NASA’s Webb Telescope Unmasks True Nature of the Cosmic Tornado

Is the ice cream sand with a cherry? This randomly alignment of Harbig Haro 49/50 can be a trick with a multi-faceted spiral galaxy of a random alignment-syllable protostar. NASA’s James Webpace provides a high resolution view to discover this new comprehensive picture and the excellent details of this bubbles activity combining the observations of the Telescope (nearest infrared camera) and Marie (middle infrared device).

Herbig Haro items are the flows made by the jets launched by the nearby, forming star. The flow, which can spread over the years of light, can stir in a large region of material. This causes trauma waves, and heat the material at high temperatures. The material then cools down the light on the visible and infrared wavelengths.

When NASA’s retired Spitzer Space Telescope Observed it in 2006Scientists, Herbig Haro 49/50 (HH 49/50), named it as the “cosmic storm” for its helical appearance, but they were uncertain about the nature of the fuzzy item at the tip of the “storm”. With its high imaging resolution, showing the excellent features of the surprising regions in the webout flu, by exposing the Fijit Object as a remote galaxy, and showing a sea of ​​remote background galaxies, the HH provides a different visual impression of 49/50.

HH is located in 49/50 Chameleon I Cloud Complex One of the closest active star -forming regions in our sky, which is making a number of low mass stars like our sun. This cloud complex is potentially similar to the environment in which our sun is formed. Past observations of the region show that the HH49/50 flow is moving away from us at a speed of 60-190 miles per second (100-300 km per second) and this is just one feature of a large emission.

HH49/50 detects the web of the web and my observations of the shining hydrogen molecules, carbon monoxide molecules, and the location of the dynamic grain of dust, which are represented by orange and red, because the region is as Protestiller jet slimes. The web observations are details of small local scales that will help astronomers model the properties of jet and understand how it is affecting the surrounding content.

The arc -shaped properties in HH49/50, which are like a water weekend by high -speed boat, point to the source of this flow. Based on past observations, scientists suspect that Ceder Blood is a viable driver of a proteostar jet activity known as 110 IRS4. The HH 49/50 (off the lower right corner of the web image) is located about 1.5 1.5 light years away, CED 110 IRS4 is a Class I Protostar. Class I Protostors are young items in the prime time (tens to one million years old) in the prime time. They usually have a comprehensible disk of the content around them that is still falling on the protostar. Scientists recently used the web’s and my observations to study this protostar Get an inventory Of the icy structure of its environment.

This detailed web images of the ARC in HH49/50 can identify the direction of the jet source, but not every arc is identified in the same direction. For example, there is an unusual outcred feature (the upper right side of the central emission), which can be another chance of a different emission of the slow urine from the jet from the jet. As an alternative, this feature can be the result of the collapse of the central emission.

https://www.youtube.com/watch?v=u_gviglw954

Video Title:
The concept examines the three -dimensional structure of Herbug Haro 49/50 (HH 49/50), as seen in the near and middle infrared light by the James WebSpace telescope. The HH49/50 is a flow that is manufactured by the nearby steel -forming star jet in our Akashiganga I Cloud Complex, one of the closest active star -forming areas in our Akashiganga. At a distance of 625 light years from the ground, it allows researchers to review its details on small scales as never before.

Visual Credit: NASA, ESA, CSA, JDPSCol (STSCI), L Histock (STSCI), G Bacon (STSCI), R Kraford (STSCI), D Krishinblat (STSCI), C News (STSCI), APAgan (STSCI).

The galaxy that appears at the tip of the HH 49/50 is far away, the face on the spiral galaxy. It is a prominent central bulge representing blue, which shows the location of old stars. The bulge also shows indicators of “side lobes”, suggesting that it may be a banned galaxy. The red flags inside the spiral arms show hot dust places and stars forming groups. Even the galaxy shows empty bubbles in these dusty areas, which are like the close galaxies observed by the web as part of the fungus program.

The web has captured these two non -connected items in the lucky alignment. In thousands of years, the edge of HH 49/50 will move out and eventually appears to hide the galaxy.

Want more? Take a Look closely at the pictureFor, for, for,. “Fill” in a concept “And Compare the web photo with Spitzers Space Telecope.

Herbug Haro is located about 62 625 light years from Earth in Chamilion in the 49/50 tower.

James Webpace Telescope is the world’s largest space science Observatory. The web will solve the mystery in our solar system, will look out of the worlds around the other stars, and it will investigate the mysterious structures and origin of our universe and our place in it. The web is an international program led by NASA with its partners, ESA (European Space Agency) and the Canadian Space Agency.

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View/Download all image products on all resolutions For this article by the Space Telescope Science Institute.

Laura Beatz – Laura.e.betz@nasa.gov
Nasa Goddard Space Flight CenterGreen Belt, MD.

Queen Hart – qhart@stsci.edu
Space Telescope Science InstituteBaltimore, MD.

Christine Plem – cpuliam@stsci.edu
Space Telescope Science InstituteBaltimore, MD.

Photographs – Web photos of other Protostar Out Floose – L483, HH 46/47And HH 211

Animation video – “”Looking for the formation of the stars and planets

Interactive – Discover jets discovered by young stars in multiple wavelengths: View Space Interactive

Article – Read more about Herbig Haro Items

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