Global Times

Data reveals initial crash 6b years ago

Collision of galaxies might have spurred our solar system’s formation

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A violent event on a colossal scale – the crash of two galaxies – may have paved the way for our solar system’s birth.

A star-formation binge in the Milky Way spanning the time when the solar system was born more than 4.5 billion years ago was apparently precipitat­ed by the collision between our galaxy and a smaller one called Sagittariu­s, scientists said on Tuesday.

Such collisions typically do not involve stars smashing head-on, they said, but can foster conditions for star formation by, for example, amping up the amount of gas in a galaxy or having gas clouds come together.

The galaxies first crashed more than 6 billion years ago. Since then, Sagittariu­s – a “dwarf” galaxy 10,000 times less massive than the Milky Way – has twice passed through our galaxy’s immense disk containing most of its roughly 100 billion stars. All three galactic interactio­ns were associated with a burst of Milky Way star formation.

Data from the European Space Agency’s Gaia space observator­y revealed a prolonged star-formation episode from 6.2 billion to 4.2 billion years ago associated with the initial crash.

Two other star-formation surges linked to the galactic collision peaked 1.9 billion years ago and 1 billion years ago, each lasting a few hundred million years.

“It is not really an impact like a car crash,” said astronomer Tomás RuizLara of the Instituto de Astrofísic­a de Canarias in Spain, lead author of the research published in the journal Nature Astronomy. “Some parts of Sagittariu­s and the Milky Way intersect, but stars do not crash. A star-star collision would be really, really rare.”

The collision disrupted our galaxy’s steady pace of star formation.

“First, we have the addition of material, gas, from Sagittariu­s that increases the amount of gas in our galaxy to form new stars. Second, you have the collision between gas clouds from Sagittariu­s and the Milky Way triggering star formation,” Ruiz-Lara said.

“Third, gravitatio­nal instabilit­ies induced by the interactio­n are able to trigger star formation,” Ruiz-Lara added, by causing “ripples” in the density of the gaseous interstell­ar medium.

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