Sunday, June 23, 2024

 

-    4510  -  WEBB  TELESCOPE'S    -  new discoveries?   When the James Webb Space Telescope was launched at the end of 2021, we expected stunning images and illuminating scientific results. So far, the powerful space telescope has lived up to our expectations. The JWST has shown us things about the early universe we never anticipated.

-


-------------------------------  4510  -  WEBB  TELESCOPE'S    -  new discoveries? 

-

-     The early universe is one of the JWST's primary scientific targets. Its infrared capabilities allow it to see the light from ancient galaxies with greater acuity than any other telescope. The telescope was designed to directly address confounding questions about the high-redshift universe.

-

-    The early universe and its transformations are fundamental to our understanding of the universe around us today. Galaxies were in their infancy, stars were forming, and black holes were forming and becoming more massive.

-

-   The Hubble Space Telescope was limited to observations at about z=11. The JWST  current high-redshift observations have reached z=14.32. Astronomers think that the JWST will eventually observe galaxies at z=20.

-

-   The first few hundred million years after the Big Bang is called the “Cosmic Dawn”. JWST showed us that ancient galaxies during the Cosmic Dawn were much more luminous and, therefore, larger than we expected. The galaxy the telescope found at z=14.32, called JADES-GS-z14-0, has several hundred million solar masses.

-

-     How can nature make such a bright, massive, and large galaxy in less than 300 million years?"   They were differently shaped, that they contained more dust than expected, and that oxygen was present. The presence of oxygen indicates that generations of stars had already lived and died.   The presence of oxygen so early in the life of this galaxy is a surprise and suggests that multiple generations of very massive stars had already lived their lives before we observed the galaxy.

-

-    JADES-GS-z14-0 is not like the types of galaxies that have been predicted by theoretical models and computer simulations to exist in the very early universe.  Active galactic nuclei (AGN) are supermassive black holes (SMBHs) that are actively accreting material and emitting jets and winds.

-

-   Quasars are a sub-type of AGN that are extremely luminous and distant, and quasar observations show that SMBHs were present in the centers of galaxies as early as 700 million years after the Big Bang. But their origins were a mystery.

-

-   Astrophysicists think that these early SMBHs were created from black hole "seeds" that were either "light" or "heavy." Light seeds had about 10 to 100 solar masses and were stellar remnants. Heavy seeds had 10 to 105 solar masses and came from the direct collapse of gas clouds.

-

-    The JWST's ability to effectively look back in time has allowed it to spot an ancient black hole at about z=10.3 that contains between 107 to 108 solar masses. The Hubble Space Telescope didn't allow astronomers to measure the stellar mass of entire galaxies the way that the JWST does.

-

-    Astronomers know that the black hole at z=10.3 has about the same mass as the stellar mass of its entire galaxy. This is in stark contrast to modern galaxies, where the mass of the black hole is only about 0.1% of the entire stellar mass.

-

-   Such a massive black hole existing only about 500 million years after the Big Bang is proof that early black holes originated from heavy seeds. This is actually in line with theoretical predictions.

-

-    We know that in the early universe, hydrogen became ionized during the Epoch of Reionization (EoR). Light from the first stars, accreting black holes, and galaxies heated and reionized the hydrogen gas in the intergalactic medium (IGM), removing the dense, hot, primordial fog that suffused the early universe.

-

-    Young stars were the primary light source for the reionization. They created expanding bubblesof ionized hydrogen that overlapped one another. Eventually, the bubbles expanded until the entire universe was ionized.

-

-   This was a critical phase in the development of the universe. It allowed future galaxies, especially dwarf galaxies, to cool their gas and form stars. But scientists aren't certain how black holes, stars, and galaxies contributed to the reionization or the exact time frame in which it took place.

-0

-    We know that hydrogen reionization happened, but exactly when and how it happened has been a major missing piece in our understanding of the first billion years.  Astronomers knew that reionization ended about 1 billion years after the Big Bang, at about redshift z=5-6. But before the JWST, it was difficult to measure the properties of the UV light that caused it. With the JWST's advanced spectroscopic capabilities, astronomers have narrowed down the parameters of reionization.

-

-    We have found spectroscopically confirmed galaxies up to z = 13.2, implying reionization may have started just a few hundred million years after the Big Bang.  JWST results also show that accreting black holes and their AGN likely contributed no more than 25% of the UV light that caused reionization.

-

-   There is still significant debate about the primary sources of reionization, in particular, the contribution of faint galaxies. Even though the JWST is extraordinarily powerful, some distant, faint objects are beyond its reach.

-

-    The JWST is not even halfway through its mission and has already transformed our understanding of the universe's first one billion years. It was built to address questions around the Epoch of Reionization, the first black holes, and the first galaxies and stars. There's definitely much more to come. Who knows what the sum total of its contributions will be?

-

-    Among the most fundamental questions in astronomy is: How did the first stars and galaxies form?    For hundreds of millions of years after the Big Bang, the universe was filled with a gaseous fog that made it opaque to energetic light. By one billion years after the Big Bang, the fog had cleared and the universe became transparent, a process known as “reionization”. Scientists have debated whether active, supermassive black holes or galaxies full of hot, young stars were the primary cause of reionization.

-

-   Almost every single galaxy that we are finding shows these unusually strong emission line signatures indicating intense recent star formation. These early galaxies were very good at creating hot, massive stars.

-

-    These bright, massive stars pumped out torrents of ultraviolet light, which transformed surrounding gas from opaque to transparent by ionizing the atoms, removing electrons from their nuclei. Since these early galaxies had such a large population of hot, massive stars, they may have been the main driver of the reionization process. The later reuniting of the electrons and nuclei produces the distinctively strong emission lines.

-

-   These young galaxies underwent periods of rapid star formation interspersed with quiet periods where fewer stars formed. These fits and starts may have occurred as galaxies captured clumps of the gaseous raw materials needed to form stars. Alternatively, since massive stars quickly explode, they may have injected energy into the surrounding environment periodically, preventing gas from condensing to form new stars.

-

-    The light from faraway galaxies is stretched to longer wavelengths and redder colors by the expansion of the universe—a phenomenon called “redshift”. By measuring a galaxy's redshift, astronomers can learn how far away it is, and therefore, when it existed in the early universe. Before Webb, there were only a few dozen galaxies observed above a redshift of 8, when the universe was younger than 650 million years old, but JADES has now uncovered nearly a thousand of these extremely distant galaxies.

-

-    Determining redshift involves looking at a galaxy's spectrum, which measures its brightness at myriad closely spaced wavelengths. But a good approximation can be determined by taking photos of a galaxy using filters that each cover a narrow band of colors to get a handful of brightness measurements. In this way, researchers can determine estimates for the distances of many thousands of galaxies at once.

-

-   More than 700 candidate galaxies existed when the universe was between 370 million and 650 million years old. The sheer number of these galaxies was far beyond predictions from observations made before Webb's launch. The observatory's exquisite resolution and sensitivity are allowing astronomers to get a better view of these distant galaxies than ever before.

-

-    James Webb Space Telescope has discovered the four most distant galaxies ever observed, one of which formed just 320 million years after the Big Bang when the universe was still in its infancy.

-

-    By the time light from the most distant galaxies reaches Earth, it has been stretched by the expansion of the universe and shifted to the infrared region of the light spectrum.  The Webb telescope's NIRCam instrument has an unprecedented ability to detect this infrared light, allowing it to quickly spot a range of never-before-seen galaxies..

-

-    The galaxies date from 300 to 500 million years after the Big Bang more than 13 billion years ago, when the universe was just two percent of its current age.  That means the galaxies are from what is called "the epoch of reionisation," a period when the first stars are believed to have emerged. The epoch came directly after the cosmic dark ages brought about by the Big Bang.

-

-    The Webb telescope confirmed the existence of JADES-GS-z10-0, which dates from 450 million years after the Big Bang and had previously been spotted by the Hubble Space Telescope.   All four galaxies are "very low in mass," weighing roughly a hundred million solar masses. The Milky Way, in comparison, weighs 1.5 trillion solar masses by some estimations.

-

-   The galaxies are very active in star formation in proportion to their mass.   The galaxies were also "very poor in metals.  This is consistent with the standard model of cosmology, science's best understanding of how the universe works, which says that the closer to the Big Bang, the less time there is for such metals to form.

-

-    However, the discovery of six massive galaxies from 500-700 million years after the Big Bang led some astronomers to question the standard model.   Those galaxies, also observed by the Webb telescope, were bigger than thought possible so soon after the birth of the universe.

-

-

June 23, 2024                            4511

------------------------------------------------------------------------------------------                                                                                                                       

--------  Comments appreciated and Pass it on to whomever is interested. ---

---   Some reviews are at:  --------------     http://jdetrick.blogspot.com ----- 

--  email feedback, corrections, request for copies or Index of all reviews

---  to:  ------    jamesdetrick@comcast.net  ------  “Jim Detrick”  -----------

--------------------- ---  Sunday, June 23, 2024  ---------------------------------

 

 

 

 

 

           

 

 

No comments:

Post a Comment