X-ray astronomy is used to detect and study astronomical objects and the Sun provides us with plenty of such data as we try and learn more about it. NASA’s Nuclear Spectroscopic Telescope Array (NuSTAR) and Solar Dynamics Observatory (SDO) provided data which was combined to form this picture of high energy x-rays streaming off the Sun. The high energy emissions, shown in blue (3 to 5 kilo-electron volts) and green (2 to 3 kilo-electron volts) are from NuSTAR’s data and come from gases that may be heated to over 3 million degrees. The SDO data in this composite image is the areas in red which consists of ultraviolet light  at 171 angstrom wavelength.