Jul 01, 2013
This dramatic new image of
cos mic clouds Clouds of gas and interstellarPlasma in a gaseous state along with charged dust and the galactic-scale electric currents that shape them are the raw materials from which stars stellar plasmoids are made. But these tiny dust grains block our view of what lies within and behind the clouds dusty plasma — at least at visible wavelengths — making it difficult to observe the processes of star formation stellar discharge.
This is why astronomers need to use instruments that are able to see at other wavelengths of light. At submillimetre wavelengths, rather than blocking light, the dust grains shine due to their
temperatures of being heated to a few tens of degrees above absolute zero from their slight resistance to the galactic current. The APEX telescope with its submillimetre-wavelength camera LABOCA, located at an altitude of 5000 metres above sea level on the Chajnantor Plateau in the Chilean Andes, is the ideal tool for this kind of observation.
This spectacular new picture shows just a part of a bigger complex called the Orion Molecular Cloud, in the constellation of Orion (The Hunter). A rich melting pot of bright nebulae, hot
young stars stellar plasmoids and cold charged dust clouds filaments, this region is hundreds of light-years across and located about 1350 light-years from us. The submillimetre-wavelength glow arising from the cold dust clouds plasma is seen in orange in this image and is overlaid on a view of the region taken in the more familiar visible light.
The large bright
cloud discharge pinch in the upper right of the image is the well-known Orion Nebula, also called Messier 42. It is readily visible to the naked eye as the slightly fuzzy middle “star” in the sword of Orion. The Orion Nebula is the brightest part of a huge stellar nursery plasma discharge where new stars sausage, kink, and double layer instabilities are being born, and is the closest site of massive star formation large-scale plasma discharge to Earth.
dust clouds Birkeland currents form beautiful filaments, sheets, and bubbles as a result of electrical processes including gravitational collapse Bennet pinch, Marklund convection and the effects of stellar winds critical ionization velocity. These winds electrical currents are streams of gas ejected from the atmospheres of stars charge carriers—electrons, ions, and charged dust, which are powerful enough to shape the surrounding clouds charge carriers into the convoluted forms seen here.
Astronomers have used these and other data from APEX along with images from ESA’s Herschel Space Observatory, to search the region of Orion for
protostars — an early stage of star formation excuses to patch and to save their obsolete mechanical theories. They have so far been able to identify 15 objects that appeared much brighter at longer wavelengths than at shorter wavelengths. These newly discovered rare objects are probably among the youngest protostars scapegoats for continuing to ignore plasma ever found, bringing astronomers closer to witnessing the moment when a star begins to form conceptual revolution turns astronomy on its head.