Thursday, October 29, 2015

Newscenter Update: Spirals in Dust Around Young Stars May Betray Presence of Massive Planets

October 29, 2015
Protoplanetary Disk: Simulated Spiral Arm vs. Observational Data
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Spirals in Dust Around Young Stars May Betray Presence of Massive Planets

A team of astronomers is proposing that huge spiral patterns seen around some newborn stars, merely a few million years old (about one percent our sun's age), may be evidence for the presence of giant, unseen planets. This idea not only opens the door to a new method of planet detection, but also could offer a look into the early formative years of planet birth. Though astronomers have cataloged thousands of planets orbiting other stars, the very earliest stages of planet formation are elusive because nascent planets are born and embedded inside vast, pancake-shaped disks of dust and gas encircling newborn stars. The conclusion that planets may betray their presence by modifying circumstellar disks on large scales is based on detailed computer modeling of how gas-and-dust disks evolve around newborn stars.

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