ALMA Opens Its Eyes
Las galaxias Antena (también conocidas como NGC 4038 y 4039) son un dúo de galaxias espiral en colisión y con formas distorsionadas que están a unos 70 millones de años-luz de distancia, en la constelación de Corvus (el Cuervo). Esta imagen combina observaciones realizadas por ALMA durante la etapa de pruebas y observaciones en longitudes de onda de luz visible hechas con el telescopio espacial Hubble de la NASA y ESA. La imagen del Hubble es la más precisa que se haya captado de este objeto y sirve de referencia en términos de resolución. ALMA realiza observaciones en longitudes de onda mucho más largas, con lo cual es más difícil obtener imágenes tan nítidas. Sin embargo, cuando el conjunto de ALMA esté construido, su capacidad de resolución será diez veces superior a la del Hubble. La mayor parte de las observaciones de prueba de ALMA usadas para crear esta imagen se hicieron utilizadando solo doce antenas -menos de las que se usarán para las primeras observaciones científicas- y con separaciones mucho menores entre ellas, por lo cual no es más que un atisbo de lo que está por venir. A medida que el observatorio crezca y se vayan incorporando nuevas antenas, aumentará exponencialmente la precisión, eficiencia y calidad de sus observaciones. Aun así, esta es la mejor imagen que se haya obtenido de las galaxias Antena en ondas submilimétricas, lo que marca un hito en la exploración del Universo submilimétrico. Mientras que la observación en luz visible (representada principalmente en azul en esta imagen) permite detectar estrellas recién formadas en las galaxias, ALMA revela objetos imposible de observar en esa longitud de onda, como lo son las densas nubes de gas frío donde se forman las estrellas. Las observaciones de ALMA (representadas aquí en rojo, rosado y amarillo) se realizaron en longitudes de onda milimétricas y submilimétricas específicas para detectar la presencia de moléculas de monóxido de carbono en nubes de hidrógeno -invisibles en otras longitudes de onda-, donde se forman las estrellas. Se descubrieron concentraciones masivas de gas no solo en el corazón de ambas galaxias, sino también en la caótica zona donde entran en colisión. Allí, la cantidad de gas supera en miles de millones de veces la masa de nuestro Sol, lo que constituye una rica reserva de material para las futuras generaciones de estrellas. Este tipo de observaciones serán vitales para comprender cómo las colisiones de galaxias pueden provocar el nacimiento de estrellas. Este es solo un ejemplo de cómo ALMA revela partes del Universo que no pueden ser observadas por los telescopios ópticos e infrarrojos. Créditos: ALMA (ESO/NAOJ/NRAO). Imagen en luz visible: telescopio espacial Hubble de NASA/ESA.
Press Releases

ALMA Opens Its Eyes

3 October, 2011 / Read time: 9 minutes

The most powerful millimeter/submillimeter-wavelength telescope in the world opens for business and reveals its first image. 

Humanity’s most complex ground-based astronomy observatory, the Atacama Large Millimeter/submillimeter Array (ALMA), has officially opened for astronomers. The first released image, from a telescope still under construction, reveals a view of the Universe that cannot be seen at all by visible-light and infrared telescopes. Thousands of scientists from around the world competed to be the first few researchers to explore some of the darkest, coldest, farthest, and most hidden secrets of the Cosmos with this new astronomical tool.

“We are living in a historic moment for science and particularly for astronomy, and perhaps also for the evolution of humanity, because we start to use the greatest observatory under construction at the moment,” said Thijs de Graauw, ALMA Director.

At present, around a third of ALMA’s eventual 66 radio antennas make up the growing array on the Chajnantor plateau in northern Chile, at an elevation of 5,000 meters. And yet, even under construction, ALMA has become the best telescope of its kind – as reflected by the extraordinary number of astronomers who requested to observe with ALMA.

“The ‘M’ in ALMA stands for ‘millimeter/submillimeter’ waves, because ALMA views the Universe in these long wavelengths of light, much longer than the optical light we see with our eyes,” said Alison Peck, ALMA Deputy Project Scientist. “With millimeter and submillimeter waves, we can watch star and planet formation, investigate astrochemistry, and detect the light that is finally reaching us from the Universe’s earliest galaxies.”

ALMA is radically different from visible-light and infrared telescopes. It is an array of linked antennas acting as a single giant telescope, and it detects much longer wavelengths than those of visible light. Its images therefore look quite unlike more familiar pictures of the cosmos.

The ALMA team has been busy testing the observatory’s systems over the past few months, in preparation for the first round of scientific observations, known as Early Science. One outcome of their tests is the first image published from ALMA, albeit from what is still very much a growing telescope. Most of the observations used to create this image of the Antennae Galaxies were made using only twelve antennas working together —fewer than will be used for the first science observations — and with the antennas much closer together as well. Both of these factors make the new image just a taster of what is to come. As the observatory grows, the sharpness, efficiency, and quality of its observations will increase dramatically as more antennas become available and the array grows in size [1].

The Antennae Galaxies is a pair of colliding galaxies with dramatically distorted shapes. While visible light shows us the stars in the galaxies, ALMA’s view reveals something that cannot be seen in visible light: the clouds of dense cold gas from which new stars form [2]. This is the best submillimeter-wavelength image ever made of the Antennae Galaxies.

Massive concentrations of gas are found not only in the hearts of the two galaxies but also in the chaotic region where they are colliding. Here, the total amount of gas is billions of times the mass of our Sun — a rich reservoir of material for future generations of stars. Observations like these open a new window on the submillimeter Universe and will be vital in helping us understand how galaxy collisions can trigger the birth of new stars. This is just one example of how ALMA reveals parts of the Universe that cannot be seen with visible-light and infrared telescopes.

ALMA could accept only about a hundred or so projects for this first nine-month phase of Early Science. “It was absolutely tremendous to receive more than nine hundred project proposals from astronomers from throughout the world wanting to use ALMA in this first ever science period!” said Lewis Ball, ALMA Deputy Director. “That represents a level of demand which is unprecedented across any ground-based or space telescope.” The successful projects were chosen based on their scientific merit, their regional diversity, and also their relevance to ALMA’s major science goals.

One of the projects chosen for ALMA Early Science observations was that of David Wilner of the Harvard-Smithsonian Center for Astrophysics in Cambridge, Massachusetts, USA. Wilner said, “My team hunts for the building blocks of solar systems, and ALMA is uniquely equipped to spot them.”

His team’s target is AU Microscopii, a star 33 light years away that is only 1% of the age of our Sun. “We will use ALMA to image the ‘birth ring’ of planetesimals that we believe orbits this young star. Only with ALMA, however, can we hope to discover clumps in these dusty asteroid belts, which can be the markers of unseen planets.” Wilner and his team will share their data with a European team who also requested ALMA observations of this nearby, dust-ringed star.

Any hunt for habitable planets around other stars often begins with a hunt for water in those distant solar systems. Debris disks, the swarms of dust, gas, and rocks around stars, are suspected also to contain craggy ice chunks filled with frozen water, gas, and possibly even organic molecules — the astrochemistry of life.

Simon Casassus, from the University of Chile, and his team will use ALMA to observe the gas and dust disk around HD142527, a young star that is 400 light years away. “The dusty disk around this star has a very large gap, which may have been carved by the formation of giant planets,” said Casassus. “Outside the gap, this disk contains enough gas to make about a dozen Jupiter-sized planets. Inside the gap, a young gaseous giant planet could still be forming, if there is gaseous material available.” Their ALMA observations will measure the mass and physical conditions of gas interior to the gap. “Thus, ALMA gives us a chance to observe planet formation, or its most recent wake,” said Casassus.

Father away, 26,000 light years from us in the center of our galaxy, sits Sagittarius A*, a supermassive black hole four million times the mass of our Sun. Gas and dust between it and us hide it from our optical telescopes. However, ALMA is tuned to see through the galactic murk and give us tantalizing views of Sgr A*.

Heino Falcke, an astronomer at Radboud University Nijmegen in the Netherlands, said, “ALMA will let us watch flares of light coming from around this supermassive black hole, and make images of the gas clouds caught by its immense pull. This will let us study this monster’s messy feeding habits. We think that some of the gas may be escaping its grip, at close to the speed of light.”

ALMA is capable of seeing cosmic dust, the cold ashes from exploded stars. Like the black outlines in a child’s coloring book, cosmic dust and cold gas trace out structures inside galaxies, even if we can’t see those galaxies clearly. At the outer fringes of our visible Universe lie the mysterious starburst galaxies, bright islands in an otherwise calm, dark Cosmos. ALMA will hunt for cold gas tracers here, as far back as a few hundred million years after the Big Bang, at a time astronomers call “cosmic dawn.”

Masami Ouchi of the University of Tokyo in Japan will use ALMA to observe Himiko, a very distant galaxy churning out at least 100 Suns’ worth of stars every year and surrounded by a giant, bright nebula. “Other telescopes cannot show us why Himiko is so bright and how it has developed such a huge, hot nebula when the ancient Universe all around it is so calm and dark,” said Ouchi.“ALMA can show us the cold gas deep in Himiko’s star-forming nebula, tracing the movements and activities inside, and we will finally see how galaxies started forming at the cosmic dawn.

During its Early Science observations, ALMA will continue its construction phase in the Chilean Andes, high on the remote Chajnantor Plateau in the harsh Atacama Desert. Each new, climate-armored antenna will join the array and be linked via fiber optic cabling. The views from each distant antenna are assembled into one large view by one of the world’s fastest, special-purpose supercomputers, the ALMA Correlator, which can perform 17 quadrillion [3] operations per second.

By 2013, ALMA will be an up to 16-km wide array of 66 ultra-precision millimeter/submillimeter wave radio antennas working together as one and built by ALMA’s multinational partners in North America, East Asia, and Europe.

Thijs de Graauw, ALMA Director, said: “Today marks the recognition of the successful coalition of thousands of people from all over the world all working with the same goal: to build the world’s most advanced radio telescope to see into the Universe’s coldest, darkest places, where galaxies and stars and perhaps the building blocks of life are created.”

The Atacama Large Millimeter/submillimeter Array (ALMA), an international astronomy facility, is a partnership of the European Organisation for Astronomical Research in the Southern Hemisphere (ESO), the U.S. National Science Foundation (NSF) and the National Institutes of Natural Sciences (NINS) of Japan in cooperation with the Republic of Chile. ALMA is funded by ESO on behalf of its Member States, by NSF in cooperation with the National Research Council of Canada (NRC) and the Ministry of Science and Technology (MOST) in Taiwan and by NINS in cooperation with the Academia Sinica (AS) in Taiwan and the Korea Astronomy and Space Science Institute (KASI).

ALMA construction and operations are led by ESO on behalf of its Member States; by the National Radio Astronomy Observatory (NRAO), managed by Associated Universities, Inc. (AUI), on behalf of North America; and by the National Astronomical Observatory of Japan (NAOJ) on behalf of East Asia. The Joint ALMA Observatory (JAO) provides the unified leadership and management of the construction, commissioning and operation of ALMA.

[1]  The quality of images from an interferometric telescope like ALMA depends on both the separations and the number of the antennas. Larger separations mean that sharper images can be created and if more antennas are working together more detailed images can be produced. More information about ALMA and interferometry.

[2]  The observations were made at specific wavelengths of millimeter and submillimeter light, tuned to detect carbon monoxide molecules in the otherwise invisible hydrogen clouds, where new stars are forming.

[3]  1.7×1016 operations per second.

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