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Massive Star's Tailed Trajectory Reaches 8 Light-Years, Positioned Edgeward in Galaxy, Poised to Settle Important Scientific Contention

Massive jet of gas, spanning an impressive 8 light-years, emerging from star within Sharpless2-284 located on the periphery of our galaxy, captured in an image taken by the James Webb Space Telescope.

Massive celestial body's jet, spanning 8 light-years, positioned on the galaxy's edge, may provide...
Massive celestial body's jet, spanning 8 light-years, positioned on the galaxy's edge, may provide insights to resolve a significant scientific controversy

Massive Star's Tailed Trajectory Reaches 8 Light-Years, Positioned Edgeward in Galaxy, Poised to Settle Important Scientific Contention

A Stellar Discovery: The Birth Announcement of a Massive Star

In the vast expanse of space, a cosmic cloud known as Sharpless2-284 has become the site of a remarkable discovery. The James Webb Space Telescope, a groundbreaking instrument in astronomical research, has captured an image of a colossal jet emanating from a star within this cloud.

This jet, a double-lobed outflow, is shooting in opposite directions, making it a rare and powerful spectacle in the cosmos. The star, approximately 10 times the mass of our Sun, is part of a proto star cluster on the edge of the Milky Way, where a few hundred stars are still forming.

The jet's eruption offers fascinating insights into the star's formation history. According to the core accretion theory, as gas falls inwards and builds up around the star, it is blasted along the star's spin axis, likely due to magnetic fields. This theory suggests that the new theoretical models imply the star is still growing, approximately 10 times the mass of the Sun.

The detection of this jet provides astronomers with a valuable insight into a key stage in stellar birth. Webb's images suggest the formation of massive stars in such environments could proceed via a stable disk around the star, as predicted by core accretion theories. The opposite sides of the jets being nearly 180 degrees apart also validates a prediction of the core accretion theory.

Moreover, the star's low metallicity makes Sh2-284 a pristine target, offering insight into early Universe star formation. The discovery of this jet can help study the formation mechanism of massive stars in low metallicity environments.

This discovery helps settle a cosmic debate around star formation, supporting the core accretion model over the chaotic 'competitive accretion' model. Massive stars, like the one found inside this cluster, have significant effects on galaxy evolution.

The tips of the jet provide further intrigue, offering clues about the star's past and the conditions under which it was born. The jet, shooting across space at hundreds of thousands of miles per hour, is 8 lightyears long.

For those interested in delving deeper into the details of this discovery, the full paper can be read at iopscience.iop.org/article/10.3847/1538-4357/addf4b. This 'birth announcement' to the Universe serves as a testament to the ongoing exploration and discovery in the field of astronomy.

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