In #Planet #Formation, It's Location, Location, Location
Issued by Inbox Astronomy
One of the top priorities for new home buyers is location. Finding a home in the right neighborhood is a key ingredient for a happy, prosperous family.
Like families hunting for a house, fledgling planets also need the proper location to grow and thrive. Astronomers using Hubble to probe the giant, young star cluster Westerlund 2 are finding that stars residing in the system's crowded central city face a rough-and-tumble neighborhood that suppresses planet formation. The Hubble observations show that lower-mass stars near the cluster's core do not have the large, dense clouds of dust that eventually could become planets in just a few million years.
But life is a lot easier for stars and would-be planets in the cluster suburbs, farther away from the dense center. Hubble detected those planet-forming clouds embedded in disks encircling stars in these neighborhoods.
The absence of planet-forming clouds around stars near the center is mainly due to their bully neighbors: bright, giant stars, some of which weigh up to 80 times the Sun's mass. Their blistering ultraviolet light and hurricane-like stellar winds of charged particles blowtorch disks around neighboring lower-mass stars, dispersing the giant dust clouds.
Understanding the importance of location and environment in nurturing planet formation is crucial for building models of planet formation and stellar evolution. Located 20,000 light-years away, Westerlund 2 is a unique laboratory to study stellar evolutionary processes because it's relatively nearby, quite young, and contains a large stellar population.
https://hubblesite.org/contents/news-releases/2020/news-2020-15
One of the top priorities for new home buyers is location. Finding a home in the right neighborhood is a key ingredient for a happy, prosperous family.
Like families hunting for a house, fledgling planets also need the proper location to grow and thrive. Astronomers using Hubble to probe the giant, young star cluster Westerlund 2 are finding that stars residing in the system's crowded central city face a rough-and-tumble neighborhood that suppresses planet formation. The Hubble observations show that lower-mass stars near the cluster's core do not have the large, dense clouds of dust that eventually could become planets in just a few million years.
But life is a lot easier for stars and would-be planets in the cluster suburbs, farther away from the dense center. Hubble detected those planet-forming clouds embedded in disks encircling stars in these neighborhoods.
The absence of planet-forming clouds around stars near the center is mainly due to their bully neighbors: bright, giant stars, some of which weigh up to 80 times the Sun's mass. Their blistering ultraviolet light and hurricane-like stellar winds of charged particles blowtorch disks around neighboring lower-mass stars, dispersing the giant dust clouds.
Understanding the importance of location and environment in nurturing planet formation is crucial for building models of planet formation and stellar evolution. Located 20,000 light-years away, Westerlund 2 is a unique laboratory to study stellar evolutionary processes because it's relatively nearby, quite young, and contains a large stellar population.
https://hubblesite.org/contents/news-releases/2020/news-2020-15
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