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'Cassiopeia' images and/or videos results page 1 of 3

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HYGINUS / CASSIOPEIA
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Cassiopeia, 2006
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Ursa Major, Polaris and Cassiopeia -
CASSIOPEIA STAR MAP
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CASSIOPEIA (CIG CARD)
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'Cassiopeia', May 1866
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Cassiopeia and Cepheus (engraving)
Cassiopeia constellation (photo)
Gamma Cassiopeia, 1890
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A false-colour image of Cassiopeia A
The constellation of Cassiopeia. 1820 (engraving)
Graptopetalum bellum/Tacitus cassiopeia
BLUNT/CASSIOPEIA/PL 30
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Stars in Cassiopeia, November 1883
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Cassiopeia A (NIRCam Image) (photo)
Constellation Cassiopee - The constellation of Cassiopei
IC 10 irregular galaxy in Cassiopeia
Nebula IC 1805 in Cassiopeia (photo)
Remains of the supernova Cassiopee - A - Supernova remnant Cassiopeia A - Cassiopee A is the rest of a supernova that exploded about 300 years ago. This image shows the expanding gas shell. From this gas will one day create new stars and planets. Cassiopee - A is located about 10,000 light years away from Earth in the constellation Cassiopee. Image obtained on September 5, 2008 with a telescope measuring 61 cm in diameter. Cassiopeia A (Cas A) is the youngest known remnant from a supernova explosion in the Milky Way. Cas A is located ten thousand light - years away from Earth in the constellation of Cassiopeia. Image taken on September 5 2008 with a 24 - inch telescope
Constellations of Andromede and Cassiopee - Andromeda and Cassiopeia constellation
Constellations of Andromede and Cassiopee - Andromeda and Cassiopeia constellation
Cassiopeia, c.1825 (card, paper, tissue )
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Constellation Cassiopee - The constellation of Cassiopei
Constellations of Cassiopeia (Cassiopee) and Cepheus (Cephee). Engraving. Colored.
Remains of a supernova explosion known as Cassiopeia A (Cas A) (photo)
Open cluster NGC 663 in Cassiopee - Open cluster NGC 663 in Cassiopei
This image from NASA's WISE shows the constellation Cassiopeia.
This image from NASA's WISE shows the constellation Cassiopeia.
Open cluster M52 in Cassiopee - Open cluster M52 in Cassiopeia - M52 (NGC 7654) is an open cluster that contains about 200 stars
Nebula VDB 2 in Cassiopee - Nebula VDB 2 in Cassiopeia - VDB 2 is a nebula by light reflexion. Other nebulae are shown in this image (LBN 585, LBN 590, GN 00.04.4, Teutsch GN J0016.8+6546, [YDM97] CO 112,115,118, Sh2 - 171). A portion of Sh2 - 171 is visible at the bottom right of the image. Numerous other faint nebulae occupy the region near VdB 2 (LBN 585, LBN 590, GN 00.04.4, Teutsch GN J0016.8+6546, [YDM97] CO 112,115,118, Sh2 - 171). Sh2 - 171 is just making an appearance in the lower right corner
Constellation Cassiopee - The constellation of Cassiopeia - On the left, the double cluster of Persee
Galaxies Maffei 1 and Maffei 2 in Cassiopee - Maffei Galaxies in Cassiopeia - Maffei 1 (right) is an elliptical galaxy, Maffei 2 (left) is a barree spiral galaxy. These two galaxies are located about 8 million light years away from Earth. Image obtained by the Oschin telescope of Mount Palomar through several filters and composed. The picture show two galaxies lying at 2.5 degrees northeast of h and Chi Persei the famous Double Cluster in Cassiopeia. Although the galaxies has been obstructed by inner galactic matters, their actual sizes are larger than 10 arc minutes, fairly large - sized neighboring galaxies. The Maffei I (on the right) is an elliptic, and the Maffei II (on the left) is classified as a bared galaxy. The galaxies are estimated about 8 million light years away. They were discovered by the Italian astronomer Paolo Maffei in 1968. Now we know about 20 galaxies belonging to Maffei Group. This image is based on data acquired by the Oschin Telescope at the Mount Palomar Observatory
Open cluster NGC 654 in Cassiopee - Open cluster NGC 654 in Cassiopei
Constellation of Cassiopee and real position of stars - Stars in the constellation of Cassiopeia 3D representation - The constellations are just imaginary drawings made from the stars. Really, the stars of the same constellation are not at the same distance from the Earth observer. The stars within a constellation rarely have any astrophysical relationship to each other. Their apparent proximity when viewed from Earth disguises the fact that they typically lie light years apart
Nebula IC 63 in Cassiopee - Nebula IC 63 in Cassiopei
'Cassiopeia', May 1866 (mythologie grecque : Cassiopee reine d'Ethiopie)
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'Cassiopeia', May 1866 (mythologie grecque : Cassiopee reine d'Ethiopie)
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Gamma Star Cassiopeia, nebulae IC 59 and IC 6
Open cluster M52 in Cassiopee - Open cluster M52 in Cassiopei
Cephee Constellation - Constellation of Cepheus - At the bottom left, the constellation Cassiopee; at the top, the bright star is the polar star. Cepheus is a representation of King Cepheus of Ethiopia, who has stellar connections, being husband to Cassiopeia and the father of Andromeda. It is a large northern constellation of 588 square degrees, 27th out of 88 in size and is best seen in the early evening in November. It is distinguished by having two unusual stars that are easily seen. Delta Cephei is the prototype for an intrinsically bright class of regularly pulsating variable stars whose period of variability is closely related to their absolute magnitudes. The brightest stars have the longest period, so distance can be estimated by measuring the period and the apparent magnitude of a star. And these stars are bright, so the method can be extended to nearby galaxies. Mu (u) Cephei is an extremely red, irregular variable star easily seen in binoculars. This too is a prototype, of a class of stars known as semi - regular variables
Open cluster NGC 7789 in Cassiopee - Open cluster NGC 7789 in Cassiopeia - The cluster of stars NGC 7789 is located about 7600 years - light from Earth. It contains about 300 stars, including a number of giant red stars. His age is estimated at 1.6 billion years. The open cluster NGC 7789 in Cassiopeia is a bright and richly populated cluster comprised of approximately 300 member stars which are evenly distributed and well detached from the background sky. This cluster lies at a distance of 7620 light - years away with an apparent diameter of 25 '. As indicated by the various red giants in the image, the cluster is advanced in age and which has been estimated to be approximately 1.6 billion years - old
Cassiopee Constellation - The constellation of Cassiopeia - Cassiopeia, was seen in mythology as the seated Queen of Ethiopia (not to be confused with the modern AEthiopia). She was the wife of Cepheus and the mother of Andromeda, beautiful but boastful. The grouping of moderately bright stars has a distinctive 'W' shape and lies in a rather faint part of the northern Milky Way. It is circumpolar for latitudes north of 50*. Occupying almost 500 square degrees of sky it is the 25th largest of the 88 modern constellations
Constellation Cassiopee - The constellation of Cassiopei
Constellation Cassiopee - The constellation of Cassiopei
The northern Milky Way, from Cassiopeia to Capella and beyond. Pleiades, Perseus, Capell
Nebula NGC 7635 in Cassiopee - The Bubble Nebula (NGC 7635) in Cassiopeia - This nebula is located about 7100 years - light from Earth. A star 40 times more massive than our Sun, called Wolf - Rayet, is responsible for the formation of this bubble; it is the star BD+60* 2522. The Bubble Nebula in Cassiopeia is one of the most dramatic emission nebulae visible in the northern hemisphere. Lying at a distance of about 7,000 light - years away and spanning six light - years in diameter, NGC 7635 is quite bright with a magnitude of 7.0. The star in the middle of the bubble, BD+602522, is responsible for this stunning site, for this very hot star emits so much UV radiation that it is able to also heat and excite the surrounding dust and gas, thus emitting its own radiation. It is a Wolf - Rayet star, a very luminous star and also very short - lived. This Wolf - Rayet star is 40 times as massive than our sun
Star Formation in Cassiopee - Star Formation in Cassiopeia - This star-forming region, called W5, is located approximately 6500 light years ago in the constellation Cassiopee. Several generations of stars appear on this cliche; the older ones are the blue stars in the centre of the two cavities; the younger stars are grouped at the edges of these cavities and at the ends of the gas pillars or they appear like pink dots; the white areas are home to the very young stars in formation. In this infrared image, heated dust appears in red, dense gas clouds appear in green. Composite image obtained by the Spitzer space telescope in 2006 and 2007. Generations of stars can be seen in this infrared portrait from Nasa's Spitzer Space Telescope. In this wispy star - forming region, called W5, the oldest stars can be seen as blue dots in the centers of the two hollow cavities (other blue dots are background and foreground stars not associated with the region). Younger stars line the rims of the cavities, and some can be seen as pink dots at the tips of the elephant - trunk - like pillars. The white knotty areas are where the youngest stars are forming. Red shows heated dust that pervades the region's cavities, while green highlights dense clouds. W5 spans an area of sky equivalent to four full moons and is about 6,500 light - years away in the constellation Cassiopeia. The Spitzer picture was taken over a period of 24 hours. Like other massive star - forming regions, such as Orion and Carina, W5 contains large cavities that were carved out by radiation and winds from the region's most massive stars. According to the theory of triggered star - formation, the carving out of these cavities pushes gas together, causing it to ignite into successive generations of new stars. This image contains some of the best evidence yet for the triggered star - formation theory. Scientists analyzing the photo have been able to sho
Star Formation in Cassiopee - Star Formation in Cassiopeia - This star-forming region, called W5, is located approximately 6500 light years ago in the constellation Cassiopee. Several generations of stars appear on this cliche; the older ones are the blue stars in the centre of the two cavities; the younger stars are grouped at the edges of these cavities and at the ends of the gas pillars or they appear like pink dots; the white areas are home to the very young stars in formation. In this infrared image, heated dust appears in red, dense gas clouds appear in green. Composite image obtained by the Spitzer space telescope in 2006 and 2007. Generations of stars can be seen in this infrared portrait from Nasa's Spitzer Space Telescope. In this wispy star - forming region, called W5, the oldest stars can be seen as blue dots in the centers of the two hollow cavities (other blue dots are background and foreground stars not associated with the region). Younger stars line the rims of the cavities, and some can be seen as pink dots at the tips of the elephant - trunk - like pillars. The white knotty areas are where the youngest stars are forming. Red shows heated dust that pervades the region's cavities, while green highlights dense clouds. W5 spans an area of sky equivalent to four full moons and is about 6,500 light - years away in the constellation Cassiopeia. The Spitzer picture was taken over a period of 24 hours. Like other massive star - forming regions, such as Orion and Carina, W5 contains large cavities that were carved out by radiation and winds from the region's most massive stars. According to the theory of triggered star - formation, the carving out of these cavities pushes gas together, causing it to ignite into successive generations of new stars. This image contains some of the best evidence yet for the triggered star - formation theory. Scientists analyzing the photo have been able to sho
Cassiopee Constellation - The constellation of Cassiopeia - Cassiopeia, was seen in mythology as the seated Queen of Ethiopia (not to be confused with the modern AEthiopia). She was the wife of Cepheus and the mother of Andromeda, beautiful but boastful. The grouping of moderately bright stars has a distinctive 'W' shape and lies in a rather faint part of the northern Milky Way. It is circumpolar for latitudes north of 50*. Occupying almost 500 square degrees of sky it is the 25th largest of the 88 modern constellations