Sunday, December 1, 2024

4627 - HOW GALAXIES FORM?

 

-  4627  -  HOW  GALAXIES  FORM?  -  The  James Webb Space Telescope (JWST) reveals new things about how planetary systems form.    Every second in the Universe, more than 3,000 new stars form as clouds of dust and gas undergo gravitational collapse. Afterward, the remaining dust and gas settle into a swirling disk that feeds the star’s growth and eventually accretes to form planets. known as a protoplanetary disk.


---------------------------------------   4627  -      HOW  GALAXIES  FORM?

-     JWST’s advanced infrared optics was used to examine protoplanetary disks around new stars. These observations provided the most detailed insights into the gas flows that sculpt and shape protoplanetary disks over time. They also confirm what scientists have theorized for a long time and offer clues about what our Solar System looked like roughly 4.6 billion years ago.

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-      In order for young stars to grow, they must draw in gas from the protoplanetary disk surrounding them. For that to happen, the gas must lose angular momentum (inertia); otherwise, it would consistently orbit the star and never accrete onto it.

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-     The mechanism that allows this to happen has remained the subject of debate among astronomers. In recent years, “magnetically driven disk” winds have emerged as a possible mechanism. Primarily powered by magnetic fields, these “winds” funnel streams of gas away from the planet-forming disk into space at dozens of kilometers per second.

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-    This causes it to lose angular momentum, allowing the leftover gas to fall inward toward the star.   Using Webb’s Near Infrared Spectrograph (NIRSpec), the astronomers could trace various wind layers by tuning the instrument to detect distinct atoms and molecules in certain transition states. The team also obtained spatially resolved spectral information across the entire field of view using the spectrograph’s Integral Field Unit (IFU).

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-    This allowed the team to trace the disk winds in unprecedented detail and revealed an intricate, three-dimensional layered structure: a central jet nested inside a cone-shaped envelop of winds at increasing distances. The team also noted a pronounced central hole inside the cones in all four protoplanetary disks.

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-    How a star accretes mass has a big influence on how the surrounding disk evolves over time, including the way planets form later on. The specific ways in which this happens have not been understood, but we think that winds driven by magnetic fields across most of the disk surface could play a very important role.

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-    However, other processes are also responsible for shaping protoplanetary disks. These include “X-wind,” where the star’s magnetic field pushes material outward at the inner edge of the disk.

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-    There are also “thermal winds,” which blow at much slower velocities and are caused by intense starlight eroding its outer edge. The high sensitivity and resolution of the JWST were ideally suited to distinguish between the magnetic field-driven wind, the X-wind, and the thermal wind. These observations revealed a nested structure of the various wind components that had never been seen before.

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-    A crucial distinction between the magnetically driven and the X-winds is how they are located farther out and cover broader regions. These winds cover regions that correspond to the inner rocky planets of our solar system, roughly between Earth and Mars. They also extend farther above the disk than thermal winds, reaching hundreds of times the distance between Earth and the Sun.

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-    The JWST observations revealed a nested structure that matched what astronomers anticipated for magnetically driven disk wind.    These observations strongly suggest that we have obtained the first detailed images of the winds that can remove angular momentum and solve the longstanding problem of how stars and planetary systems form.

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November 29, 2024         HOW  GALAXIES  FORM?                     4627

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--------------------- ---  Sunday, December 1, 2024  ---------------------------------

 

 

 

 

 

           

 

 

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