Scientists Discover First Astrosphere Around Sunlike Star: What You Need to Know?

Astronomers have detected the first-ever astrosphere surrounding a sunlike star, revealing insights into early solar winds

Written by Gadgets 360 Staff | Updated: 9 December 2024 17:00 IST

Scientists Discover First Astrosphere Around Sunlike Star: What You Need to Know?

Photo Credit: Goddard Space Flight Center/NASA

A young star, the Moth, alters its dust disk shape while its stellar wind bubble remains intact

Astronomers have detected an astrosphere around a star resembling the Sun, marking a significant milestone in understanding stellar evolution. This finding, shared during the 25 Years of Science with Chandra symposium on December 3, 2024, provides a rare view into the early conditions of stars like the Sun. An astrosphere, described as a bubble of ionised gas formed by stellar wind, acts as a protective shell around stars. The discovery has shed light on how these structures are formed and their role in shielding planetary systems from cosmic radiation.

What Defines an Astrosphere?

Astrospheres are created by a star's stellar wind, a continuous stream of charged particles. For instance, the Sun's heliosphere serves as an example, extending beyond Pluto and safeguarding the solar system from cosmic rays. Despite extensive research, such phenomena had not been observed around stars with characteristics similar to the Sun. As per reports, Carey Lisse, a researcher at Johns Hopkins Applied Physics Laboratory, noted in an interview with a prominent science publication that the detection of astrospheres around average stars has been elusive for over two decades.

Key Target: HD 61005, Known as "The Moth"

The star HD 61005, dubbed “The Moth” for its distinctive wing-like dust disk, became the focus of this investigation. Its rapid movement through a dense interstellar gas cloud at approximately 10 kilometres per second has resulted in the unique shape of its surrounding disk. According to sources, HD 61005, which mirrors the size and mass of the Sun, was chosen for its youthful stage at 100 million years old. Young stars like this typically emit stronger stellar winds, providing ideal conditions for studying astrospheres.

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X-ray Data Unveil Unexpected Details

Observations captured by NASA's Chandra X-ray Observatory revealed a halo of X-rays encasing HD 61005. This structure extends nearly 100 times farther than the Sun's heliosphere. Contrary to expectations, the astrosphere displayed a spherical shape, suggesting the star's intense wind counteracts external pressures.

Insights into Solar Evolution

The findings are believed to offer clues about the early behaviour of the Sun and its protective influences on the young Earth. Understanding such phenomena could also aid in evaluating the habitability of planets orbiting stars with similar properties. The study represents a leap in comprehending the protective role of astrospheres across stellar systems.

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