Archive for european southern observatory

ESO Planning First Astronomy Camp For Secondary School Students

ESO

The European Southern Observatory (ESO) and its Science Outreach Network is collaborating with the science communication event organizer Sterrenlab to arrange the first ESO Astronomy Camp. The camp will take place from 26-31 December 2013 at the Astronomical Observatory of the Aosta Valley, located in Saint-Barthelemy, Nus, Italy. Several partners, including ESO, are providing for a total of, so far, five bursaries that will be awarded to the winning applicants.

The camp will explore the theme of the visible and the invisible Universe through lectures, hands-on activities, and nighttime observations with the telescopes and instruments at the observatory. Social activities, winter sports, and excursions will contribute to making the camp a memorable experience for the participants. ESO will be responsible for the scientific program for the ESO Astronomy Camp, and will, together with other partners, provide lecturers and material.

Sterrenlab specializes in the organization of international science camps for children and teenagers, and offers a variety of services in consultancy, and in the design, and implementation of projects and events in the areas of science education and communication.

The camp will be available for a maximum of 55 secondary school students aged between 16 and 18 from the ESO Member States and ESO Science Outreach Network countries. Students wishing to apply should fill out the form on the Camp website before 15 October 2013. The selection of the candidates will take place on 31 October 2013. Final confirmation from the participants is due by 8 November 2013. The selection criteria and other instructions for participation are given on the Camp website.

The registration fee of 480 euros covers full board accommodation at the hostel of Saint Barthelemy, supervision by professional staff, all astronomical and leisure activities, materials, excursions, internal transport, and insurance. Bus transport between the observatory and the airport of Milan Malpensa will be provided.

The applicant with the best entry will win a free trip sponsored by ESO. This bursary will cover the complete cost of the camp and transport to the camp, and will go to the best application from a student residing in one of ESO’s Member States. Four national partners are also providing free Camp registrations to the best applications from a student residing in their respective countries (but not travel funding):

  • Italy: Istituto Nazionale di Astrofisica and University of Milan
  • Poland: Polish Astronomical Society and Urania — Postępy Astronomii and Urząd Marszałkowski Województwa Kujawsko-Pomorskiego
  • Spain: Sociedad Española de Astronomía
  • Switzerland: Université de Gèneve

The ESO Astronomy Camp has so far been endorsed by the following institutions:

  • Austrian Planetarium Society
  • Planétarium de l’Observatorire Royal de Belgique
  • Tähtitieteellinen yhdistys Ursa (Ursa Astronomical Association)
  • Haus der Astronomie
  • Istituto Nazionale di Astrofisica
  • Società Astronomica Italiana
  • University of Milan – COSMO group
  • Netherlands Research School for Astronomy (NOVA)
  • Polish Astronomical Society
  • Urania — Postępy Astronomii
  • Astronomical Observatory of the University of Coimbra
  • Observatorio Astronómico — Universidad de Valencia
  • Sociedad Española de Astronomía
  • Onsala Space Observatory
  • University of Geneva
  • University of Cag — Space Observation Research Centre
  • Las Cumbres Observatory Global Telescope Network
  • UK National STEM Centre

Follow the Camp website for updates.

On The Net:

Article source: http://www.redorbit.com/news/space/1112847497/eso-astronomy-camp-secondary-school-students-051513/

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An anarchic region of star formation captured

NGC-6559The Danish 1.54-meter telescope located at the European Southern Observatory (ESO) La Silla Observatory in Chile has captured a striking image of NGC 6559, an object that showcases the anarchy that reigns when stars form inside an interstellar cloud.

NGC 6559 is a cloud of gas and dust located at a distance of about 5,000 light-years from Earth in the constellation Sagittarius the Archer. The glowing region is a relatively small object, just a few light-years across, in contrast to the 100 light-years and more spanned by its famous neighbor, the Lagoon Nebula (M8). Although it is usually overlooked in favor of its distinguished companion, NGC 6559 has the leading role in this new picture.

The gas in the clouds of NGC 6559, mainly hydrogen, is the raw material for star formation. When a region inside this nebula gathers enough matter, it starts to collapse under its own gravity. The center of the cloud grows ever denser and hotter until thermonuclear fusion begins and a star is born. The hydrogen atoms combine to form helium atoms, releasing energy that makes the star shine.

These brilliant hot young stars born out of the cloud energize the hydrogen gas still present around them in the nebula. The gas then re-emits this energy, producing the glowing threadlike red cloud seen near the center of the image. This object is known as an emission nebula.

But NGC 6559 is not just made of hydrogen gas. It also contains solid particles of dust made of heavier elements such as carbon, iron, or silicon. The bluish patch next to the red emission nebula shows the light from the recently formed stars being scattered — reflected in many different directions — by the microscopic particles in the nebula. Known to astronomers as a reflection nebula, this type of object usually appears blue because the scattering is more efficient for these shorter wavelengths of light.

In regions where it is very dense, the dust completely blocks the light behind it, as is the case for the dark isolated patches and sinuous lanes to the bottom left-hand side and right-hand side of the image. To look through the clouds at what lies behind, astronomers would need to observe the nebula using longer wavelengths that would not be absorbed.

The Milky Way fills the background of the image with countless yellowish older stars. Some of them appear fainter and redder because of the dust in NGC 6559.

Article source: http://www.astronomy.com/~/link.aspx?_id=c52e443a-b953-4219-9cbf-12eca04e1b7f

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Young Blue Stars Shine in Cosmic Photo

A beautiful cluster of stars shines brightly in a new photo from the European Southern Observatory.

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Herschel discovers some of the youngest stars ever seen

Youngest-starsAstronomers have found some of the youngest stars ever seen, thanks to the Herschel Space Observatory, a European Space Agency (ESA) mission.

Observations from NASA’s Spitzer Space Telescope and the Atacama Pathfinder Experiment (APEX) telescope in Chile, a collaboration involving the Max Planck Institute for Radio Astronomy in Germany, the Onsala Space Observatory in Sweden, and the European Southern Observatory in Germany, contributed to the findings.

Dense envelopes of gas and dust surround the fledging stars known as protostars, making their detection difficult. The 15 newly observed protostars turned up by surprise in a survey of the biggest site of star formation near our solar system, located in the constellation Orion. The discovery gives scientists a peek into one of the earliest and least understood phases of star formation.

“Herschel has revealed the largest ensemble of such young stars in a single star-forming region,” said Amelia Stutz of the Max Planck Institute for Astronomy. “With these results, we are getting closer to witnessing the moment when a star begins to form.”

Stars spring to life from the gravitational collapse of massive clouds of gas and dust. This changeover from stray cool gas to the ball of super-hot plasma we call a star is relatively quick by cosmic standards, lasting only a few hundred thousand years. Finding protostars in their earliest, most short-lived and dimmest stages poses a challenge.

Astronomers long had investigated the stellar nursery in the Orion Molecular Cloud Complex, a vast collection of star-forming clouds, but had not seen the newly identified protostars until Herschel observed the region.

“Previous studies have missed the densest, youngest, and potentially most extreme and cold protostars in Orion,” Stutz said. “These sources may be able to help us better understand how the process of star formation proceeds at the very earliest stages, when most of the stellar mass is built up and physical conditions are hardest to observe.”

Herschel spied the protostars in far-infrared, or long-wavelength light, which can shine through the dense clouds around burgeoning stars that block out higher-energy, shorter wavelengths, including the light our eyes see.

The Herschel Photodetector Array Camera and Spectrometer (PACS) instrument collected infrared light at 70 and 160 micrometers in wavelength, comparable to the width of a human hair. Researchers compared these observations to previous scans of the star-forming regions in Orion taken by Spitzer. Extremely young protostars identified in the Herschel views but too cold to be picked up in most of the Spitzer data were further verified with radio wave observations from the APEX ground telescope.

“Our observations provide a first glimpse at protostars that have just begun to ‘glow’ at far-infrared wavelengths,” said Elise Furlan from the National Optical Astronomy Observatory in Tucson, Arizona.

Of the 15 newly discovered protostars, 11 possess red colors, meaning their light output trends toward the low-energy end of the electromagnetic spectrum. This output indicates the stars are still embedded deeply in a gaseous envelope, meaning they are very young. An additional seven protostars previously seen by Spitzer share this characteristic. Together, these 18 budding stars constitute only 5 percent of the protostars and candidate protostars observed in Orion. That figure implies the very youngest stars spend perhaps 25,000 years in this phase of their development, a mere blink of an eye considering a star like our Sun lives for about 10 billion years.

Researchers hope to document chronologically each stage of a star’s development rather like a family album, from before birth to early infancy, when planets also take shape.

“With these recent findings, we add an important missing photo to the family album of stellar development,” said Glenn Wahlgren from NASA Headquarters in Washington, D.C. “Herschel has allowed us to study stars in their infancy.”

Article source: http://www.astronomy.com/~/link.aspx?_id=3a45f49b-9cce-4fbc-a8cc-b3daef938672

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Rare triple quasar found

triple-quasarFor only the second time in history, a team of scientists, including Michele Fumagalli from the Carnegie Institution for Science in Washington, D.C., has discovered an extremely rare triple quasar system.

Quasars are extremely bright and powerful sources of energy that sit in the center of a galaxy, surrounding a black hole. In systems with multiple quasars, the bodies are held together by gravity and are believed to be the product of galaxies colliding.

It is difficult to observe triplet quasar systems because of observational limits that prevent researchers from differentiating multiple nearby bodies from one another at astronomical distances. Moreover, such phenomena are presumed to be rare.

The team led by Emanuele Farina of the University of Insubria in Como, Italy, combined observations from the New Technology Telescope of the European Southern Observatory at La Silla, Chile, and from the Calar Alto Observatory in Spain with advanced modeling. This enabled them to find the triplet quasar, called QQQ J1519+0627. The light from the three quasars has traveled 9 billion light-years to reach us, which means the light was emitted when the universe was only a third of its current age.

Advanced analysis confirmed that what the team found was, indeed, three distinct sources of quasar energy and that the phenomenon is extremely rare.

Two members of the triplet are closer to each other than the third. This means that the system could have been formed by interaction between the two adjacent quasars, but was probably not triggered by interaction with the more-distant third quasar. Furthermore, no evidence was seen of any ultraluminous infrared galaxies — galaxies with strong emission in infrared light — which is where quasars are commonly found. As a result, the team proposes that this triplet quasar system is part of some larger structure that is still undergoing formation.

“Honing our observational and modeling skills and finding this rare phenomenon will help us understand how cosmic structures assemble in our universe and the basic processes by which massive galaxies form,” Fumagalli said.

“Further study will help us figure out exactly how these quasars came to be and how rare their formation is,” Farina said.

Article source: http://www.astronomy.com/~/link.aspx?_id=be73bc40-04e1-4974-a2a3-81eb3be57429

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Rare triple quasar found

triple-quasarFor only the second time in history, a team of scientists, including Michele Fumagalli from the Carnegie Institution for Science in Washington, D.C., has discovered an extremely rare triple quasar system.

Quasars are extremely bright and powerful sources of energy that sit in the center of a galaxy, surrounding a black hole. In systems with multiple quasars, the bodies are held together by gravity and are believed to be the product of galaxies colliding.

It is difficult to observe triplet quasar systems because of observational limits that prevent researchers from differentiating multiple nearby bodies from one another at astronomical distances. Moreover, such phenomena are presumed to be rare.

The team led by Emanuele Farina of the University of Insubria in Como, Italy, combined observations from the New Technology Telescope of the European Southern Observatory at La Silla, Chile, and from the Calar Alto Observatory in Spain with advanced modeling. This enabled them to find the triplet quasar, called QQQ J1519+0627. The light from the three quasars has traveled 9 billion light-years to reach us, which means the light was emitted when the universe was only a third of its current age.

Advanced analysis confirmed that what the team found was, indeed, three distinct sources of quasar energy and that the phenomenon is extremely rare.

Two members of the triplet are closer to each other than the third. This means that the system could have been formed by interaction between the two adjacent quasars, but was probably not triggered by interaction with the more-distant third quasar. Furthermore, no evidence was seen of any ultraluminous infrared galaxies — galaxies with strong emission in infrared light — which is where quasars are commonly found. As a result, the team proposes that this triplet quasar system is part of some larger structure that is still undergoing formation.

“Honing our observational and modeling skills and finding this rare phenomenon will help us understand how cosmic structures assemble in our universe and the basic processes by which massive galaxies form,” Fumagalli said.

“Further study will help us figure out exactly how these quasars came to be and how rare their formation is,” Farina said.

Article source: http://www.astronomy.com/~/link.aspx?_id=be73bc40-04e1-4974-a2a3-81eb3be57429

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Capturing the "wings" of the Seagull Nebula

Seagull-Nebula-wingThis new image from the European Southern Observatory (ESO) shows a section of a cloud of dust and glowing gas called the Seagull Nebula. These wispy red clouds form part of the “wings” of the celestial bird, and this picture reveals an intriguing mix of dark and glowing red clouds, weaving between bright stars. This new view was captured by the Wide Field Imager on the MPG/ESO 2.2-meter telescope at ESO’s La Silla Observatory in Chile.

Running along the border between the constellations of Canis Major the Big Dog and Monoceros the Unicorn in the southern sky, the Seagull Nebula is a huge cloud mostly made of hydrogen gas. It’s an example of what astronomers refer to as an HII region. Hot new stars form within these clouds, and their intense ultraviolet radiation causes the surrounding gas to glow brightly.

The reddish hue in this image is a telltale sign of the presence of ionized hydrogen. The Seagull Nebula, known more formally as IC 2177, is a complex object with a bird-like shape that is made up of three large clouds of gas: Sharpless 2-292 forms the “head”; this new image shows part of Sharpless 2-296, which comprises the large “wings”; and Sharpless 2-297 is a small, knotty addition to the tip of the gull’s right “wing”.

These objects are all entries in the Sharpless nebula catalog, a list of more than 300 glowing clouds of gas compiled by American astronomer Stewart Sharpless in the 1950s. Before he published this catalog, Sharpless was a graduate student at Yerkes Observatory in Wisconsin, where he and his colleagues published observational work that helped show that the Milky Way is a spiral galaxy with vast, curved arms.

Spiral galaxies can contain thousands of HII regions, almost all of which are concentrated along their spiral arms. The Seagull Nebula lies in one of the spiral arms of the Milky Way. But this is not the case for all galaxies; while irregular galaxies do contain HII regions, these are jumbled up throughout the galaxy, and elliptical galaxies are different yet again — appearing to lack these regions altogether. The presence of HII regions indicates that active star formation is still in progress in a galaxy.

This image of Sharpless 2-296 was captured by the Wide Field Imager (WFI), a large camera mounted on the MPG/ESO 2.2-meter telescope at ESO’s La Silla Observatory in Chile. It shows only a small section of the nebula, a large cloud that is furiously forming hot stars in its interior. The frame shows Sharpless 2-296 lit up by several particularly bright young stars — there are many other stars scattered across the region, including one so bright that stands out as the gull’s “eye” in pictures of the entire complex.

Article source: http://www.astronomy.com/~/link.aspx?_id=124342df-d4e5-4786-9ff0-dfed6c87a154

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GALEX reveals the largest-known spiral galaxy

NGC-6872The spectacular barred spiral galaxy NGC 6872 has ranked among the biggest stellar systems for decades. Now a team of astronomers from the United States, Chile, and Brazil has crowned it the largest-known spiral based on archival data from NASA’s Galaxy Evolution Explorer (GALEX) mission.

Measuring tip-to-tip across, its two outsized spiral arms, NGC 6872 spans more than 522,000 light-years, making it more than five times the size of our Milky Way Galaxy.

“Without GALEX’s ability to detect the ultraviolet light of the youngest, hottest stars, we would never have recognized the full extent of this intriguing system,” said Rafael Eufrasio from NASA’s Goddard Space Flight Center in Greenbelt, Maryland.

The galaxy’s unusual size and appearance stem from its interaction with a much smaller disk galaxy named IC 4970, which has only about one-fifth the mass of NGC 6872. The odd couple is located 212 million light-years from Earth in the southern constellation Pavo.

Astronomers think large galaxies, including our own, grew through mergers and acquisitions — assembling over billions of years by absorbing numerous smaller systems.

Intriguingly, the gravitational interaction of NGC 6872 and IC 4970 may have done the opposite, spawning what may develop into a new small galaxy.

“The northeastern arm of NGC 6872 is the most disturbed and is rippling with star formation, but at its far end, visible only in the ultraviolet, is an object that appears to be a tidal dwarf galaxy similar to those seen in other interacting systems,” said Duilia de Mello from Catholic University in Washington, D.C.

The tidal dwarf candidate is brighter in the ultraviolet than other regions of the galaxy, a sign that it bears a rich supply of hot young stars less than 200 million years old.

The researchers studied the galaxy across the spectrum using archival data from the European Southern Observatory’s (ESO) Very Large Telescope (VLT), the Two Micron All Sky Survey, and NASA’s Spitzer Space Telescope, as well as GALEX.

By analyzing the distribution of energy by wavelength, the team uncovered a distinct pattern of stellar age along the galaxy’s two prominent spiral arms. The youngest stars appear in the far end of the northwestern arm, within the tidal dwarf candidate, and stellar ages skew progressively older toward the galaxy’s center.

The southwestern arm displays the same pattern, which is likely connected to waves of star formation triggered by the galactic encounter.

A 2007 study by Cathy Horellou of Onsala Space Observatory in Sweden and Baerbel Koribalski of the Australia National Telescope Facility developed computer simulations of the collision that reproduced the overall appearance of the system as we see it today. According to the closest match, IC 4970 made its closest approach about 130 million years ago and followed a path that took it nearly along the plane of the spiral’s disk in the same direction it rotates. The current study is consistent with this picture.

As in all barred spirals, NGC 6872 contains a stellar bar component that transitions between the spiral arms and the galaxy’s central regions. Measuring about 26,000 light-years in radius, or about twice the average length found in nearby barred spirals, it is a bar that befits a giant galaxy.

The team found no sign of recent star formation along the bar, which indicates it formed at least a few billion years ago. Its aged stars provide a fossil record of the galaxy’s stellar population before the encounter with IC 4970 stirred things up.

“Understanding the structure and dynamics of nearby interacting systems like this one brings us a step closer to placing these events into their proper cosmological context, paving the way to decoding what we find in younger, more distant systems,” said Eli Dwek from Goddard.

The study also included Fernanda Urrutia-Viscarra and Claudia Mendes de Oliveira of the University of Sao Paulo in Brazil and Dimitri Gadotti at the European Southern Observatory in Santiago, Chile.

Article source: http://www.astronomy.com/~/link.aspx?_id=0d68927e-081b-4142-a089-17f391112488

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NASA’s Galex Reveals the Largest-Known Spiral Galaxy

This composite of the giant barred spiral galaxy NGC 6872 combines visible light
This composite of the giant barred spiral galaxy NGC 6872 combines visible light images from the European Southern Observatory’s Very Large Telescope with far-ultraviolet (1,528 angstroms) data from NASA’s GALEX and 3.6-micron infrared data acquired by NASA’s Spitzer Space Telescope. Image credit: NASA’s Goddard Space Flight Center/ESO/JPL-Caltech/DSS
› Full image and caption

January 10, 2013

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PASADENA, Calif. — The spectacular barred spiral galaxy NGC 6872 has ranked among the biggest stellar systems for decades. Now a team of astronomers from the United States, Chile and Brazil has crowned it the largest known spiral, based on archival data from NASA’s Galaxy Evolution Explorer (GALEX) mission, which has since been loaned to the California Institute of
Technology in Pasadena.

Measuring tip-to-tip across its two outsized spiral arms, NGC 6872 spans more than 522,000 light-years, making it more than five times the size of our Milky Way galaxy.

“Without GALEX’s ability to detect the ultraviolet light of the youngest, hottest stars, we would never have recognized the full extent of this intriguing system,” said lead scientist Rafael Eufrasio, a research assistant at NASA’s Goddard Space Flight Center in Greenbelt, Md., who is a doctoral student at Catholic University of America in Washington. He presented the findings Thursday at the American Astronomical Society meeting in Long Beach, Calif.

The galaxy’s unusual size and appearance stem from its interaction with a much smaller disk galaxy named IC 4970, which has only about one-fifth the mass of NGC 6872. The odd couple is located 212 million light-years from Earth in the southern constellation Pavo.

Astronomers think large galaxies, including our own, grew through mergers and acquisitions — assembling over billions of years by absorbing numerous smaller systems.

Intriguingly, the gravitational interaction of NGC 6872 and IC 4970 may have done the opposite, spawning what may develop into a new small galaxy.

“The northeastern arm of NGC 6872 is the most disturbed and is rippling with star formation, but at its far end, visible only in the ultraviolet, is an object that appears to be a tidal dwarf galaxy similar to those seen in other interacting systems,” said team member Duilia de Mello, a professor of astronomy at Catholic University.

The tidal dwarf candidate is brighter in ultraviolet than other regions of the galaxy, a sign it bears a rich supply of hot young stars less than 200 million years old.

The researchers studied the galaxy across the spectrum using archival data from the European Southern Observatory’s Very Large Telescope, the Two Micron All Sky Survey, and NASA’s Spitzer Space Telescope, as well as GALEX.

By analyzing the distribution of energy by wavelength, the team uncovered a distinct pattern of stellar age along the galaxy’s two prominent spiral arms. The youngest stars appear in the far end of the northwestern arm, within the tidal dwarf candidate, and stellar ages skew progressively older toward the galaxy’s center.

The southwestern arm displays the same pattern, which is likely connected to waves of star formation triggered by the galactic encounter.

A 2007 study by Cathy Horellou at Onsala Space Observatory in Sweden and Baerbel Koribalski of the Australia National Telescope Facility developed computer simulations of the collision that reproduced the overall appearance of the system as we see it today. According to the closest match, IC 4970 made its closest approach about 130 million years ago and followed a path that took it nearly along the plane of the spiral’s disk in the same direction it rotates. The current study is consistent with this picture.

As in all barred spirals, NGC 6872 contains a stellar bar component that transitions between the spiral arms and the galaxy’s central regions. Measuring about 26,000 light-years in radius, or about twice the average length found in nearby barred spirals, it is a bar that befits a giant galaxy.

The team found no sign of recent star formation along the bar, which indicates it formed at least a few billion years ago. Its aged stars provide a fossil record of the galaxy’s stellar population before the encounter with IC 4970 stirred things up.

“Understanding the structure and dynamics of nearby interacting systems like this one brings us a step closer to placing these events into their proper cosmological context, paving the way to decoding what we find in younger, more distant systems,” said team member and Goddard astrophysicist Eli Dwek.

The study also included Fernanda Urrutia-Viscarra and Claudia Mendes de Oliveira at the University of Sao Paulo in Brazil and Dimitri Gadotti at the European Southern Observatory in Santiago, Chile.

The GALEX mission is led by the California Institute of Technology in Pasadena, which is responsible for science operations and data analysis. NASA’s Jet Propulsion Laboratory, also in Pasadena, manages the mission and built the science instrument. GALEX was developed under NASA’s Explorers Program managed by NASA’s Goddard Space Flight Center. In May 2012, NASA loaned GALEX to Caltech, which continues spacecraft operations and data management using private funds.

For more information about GALEX, visit http://www.nasa.gov/galex and http://www.galex.caltech.edu/ .

Whitney Clavin 818-354-4673
Jet Propulsion Laboratory, Pasadena, Calif.
whitney.clavin@jpl.nasa.gov

Lynn Chandler 301-286-2806
Goddard Space Flight Center, Greenbelt, Md.

lynn.chandler-1@nasa.gov

J.D. Harrington 202-358-5241
Headquarters, Washington

j.d.harrington@nasa.gov

2013-016

Article source: http://www.jpl.nasa.gov/news/news.php?release=2013-016

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World’s largest telescope being built in Chile

When it is complete, the European Extremely Large Telescope in Chile will be the crown astronomical jewel of the European Southern Observatory, which celebrates its 50th birthday this year.

But construction of the world’s largest telescope will take $1.4 billion, a decade of work and an iron will on the part of the countries participating.

Most of the 14 member nations of the European Southern Observatory (ESO) are countries stricken by money difficulties sparked by the global recession that began in 2007. This pushed back construction of the 128-foot telescope from an expected start date of this year.

The project was approved in June. Most of the member countries have now committed financially, with the final ones expected to make their approvals in late 2012 or early 2013, ESO officials said. [European Southern Observatory's Top 10 Amazing Discoveries]

“We remain confident that the European member states will give the green light,” Lars Lindberg Christensen, an ESO spokesperson, told SPACE.com during an interview from the organization’s headquarters in Germany. “In a situation where you have a slowdown of the economy, you need to invest in research and development. You need to invest in industry.”

Chilean choice

Over the past 50 years, ESO telescopes have made stunning discoveries, including aiding the Nobel-prize winning find showing that the universe is accelerating as it expands.

When ESO was formed in 1962, there were few southern hemisphere telescopes available to do astronomy. The telescopes available in Chile, South Africa and Australia were typically no more than 6.5 feet in diameter. This made it difficult to look at the Milky Way’s center, or observe the Magellanic Clouds nearby Earth, or watch comets that graced southern hemisphere skies.

Countries in southern Africa were initially considered to host ESO’s facilities, but officials chose a remote location in Chile instead. Everything needs to be trucked in — water, food, telescopic equipment — at great expense. [Video: Exploring the Southern Sky - ESO at 50]

But the money is worth it, ESO determined, because the site has 330 cloud-free days a year. A typical astronomer travels roughly 6,200 to 7,500 miles to work there, so the weather patterns offer them a very high probability of getting usable telescope time.

“Basically, weather was the main driving force for the location,” Christensen said. “The more cloud-free conditions and the more stable atmosphere [one has], the more astronomy you can do.”

With ESO in the country, Chilean astronomers have immeasurably increased their activities in the field. They are granted a percentage of ESO telescope time in recognition of their agreement to host ESO, and officials noted they are contributing great science in their own right. Earlier this year, for example, Chileans led an ESO effort to catalog 84 million stars in the central part of the Milky Way.

Relations weren’t always this smooth. In 1995, Chile briefly ordered a work stoppage on the Very Large Telescope’s construction amid loud protests from ESO. At the time, Chile was facing lawsuits from private citizens who disputed the government’s claim to land that ESO was using for the construction.

The dispute was swiftly resolved, the VLT completed construction, and relations today are “close and collaborative” between ESO and Chile, the organization said.

Desert mountaintop sites

ESO’s facilities include 15 operational telescopes that it owns or shares, scattered across three mountaintop sites in the Atacama Desert of Chile.

La Silla is the site where ESO’s first telescope saw light in 1966, and where the New Technology Telescope first tested “active” optics to correct for external distortions such as temperature that affect telescopic mirrors. More recently, the site added an exoplanet seeker dubbed HARPS, for High Accuracy Radial Velocity Planet Searcher.

Paranal is ESO’s most famous location. The observatory hosts the Very Large Telescope, which is a collection of four 27-foot telescopes that can all link together to observe one object. The VLT can even hook up with four movable auxiliary telescopes – each about six feet in size – for a baseline of up to 656 feet.

The last site, Llano de Chajnantor, is the location of the world’s most complex radio telescope: the Atacama Large Millimeter/submillimeter Array (ALMA), which just started science observing in 2011.

As the site has grown, so has the maturity of the organization. ESO began with five founding countries and has now expanded to 14. Brazil is awaiting ratification to be the 15th member country.

ESO fields 1800 proposals for telescope time a year, generally receiving requests for 3 to 6 times more than the number of observing nights available. (The most oversubscribed telescopes are VLT and HARPS.) Work from ESO telescopes generates roughly 800 refereed papers a year.

The origins of the universe

While the science goes on in Chile, ESO is improving its headquarters in Germany.

The E-ELT prompted a badly needed expansion of ESO’s facilities that will essentially double the amount of space available to employees. The “green-friendly” construction will include a new office and a technical building, as well as a bridge that will span the two locations.

The more than 200,000-square-foot expansion is on time and budget, and should finish in 2013.

“Storage in the current building is short of space, so [more storage] is one little silly thing that people are looking forward to,” joked Christenson.

More importantly, the new headquarters is being put in place to better support the E-ELT. Officials are expecting a bevy of discoveries from the telescope.

The E-ELT will measure the properties of the first stars and galaxies, and — astronomers hope — will shed some light on the mysterious dark matter and dark energy that makes up most of the universe.

Most exciting to ESO is the potential to see how the universe operated in its early years.

“It is actually possible with this bigger telescope to go back in time and measure changes to the [universe's] fundamental physical constants,” Christenson said.

“It might be that the physical constants remain the same, but it could also be that they change. If they change, that would give us a view into some completely new physics that we don’t know about.”

Follow Elizabeth Howell @howellspace, or SPACE.com @Spacedotcom. We’re also on Facebook and Google+.

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Article source: http://www.cbsnews.com/8301-205_162-57556768/worlds-largest-telescope-being-built-in-chile/

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