Iron Ions (Fe XII) in the Sun's Atmosphere
Under conditions (temperatures around 1,500,000 kelvins) that exist in the Sun's corona (upper atmosphere), an iron atom loses 11 electrons and becomes an Fe XII ion. These ions emit extreme ultraviolet (EUV) radiation at a wavelength of 19.5 nm (195 Å). Radiation at this wavelength allows scientists to see structures and processes at a certain height in the solar atmosphere. These high energy UV emissions are (thankfully!) blocked by Earth's atmosphere, so scientists must use orbiting solar telescopes on satellites above the atmosphere to view the Sun at this wavelength. On Earth, iron is a silvery-white metal that is found throughout the Earth's crust. It is also a critical component of the human body found in blood cells and necessary for the proper functioning of cells and muscles. |
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Iron exists in small amounts in the 









