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Immagini di 'Cassiopeia' trovate, 187

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Constellation Cassiopee - The constellation of Cassiopei

Constellation Cassiopee - The constellation of Cassiopei

PIX4589563

Cassiopee Constellation - Constellation of Cassiopeia - Map of the constellation Cassiopee with its main Celestial objects. The Great Bear is indicated for the scale. Map showing the constellation of Cassiopeia with its main celestial objects. Constellation of Big Dipper is shown at scale

Cassiopee Constellation - Constellation of Cassiopeia - Map of the constellation Cassiopee with its main Celestial objects. The Great Bear is indicated for the scale. Map showing the constellation of Cassiopeia with its main celestial objects. Constellation of Big Dipper is shown at scale

Sebastien Beaucourt

PIX4589711

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

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

PIX4589796

Nebula VdB 4 in Cassiopee - Nebula VdB 4 in Cassiopeia - van den Bergh 4 is a reflexion nebula in the constellation Cassiopee. The adjacent dark nebulae and dust appear not to be cataloged

Nebula VdB 4 in Cassiopee - Nebula VdB 4 in Cassiopeia - van den Bergh 4 is a reflexion nebula in the constellation Cassiopee. The adjacent dark nebulae and dust appear not to be cataloged

Adam Block

PIX4621721

Constellation Cassiopee - The constellation of Cassiopei

Constellation Cassiopee - The constellation of Cassiopei

B&S.Fletcher

PIX4589568

Cassiopee Constellation - Constellation of Cassiopeia - Cassiopee Constellation extracted from the Hevelius Uranographia. Recolorised image. Map showing the constellation of Cassiopeia with its mythological form from “” Uranographia”” star atlas by Hevelius (1690). Recolored Image

Cassiopee Constellation - Constellation of Cassiopeia - Cassiopee Constellation extracted from the Hevelius Uranographia. Recolorised image. Map showing the constellation of Cassiopeia with its mythological form from “” Uranographia”” star atlas by Hevelius (1690). Recolored Image

Sebastien Beaucourt

PIX4589721

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 cavi

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 cavi

PIX4621152

Constellations of Cassiopee and Cephee - Cassiopeia and Cepheus with constellation lines - Constellations Cassiopeia and Cepheus are two of the most famous constellations in the Northern skies. The shapes of the constellations were drawn on top and some important objects were highlited

Constellations of Cassiopee and Cephee - Cassiopeia and Cepheus with constellation lines - Constellations Cassiopeia and Cepheus are two of the most famous constellations in the Northern skies. The shapes of the constellations were drawn on top and some important objects were highlited

Alex Conu

PIX4589747

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 Obse

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 Obse

D. De Martin

PIX4613894

Constellation Cassiopee - The constellation of Cassiopeia - On the left, the double cluster of Persee

Constellation Cassiopee - The constellation of Cassiopeia - On the left, the double cluster of Persee

Vincent Toporenko

PIX4589595

Nebula NGC 7635 in Cassiopee - Bubble Nebula (NGC 7635) in Cassiopeia - This nebula is located about 7100 years - light from Earth. A massive star, 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

Nebula NGC 7635 in Cassiopee - Bubble Nebula (NGC 7635) in Cassiopeia - This nebula is located about 7100 years - light from Earth. A massive star, 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

PIX4620681

Nebula VdB 4 in Cassiopee - Nebula VdB 4 in Cassiopeia - van den Bergh 4 is a reflexion nebula in the constellation Cassiopee. The adjacent dark nebulae and dust appear not to be cataloged

Nebula VdB 4 in Cassiopee - Nebula VdB 4 in Cassiopeia - van den Bergh 4 is a reflexion nebula in the constellation Cassiopee. The adjacent dark nebulae and dust appear not to be cataloged

Tom Davis

PIX4621717

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

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

PIX4589602

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 cavi

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 cavi

PIX4621160

Constellations of Cephee, Cassiopee and Little Bear - Across the North Celestial Pole, Cassiopeia to Ursa Mino

Constellations of Cephee, Cassiopee and Little Bear - Across the North Celestial Pole, Cassiopeia to Ursa Mino

PIX4589857

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

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

Adam Block

PIX4620709

Shooting star rain, Perseides - Illustration - Perseid meteor shower. Artwork - The double cluster of Persee is surrounded. The double cluster in Perseus is circled

Shooting star rain, Perseides - Illustration - Perseid meteor shower. Artwork - The double cluster of Persee is surrounded. The double cluster in Perseus is circled

S. Numazawa

PIX4599307

Cassiopeia and Pole Star (chromolitho)

Cassiopeia and Pole Star (chromolitho)

English School, (20th century)

LLM3651668

Nebula NGC 281 in Cassiopee - Nebula NGC 281 in Cassiopeia - NGC 281 is a star-forming region about 10,000 light years away from Earth in the constellation Cassiopee. At the center of this nebula is the cluster of stars IC 1590 whose stars are only a few million years old. NGC 281 is a busy workshop of star formation. Prominent features include a small open cluster of stars, a diffuse red - glowing emission nebula, large lanes of obscuring gas and dust, and dense knots of dust and gas in which stars may still be forming. The open cluster of stars IC 1590 visible around the center has formed only in the last few million years. The brightest member of this cluster is actually a multiple - star system shining light that helps ionize the nebula's gas, causing the red glow visible throughout. The lanes of dust visible below the center are likely homes of future star formation. The entire NGC 281 system lies about 10 thousand light years distant

Nebula NGC 281 in Cassiopee - Nebula NGC 281 in Cassiopeia - NGC 281 is a star-forming region about 10,000 light years away from Earth in the constellation Cassiopee. At the center of this nebula is the cluster of stars IC 1590 whose stars are only a few million years old. NGC 281 is a busy workshop of star formation. Prominent features include a small open cluster of stars, a diffuse red - glowing emission nebula, large lanes of obscuring gas and dust, and dense knots of dust and gas in which stars may still be forming. The open cluster of stars IC 1590 visible around the center has formed only in the last few million years. The brightest member of this cluster is actually a multiple - star system shining light that helps ionize the nebula's gas, causing the red glow visible throughout. The lanes of dust visible below the center are likely homes of future star formation. The entire NGC 281 system lies about 10 thousand light years distant

Jerry Lodriguss

PIX4617441

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

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

PIX4589805

Cassiopee Constellation - The constellation of Cassiopeia - Cassiopee Constellation with near the horizon, part of the constellation Persee. Cassiopeia constellation; near the horizon, Perseus constellation

Cassiopee Constellation - The constellation of Cassiopeia - Cassiopee Constellation with near the horizon, part of the constellation Persee. Cassiopeia constellation; near the horizon, Perseus constellation

S. Numazawa

PIX4589608

Constellations of Cephee, Cassiopee and Little Bear - Across the North Celestial Pole, Cassiopeia to Ursa Mino

Constellations of Cephee, Cassiopee and Little Bear - Across the North Celestial Pole, Cassiopeia to Ursa Mino

PIX4589859

Nebulae NGC 7635, NGC 7538 and M52 clusters in Cassiopee - M52, The Bubble Nebula, and NGC 7538 in Cassiopeia - Open cluster M52 is on the left, NGC 7635, is in the center. The nebula emitted NGC 7538 is on the top right. Open cluster M52 is at left in this photo, and NGC 7635, the Bubble Nebula is near the center. Bright emission nebula NGC 7538 is at the upper right

Nebulae NGC 7635, NGC 7538 and M52 clusters in Cassiopee - M52, The Bubble Nebula, and NGC 7538 in Cassiopeia - Open cluster M52 is on the left, NGC 7635, is in the center. The nebula emitted NGC 7538 is on the top right. Open cluster M52 is at left in this photo, and NGC 7635, the Bubble Nebula is near the center. Bright emission nebula NGC 7538 is at the upper right

R. Gendler

PIX4620669

The Lactee Way in the North Hemisphere - Panorama - Northern Milky Way Panorama - Part of the Lactee Way that extends here from the Swan, on the left, to Cassiopee, on the right. This portion of the Milky Way, our own galaxy as seen from the inside, is best placed in the northern sky in the fall. Stretching from Deneb and the North America Nebula in Cygnus at the left, the Milky Way runs across the photo to Cassiopeia at the right

The Lactee Way in the North Hemisphere - Panorama - Northern Milky Way Panorama - Part of the Lactee Way that extends here from the Swan, on the left, to Cassiopee, on the right. This portion of the Milky Way, our own galaxy as seen from the inside, is best placed in the northern sky in the fall. Stretching from Deneb and the North America Nebula in Cygnus at the left, the Milky Way runs across the photo to Cassiopeia at the right

Jerry Lodriguss

PIX4636889

Constellations of Andromede and Cassiopee - Andromeda and Cassiopeia constellations - Field around the constellations of Andromede and Cassiopee. Star field around constellations of Andromeda and Cassiopeia

Constellations of Andromede and Cassiopee - Andromeda and Cassiopeia constellations - Field around the constellations of Andromede and Cassiopee. Star field around constellations of Andromeda and Cassiopeia

PIX4588941

Constellations of Andromede and Cassiopee - Andromeda and Cassiopeia constellations - Field around the constellations of Andromede and Cassiopee. Star field around constellations of Andromeda and Cassiopeia

Constellations of Andromede and Cassiopee - Andromeda and Cassiopeia constellations - Field around the constellations of Andromede and Cassiopee. Star field around constellations of Andromeda and Cassiopeia

PIX4588948

Constellations of Cassiopee, Cephee and Lizard - Cassiopeia, Cepheus, Lacerta constellations - On the top left the constellation of Cephee, on its right the Lizard, in the center of Cassiopee, below part of the constellation of Persee, on the right, part of Andromede. Top left Cepheus constellation with Lacerta to its right; in the middle Cassiopeia constellation, and part of Andromeda to its right; bottom part of Perseus

Constellations of Cassiopee, Cephee and Lizard - Cassiopeia, Cepheus, Lacerta constellations - On the top left the constellation of Cephee, on its right the Lizard, in the center of Cassiopee, below part of the constellation of Persee, on the right, part of Andromede. Top left Cepheus constellation with Lacerta to its right; in the middle Cassiopeia constellation, and part of Andromeda to its right; bottom part of Perseus

S. Numazawa

PIX4589645

Mel 15 star cluster in the nebula IC 1805 - IC1805 Heart Nebula - Melotte 15 is a cluster of young stars composed of massive OB-type stars. Age about 1.5 million years, this cluster is located 50 years - light in front of the nebula it illuminates. Melotte 15 is an extremely young cluster of massive OB stars with a mean age of only 1.5 million years. The cluster is positioned some 50 light years in front of the nebula it illuminates

Mel 15 star cluster in the nebula IC 1805 - IC1805 Heart Nebula - Melotte 15 is a cluster of young stars composed of massive OB-type stars. Age about 1.5 million years, this cluster is located 50 years - light in front of the nebula it illuminates. Melotte 15 is an extremely young cluster of massive OB stars with a mean age of only 1.5 million years. The cluster is positioned some 50 light years in front of the nebula it illuminates

PIX4622391

Constellations of Andromede and Cassiopee - Andromeda and Cassiopeia constellations - On the left the constellation of Cassiopee, on the right Andromede, up part of Pegase. Left Cassiopeia constellation, right Andromeda and part of Pegasus

Constellations of Andromede and Cassiopee - Andromeda and Cassiopeia constellations - On the left the constellation of Cassiopee, on the right Andromede, up part of Pegase. Left Cassiopeia constellation, right Andromeda and part of Pegasus

PIX4588933

Constellations of Andromede and Cassiopee - Andromeda and Cassiopeia constellation

Constellations of Andromede and Cassiopee - Andromeda and Cassiopeia constellation

PIX4588898

Rain d'étoiles filantes-Perseides - Perseid meteor shower - Composite of different images. The constellation Cassiopee is traced. Composite of different images. Constellation of Cassiopeia is drawn

Rain d'étoiles filantes-Perseides - Perseid meteor shower - Composite of different images. The constellation Cassiopee is traced. Composite of different images. Constellation of Cassiopeia is drawn

S. Numazawa

PIX4598809

Cassiopeia and Stephalia (chromolitho)

Cassiopeia and Stephalia (chromolitho)

European School, (19th century)

LLM2783031

Nebulae NGC 7635, NGC 7538 and M52 clusters in Cassiopee - M52, The Bubble Nebula, and NGC 7538 in Cassiopeia - Open cluster M52 is on the left, NGC 7635, is in the center. The nebula emitted NGC 7538 is on the top right. Open cluster M52 is at left in this photo, and NGC 7635, the Bubble Nebula is near the center. Bright emission nebula NGC 7538 is at the upper right

Nebulae NGC 7635, NGC 7538 and M52 clusters in Cassiopee - M52, The Bubble Nebula, and NGC 7538 in Cassiopeia - Open cluster M52 is on the left, NGC 7635, is in the center. The nebula emitted NGC 7538 is on the top right. Open cluster M52 is at left in this photo, and NGC 7635, the Bubble Nebula is near the center. Bright emission nebula NGC 7538 is at the upper right

PIX4620688

Nebula NGC 7635 in Cassiopee - The Bubble Nebula: This nebula is located about 8000 light years 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. Image obtained by the space telescope Hubble - The Bubble Nebula, also known as NGC 7635, is an emission nebula located 8 000 light-years away - This complete view of the Bubble Nebula allows us to fully appreciate the almost perfectly symmetrical shell which gives the nebula its name. This shell is the result of a powerful flow of gas - known as a stellar wind - from the bright star visible just to the left of centre in this image. The star, SAO 20575, is between ten and twenty times the mass of the Sun and the pressure created by its stellar wind forces the surrounding interstellar material outwards into this bubble-like form - The giant molecular cloud that surrounds the star - glowing in the star's intense ultraviolet radiation - tries to

Nebula NGC 7635 in Cassiopee - The Bubble Nebula: This nebula is located about 8000 light years 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. Image obtained by the space telescope Hubble - The Bubble Nebula, also known as NGC 7635, is an emission nebula located 8 000 light-years away - This complete view of the Bubble Nebula allows us to fully appreciate the almost perfectly symmetrical shell which gives the nebula its name. This shell is the result of a powerful flow of gas - known as a stellar wind - from the bright star visible just to the left of centre in this image. The star, SAO 20575, is between ten and twenty times the mass of the Sun and the pressure created by its stellar wind forces the surrounding interstellar material outwards into this bubble-like form - The giant molecular cloud that surrounds the star - glowing in the star's intense ultraviolet radiation - tries to

PIX4620728

Nebula NGC 281 in Cassiopee - Nebula NGC 281 in Cassiopeia - NGC 281 is a star-forming region about 10,000 light years away from Earth in the constellation Cassiopee. At the center of this nebula is the cluster of stars IC 1590 whose stars are only a few million years old. Image obtained by combining light through 3 different filters that highlight oxygen, hydrogen, and sulfur. NGC 281 is a busy workshop of star formation. Prominent features include a small open cluster of stars, a diffuse emission nebula, large lanes of obscuring gas and dust, and dense knots of dust and gas in which stars may still be forming. The open cluster of stars IC 1590 visible around the center has formed only in the last few million years. The brightest member of this cluster is actually a multiple - star system shining light that helps ionize the nebula's gas. The lanes of dust visible below the center are likely homes of future star formation. The entire NGC 281 system lies about 10 thousand light years di

Nebula NGC 281 in Cassiopee - Nebula NGC 281 in Cassiopeia - NGC 281 is a star-forming region about 10,000 light years away from Earth in the constellation Cassiopee. At the center of this nebula is the cluster of stars IC 1590 whose stars are only a few million years old. Image obtained by combining light through 3 different filters that highlight oxygen, hydrogen, and sulfur. NGC 281 is a busy workshop of star formation. Prominent features include a small open cluster of stars, a diffuse emission nebula, large lanes of obscuring gas and dust, and dense knots of dust and gas in which stars may still be forming. The open cluster of stars IC 1590 visible around the center has formed only in the last few million years. The brightest member of this cluster is actually a multiple - star system shining light that helps ionize the nebula's gas. The lanes of dust visible below the center are likely homes of future star formation. The entire NGC 281 system lies about 10 thousand light years di

PIX4617475

Remnants of the supernova Cassiopee A in X-rays - visible and infrared - This stunning picture of the supernova remnant Cassiopeia A (Cas A) is a composite of images taken by three of Nasa's Great Observatories. Infrared data from the Spitzer Space Telescope are colored red; optical data from the Hubble Space Telescope are yellow; and X - ray data from the Chandra X - ray Observatory are green and blue. Cas A is the 300 - year - old remnant created by the supernova explosion of a massive star. Each Great Observatory image highlights different characteristics of the remnant. Spitzer reveals warm dust in the outer shell with temperatures of about 10 degrees Celsius (80 degrees Fahrenheit), and Hubble sees the delicate filamentary structures of warmer gases about 10,000 degrees Celsius. Chandra shows hot gases at about 10 million degrees Celsius. This hot gas was created when ejected material from the supernova smashed into surrounding gas and dust at speeds of about ten million miles per

Remnants of the supernova Cassiopee A in X-rays - visible and infrared - This stunning picture of the supernova remnant Cassiopeia A (Cas A) is a composite of images taken by three of Nasa's Great Observatories. Infrared data from the Spitzer Space Telescope are colored red; optical data from the Hubble Space Telescope are yellow; and X - ray data from the Chandra X - ray Observatory are green and blue. Cas A is the 300 - year - old remnant created by the supernova explosion of a massive star. Each Great Observatory image highlights different characteristics of the remnant. Spitzer reveals warm dust in the outer shell with temperatures of about 10 degrees Celsius (80 degrees Fahrenheit), and Hubble sees the delicate filamentary structures of warmer gases about 10,000 degrees Celsius. Chandra shows hot gases at about 10 million degrees Celsius. This hot gas was created when ejected material from the supernova smashed into surrounding gas and dust at speeds of about ten million miles per

PIX4582940

Comete Hale - Bopp et observers 01/04/1997 - Comet Hale - Bopp with observers 1 April 1997 - The two children of the photographer (12 and 15 years old) observe the Hale - Bopp comete on 1 April 1997. Pennsylvania - USA. The photographers two sons, 12 year - old and 15 year - old watch comet Hale - Bopp on April 1st, 1997

Comete Hale - Bopp et observers 01/04/1997 - Comet Hale - Bopp with observers 1 April 1997 - The two children of the photographer (12 and 15 years old) observe the Hale - Bopp comete on 1 April 1997. Pennsylvania - USA. The photographers two sons, 12 year - old and 15 year - old watch comet Hale - Bopp on April 1st, 1997

Jerry Lodriguss

PIX4569601

Constellations of Cassiopee, Cephee and Lizard - Cassiopeia, Cepheus, Lacerta constellations - On the top left the constellation of Cephee, on its right the Lizard, in the center of Cassiopee, below part of the constellation of Persee, on the right, part of Andromede. Top left Cepheus constellation with Lacerta to its right; in the middle Cassiopeia constellation, and part of Andromeda to its right; bottom part of Perseus

Constellations of Cassiopee, Cephee and Lizard - Cassiopeia, Cepheus, Lacerta constellations - On the top left the constellation of Cephee, on its right the Lizard, in the center of Cassiopee, below part of the constellation of Persee, on the right, part of Andromede. Top left Cepheus constellation with Lacerta to its right; in the middle Cassiopeia constellation, and part of Andromeda to its right; bottom part of Perseus

S. Numazawa

PIX4589653

Constellations of Andromede and Cassiopee - Andromeda and Cassiopeia constellations - Star sky around the constellations of Andromede and Cassiopee. 19/10/2007. Starry sky above an oak. October 19, 200

Constellations of Andromede and Cassiopee - Andromeda and Cassiopeia constellations - Star sky around the constellations of Andromede and Cassiopee. 19/10/2007. Starry sky above an oak. October 19, 200

Laurent Laveder

PIX4588930

Constellation of Perseus and Andromeda, from 'Atlas Coelestis', by John Flamsteed (1646-1719), pub. in 1729 (hand coloured engraving)

Constellation of Perseus and Andromeda, from 'Atlas Coelestis', by John Flamsteed (1646-1719), pub. in 1729 (hand coloured engraving)

Thornhill, James (1675-1734) (after)

STC128638

Constellations of Andromede and Cassiopee - Andromeda and Cassiopeia constellations - On the left the constellation of Cassiopee, on the right Andromede, up part of Pegase. Left Cassiopeia constellation, right Andromeda and part of Pegasus

Constellations of Andromede and Cassiopee - Andromeda and Cassiopeia constellations - On the left the constellation of Cassiopee, on the right Andromede, up part of Pegase. Left Cassiopeia constellation, right Andromeda and part of Pegasus

PIX4588919

Constellations of Andromede and Cassiopee - Andromeda and Cassiopeia constellations - Star sky around the constellations of Andromede and Cassiopee. 16/10/2007. Starry sky above an oak. October 16, 200

Constellations of Andromede and Cassiopee - Andromeda and Cassiopeia constellations - Star sky around the constellations of Andromede and Cassiopee. 16/10/2007. Starry sky above an oak. October 16, 200

Laurent Laveder

PIX4588938

Nebula NGC 281 in Cassiopee - Nebula NGC 281 in Cassiopeia - NGC 281 is a star-forming region about 10,000 light years away from Earth in the constellation Cassiopee. At the center of this nebula is the cluster of stars IC 1590 whose stars are only a few million years old. A composite of X-ray images obtained by the Chandra Space Telescope in purple and infrared by Spitzer in red green and blue. High - mass stars are important because they are responsible for much of the energy pumped into our galaxy over its lifetime. Unfortunately, these stars are poorly understood because they are often found relatively far away and can be obscured by gas and dust. The star cluster NGC 281 is an exception to this rule. It is located about 6,500 light years from Earth and, remarkably, almost 1,000 light years above the plane of the galaxy, giving astronomers a nearly unfettered view of the star formation within IT.This composite image of NGC 281 contains X - ray data from Chandra, in purple, with inf

Nebula NGC 281 in Cassiopee - Nebula NGC 281 in Cassiopeia - NGC 281 is a star-forming region about 10,000 light years away from Earth in the constellation Cassiopee. At the center of this nebula is the cluster of stars IC 1590 whose stars are only a few million years old. A composite of X-ray images obtained by the Chandra Space Telescope in purple and infrared by Spitzer in red green and blue. High - mass stars are important because they are responsible for much of the energy pumped into our galaxy over its lifetime. Unfortunately, these stars are poorly understood because they are often found relatively far away and can be obscured by gas and dust. The star cluster NGC 281 is an exception to this rule. It is located about 6,500 light years from Earth and, remarkably, almost 1,000 light years above the plane of the galaxy, giving astronomers a nearly unfettered view of the star formation within IT.This composite image of NGC 281 contains X - ray data from Chandra, in purple, with inf

PIX4617483

Star cluster IC 1590 in NGC 281 (Cassiopee) - Open cluster and Bok globules in NGC 281 - View of a detail in the center of the nebula NGC 281 in Cassiopee. The brightest stars of the open cluster IC 1590 are visible, accompanied by Bok's blood cells, dark interstellar clouds consisting of gas and dust that absorb light. Image obtained by the Hubble Space Telescope (HST). Astronomers have used the NASA/ESA Hubble Space Telescope to study the young open star cluster IC 1590, which is found within the star formation region NGC 281 - - nicknamed the Pacman Nebula due to its resemblance to the famous arcade game character. This image only shows the central part of the nebula, where the brightest stars at the core of the cluster are found, with part of the Pacman's hungry mouth visible as the dark region below. But Pacman isn't gobbling up these stars. Instead, the nebula's gas and dust are being used as raw ingredients to make new stars. However, the stars in IC 1590 are still plotting thei

Star cluster IC 1590 in NGC 281 (Cassiopee) - Open cluster and Bok globules in NGC 281 - View of a detail in the center of the nebula NGC 281 in Cassiopee. The brightest stars of the open cluster IC 1590 are visible, accompanied by Bok's blood cells, dark interstellar clouds consisting of gas and dust that absorb light. Image obtained by the Hubble Space Telescope (HST). Astronomers have used the NASA/ESA Hubble Space Telescope to study the young open star cluster IC 1590, which is found within the star formation region NGC 281 - - nicknamed the Pacman Nebula due to its resemblance to the famous arcade game character. This image only shows the central part of the nebula, where the brightest stars at the core of the cluster are found, with part of the Pacman's hungry mouth visible as the dark region below. But Pacman isn't gobbling up these stars. Instead, the nebula's gas and dust are being used as raw ingredients to make new stars. However, the stars in IC 1590 are still plotting thei

PIX4617504

Comete Hale - Bopp et observers 01/04/1997 - Comet Hale - Bopp with observers 1 April 1997 - Two boys watch the Comete Hale - Bopp. Two boys watch comet Hale - Bopp on April 1st, 1997

Comete Hale - Bopp et observers 01/04/1997 - Comet Hale - Bopp with observers 1 April 1997 - Two boys watch the Comete Hale - Bopp. Two boys watch comet Hale - Bopp on April 1st, 1997

Jerry Lodriguss

PIX4569599

Constellations of Cassiopee, Persee - Cassiopeia, Perseus, Cepheus constellations - On the top right the constellation of Cephee, in the center of Cassiopee, below the left of the constellation Persee, on the bottom right, part of Andromede. Top right Cepheus constellation, in the middle Cassiopeia constellation, bottom right part of Andromeda, bottom left Perseus

Constellations of Cassiopee, Persee - Cassiopeia, Perseus, Cepheus constellations - On the top right the constellation of Cephee, in the center of Cassiopee, below the left of the constellation Persee, on the bottom right, part of Andromede. Top right Cepheus constellation, in the middle Cassiopeia constellation, bottom right part of Andromeda, bottom left Perseus

PIX4589673

Cassiopeia (colour litho)

Cassiopeia (colour litho)

European School, (19th century)

LLH5234695

Constellations of Cassiopee, Persee - Cassiopeia, Perseus, Cepheus constellations - On the top right the constellation of Cephee, in the center of Cassiopee, below the left of the constellation Persee, on the bottom right, part of Andromede. Top right Cepheus constellation, in the middle Cassiopeia constellation, bottom right part of Andromeda, bottom left Perseus

Constellations of Cassiopee, Persee - Cassiopeia, Perseus, Cepheus constellations - On the top right the constellation of Cephee, in the center of Cassiopee, below the left of the constellation Persee, on the bottom right, part of Andromede. Top right Cepheus constellation, in the middle Cassiopeia constellation, bottom right part of Andromeda, bottom left Perseus

PIX4589683

Bok's cells in NGC 281 (Cassiopee) - Bok globules in NGC 281 - View of a detail of the nebula NGC 281 in Cassiopee center on Bok's Globules. A Bok's blood cell is a dark interstellar cloud of gases and dust that absorb light. If it condenses enough, it gives birth to new stars. Near these blood cells shine blue stars; they belong to the young cluster of stars IC 1590. Image obtained by the Hubble Space Telescope in October 2005. These opaque, dark knots of gas and dust are called “” Bok globules,””” and they are absorbing light in the center of the nearby emission nebula and star - forming region. Bok hypothesized that giant molecular clouds, on the order of hundreds of light - years in size, can become perturbed and form small pockets where the dust and gas are highly concentrated. These small pockets become gravitationally bound and accumulate dust and gas from the surrounding area. If they can capture enough mass, they have the potential of creating stars in their cores; however, no

Bok's cells in NGC 281 (Cassiopee) - Bok globules in NGC 281 - View of a detail of the nebula NGC 281 in Cassiopee center on Bok's Globules. A Bok's blood cell is a dark interstellar cloud of gases and dust that absorb light. If it condenses enough, it gives birth to new stars. Near these blood cells shine blue stars; they belong to the young cluster of stars IC 1590. Image obtained by the Hubble Space Telescope in October 2005. These opaque, dark knots of gas and dust are called “” Bok globules,””” and they are absorbing light in the center of the nearby emission nebula and star - forming region. Bok hypothesized that giant molecular clouds, on the order of hundreds of light - years in size, can become perturbed and form small pockets where the dust and gas are highly concentrated. These small pockets become gravitationally bound and accumulate dust and gas from the surrounding area. If they can capture enough mass, they have the potential of creating stars in their cores; however, no

PIX4617491

Summer Sky, Cassiopee Constellation - Summer Starry Sky, constellation of Cassiopeia - To the north - east, the constellation Persee to the left of the tree; Cassiopee and its W shape is higher. Glue at the top right of the tree, the great galaxy of Andromede M 31. Then following the lactee route, the constellation of Cephee. August 18, 2009. Top left is Cepheus constellation with Lacerta to its right; in the middle Cassiopeia constellation, with the great galaxy of Andromeda to its right; bottom is Perseus. August 18, 2009

Summer Sky, Cassiopee Constellation - Summer Starry Sky, constellation of Cassiopeia - To the north - east, the constellation Persee to the left of the tree; Cassiopee and its W shape is higher. Glue at the top right of the tree, the great galaxy of Andromede M 31. Then following the lactee route, the constellation of Cephee. August 18, 2009. Top left is Cepheus constellation with Lacerta to its right; in the middle Cassiopeia constellation, with the great galaxy of Andromeda to its right; bottom is Perseus. August 18, 2009

Laurent Laveder

PIX4589688

Nebulas IC 1805 and IC 1848 in Cassiopee - Nebulas IC 1805 and IC 1848 in Cassiopeia - IC 1848 (left) is an emission nebula associated with a cluster of stars; it also houses the CR 34 star cluster. On the right, the largest nebula, IC 1805. LBN 667 is the large area of red emission nebulosity on the left side of the image. Open clusters CR 34 and IC 1848 are embedded in the nebula. IC 1805 is the large area of nebulosity on the right side of the image. NGC 896, a bright knot of nebulosity, is at the upper right of the photo. IC 1805 looks vaguely like a heart if you rotate your head 90 degrees counterclockwise and use your imagination when you look at the photo. The loose open cluster Mel 15 lies at the center of IC 1805, and open cluster NGC 1027 is just above right of the center of the image at top

Nebulas IC 1805 and IC 1848 in Cassiopee - Nebulas IC 1805 and IC 1848 in Cassiopeia - IC 1848 (left) is an emission nebula associated with a cluster of stars; it also houses the CR 34 star cluster. On the right, the largest nebula, IC 1805. LBN 667 is the large area of red emission nebulosity on the left side of the image. Open clusters CR 34 and IC 1848 are embedded in the nebula. IC 1805 is the large area of nebulosity on the right side of the image. NGC 896, a bright knot of nebulosity, is at the upper right of the photo. IC 1805 looks vaguely like a heart if you rotate your head 90 degrees counterclockwise and use your imagination when you look at the photo. The loose open cluster Mel 15 lies at the center of IC 1805, and open cluster NGC 1027 is just above right of the center of the image at top

Jerry Lodriguss

PIX4622386

False-colour image of supernova remnant Cassiopeia A in constellation Cassiopeia, 10,000 light-years away. It is the remnant of a once massive star that died in a supernova explosion. Credit NASA. Science Astronomy

False-colour image of supernova remnant Cassiopeia A in constellation Cassiopeia, 10,000 light-years away. It is the remnant of a once massive star that died in a supernova explosion. Credit NASA. Science Astronomy

UIG528814

Perseus and Adromeda (colour litho)

Perseus and Adromeda (colour litho)

Spence, Thomas Ralph (1848-1918)

LLM5998214

Lactee route between Cephee and Cassiopee - Cepheus to Cassiopeia - This rich area of the northern Milky Way stretches from Cepheus on the lower left to Cassiopeia on the upper right. Numerous bright red emission nebulas, dark nebulas and star clusters can be seen. The large emission nebula IC 1396 is in the lower left corner, next of Herschel's Garnet Star (Mu Cephei). Open cluster M52 and the Bubble Nebula, NGC 7635, are at the right center of the frame. At the lower right is a pair of large emission nebulas, CED 214 (Sh2-171) and NGC 7822. Large open cluster NGC 7789 is at the upper right corner, about two and a half degrees from Caph (Beta Cassiopeiae). Other red emission nebulas in the field are: Sh2-132, Sh2-142, Sh2-155 (the Cave Nebula), and Sh2-157

Lactee route between Cephee and Cassiopee - Cepheus to Cassiopeia - This rich area of the northern Milky Way stretches from Cepheus on the lower left to Cassiopeia on the upper right. Numerous bright red emission nebulas, dark nebulas and star clusters can be seen. The large emission nebula IC 1396 is in the lower left corner, next of Herschel's Garnet Star (Mu Cephei). Open cluster M52 and the Bubble Nebula, NGC 7635, are at the right center of the frame. At the lower right is a pair of large emission nebulas, CED 214 (Sh2-171) and NGC 7822. Large open cluster NGC 7789 is at the upper right corner, about two and a half degrees from Caph (Beta Cassiopeiae). Other red emission nebulas in the field are: Sh2-132, Sh2-142, Sh2-155 (the Cave Nebula), and Sh2-157

Jerry Lodriguss

PIX4636596

Constellations around Persee - Constellations around Perseus - Star sky photography on November 6, 2007. At the bottom of the picture is the planet Mars in the Gemels. Above it is the constellation of the Coach, then Persee, a part of Andromede with its left Cassiopee and its right, the Triangle. Starry sky on november 6 2007. Bottom is the bright planet Mars in Gemini; above it the constellation of Auriga, then Perseus, a part of Andromeda with on its left Cassiopeia and on its right Triangulum

Constellations around Persee - Constellations around Perseus - Star sky photography on November 6, 2007. At the bottom of the picture is the planet Mars in the Gemels. Above it is the constellation of the Coach, then Persee, a part of Andromede with its left Cassiopee and its right, the Triangle. Starry sky on november 6 2007. Bottom is the bright planet Mars in Gemini; above it the constellation of Auriga, then Perseus, a part of Andromeda with on its left Cassiopeia and on its right Triangulum

Laurent Laveder

PIX4593248

Constellations around Persee - Constellations around Perseus - Star sky photography on November 6, 2007. At the bottom of the picture is the planet Mars in the Gemels. above, the constellation of the Coach, then Persee, a part of Andromede with on its left Cassiopee and on its right, the Triangle. Starry sky on november 6 2007. Bottom is the bright planet Mars in Gemini; above it the constellation of Auriga, then Perseus, a part of Andromeda with on its left Cassiopeia and on its right Triangulum

Constellations around Persee - Constellations around Perseus - Star sky photography on November 6, 2007. At the bottom of the picture is the planet Mars in the Gemels. above, the constellation of the Coach, then Persee, a part of Andromede with on its left Cassiopee and on its right, the Triangle. Starry sky on november 6 2007. Bottom is the bright planet Mars in Gemini; above it the constellation of Auriga, then Perseus, a part of Andromeda with on its left Cassiopeia and on its right Triangulum

Laurent Laveder

PIX4593253

Constellations around Persee - Constellations around Perseus - Star sky photography on November 6, 2007. At the bottom of the picture is the planet Mars in the Gemels. Above it is the constellation of the Coach, then Persee, a part of Andromede with its left Cassiopee and its right, the Triangle. The constellations are traced and their Latin name is indicated. Starry sky on november 6 2007. Bottom is the bright planet Mars in Gemini; above it the constellation of Auriga, then Perseus, a part of Andromeda with on its left Cassiopeia and on its right Triangulum. Constellations are drawn with their latin names

Constellations around Persee - Constellations around Perseus - Star sky photography on November 6, 2007. At the bottom of the picture is the planet Mars in the Gemels. Above it is the constellation of the Coach, then Persee, a part of Andromede with its left Cassiopee and its right, the Triangle. The constellations are traced and their Latin name is indicated. Starry sky on november 6 2007. Bottom is the bright planet Mars in Gemini; above it the constellation of Auriga, then Perseus, a part of Andromeda with on its left Cassiopeia and on its right Triangulum. Constellations are drawn with their latin names

Laurent Laveder

PIX4593268

The Cassiopeia A supernova's first flash of radiation makes six clumps of dust (circled in annotated version) unusually hot. The supernova remnant is the large white ball in the center. This infrared picture was taken by NASA's Spitzer Space Telescope.

The Cassiopeia A supernova's first flash of radiation makes six clumps of dust (circled in annotated version) unusually hot. The supernova remnant is the large white ball in the center. This infrared picture was taken by NASA's Spitzer Space Telescope.

UIG867116

Cassiopeia and Cepheus (engraving)

Cassiopeia and Cepheus (engraving)

TRK3071533

This image from NASA's WISE shows the constellation Cassiopeia.

This image from NASA's WISE shows the constellation Cassiopeia.

UIG867182

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