
© Iztok Bončina/ALMA (ESO/NAOJ/NRAO)Two of the telescopes comprising ALMA (the Atacama Large Millimeter/submillimeter Array) in Chile.
The galaxies of the Universe's youth worked busily at making stars - that much is certain. However, what did those galaxies look like? How many were there, and how were they distributed in space and time?
Over such huge distances, those galaxies appear faint to us, so it's only within the last decade or so that astronomers have been able to start obtaining a reasonable view of them. The newly inaugurated ALMA (Atacama Large Millimeter/submillimeter Array) is one of the most promising telescope arrays in the world for making observations of the early Universe.
As reported in a new
Nature paper, ALMA scientists measured the distances to 23 early star-forming galaxies in a patch of sky in the Southern Hemisphere. Out of that sample, at least 10 emitted their light when the Universe was less than 1.5 billion years old, placing them among some of the earliest galaxies observed.
Over the last ten years, astronomers discovered that the ratios of galaxy types shifted greatly over time. One particular type of galaxy - known as a dusty starburst galaxy - was nearly 1,000 times more common in the past than it is today. These galaxies, as their name suggests, form stars at a high rate and are swathed in the molecules collectively known as dust. (Lighter molecules, such as hydrogen H2, oxygen O2, or water H2O, behave as gases, whereas heavier molecules can stick together via static electricity, much as dust bunnies gather under your bed.)
Unshielded light from newborn stars is frequently dominated by blue and ultraviolet emission, but dust absorbs most of those wavelengths. This heats the dust, however, making it glow strongly in the infrared. The result: dusty starburst galaxies are intense infrared emitters.
Comment: Check out last week's SOTT Talk Radio show on this very topic:
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