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The Sciences

Researchers Close In On Birthdate of First Stars

D-briefBy Jake ParksMay 16, 2018 10:15 PM

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With the help of the Atacama large Millimeter/submillimeter Array, astronomers have detected the earliest signs of oxygen (red) distributed in the galaxy MACS1149-JD1. The discovery provides the strongest evidence yet that stars in the fledgling universe started forming earlier than previously thought — when it was less than 2 percent its current age. (Credit: ALMA (ESO/NAOJ/NRAO), NASA/ESA Hubble Space Telescope, W. Zheng (JHU), M. Postman (STScI), the CLASH Team, Hashimoto et al.) The Atacama Large Millimeter/submillimeter Array (ALMA) is not your standard, run-of-the-mill telescope. Instead, ALMA, which is located in the high-and-dry Atacama Desert of northern Chile, is a radio telescope made up of 66 high-precision antennas that operate in perfect harmony. When ALMA’s antennas (which range from 7 to 12 meters in diameter) are configured in different ways, the array is capable of zooming in on some of the most distant cosmic objects in the universe, as well as capturing images that are clearer than those produced by the Hubble Space Telescope.

First Starlight

In a new study set for publication tomorrow in the journal Nature, an international team of astronomers used this impressive array to observe an extremely distant galaxy called MACS1149-JD1. Within the galaxy, the team was surprised to discover faint signals of ionized oxygen that were emitted almost 13.3 billion years ago (or 500 million years after the Big Bang). This is not only the most distant detection of oxygen ever made by any telescope, but more importantly, the discovery of the ancient oxygen serves as clear evidence that stars began forming just 250 million years after the Big Bang, when the universe was less than 2 percent its current age. https://www.youtube.com/watch?v=_spfSRxR4lQ

Before the first stars kicked on, the universe was a relatively boring place, consisting primarily of radiation leftover from the Big Bang, as well as hydrogen and helium. However, many of the heavier elements we take for granted today (such as carbon and oxygen) did not exist before the first stars. This is because stars are the burning crucibles that convert hydrogen and helium into larger elements — without stars, there is no oxygen.“I was thrilled to see the signal of the distant oxygen in the ALMA data,” said lead author Takuya Hashimoto, a researcher at Osaka Sangyo University and the National Astronomical Observatory of Japan, in a press release. “This detection pushes back the frontiers of the observable universe.” One of the most burning questions on astronomers’ minds is: When did the first galaxies emerge from total darkness? This period, commonly referred to as ‘cosmic dawn,’ is of particular interest because it marked the transition from a hot, dense, and nearly homogeneous universe to the universe we are more familiar with today — one filled with stars, planets, nebulae, and people. “Determining when cosmic dawn occurred is akin to the Holy Grail of cosmology and galaxy formation,” said co-author Richard Ellis, an astronomer at University College London, in a press release. “With these new observations of MACS1149-JD1, we are getting closer to directly witnessing the birth of starlight! Since we are all made of processed stellar material, this is really finding our own origins.”

[This article originally appeared on Astronomy.com]

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