The powerful “space tornado” received high resolution glow thanks to NASA’s James Webb Space Telescope (JWST). Herbig-Haro49/50 (HH 49/50) new look Released today We also answer questions that astronomers have been curious about, as we first spotted the distant layers nearly 20 years ago.

The HH 49/50 was first glimpsed in 2006 by NASA’s now-retired Spitzer Space Telescope. Located approximately 625 light years from Earth in the constellation Chamayleon, astronomers were quickly called HH 49/50 “Cosmic Trnado”. Such Herbig-Haro objects are not rare, but when known as protostals, they only occur in very specific situations related to the earliest stages of the star.

Protostal’s journey to become the sun on a distant planet covers multiple stages and spans millions of years. During this time, including the creation of Herbig Halo objects, a huge amount of energy is required and generated. These arrangements are created after the high-energy jets are striped for several light years and collide with areas of more dense material. The resulting shock waves can heat the surrounding material. It cools through the emission of light at both infrared and visible wavelengths.

When Spitzer first spotted the HH 49.50, astronomers noticed a small, bright, conflicting location at the top tip of a tornado in space. Since then, experts have been following the identity of fuzzy mystery objects. Using JWST’s powerful toolkit, astronomers have got the answer.

The latest look of the HH 49/50 is one of the best looks of the Herbig-Haro object, created by photographing on the space telescope’s near-infrared camera (Nircam) and mid-infrared instrument (Miri). Estimated to be far from us at 60-190 mph, the swirl rocks consist of sparkling carbon monoxide and hydrogen molecules, as well as highly energyed cosmic dustmots.

This side-by-side comparison shows a Spitzerspace infrared infrared array camera image on HH 49/50 (left) for a Webb image of the same object (right) using NIRCAM (near-infrared) instruments and MIRI (mid-infrared instruments). Webb’s image shows intricate details of heated gas and dust as Protosterjet pounds onto the material. Webb also resolves “fuzzy” objects at the tip of the runoff into a distant, spiral galaxy. Images of Spitzer show 3.6 micron light in blue, 4.5 micron green and 8.0 microns in red (IRAC1, IRAC2, IRAC4). In the Webb image, blue represents 2.0 microns (F200W) of light, cyan represents light at 3.3 microns (F335M), green represents 4.4 microns (F444W), orange represents 4.7 microns (F470N), and red represents 7.7 microns (F770W). credit: NASA, ESA, CSA, STSCI, NASA-JPL, SSC

“The arc-shaped feature of the HH 49/50 refers to the source of this spill, similar to the water wake created by speeding boats.” NASA explained in the announcement. “Based on past observations, scientists suspect that the Protostal, known as the Cederblad 110 IRS4, is a plausible driver of jet activity.”

The CED 110 IRS4 can be seen near the bottom right corner of the image, and is about 1.5 light years away from HH 49/50. As a Class I primitive group, astronomers estimate it is less than a million years, and have won mass at its peak period.

For Bright Dot, first captured in 2006, no professional astronomers are required to identify well-defined publications documented by JWST. According to NASAIt is a spiral galaxy located against the “sea of ​​a distant background galaxy.” If you see it clearly, the blue “notable central bulge” of the old stars is on display, but the red area inside the spiral arm shows galaxy gas and protostal clouds.

HH 49/50 Lucky Alignment and Face-On Spiral Galaxy offer the unique look of two universes. Given the jet stream speed of the HH 49/50, the energy plume could completely obscure spiral galaxies within thousands of years.

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Andrew Paul is a staff writer for popular science covering Tech News.



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