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'Ursa Major' Bilder und Clips Suchergebnisse page 1 of 3

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Constellation Ursa - Constellation of Ursa Major - Grand Chariot, asterism of the constellation Ursa Ursa
Constellations of the Great Bear and Little Bear - Constellations of Ursa Major and Ursa Mino
Ursa Major, Polaris and Cassiopeia -
The constellation of Ursa Major.
WHITTAKER/URSA MAJOR
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Constellation Ursa - Constellation of Ursa Major - Grand Chariot, asterism of the constellation Ursa Ursa
URSA MAJOR STAR MAP
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URSA MAJOR & URSA MINOR, 2017 (tinted gesso on wood)
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The constellation Ursa Major, 1603
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Constellation of the Great Ursa - Constellation of Ursa Major - Lofoten, Norway
Great Dipper Constellation - Ursa Major
BLUNT/URSA MAJOR/PL 24
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Constellations of the Great Bear and Little Bear - Constellations of Ursa Major and Ursa Mino
Constellation of the Great Ursae - Constellation of Ursa Majo
Shooting star and constellation of the Great Ursa - Meteor and constellation of Ursa Major - Geminide
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Ursa Minor and Ursa Major. Birds, prince and an angel in the border.
Illustrations to a treatise on astrology
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Galaxies NGC 3718 and NGC 3729 in Ursa Major
Comete Hyakutake et galaxy M101 - Comet Hyakutake with M101 galaxy - 25 March 1996. 25 March 199
Constellation of Ursa Major - Constellation of Ursa Major - Grand Chariot, asterism of the constellation Ursa Ursa. Composite of two images. The sky is enlarged in relation to reality. This photo of the constellation Ursa Major, better known as The Big Dipper clearly shows the main “” naked eye”” stars that make up the shape of “” the dipper”” enlarged in their true color. The Big Dipper is actually just the tail section of Usa Major, “” The Great Bear””, which is a very large constellation in the Northern sky
Double star M40 in the Great Bear - M40 in Ursa Major - At the bottom of the picture, the spiral galaxy barree NGC 4290. Double star system in Ursa Major; bottom is the barred spiral galaxy NGC 4290
An irregular galaxy (NGC 3556) in constellation Ursa Major.
Spiral galaxy NGC 2841 in the Great Bear - Spiral galaxy NGC 2841 in Ursa Majo
Constellations of the Great Bear and Hunting Dogs - Constellations of Ursa Major and Canes Venatic
Ursa Major, c.1825 (card, paper, tissue)
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Spiral galaxy NGC 5474 in the Great Bear - Spiral galaxy NGC 5474 in Ursa Majo
Spiral galaxy NGC 3184 in the Great Bear - Spiral galaxy NGC 3184 in Ursa Majo
Comete Hyakutake and Big Bear - Comet Hyakutake and Big Dipper March 25 199
Polaris System - Polaris is a triple system consisting of a supergiant star and two dwarf stars. It is a pulsating variable star, cepheide of low amplitude. This montage shows the polar star and constellations of the Little Bear and the Big Bear (left), Polaris A and his companion Polaris B seen by the Hubble Space Telescope (top right), and Polaris Ab photographed for the first time by the Hubble Space Telescope (bottom right). This sequence of images shows that the North Star, Polaris is really a triple star system. For the first time, the close companion of Polaris has been seen directly. The left frame shows Polaris's location very close to the position of Earth's north celestial pole in Ursa Minor (the Small Bear). The upper right image shows Polaris A and its distant companion Polaris B, as viewed by Hubble. They are separated by approximately 240 billion miles. Polaris B, the wide companion, is visible in small telescopes, and was first noticed by William Herschel in 1780. The close companion, Polaris Ab was known to exist from its gravitational tug on Polaris A, but has only been seen directly now using Hubble (lower right image). The companion is only 2 trillion miles from Polaris A. The triple system is 430 light - years away
Twin galaxies in the constellation of Ursa Major, 31 March 1889
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Cepheides in the galaxy M81 - Cepheids in the galaxy M81 - Cepheides are very bright variable stars that serve as cosmic beacons to measure distance from nearby galaxies. Their pulse period is measured and their absolute luminosite is calculated. By comparing the result to their apparent luminosite in the sky, they can be calculated accurately. Here, the space telescope identified cepheides in the M81 galaxy; astronomers were able to deduce a new distance for this galaxy; it would be 11 million years - light from Earth; previous estimates gave a figure of 18 million light years. Image obtained in 1993. Astronomers have discovered variable stars in the spiral galaxy M81, and measured the distance of the galaxy to be 11 million light - years (3.4 megaparsecs). They quote a 10% uncertainty in this result (plus or minus approximately one million light - years). Previous estimates of the galaxy's distance have ranged from 4.5 to 18 million light - years (1.4 to 5.6 megaparsecs). The astronomers used the Hubble '5 Wide Field & Planetary Camera to study two fields in M81. In each field they took 22 twenty - minute exposures spread over 14 months to find the variable stars and measure their periods and brightness. Cepheids are pulsating stars that become alternately brighter and fainter with periods ranging from 10 to 50 days. Astronomers have known for over 50 years that the periods of these stars precisely predict their total luminous power, which allows their distance to be measured. Messier 81 is a large spiral galaxy in the constellation Ursa Major. It is a rotating system of gas and stars similar to our own Galaxy, the Milky Way, but approximately twice as massive. This galaxy achieved prominence three months ago when the brightest northern supernova this century was discovered. In the expanding universe, the Hubble Constant (H0) is the ratio of the rec
Constellation Big Dipper - The Big Dipper - Asterism forms by the seven brightest stars in the constellation Big Dipper. Asterism formed by the seven brightest stars of the constellation Ursa Major
Dragon Constellation - Constellation of Draco - Dragon Constellation with part of the Big Bear and Little Bear. Draco (the Dragon) is said to represent Ladon, the multi - headed dragon slaughtered by Hercules, an act necessary to obtain the golden apples from the garden of Hesperides as the 11th of his 12 labours. Other ancient, dragonocentric legends exist. The constellation itself is rather indistinct with few bright stars, but it is a large and rambling construction wrapped around the north celestial pole. It extends from close to the Pole Star to more than 40 degrees of delination south of it and wanders over 11 hours of Right Ascension between Hercules and the Big Dipper. It is the 8th largest constelation in terms of area, which is over 1000 square degrees. This image also contains the constellation of Ursa Minor
Star constellations, Big Dipper or Plough, part of Ursa Major, astronomy diagram
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An image of the Pinwheel Galaxy, or M101. Located in the constellation of Ursa Major.
Constellation of the Great Bear - Constellation of Ursa Major: Constellation of the Great Bear seen above Burg Heid in Germany. - Ursa Major above Burg Heid, Germany
Constellation Hunting Dogs - Constellation of Canes Venatici - The small constellation of Hunting Dogs and the constellations of Bovier and Big Bear. Canes Venatici (CVN, the Hunting Dogs) is an inconspicuous constellation introduced by Johannes Hevelius in 1690, nestling beneath the tail of Ursa Major. It represents the dogs Asterion and Chara, held on a leash by Booetes as the attack the Great Bear. The brightest star is Cor Caroli, named by Edmund Halley in memory of the king Charles I, King of England, or his son, Charles II. Booetes is also visible on the left
Spiral galaxy seen by the slice NGC 4013 in the Great Bear - Edge - on view of NGC 4013 spiral galaxy in Ursa Major - The spiral galaxy Ngc 4013 is located 55 million years - light in the constellation Big Bear. A bright star seems to radiate from this galaxy; in reality, this star is much closer and belongs to our galaxy. Edge - on view of NGC 4013 spiral galaxy located about 55 million light years in Ursa Major. In its center, the very bright star is very much closer to us than it appears and belongs to our galaxy
Spiral galaxy NGC 3949 in the Great Bear - Spiral galaxy NGC 3949 in Ursa Major - The spiral galaxy NGC 3949 is located about 50 million years away - light from Earth. This image was taken by the Hubble Space Telescope in October 2001. Like our Milky Way, this galaxy has a blue disk of young stars peppered with bright pink star - birth regions. In contrast to the blue disk, the bright central bulge is made up of mostly older, redder stars. NGC 3949 lies about 50 million light - years from Earth. It is a member of a loose cluster of some six or seven dozens of galaxies located in the direction of the Big Dipper, in the constellation Ursa Major (the Great Bear). It is one of the larger galaxies of this cluster. This image was created from Hubble data taken with the Wide Field Planetary Camera 2 in October 2001. Separate exposures through blue, visible, and near - infrared filters have been combined to make the natural color picture
Spiral galaxy NGC 4013 in the Great Bear - Edge - on galaxy NGC 4013 in Ursa Major - The spiral galaxy NGC 4013 is located 55 million years - light in the constellation Big Bear. In this image, traces left by the passage of a dwarf galaxy appear as a stellar current around that galaxy. A bright star seems to radiate from this galaxy; in reality, this star is much closer and belongs to our galaxy. Edge - on view of NGC 4013 spiral galaxy located about 55 million light years in Ursa Major. This deep color image reveals an enormous faint looping structure extending over 80,000 light years from the galaxy center. This is a stream of stars coming from a smaller galaxy who merged with NGC 4013. The very bright star in the center of the galaxy is very much closer to us than it appears and belongs to our 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. Image obtained with a 50 cm telescope, composite of several poses. 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
Constellation of the Great Bear - Constellation of Ursa Major - Map of the constellation of the Great Bear with its main Celestial objects. Map showing the constellation of the Big Dipper with its main celestial objects
Spiral galaxy M101 in the Great Bear - Large field - Wide field view of the Pinwheel Galaxy (M101) - The galaxy M101 (NGC 5457) is located about 27 million years away - light from Earth. It spans more than 170,000 light years, almost double the size of our galaxy. We think that of the trillion stars in it, 100 billion stars could be similar to our Sun. In this image, other galaxies are visible: NGC 5474 (below M101), NGC 5473 (just above M101), NGC 5485 (upper left), NGC 5422 (upper center) and UGC 8837 (near star 86 uA, lower left). Image obtained by the Oschin telescope of Mount Palomar through several filters and composed. Catalogued as M101, the Pinwheel is a nice face - on spiral galaxy. It lies in the northern circumpolar constellation Ursa Major (The Big Bear), at a distance of about 25 million light - years from Earth. The bright blue star at right is 86 Uma, barely visible at the naked eye from a dark site. Also visible some other nice galaxies like NGC 5474 (below under M101), NGC 5473 (just above M101), NGC 5485 (at left edge), NGC 5422 (at top edge) and UGC 8837 (near 86 UMA, the bright star at bottom right). This image is based on data acquired by the Oschin Telescope at the Mount Palomar Observatory
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
Spiral Galaxy NGC 3079 in the Great Bear - Spiral galaxy NGC 3079 - NGC 3079 is a spiral galaxy distant about 50 million years - light from Earth. His disc measures about 70,000 years - light. Also visible in this photo is the quasar Q0957+561, 9 billion years away - light. The NGC 3079 spiral galaxy is located at about 50 million light years from Earth. Its dics is approximately 70,000 light years wide. The Q0957+561 twin quasar, roughly at 9 billion light years away, is also visible in this image
Constellation of the Great Bear and Spring Triangle - The Big Dipper and spring triangle - View of the Great Bear with on its left the brilliant star Arcturus du Bouvier. Also visible are the star Spica and the constellation of the Lion. The stars Arcturus, Spica and Denebola form an asterism called the Spring Triangle. The Big Dipper with at left the bright star Arcturus in Bootes. Also visible the star Spica and the constellations of Leo. The stars Arcturus, Spica and Denebola are forming the asterism called the spring triangle
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
Supernova in Galaxy M82 in Ursa Major - SN 2014J is a supernova of type Ia discovered on January 21, 2014 in the M82 galaxy. The supernova appears to the right of the center of the image. M82 is an irregular galaxy distant about 12 million years - light from Earth. Image obtained by the Hubble Space Telescope on January 31, 2014. SN 2014J is a type Ia supernova discovered on January 21 2014 in M82. 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. This Hubble photograph was taken on January 31 2014, as the supernova approached its peak brightness
Spiral galaxy M81 in the Great Bear - Spiral galaxy M81 in Ursa Major - The spiral galaxy M81 is located 12 million years ago - light from Earth. Its arms are home to star-forming regions while its core is surrounded by much older yellow stars. In the background at the top, an irregular dwarf galaxy, Holmberg IX. This image obtained by a 50 cm amateur telescope, in February 2010 for 23 hours of poses, shows gas filaments whose origin is uncertain. Located about 12 million light - years from our planet, M81 (NGC 3031) together with M82 (NGC 3034), NGC 3077 and NGC 2976 forms one of the most iconic groups of interacting galaxies. The M81 group has also been the subject of many studies searching for and analyzing evidence of strong interactions among its components. In 1965, Halton Arp detected an unusual looping feature near M81 while examining photographic plates produced with the 48 - inch Schmidt on Mount Palomar. Traditionally, ARP's loop has been interpreted as a tail resulting from the tidal interaction between M81 and M82. However, since its discovery that explanation has been doubted by many researchers. Interestingly, the region of the sky containing the M81 group of galaxies is filled with Galactic cirrus and ARP's loop exhibits colors and emission properties similar to those observed in Galactic cirrus clouds. This optical image suggests that the light observed at optical wavelengths is a combination of emissions from: recent star forming regions situated near M81, the extended disk of M81 and scattered light from the same Galactic cirrus that is responsible for the bulk of the far infrared emissions. Although our observations cannot exclude the presence of some material stripped from the disk of M81 (NGC 3031) and/or M82 (NGC 3034) that is chance located in our line of sight to and far behind this intruiging structure, our findings suggest that ARP's Loop is situated between the observer and M81 (