Cosmic Chemistry: Unlocking the Unexpected Secrets of Early Universe’s Star Factories

Unexpected Chemistry Reveals Cosmic Star Factory Secrets

Researchers at Chalmers University of Technology have uncovered new insights into two early-universe galaxies, observing a variety of molecules and illuminating the star-formation processes of these distant galaxies through advanced telescope observations. Credit:

A groundbreaking study by Chalmers University scientists reveals unprecedented molecular details in two early-universe galaxies, advancing our understanding of their star-formation activities.

Two galaxies in the early universe, which contain extremely productive star factories, have been studied by a team of scientists led by Chalmers University of Technology in Sweden. Using powerful telescopes to split the galaxies’ light into individual colors, the scientists were amazed to discover light from many different molecules – more than ever before at such distances. Studies like this could revolutionize our understanding of the lives of the most active galaxies when the universe was young, the researchers believe.

Unveiling the Nature of Early Galaxies

When the universe was young, galaxies were very different from today’s stately spirals, which are full of gently-shining suns and colorful gas clouds. New stars were being born, at rates hundreds of times faster than in today’s universe. Most of this, however, was hidden behind thick layers of dust, making it a challenge for scientists to discover these star factories’ secrets – until now. By studying the most distant galaxies visible with powerful telescopes, astronomers can get glimpses of how these factories managed to create so many stars.

Molecules Found in Galaxy NCv1.143

Light from many different molecules reveals the secrets of distant star factories. The illustration shows representations of the molecules found in the distant galaxy NCv1.143, superimposed on an image of a similar galaxy in the nearby universe – NGC 572 – taken in visible light by the Hubble telescope. Credit: ESA/Hubble, NASA, L. Ho; Jmol (molecules); R. Cumming (montage)

In a new study, published on December 14 in the journal Astronomy & Astrophysics, a team of scientists led by Chalmers astronomer Chentao Yang, used the telescopes of NOEMA (NOrthern Extended Millimetre Array) in France to find out more about how these early star factories managed to create so many stars. Yang and his colleagues measured light from two luminous galaxies in the early universe – one of them classified as a quasar, and both with high rates of star formation.

“We knew these galaxies were prodigious star factories, perhaps amongst the biggest the universe has ever seen. To be able to find out how they work, we measured their light at wavelengths around one millimeter, hoping to collect new clues,” says Chentao Yang.

Molecular Insights From Distant Galaxies

The measurements proved to be successful beyond the scientists’ expectations. In the light they recorded from both galaxies, they identified traces of many different kinds of molecules. From deep within these galaxies, light is emitted in many different wavelengths from the clouds of gas and dust where new stars are born.

“It’s an amazing explosion of color, in shades that the human eye can’t see. But by combining our observations with our knowledge of physics and chemistry, we can understand what the colors mean, and see what differences there are between different galaxies,” explains Sergio Martín, astronomer at ESO and Joint ALMA Observatory, Chile, and member of the research team.

Molecules Found in Galaxy APM 08279+5255

Light from many different molecules reveals the secrets of distant star factories. The illustration shows representations of the molecules found in the distant galaxy APM 08279+5255, superimposed on an image of a similar galaxy in the nearby universe – IC 5063 – taken in visible light by the Hubble telescope. Both of these galaxies have an active supermassive black hole at their center. Credit: NASA, ESA & W. P. Maksym (CfA); Jmol (molecules); R. Cumming (montage)

By analyzing each galaxy’s spectrum – the individual colors of their light – the scientists were able to identify 13 molecules, several of which have never been seen before in such distant galaxies. Each molecule gives different clues about the temperature, pressure, and density in the space between the stars, and about how starlight, radiation, and matter interact – providing key new information on the physical and chemical conditions in these galaxies.

“Interpreting the signals is a challenge. We are seeing part of the electromagnetic spectrum that is hard to observe in nearby galaxies. But thanks to the expansion of the universe, the light from distant galaxies like these is shifted to longer wavelengths that we can see with radio telescopes observing in the sub-millimeter,” says Chentao Yang.

More Like a Neon-Lit City Than a Night Under the Stars

The two galaxies studied by the team are so far away that their light takes almost 13 billion years to reach us.

“Looking at these galaxies is less like a night under the stars and more like seeing a city lit with neon lights,” says Susanne Aalto, Chalmers astronomer and team member.

Astronomers are used to taking pictures of our galaxy’s star factories, like the Orion Nebula and the Carina Nebula, she explains.

“In these two distant galaxies, we are instead seeing star factories that are bigger, brighter, full of dust, and different in many ways. The Orion and Carina nebulae are lit up thanks to ultraviolet light from hot, newborn stars. In these two distant galaxies, ultraviolet light can’t get past the layers of dust. Much of the illumination is instead thanks to cosmic rays – high energy particles that can be created by exploding stars, or close to a supermassive black hole,” says Susanne Aalto.

Light From the Distant Galaxies NCv1.143 and APM 08279+5255

Light from two distant galaxies showing signs of many different molecules. The sharp peaks in these graphs, known as spectral lines, tell astronomers about the gas clouds that emit the light. The horizontal axis shows both wavelength and frequency of the light; the vertical axis shows relative brightness. The top spectrum has been shifted upwards for clarity. In red, the graph shows the galaxy NCv1.143 and in purple, APM 08279+5255. Credit: Chentao Yang et al.

The Uniqueness of Early-Universe Galaxies

While galaxies like these two are rare, the scientists have plans to study more of them, using both NOEMA and its even bigger sister telescope, ALMA (the Atacama Large Millimetre/Submillimetre Array) in Chile. Both telescopes are sensitive to light with wavelengths of around one millimeter.

“Our results show how NOEMA, with its broadband receivers and powerful correlator computer, has opened up new opportunities for studying extreme galaxies like these in the northern sky. From the southern hemisphere, ALMA’s planned wideband sensitivity upgrades will offer even more exciting prospects. The most remarkable galaxies in the early universe are finally able to tell their stories through their molecules,” says Pierre Cox, astronomer at CNRS and Sorbonne Université, France.

More About the Research Results

Over a hundred different molecules have been detected in interstellar space. In this study, the astronomers identified molecules of carbon monoxide (CO), the cyano radical (CN), the ethynyl radical (CCH), hydrogen cyanide (HCN), the formyl cation (HCO+), hydrogen isocyanide (HNC), carbon monosulphide (CS), water (H2O), the hydronium ion (H3O+), nitric oxide (NO), diazenylium (N2H+), the methylidyne radical (CH), and cyclopropenylidene (c-C3H2). Several of these (CH, CCH, c-C3H2, N2H+, and H3O+) have never been seen before at such large distances.

The two galaxies in the study have catalog numbers APM 08279+5255 and NCv1.143. Previous studies have shown that they are so far away that their light has been traveling towards us for nearly 13 billion years, corresponding to redshifts of 3.911 and 3.565, respectively. Redshift means that the expansion of the universe stretches the light from distant galaxies to longer wavelengths, which can be observed with radio telescopes.

Despite their distance, the galaxies shine brightly at radio wavelengths. Their signals are amplified thanks to clusters of other galaxies that lie along the light’s path – an effect known as gravitational lensing. One of the galaxies, APM 08279+5255, is also a quasar, a galaxy whose center glows brightly all the way from radio waves to X-rays, due to material swirling around a supermassive black hole. NCv1.143 may also contain a central black hole.

Reference: “SUNRISE: The rich molecular inventory of high-redshift dusty galaxies revealed by broadband spectral line surveys” by Chentao Yang, Alain Omont, Sergio Martín, Thomas G. Bisbas, Pierre Cox, Alexandre Beelen, Eduardo González-Alfonso, Raphaël Gavazzi, Susanne Aalto, Paola Andreani, Cecilia Ceccarelli, Yu Gao, Mark Gorski, Michel Guélin, Hai Fu, R. J. Ivison, Kirsten K. Knudsen, Matthew Lehnert, Hugo Messias, Sebastien Muller, Roberto Neri, Dominik Riechers, Paul van der Werf and Zhi-Yu Zhang, 14 December 2023, Astronomy & Astrophysics.
DOI: 10.1051/0004-6361/202347610

More about the research group:

The team is composed of: Chentao Yang (Chalmers University of Technology, Sweden), Alain Omont (CNRS and Sorbonne Université, France), Sergio Martín (ESO and Joint ALMA Observatory, Chile), Thomas G. Bisbas (Zhejiang Laboratory, China), Pierre Cox (CNRS and Sorbonne Université, France), Alexandre Beelen (Aix Marseille University, France), Eduardo González-Alfonso (Universidad de Alcalá, Spain), Raphaël Gavazzi (Aix Marseille University), Susanne Aalto (Chalmers University of Technology), Paola Andreani (ESO), Cecilia Ceccarelli (Université Grenoble Alpes, CNRS), Yu Gao (Xiamen University, China), Mark Gorski (Chalmers University of Technology), Michel Guélin (IRAM, France), Hai Fu (University of Iowa, USA), Rob J. Ivison (ESO, Macquarie University, Dublin IAS, University of Edinburgh), Kirsten K. Knudsen (Chalmers University of Technology), Matthew Lehnert (Centre de Recherche Astrophysique de Lyon, CRAL, France), Hugo Messias (ESO and Joint ALMA Observatory), Sebastien Muller (Chalmers University of Technology), Roberto Neri (IRAM), Dominik Riechers (Universität zu Köln), Paul van der Werf (Leiden University, Netherlands) and Zhi-Yu Zhang (Nanjing University, China).

More about NOEMA:

NOEMA, the Northern Extended Millimetre Array, is the most powerful millimeter observatory in the Northern Hemisphere, located on 2500 meters above sea level on the Plateau de Bure in the French Alps and run by IRAM. It consists of an array of 12 individual 15-metre antennas. During observations, the antennas function as a single telescope by using a technique called interferometry.

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