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Hubble Telescope Gallery

Choose from 262 pictures in our Hubble Telescope collection for your Wall Art or Photo Gift. All professionally made for Quick Shipping.


Orion nebula Featured Hubble Telescope Print

Orion nebula

Orion nebula. Coloured composite infrared and visible light image of the Orion nebula M42. This emission nebula, a cloud of gas and dust in which starbirth takes place, is found in the constellation Orion, some 1500 light years from Earth. Glowing clouds of ionised hydrogen and sulphur gases are green, and cool clouds of polycyclic aromatic hydrocarbons are orange and red. The gases are ionised by radiation from the four young Trapezium stars at the core (centre left). The small orange dots are embryonic stars, growing as they accumulate dust and gas. M42's neighbour, the M43 nebula, can also be seen (pale blue, top left). Infrared data from the Spitzer Space Telescope, visible light data from the Hubble Space Telescope

© NASA/JPL-CALTECH/STSCI/SCIENCE PHOTO LIBRARY

Gas pillar in the Eagle nebula Featured Hubble Telescope Print

Gas pillar in the Eagle nebula

Gas pillar in the Eagle nebula (M16), Hubble Space Telescope image. This is a 9.5-light-year-tall pillar of cold gas and dust silhouetted against a bright emission nebula. The dense pockets of dust and gas in this pillar may be in the process of condensing into stars. The upper part of the pillar is glowing as it is heated and compressed by radiation from hot young stars out of frame at upper left. The colours here come from ionised gases; the blue from oxygen and the orange from hydrogen. The Eagle nebula lies around 7000 light years from Earth in the constellation Serpens Cauda. This image was taken in November 2004 by the Advanced Camera for Surveys (ACS) on the HST

© Nasa/Esa/Stsci/Hubble Heritage Team/Science Photo Library

International Year of Astronomy 2009 Featured Hubble Telescope Print

International Year of Astronomy 2009

In celebration of the International Year of Astronomy 2009, NASA's Great Observatories -- the Hubble Space Telescope, the Spitzer Space Telescope, and the Chandra X-ray Observatory -- have produced a matched trio of images of the central region of our Milky Way galaxy. Each image shows the telescope's different wavelength view of the galactic center region, illustrating the unique science each observatory conducts. In this spectacular image, observations using infrared light and X-ray light see through the obscuring dust and reveal the intense activity near the galactic core. Note that the center of the galaxy is located within the bright white region to the right of and just below the middle of the image. The entire image width covers about one-half a degree, about the same angular width as the full moon. Spitzer's infrared-light observations provide a detailed and spectacular view of the galactic center region [Figure 1 (top frame of poster)]. The swirling core of our galaxy harbors hundreds of thousands of stars that cannot be seen in visible light. These stars heat the nearby gas and dust. These dusty clouds glow in infrared light and reveal their often dramatic shapes. Some of these clouds harbor stellar nurseries that are forming new generations of stars. Like the downtown of a large city, the center of our galaxy is a crowded, active, and vibrant place. Although best known for its visible-light images, Hubble also observes over a limited range of infrared light [Figure 2 (middle frame of poster)]. The galactic center is marked by the bright patch in the lower right. Along the left side are large arcs of warm gas that have been heated by clusters of bright massive stars. In addition, Hubble uncovered many more massive stars across the region. Winds and radiation from these stars create the complex structures seen in the gas throughout the image.This sweeping panorama is one of the sharpest infrared pictures ever made of the galactic center region. X-rays detected by Chandra expose a wealth of exotic objects and high-energy features [Figure 3 (bottom frame of poster)]. In this image, pink represents lower energy X-rays and blue indicates higher energy. Hundreds of small dots show emission from material around black holes and other dense stellar objects. A supermassive black hole -- some four million times more massive than the Sun -- resides within the bright region in the lower right. The diffuse X-ray light comes from gas heated to millions of degrees by outflows from the supermassive black hole, winds from giant stars, and stellar explosions. This central region is the most energetic place in our galaxy

© NASA/JPL-Caltech/ESA/CXC/STScI