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By spying on a neighboring galaxy, NASA Hubble Space Telescope has captured an image of a young, globular-like star cluster—a type of object unknown in our Milky Way Galaxy.
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NASA Spitzer Space Telescope shows the supernova remnant 1E0102.2-7219 sits next to the nebula N76 in a bright, star-forming region of the Small Magellanic Cloud, a satellite galaxy to our Milky Way galaxy.
Ver en NASA ↗A rich collection of colorful astronomical objects is revealed in this picturesque image of the Rho Ophiuchi cloud complex from NASA Wide-field Infrared Explorer; the cloud is found rising above the plane of the Milky Way in the night sky.
Ver en NASA ↗This composite of 30 Doradus, the Tarantula Nebula, contains data from Chandra blue, Hubble green, and Spitzer red. Located in the Large Magellanic Cloud, the Tarantula Nebula is one of the largest star-forming regions close to the Milky Way.
Ver en NASA ↗This image from NASA Herschel, in the constellation of Vulpecula, shows an entire assembly line of newborn stars. The diffuse glow reveals the widespread cold reservoir of raw material that our Milky Way galaxy has in stock for building stars.
Ver en NASA ↗This image of the microwave sky was synthesized using data spanning the range of light frequencies detected by ESA Planck. A vast portion of the sky is dominated by the diffuse emission from gas and dust in our Milky Way galaxy.
Ver en NASA ↗This artist concept shows NASA Voyager spacecraft against a field of stars in the darkness of space as they travel farther away from Earth, on a journey to interstellar space, and will eventually circle around the center of the Milky Way galaxy.
Ver en NASA ↗This infrared view of the whole sky highlights the flat plane of our Milky Way galaxy line across middle of image. NASA WISE, will take a similar infrared census of the whole sky, only with much improved resolution and sensitivity.
Ver en NASA ↗The Milky Way and other galaxies in the universe harbor many young star clusters and associations that each contain hundreds to thousands of hot, massive, young stars known as O and B stars.
Ver en NASA ↗The galaxy Messier 101 is a swirling spiral of stars, gas, and dust. Messier 101 is nearly twice as wide as our Milky Way galaxy in this image as seen by NASA Spitzer Space Telescope.
Ver en NASA ↗The color scale in this image from the Planck mission represents the emission from dust, a minor but crucial component that pervades our Milky Way galaxy. The texture indicates the orientation of the galactic magnetic field.
Ver en NASA ↗On the morning of February 1, 2011, NASA Wide-field Infrared Survey Explorer, or WISE, took its last snapshot of the sky. WISE final picture shows thousands of stars in a patch of the Milky Way galaxy in the constellation Perseus.
Ver en NASA ↗New data from NASA Cassini spacecraft suggest that the shape of our solar system moving through the local Milky Way galaxy looks like a bubble -- or a rat -- traveling through a boa constrictor belly.
Ver en NASA ↗This is a mosaic of the images covering the entire sky as observed by NASA Wide-field Infrared Survey Explorer WISE, part of its All-Sky Data Release. In this mosaic, the Milky Way Galaxy runs horizontally across the map.
Ver en NASA ↗This mosaic reveals a panorama of the Milky Way from NASA Spitzer Space Telescope. This picture covers only about three percent of the sky, but includes more than half of the galaxy stars and the majority of its star formation activity.
Ver en NASA ↗Resembling an opulent diamond tapestry, this image from NASA Hubble Space Telescope shows a glittering star cluster that contains a collection of some of the brightest stars seen in our Milky Way galaxy called Trumpler 14.
Ver en NASA ↗This image is from NASA Galaxy Evolution Explorer is an observation of the large galaxy in Andromeda, Messier 31. The Andromeda galaxy is the most massive in the local group of galaxies that includes our Milky Way.
Ver en NASA ↗The center of the Milky Way galaxy imaged by NASA Spitzer Space Telescope is displayed on a quarter-of-a-billion-pixel, high-definition 23-foot-wide 7-meter LCD science visualization screen at NASA Ames Research Center.
Ver en NASA ↗The galaxy NGC 4395 is shown here in infrared light, captured by NASA Spitzer Space Telescope. This dwarf galaxy is relatively small in comparison with our Milky Way galaxy, which is nearly 1,000 times more massive.
Ver en NASA ↗This enormous section of the Milky Way galaxy is a mosaic of images from NASA Wide-field Infrared Survey Explorer. The constellations Cassiopeia and Cepheus are featured in this 1,000-square degree expanse.
Ver en NASA ↗Yellow balls -- which are several hundred to thousands times the size of our solar system -- are pictured here in the center of this image taken by NASA Spitzer Space Telescope.
Ver en NASA ↗This mosaic image from NASA Wide-field Infrared Survey Explorer is located in a constellation in the southern sky, Pavo, which is Latin for peacock.
Ver en NASA ↗This image from NASA's Spitzer Space telescope shows the star-forming nebula W51, one of the largest star factories in the Milky Way galaxy.
Ver en NASA ↗This map of the entire sky was captured by the European Space Agency Planck mission. The band running through the middle corresponds to dust in our Milky Way galaxy.
Ver en NASA ↗Contenido y metadatos proporcionados por la NASA Image and Video Library.