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Untangling a Knot of Galaxy Clusters
Jan 30, 2023
Astronomers have captured a spectacular, ongoing collision between at least three galaxy clusters. Data from NASA’s Chandra X-ray Observatory, ESA’s (European Space Agency’s) XMM-Newton, and a trio of radio telescopes is helping astronomers sort out what is happening in this jumbled scene. Collisions and mergers like this are the main way that galaxy clusters can grow into the gigantic cosmic edifices seen today. These also act as the largest particle accelerators in the universe.
The giant galaxy cluster forming from this collision is Abell 2256, located 780 million light-years from Earth. This composite image of Abell 2256 combines X-rays from Chandra and XMM in blue with radio data collected by the Giant Metrewave Radio Telescope (GMRT), the Low Frequency Array (LOFAR), and the Karl G. Jansky Very Large Array (VLA) all in red, plus optical and infrared data from Pan-STARRs in white and pale yellow.
Astronomers studying this object are trying to tease out what has led to this unusual-looking structure. Each telescope tells a different part of the story. Galaxy clusters are some of the biggest objects in the universe containing hundreds or even thousands of individual galaxies. In addition, they contain enormous reservoirs of superheated gas, with temperatures of several million degrees Fahrenheit. Only X-ray telescopes like Chandra and XMM can see this hot gas. A labeled version of the figure shows gas from two of the galaxy clusters, with the third blended too closely to separate from the others.
The radio emission in this system arises from an even more complex set of sources. The first are the galaxies themselves, in which the radio signal is generated by particles blasting away in jets from supermassive black holes at their centers. These jets are either shooting into space in straight and narrow lines (those labeled “C” and “I” in the annotated image, using the astronomer’s naming system) or slowed down as the jets interact with gas they are running into, creating complex shapes and filaments (“A”, “B,” and “F”). Source F contains three sources, all created by a black hole in a galaxy aligning with the left-most source of this trio.
Radio waves are also coming from huge filamentary structures (labeled "relic"), mostly located to the north of the radio-emitting galaxies, likely generated when the collision created shock waves and accelerated particles in the gas across over two million light-years. A paper analyzing this structure was published earlier this year by Kamlesh Rajpurohit from the University of Bologna in Italy in the March 2022 issue of The Astrophysical Journal, and is available online. This is Paper I in an ongoing series studying different aspects of this colliding galaxy cluster system.
Finally, there is a "halo" of radio emission located near the center of the collision. Because this halo overlaps with the X-ray emission and is dimmer than the filamentary structure and the galaxies, another radio image has been produced to emphasize the faint radio emission. Paper II led by Rajpurohit, recently published in the journal Astronomy and Astrophysics and available online, presents a model that the halo emission may be caused by the reacceleration of particles by rapid changes in the temperature and density of the gas as the collision and merging of the clusters proceed. This model, however, is unable to explain all the features of the radio data, highlighting the need for more theoretical study of this and similar objects.
Paper III by Rajpurohit and collaborators will study the galaxies producing radio waves in Abell 2256. This cluster contains an unusually large number of such galaxies, possibly because the collision and merger are triggering the growth of supermassive black holes and consequent eruptions. More details about the LOFAR image of Abell 2256 will be reported in an upcoming paper by Erik Osinga.
https://www.nasa.gov/mission_pages/chandra/news/untangling-a-knot-of-galaxy-clusters.html
Flora, Fauna at NASA’s Kennedy Space Center
Jan 31, 2023
In this photo from Oct. 14, 2008, a great blue heron stands watch among a pond of water lilies on NASA's Kennedy Space Center. It is one of 310 species of birds that inhabit the National Merritt Island Wildlife Refuge, which shares a boundary with Kennedy. The marshes and open water of the refuge also provide wintering areas for 23 species of migratory waterfowl, as well as a year-round home for great blue herons, great egrets, wood storks, cormorants, brown pelicans, and other species of marsh and shore birds. Kennedy is responsible for more protected species than any other federal property in the continental United States.
https://www.nasa.gov/image-feature/flora-fauna-at-nasa-s-kennedy-space-center
What Could Go Wrong? Scientists Launch Project To Bring The Dodo Bird Back From The Dead
Published January 31, 2023 at 3:15pm
Scientists believe they have found a way to bring back the animal most synonymous with the extinction, the dodo bird. Should their endeavor prove successful, this could open the door for the resurrection of several other animals that were thought to be long gone.
A “de-extinction company” known as Colossal Biosciences has decided to play God and right a “wrong” done by humans by using edited DNA to create a so-called proxy version of the dodo since an exact clone is not possible. Should the recreation prove successful, the next step would be to re-introduce the dodo to its original habitat in Mauritius.
The founders of the company believes reintroducing the dodo will benefit conservation and the wildlife ecosystem. They do not elaborate on why, however.
Colossal Biosciences is also working bringing other endangered species back from the dead, such as the Tasmanian tiger and wooly mammoth.
https://www.thegatewaypundit.com/2023/01/go-wrong-scientists-launch-project-bring-dodo-bird-back-dead/