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When the universe was young, there were no stars, galaxies, or fifty-fifty atoms. As space expanded, hydrogen atoms formed and coalesced into stars. Eventually, the first galaxies emerged, and some of those galaxies may nevertheless be. New information from researchers at Durham Academy in the Britain and Harvard in the Us suggests several of those ancient galaxies could be in our ain lawn. This discovery also lends credence to a leading model of the early universe.

Our electric current understanding holds that the early universe was not fifty-fifty transparent to radiation. It took thousands of years for that to change, and the first atoms of hydrogen formed about 380,000 years later on the Big Bang. This menstruation is sometimes called the Cosmic Dark Ages because at that place were no stars or other objects producing light or other frequencies in the electromagnetic spectrum. It would take almost 100 million years longer for the universe to cool enough that the atoms could dodder together to form stars that populated the very first galaxies. But then, galaxy germination stopped for most a billion years.

The intense ultraviolet radiations from those early galaxies ionized the remaining hydrogen atoms, making information technology harder for them to cool and form stars. That hydrogen did somewhen absurd and formed massive dark thing halos around galaxies. This, in plough, shielded ionized gas from radiation, allowing it to cool and class stars. Thus, milky way germination resumed. This is a key component of the widely accepted Lambda-cold-night-matter model, and the team behind the latest research says its results support the model.

The team found two singled-out populations of dwarf galaxies orbiting our Milky Style galaxy. One group formed during the era before nighttime matter halos were built up. The other is more contempo and brighter. The offset set is over 13 billion years one-time — among the oldest in the universe. The brighter ones are at least several hundred million years younger. In the "old" set are Segue-1, Bootes I, Tucana 2, and Ursa Major I. The team found a similar distribution among observable dwarf galaxies in orbit of M31 (Andromeda).

This distribution of older and younger galaxies are in line with the Lambda-cold-night-matter model. Information technology would have been impossible to clarify the older dwarf galaxies even ten years agone, only improved instruments allowed the team to make up one's mind the properties of these tiny galaxies.

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