Astronomers detected a faint but definite signal of oxygen in a galaxy located 13.28 billion light-years away from us, through observations using the Atacama Large Millimeter/submillimeter Array (ALMA). Breaking their own records, this marks the most distant oxygen ever detected in the Universe. Referencing infrared observations, the team determined that star formation in the galaxy started at an unexpectedly early stage; 250 million years after the Big Bang.

“Rather than saying I was happy, it would be more accurate to say I was thrilled to see the signal of the most distant oxygen,” explains Takuya Hashimoto, the lead author of the research paper published in the journal Nature and a researcher at Osaka Sangyo University and the National Astronomical Observatory of Japan. “I was excited enough that the signal appeared in my dreams and I had difficulty sleeping that night.”

An international team of astronomers led by Hashimoto used ALMA to observe a distant galaxy called MACS1149-JD1. They detected a signal from ionized oxygen in the galaxy. The infrared light emitted from oxygen was stretched to microwave wavelengths by the expansion of the Universe before it reached Earth and was observed by ALMA. The team measured the change in the wavelength of the light and found that the signal had traveled 13.28 billion light-years ^[1] to reach us, making it the most distant, or oldest, oxygen ever detected by any telescope. In addition, a weaker signal of neutral hydrogen emissions was independently found with the European Southern Observatory’s Very Large Telescope; the distance determined from this observation is consistent with the distance based on the oxygen observation. MACS1149-JD1 is the most distant galaxy with a precise distance measurement ^[2] .

For a certain period after the Big Bang, there was no oxygen in the Universe. Oxygen was created in stars and then released when the stars died. The detection of oxygen in MACS1149-JD1 indicates that an earlier generations of stars had been already formed and expelled processed oxygen by the epoch of observation, which is only about 500 million years after the beginning of the Universe.

The team then reconstructed the star formation history in the galaxy using infrared data taken with the NASA/ESA Hubble Space Telescope and NASA Spitzer Space Telescope. The observed brightness of the galaxy is well explained by a model where the onset of star formation was another 250 million years ago. The model indicates that the star formation became inactive once after the first ignition, and then revived at the epoch of the ALMA observations; 500 million years after the Big Bang. The astronomers suppose that the first star formation burst blew the gas away from the galaxy, which would suppress the star formation. Then, the gas returned to the galaxy leading to the second burst of star formation. The massive newborn stars in the second burst ionize oxygen, and it’s those emissions that have been detected with ALMA.

“The mature stellar population in MACS1149-JD1 implies that stars were forming back to even earlier times, beyond what we can currently see with our telescopes. This has very exciting implications for finding `cosmic dawn’ when the first galaxies emerged” adds Nicolas Laporte, a researcher at University College London/Université de Toulouse and a member of the research team.

ALMA has set the record for the most distant oxygen several times. In 2016, Akio Inoue at Osaka Sangyo University and his colleagues found the signal of oxygen at 13.1 billion light-years away with ALMA ^[3] . Several months later, Nicolas Laporte and his team used ALMA to detect oxygen at 13.2 billion light-years away ^[4] . Now, the two teams merged into one and achieved this new record. “This reflects the both competitive and collaborative nature of the forefront of scientific research,” said Inoue.

“With this discovery we managed to reach the earliest phase of cosmic star formation history,” said Hashimoto. “We are eager to find oxygen in even farther parts of the Universe and expand the horizon of human knowledge.”

 

 

 

Computer graphics movie of the star formation history in the galaxy MACS1149-JD1. The self-gravity of matter creates filamentary structures and the density at the intersections of the filaments increases. Around 200 million years after the Big Bang, active star formation ignites in the high density regions, which leads to the formation of galaxies. The gas in the galaxy is blown off by active stellar wind and supernovae, then the gas returns to the galaxy and causes another burst of star formation.
Download the movie file with English caption.
Download the movie file without caption.
Credit: ALMA (ESO/NAOJ/NRAO)

 

 

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Paper and research team

These observation results are published as Hashimoto et al. “The onset of star formation 250 million years after the Big Bang” in Nature on May 16, 2018.

The research team members are:
Takuya Hashimoto (Osaka Sangyo University/National Astronomical Observatory of Japan), Nicolas Laporte (University College London//Université de Toulouse), Ken Mawatari (Osaka Sangyo University/The University of Tokyo), Richard S. Ellis (University College London), Akio. K. Inoue (Osaka Sangyo University), Erik Zackrisson (Uppsala University), Guido Roberts-Borsani (University College London), Wei Zheng (Johns Hopkins University), Yoichi Tamura (Nagoya University), Franz E. Bauer (Pontificia Universidad Católica de Chile), Thomas Fletcher (University College London), Yuichi Harikane (The University of Tokyo), Bunyo Hatsukade (The University of Tokyo), Natsuki H. Hayatsu (The University of Tokyo/European Southern Observatory), Yuichi Matsuda (National Astronomical Observatory of Japan/SOKENDAI), Hiroshi Matsuo (National Astronomical Observatory of Japan/SOKENDAI), Takashi Okamoto (Hokkaido University), Masami Ouchi (The University of Tokyo), Roser Pelló (Université de Toulouse), Claes-Erik Rydberg (Universität Heidelberg), Ikkoh Shimizu (Osaka University), Yoshiaki Taniguchi (The Open University of Japan), Hideki Umehata (The Open University of Japan/The University of Tokyo/RIKEN), Naoki Yoshida (The University of Tokyo)

This research was supported by JSPS KAKENHI (Grant Numbers 26287034, 17H01114, 17H06130, 17H04831, 16H01085, 16H02166, 15K17616, 17K14252, JP17H01111, 16J03329, and 15H02064), NAOJ ALMA Scientific Research Grant Number 2016-01A, European Research Council Advanced Grant FP7/669253 and 339177, CONICYT-Chile Basal-CATA PFB-06/2007, FONDECYT Regular 1141218, and NAOJ Visiting Fellow Program.

 

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 National Science Council of Taiwan (NSC) 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.