The V light curve [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Supernova progenitor stars in the initial range of 23 to 33 solar masses and their relation with the SNR Cassiopeia A [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- The Hertzsprung-Russell Diagram of Star Clusters [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Table of the 10 Brightest stars within 10 Parsecs of the Sun [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- The Hertzsprung-Russell Diagram of the Nearest Stars [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Magnitude and Color in Astronomy [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Stellar Types [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Brown Dwarfs [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Spotting the Minimum [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- The Structure and Evolution of Brown Dwarfs [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- No Bang from the Big Bang Machine [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- The Sizes of the Stars and the Planets [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- An Implausible Light Thrust [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- the Masses of Degenerate Objects [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Degeneracy Pressure [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Introduction to Degenerate Objects [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- The Radii of Degenerate Objects [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- The Inevitability of Black Holes [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Scientific Pig-Out [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- The Neutrino Cooling of Degenerate Dwarfs [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- The Neutrino Cooling of Neutron Stars [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Overview of Supernovae [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Energetics of Thermonuclear Supernovae [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Thermonuclear Supernovae [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Nuclear Reactions in Thermonuclear Supernovae [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Core-Collapse Supernovae [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Neutrinos and SN 1987A [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Revealing the sub-AU asymmetries of the inner dust rim in the disk around the Herbig Ae star R Coronae Austrinae [Last Updated On: December 13th, 2009] [Originally Added On: December 13th, 2009]
- Probing the dust properties of galaxies up to submillimetre wavelengths - I. The spectral energy distribution of dwarf galaxies using LABOCA [Last Updated On: December 13th, 2009] [Originally Added On: December 13th, 2009]
- On the physical origin of the second solar spectrum of the Sc II line at 4247 Å [Last Updated On: December 13th, 2009] [Originally Added On: December 13th, 2009]
- On detecting the large separation in the autocorrelation of stellar oscillation times series [Last Updated On: December 13th, 2009] [Originally Added On: December 13th, 2009]
- Imaging the spotty surface of Betelgeuse in the H band [Last Updated On: December 13th, 2009] [Originally Added On: December 13th, 2009]
- Chandra observation of Cepheus A: the diffuse emission of HH 168 resolved [Last Updated On: December 13th, 2009] [Originally Added On: December 13th, 2009]
- A planetary eclipse map of CoRoT-2a - Comprehensive lightcurve modeling combining rotational-modulation and transits [Last Updated On: December 13th, 2009] [Originally Added On: December 13th, 2009]
- The chemical composition of carbon stars. The R-type stars [Last Updated On: December 13th, 2009] [Originally Added On: December 13th, 2009]
- Flow instabilities of magnetic flux tubes - IV. Flux storage in the solar overshoot region [Last Updated On: December 13th, 2009] [Originally Added On: December 13th, 2009]
- Fragmentation of a dynamically condensing radiative layer [Last Updated On: December 13th, 2009] [Originally Added On: December 13th, 2009]
- Temporal variations of the CaXIX spectra in solar flares [Last Updated On: December 13th, 2009] [Originally Added On: December 13th, 2009]
- Deuterium chemistry in the Orion Bar PDR - “Warm” chemistry starring CH_{2}D^+ [Last Updated On: December 13th, 2009] [Originally Added On: December 13th, 2009]
- Metal abundances in the cool cores of galaxy clusters [Last Updated On: December 13th, 2009] [Originally Added On: December 13th, 2009]
- The nature of the X-ray binary IGR J19294+1816 from INTEGRAL, RXTE, and Swift observations [Last Updated On: December 13th, 2009] [Originally Added On: December 13th, 2009]
- Relating basic properties of bright early-type dwarf galaxies to their location in Abell 901/902 [Last Updated On: December 13th, 2009] [Originally Added On: December 13th, 2009]