RF2BE3WJD–Carina Nebula in outer space. Elements of this image furnished by NASA.
RM2GNHKAN–The famous Pillars of Creation,a part of a small region of the Eagle Nebula, a vast star-forming region 6,500 light-years from Earth.The colors in the image highlight emission from several chemical elements. Oxygen emission is blue, sulfur is orange, and hydrogen and nitrogen are green. . Image source NASA/ESA Hubble Space Telescope
RF2A81F05–Awesome beauty of starfield somewhere in deep space. Elements of this image furnished by NASA
RF2FMG5XD–Collage of a spaceship telescope on the background of stripes in the form of louvers of a galaxy with stars with copy space. Elements of this image fu
RMEN8HKG–NASA’s Hubble Space Telescope measures in at just over 43 feet long and is 14 feet in diameter. When upright, it is a five story tower that, when readied for launch, filled out the orbiter’s entire payload bay. Hubble is made up of three major elements: the Optical Telescope Assembly, the focal plane scientific instruments, and the Support Systems Module, which is divided into four sections, stacked together like canisters. In this photo, all of Hubble's main structures are present as the forward shell is being moved into position for mating at Lockheed Martin’s 535,000 cubic foot, Vertical As
RF2KFNKG4–Clouds of interstellar gas & dust in the Carina Nebula, southern constellation Carina. Pillar of dust and gas. Elements of image furnished by NASA.
RF2B0YKTN–Hubble space telescope photo of Pillars of Creation. Interstellar gas and dust in the Eagle Nebula, in Serpens constellation 6,500 light years away.
RF2AB6G36–The Lagoon Nebula in bright colours. Deep space look. Science fiction wallpaper. Elements of this image were furnished by NASA.
RFKDB1R9–Deep space object: Pillars of creation in Eagle Nebula (M16) in the constellation Serpens, elements of this image furnished by NASA
RM2ABAJ28–For this image, the NASA/ESA Hubble Space Telescope turned its powerful eye toward an emission-line galaxy called NGC 3749. When astronomers explore the contents and constituent parts of a galaxy somewhere in the Universe, they use various techniques and tools. By hunting for specific signs of emission from various elements within a galaxy's spectrum of light - so-called emission lines - or, conversely, the signs of absorption from other elements, so-called absorption lines, astronomers can start to deduce what might be happening within. While not all galaxies display strong emission lines, NG
RMKRB7PG–New Chandra observations have been used to make the first detection of X-ray emission from young stars with masses similar to our Sun outside our Milky Way galaxy. The Chandra observations of these low-mass stars were made of the region known as the 'Wing' of the Small Magellanic Cloud (SMC), one of the Milky Way's closest galactic neighbors. In this composite image of the Wing the Chandra data is shown in purple, optical data from the Hubble Space Telescope is shown in red, green and blue and infrared data from the Spitzer Space Telescope is shown in red. Astronomers call all elements heavier
RF2HC89J8–James Webb Telescope and Hubble Telescope facing each other in barner. copy space. Elements of this image were furnished by NASA.