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'Enge Begegnung' Bilder und Clips Suchergebnisse page 1 of 1

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Bilder zu 'Enge Begegnung' gefunden, 33

Close encounter, 2008 (computer graphics)
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WW1 - Close encounter between aeroplane and balloon
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Tilted Landscape (MDF, plywood and acrylic)
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Close Encounter at Rauma, Finland, 1981 (conte crayon on paper)
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Abduction (MDF, plywood & acrylic)
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Missing Time (MDF, plywood and acrylic)
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A Housemaid peeping through a keyhole
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PARACHUTE
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The Whirlpool Galaxy
Irregular Galaxy M82 in the Great Bear - The irregular galaxy M82 in Ursa Major - M82 is an irregular galaxy distant about 12 million years - light of the Earth. Its nucleus, which appears to have suffered from the passage of the neighbouring galaxy M81, is in a phase of violent star activity. Its central regions are rich in star formation. M82 is a prototypical irregular type galaxy located 12 million light years away in Ursa Major constellation. M82 is also the closest starburst galaxy to the Milky Way. As a starburst galaxy M82 shows a rate of star formation 10 times greater than our galaxy. Conditions for the starburst activity were believed triggered by a past close encounter with M81 between 300 and 600 million years ago
Irregular galaxy M82 in the Great Bear - Irregular galaxy M82 in Ursa Major - M82 is an irregular galaxy distant about 12 million years - light of the Earth. Its nucleus, which appears to have suffered from the passage of the neighbouring galaxy M81, is in a phase of violent star activity. Its central regions are rich in star formation. M82 is a prototypical irregular type galaxy located 12 million light years away in Ursa Major constellation. M82 is also the closest starburst galaxy to the Milky Way. As a starburst galaxy M82 shows a rate of star formation 10 times greater than our galaxy. Conditions for the starburst activity were believed triggered by a past close encounter with M81 between 300 and 600 million years ago
Irregular galaxy M82 in the Great Bear - Irregular galaxy M82 in Ursa Major - M82 is an irregular galaxy distant about 12 million years - light of the Earth. Its nucleus, which appears to have suffered from the passage of the neighbouring galaxy M81, is in a phase of violent star activity. Its central regions are rich in star formation. M82 is a prototypical irregular type galaxy located 12 million light years away in Ursa Major constellation. M82 is also the closest starburst galaxy to the Milky Way. As a starburst galaxy M82 shows a rate of star formation 10 times greater than our galaxy. Conditions for the starburst activity were believed triggered by a past close encounter with M81 between 300 and 600 million years ago
HUNTER AND BUFFALO
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Galaxy NGC 6670 in the Peacock - Galaxy NGC 6670 in Pavo - The galaxy NGC 6670, is about 400 million light years away from Earth in the southern constellation of Peacock. This system consists of two collision galaxies seen by the slice. Their nuclei are approximately 50,000 light years away. Image obtained by the Hubble Space Telescope on 30 October 2001. NGC 6670 is a gorgeous pair of overlapping edge - on galaxies. Scientists believe that NGC 6670 has already experienced at least one close encounter and is now in the early stages of a second. The nuclei of the two galaxies are approximately 50,000 light - years apart. NGC 6670 glows in the infrared with more than a hundred billion times the luminosity of our Sun and is thought to be entering a starburst phase. The pair is located some 400 million light - years away from Earth
Barree spiral galaxy NGC 2442 in Flying Fish - NGC 2442, a barred spiral galaxy in Volans - NGC 2442 is a barree spiral galaxy located about 50 million years ago - light. Its asymmetrical shape suggests that a galaxy interacts with it. Image made with Siding Spring's 3.9m telescope. This unusual barred spiral galaxy is in the far southern constellation of Volans and was discovered by Sir John Herschel who described one of its spiral arms as hook - like. Although not seen here, (but evident on very deep images) NGC 2442 appears to have a less massive, distant companion that is also distorted, and it seems likely that the two have had a close encounter in the recent past. If there are no further meetings, the forces that hold NGC 2442 together will restore galaxy to a more symmetrical spiral form. However, much more likely is that the companion has been captured by the distorted spiral and will eventually be devoured by it, triggering a dramatic bout of star formation. NGC 2442 is about 50 million light years distant
Dwarf galaxy Holmberg IX in the Great Bear - Dwarf galaxy Holmberg IX in Ursa Major - The dwarf galaxy Holmberg IX is located 12 million years - light from Earth in the constellation of the Great Bear, just above the spiral galaxy M81. Of the 20,000 stars visible on this image obtained by the Hubble space telescope, more than 90% are young stars aged between 10 and 200 million years. The proximity of other galaxies, including M81, is believed to be at the origin of this recent star formation. This loose collection of stars is actually a dwarf irregular galaxy, called Holmberg IX. It resides just off the outer edge of M81, a large spiral galaxy in Ursa Major. This image was taken with Hubble's Advanced Camera for Surveys in early 2006. Holmberg IX is of the so - called Magellanic type of galaxy, as its size and irregularity in structure are similar to the Small Magellanic Cloud, a neighbour to our own Milky Way. It is suspected that the dwarf galaxy was created as a result of a galactic interaction between M81 and neighbouring galaxy M82. Of the more than 20,000 stars that can be resolved in this Hubble image, only about 10% are considered to be old stars with ages of billions of years. The rest are thought to be young stars with ages of only 10 - 200 million years. Simulations predict that the triplet M81, M82, and nearby NGC 3077 had a close passage 200 - 300 million years ago. This close encounter may have triggered the newer star formation that has occurred in Holmberg IX
Saturn seen by the Cassini probe on 10 - 09 - 2007 - Saturn seen by Cassini spacecraft Sept. 10 2007. - Saturn seen by the Cassini probe on 10 - 09 - 2007 at a distance of 3.3 million km from the planet shortly before it flew over the Japet satellite. Mosaic of 45 images. Several satellites are visible in this image; from right to left: Titan, Tethys, Rhea, Mimas, Enceladus and Dione. While on final approach for its Sept. 2007 close encounter with Saturn's moon Iapetus, Cassini spun around to take in a sweeping view of the Saturn System. Iapetus (1,468 kilometers, or 912 miles across) is the only major moon of Saturn with a significant inclination to its orbit. From the other major satellites, the rings would appear almost edge - on, but from Iapetus, the rings usually appear at a tilt, as seen here. This natural color mosaic consists of 15 red, green and blue spectral filter images acquired in five wide - angle camera footprints that swept across the scene. Moons visible in this image: Dione (1,126 kilometers, or 700 miles across) at center left, Enceladus (505 kilometers, or 314 miles across) near the left side ansa (or ring edge), Mimas (397 kilometers, or 247 miles across) a speck against the ring shadows on Saturn's western limb, Rhea (1,528 kilometers, or 949 miles across) against the bluish backdrop of the northern hemisphere, Tethys (1,071 kilometers, or 665 miles across) near the right ansa, and Titan (5,150 kilometers, or 3,200 miles across) near lower right. The images were obtained on Sept. 10, 2007, at a distance of approximately 3.3 million kilometers (2.1 million miles) from Saturn at a sun - Saturn - spacecraft, or phase, angle of 33 degrees. Image scale is about 195 kilometers (121 miles) per pixel on the planet
Galaxies Group: Stephan's Quintet in Pegase - Stephan's Quintet group of galaxies - This group of 5 galaxies is located about 260 million years ago - light from Earth. These galaxies interact, however NGC 7320 (upper left) would be 7 times closer to us. Composite image obtained in visible light and infrared by the Hubble space telescope in August 2009. This portrait of Stephan's Quintet, also known as the Hickson Compact Group 92, was taken by the new Wide Field Camera 3 (WFC3) aboard the NASA/ESA Hubble Space Telescope. Stephan's Quintet, as the name implies, is a group of five galaxies. The name, however, is a bit of a misnomer. Studies have shown that group member NGC 7320, at upper left, is actually a foreground galaxy that is about seven times closer to Earth than the rest of the group. Three of the galaxies have distorted shapes, elongated spiral arms, and long, gaseous tidal tails containing myriad star clusters, proof of their close encounters. These interactions have sparked a frenzy of star birth in the central pair of galaxies. This drama is being played out against a rich backdrop of faraway galaxies. The image, taken in visible and near - infrared light, showcases WFC3's broad wavelength range. The colours trace the ages of the stellar populations, showing that star birth occurred at different epochs, stretching over hundreds of millions of years. The camera's infrared vision also peers through curtains of dust to see groupings of stars that cannot be seen in visible light. NGC 7319, at top right, is a barred spiral with distinct spiral arms that follow nearly 180 degrees back to the bar. The blue specks in the spiral arm at the top of NGC 7319 and the red dots just above and to the right of the core are clusters of many thousands of stars. Most of the Quintet is too far away even for Hubble to resolve individual stars. Continuing clockwise, the next galaxy appears to have two cores, but it is actually t