NASA's Webb Snaps Supersonic Outflow of Young Star

September 14, 2023 10:00AM (EDT)Release ID: 2023-141
At the center is a thin horizontal pinkish cloud known as Herbig-Haro 211 that is uneven with rounded ends, and tilted from bottom left to top right. It takes up about two-thirds of the length of this angle, but is thinner and longer at the opposite angle. At its center is a dark spot. On either side of the dark spot, there are orangish-yellow wisps that extend to light blue wisps. Within the center of those clouds, a pink fluffy streak runs through each lobe. At the ends of each lobe, pink becomes the dominant color. The lobe to the left is fatter. The right lobe is thinner, and ends in a smaller pink semi-circle. Just off the edge of this lobe is a slightly smaller pink semicircle, then a pink sponge-like blob.

Summary

Infrared capabilities map out molecular structure of outflow

NASA’s James Webb Space Telescope has captured a high-resolution look at Herbig-Haro 211 (HH 211), a bipolar jet traveling through interstellar space at supersonic speeds. At roughly 1,000 light-years away from Earth in the constellation Perseus, the object is one of the youngest and nearest protostellar outflows, making it an ideal target for Webb.

Full Article

Herbig-Haro (HH) objects are luminous regions surrounding newborn stars, formed when stellar winds or jets of gas spewing from these newborn stars form shock waves colliding with nearby gas and dust at high speeds. This image of HH 211 from NASA’s James Webb Space Telescope reveals an outflow from a Class 0 protostar, an infantile analog of our Sun when it was no more than a few tens of thousands of years old and with a mass only 8% of the present-day Sun. (It will eventually grow into a star like the Sun.) Infrared imaging is powerful in studying newborn stars and their outflows, because ...

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