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Protoplanetary disc’s spiral arms embrace young star

Swirling around the young star Elias 2-27 is a stunning spiral-shape pinwheel of dust. This striking feature, seen with the Atacama Large Millimetre/submillimetre Array (ALMA), is the product of density waves — gravitational perturbations in the star’s protoplanetary disc that produce sweeping arms reminiscent of a spiral galaxy, but on a much smaller scale.

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Gluttonous young star may hold clues to planet formation

In 1936, infant star FU Orionis began gobbling material from its surrounding disc of gas and dust with a sudden voraciousness, eating the equivalent of 18 Jupiters in the last 80 years. During a three-month binge, as matter turned into energy, the star became 100 times brighter, heating the disc around it to temperatures of up to 6,650 °C.

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Light echoes give clues to young star’s protoplanetary disc

Protoplanetary discs are ‘doughnuts’ of gas and dust surrounding young stars, the sites where planets form over the course of millions of years. Researchers studying the one-million-year-old infant star YLW 16B, some 400 light-years from Earth, were able to determine the distance from the star to the inner rim of its surrounding protoplanetary disc by observing its light echo.

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Exiled exoplanet kicked out of star’s local neighbourhood?

A planet discovered last year sitting at an unusually large distance from its star — 16 times farther than Pluto is from the Sun — may have been kicked out of its birthplace close to the star in a process similar to what may have happened early in our own solar system’s history. The planet’s 13-million-year-old parent star is known as HD 106906 and lies 300 light-years away.

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Surprising chemistry seen in molecular rings around young star

Astronomers using the Atacama Large Millimeter/submillimetre Array (ALMA) have discovered two spectacular rings of molecules encircling the young, Sun-like star IM Lup. The rings are made up of one of the most common heavy ions in space — DCO+ (deuterium, carbon, oxygen). This chemistry reveals new insights into the conditions of the planet-forming disc surrounding this star.