The new discoveries were made from observations made by radio telescopes from ALMA (Atacama Large Millimeter Array), an observatory located in the Atacama Desert, in Chile. The results were reported in the study published in The Astrophysical Journal. This is considered the most detailed investigation ever done into molecular gas content in a galaxy in the early universe. It is also the most distant detection of water in a star-forming galaxy. “Oxygen and carbon, in particular, are first generation elements. In the molecular forms of carbon monoxide and water, they are essential for life as we know it,” said Sreevani Jarugula, an astronomer at the University of Illinois, USA, and lead author of the study. The fact that SPT0311-58 is a massive galaxy helped with the discoveries: “There is more gas and dust compared to other galaxies in the early universe”, says the researcher. "This gives us many potential opportunities to observe abundant molecules and better understand how these life-creating elements impacted the development of the universe."
There is a correlation between the infrared emission of dust and the presence of water: “Dust absorbs ultraviolet radiation from stars and re-emits it as infrared photons”, explains Jarugula. "This stimulates the molecules, causing an emission of water that scientists can see." Studying the formation of the first galaxies helps scientists better understand their properties and how they interact with each other, as well as the emergence and evolution of the universe.
Post a Comment