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'Cepheus' Bilder und Clips Suchergebnisse page 1 of 2

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Bilder zu 'Cepheus' gefunden, 116

Stars for November as shown in 1923
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  • Content within this photograph may require additional clearances (eg: trademark and personality rights) depending on Licensee's specific use of material, which may include book and magazine cover use.
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
The constellation of Cepheus, 1488
Open cluster NGC 7142 in Cephee - Open cluster NGC 7142 in Cepheu
Constellation of Cephee - Constellation of Cepheu
Cassiopeia and Cepheus (engraving)
Variable star PV Cephei and nebula Gyulbudagyan - Variable star PV Cephei with Gyulbudagyan's nebula - PV Cephei is an excessively fast variable star, moving almost 20 km per second in the interstellar medium. This young star, formed about 500,000 years ago, is now more than 30 years ago - light from its birthplace, the cluster of stars of the Iris nebula, NGC 7023. PV Cephei is the small orange star with a gas cloud located in the upper left middle of the image. Image obtained on October 19, 2008 with a telescope measuring 61 cm in diameter. PV Cephei is a variable star moving at roughly 20 km/sec through the interstellar medium. This young star was formed about 500,000 years ago and is located now at about 30 light years from its birth place, the star cluster of Iris nebula (NGC 7023). PV Cephei is the small oranged star visible near the middle of the image, at right of the brilliant blue star. It is associated with a small cloud of gas. Image taken on October 19 2008 with a 24 - inch telescope
Open cluster NGC 7762 in Cephee - Open cluster NGC 7762 in Cepheu
Comete Panstarrs C/2011 L4 and Gamma Cephei - Comete PanStarrs (C/2011 L4) near the star Gamma Cephei (the brightest star at the top left), May 12, 2013. Due to the precession of equinoxes, Gamma Cephei (Errai) will indicate the northern Celestial pole in a few thousand years. Image taken on May 12 2013, when this comet developed a very interesting fan-shaped tail. The bright star in the image is Gamma Cephei, aka Errai. Due to the precession of the equinoxes, Gamma Cephei will be our next bright northern pole star, in a couple thousand years
VDB 149 nebula in Cephee - VDB 149 is a reflexion nebula
Constellation of Cephee - Constellation of Cepheu
Open cluster NGC 7510 in Cephee - Open cluster NGC 7510 in Cepheu
Open cluster NGC 6939 and galaxy NGC 6946 - Spiral galaxy NGC 6946 and open cluster NGC 6939 - The spiral galaxy NGC 6946 is located about 10 million years ago - light in Cephee. Many star formations are observed here. The cluster of stars NGC 6939, on the right, belongs to our galaxy. Spiral Galaxy NGC 6946 and Open Cluster NGC 6939 are located about 2 degrees southwest of Eta Cepheus. 6946 is a 9.7 magnitude spiral galaxy that was discovered by William Herschel on September 9, 1798 and is about 10 arc minutes in diameter. It is a relatively close galaxy at a distance of about 10 million light years, and was once suspected by Edwin Hubble of being a member of the Local Group of galaxies that includes the Milky Way, but today it is not believed to be a member. Because we are looking at it through the plane of our own galaxy, it is highly obscured by dust. NGC 6946 is sometimes called the Fireworks galaxy because of the number of supernovae that have been discovered there and the galaxy's prodigious rate of star formation. By contrast, open cluster NGC 6939, seen about 40 arc minutes northwest of NGC 6946, is located inside of our own galaxy at a distance of approximately 36 light years. It is just by coincidence that these two objects lie close to each other in the same line of sight
Nebulae NGC 7023 and VDB 141 in Cephee - Iris Nebula and Ghost nebula in Cepheus - The nebula of the Iris (NGC 7023) is a reflexion nebula illuminated by the star HD 200775. VDB 141, lower left, is a reflexion nebula illuminated by young stars. The bright star HD 200775 shining through the nebula NGC 7023 is a 10 solar mass star centrally imbedded in a region surrounded by ambient molecular cloud material. Bottom left is the reflection nebula VDB 141, the Ghost nebula illuminated by young stars
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
Nebula NGC 7129 in Cephee - Reflection nebula NGC 7129 in Cepheus - Nebula by reflexion located 3300 years - light of the Earth. This nebula houses very young stars, aged less than a million years old. NGC 7129 is a star forming region located in Cepheus constellation, 3300 light years from us. Several Herbig Haro objects are visible in this nebula. Herbig - Haro objects are small emission nebulae found around young developing stars (protostars) and which are believed to be transient in their nature, for they only exist for a few thousand years
Nebula NGC 7023 in Cephee - NGC 7023 (The Iris Nebula) in Cepheus - The Iris Nebula (NGC 7023) is a reflexion nebula illuminated by the massive star HD 200775. The bright star HD 200775 shining through the nebula NGC 7023 is a 10 solar mass star centrally imbedded in a region surrounded by ambient molecular cloud material. Suns are born from vast clouds of dust and gas that gather in the dark places between the stars. Gravity causes these interstellar vapors to collapse inward until the pressure causes high enough temperatures at its center to fuse hydrogen, the university's basic building block, into helium - an event that also releases gamma - ray photons. These photons can take a million years to travel outward through the overlying matter until they reach the surface and escape into space as visible light. The push of the photon's rush to make an exit also stops the cloud's collapse and thus what began as thin gas and dust becomes a brilliant star illuminating the heavens and possibly warming near - by planets. This picture shows a place in deep space where these kinds of events have occurred. The brilliant star near the center of the picture is young and very hot - in relative terms, it was only recently created. The cloud from which it formed still surrounds this young Sun but is being blown away by the push of star's massive radiation. This picture shows the way it looked 1,300 years ago due to the distance that separates it from Earth and the speed that light travels
Elephant tube nebula (VDB 142) in Cephee - The Elephant Trunk Nebula (VDB 142) in Cepheus - IC1396, VDB 142. Nebula located about 2700 years - light from Earth. Image obtained with a telescope 61 cm in diameter. The Elephant Trunk Nebula (IC 1396A) in Cepheus is part of the larger IC 1396 complex which spans a large area of the sky measuring 170 by 140 arc - minutes and is one of the brightest emission nebulae with a magnitude of 3.5. The western portion of IC 1396 contains the Elephant Trunk Nebula (IC 1396A) which is characterized with H - II emissions, dark lanes and globules as well as a small reflection nebula. This stellar nursery lies at a distance of 2,720 light - years away. Image taken with a 24 - inch telescope
Dust in Iris Nebula - Dust in Iris Nebula - The Iris Nebula (NGC 7023) is a reflexion nebula illuminated by the star HD 200775. This image obtained by the Hubble Space Telescope shows a detail of the nebula or HD star 200775 (at the top of the image, out of the field) illuminates tiny particles of dust. This close - up of an area in the northwest region of the large Iris Nebula (NGC 7023) seems to be clogged with cosmic dust. With bright light from the nearby star HD 200775 illuminating it from above, the dust resemble thick mounds of billowing cotton. It is actually made up of tiny particles of solid matter, with sizes from ten to a hundred times smaller than those of the dust grains we find at home. Both background and foreground stars are dotted throughout the image. North is down, East is right. The field of view is 3.3 arcminutes. The image is a composite of four images obtained by the Hubble space Telescope through blue, green, near - infrared and H - alpha filters
Nebula NGC 7023 in Cephee - Iris Nebula in Cepheus - The nebula of the Iris (NGC 7023) is a reflexion nebula illuminated by the star HD 200775. Infrared observations indicate that this nebula contains PAH (aromatic polycyclic hydrocarbons), molecules composed of carbon atoms and hydrogen. NGC 7023 (The Iris Nebula) is located 1400 Light Years away. The bright star HD 200775 shining through the nebula NGC 7023 is a 10 solar mass star centrally imbedded in a region surrounded by ambient molecular cloud material. Infrared observations indicate that this nebula may contain complex carbon molecules known as PaHS
Elephant tube nebula (VDB 142) in Cephee - The Elephant Trunk Nebula (VDB 142) in Cepheus - IC1396, VDB 142. Nebula located about 2700 years - light from Earth. Image obtained with a telescope 40 cm in diameter, through 3 different filters that highlight oxygen, hydrogen, and sulfur. The Elephant Trunk Nebula (IC 1396A) in Cepheus is part of the larger IC 1396 complex which spans a large area of the sky measuring 170 by 140 arc - minutes and is one of the brightest emission nebulae with a magnitude of 3.5. The western portion of IC 1396 contains the Elephant Trunk Nebula (IC 1396A) which is characterized with H - II emissions, dark lanes and globules as well as a small reflection nebula. The IC 1396 complex is technically a star cluster (aka Cr 439, Trumpler 37) owing to the presence of a developing open but loose cluster at the heart of this rich nebulosity. This open star cluster is comprised of 50 - 100 member stars which vary in brightness spanning an area of approximately 50 'in diameter and which are not very well detached from the background sky. This stellar nursery lies at a distance of 2,720 light - years away. Image taken with a 16 inch telescope in combining the light from 3 different filters tracing emission from oxygen, hydrogen, and sulphur
Sharpless - 136: 'Ghost' in Cepheus, 2011 (digital photo)
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Cepheus. Marginal drawings of animals. Illustrations to a treatise on astrology
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Constellations of Cassiopeia (Cassiopee) and Cepheus (Cephee). Engraving. Colored.
Nebula NGC 7129 in Cephee: Nebula by reflexion located 3300 light years from Earth. This nebula houses very young stars, aged less than a million years old. - NGC 7129 is a young compact star forming region which displays an unusual patchwork of colorful nebulosity and bright stars contrasted against the dust clouds of the Milky Way. NGC 7129 contains several bright reflection nebulae including the large blue reflection cloud NGC 7133 and the unusual small yellow reflection cloud LBN497. Also conspicuous in the field are several bright Herbig-Haro objects, the signatures of young stellar objects soon to emerge in the main sequence. The dominant blue reflection nebula, NGC 7133 is illuminated by two young B-type stars BD+65* 1637 and BD+65* 1638. Both stars are less than one million years old and represent the core of NGC 7129, a small cluster of low mass stars which populate the 36 light year wide cavity
Elephant tube nebula (VDB 142) in Cephee - The Elephant Trunk Nebula (VDB 142) in Cepheus: IC1396, VDB 142. Nebula located about 2700 light years from Earth. Image obtained with a bezel Tele Vue NP127iS, through 3 different filters that demonstrate oxygen, hydrogen, and sulfur - The Elephant Trunk Nebula (IC 1396A) in Cepheus is part of the larger IC 1396 complex which spans a large area of the sky measuring 170 by 140 arc-minutes and is one of the brightest emission nebulae with a magnitude of 3.5. The western portion of IC 1396 contains the Elephant Trunk Nebula (IC 1396A) which is characterized with H-II emissions, dark lanes and globules as well as a small reflection nebula. The IC 1396 complex is technically a star cluster (aka Cr 439, Trumpler 37) owing to the presence of a developing open but loose cluster at the heart of this rich nebulosity. This open star cluster is comprised of 50-100 member stars which vary in brightness spanning an area of approximately 50 'in diameter and which are not very well detached from the background sky. This stellar nursery lies at a distance of 2,720 light-years away - Image taken in combining the light from 3 different filters tracing emission from oxygen, hydrogen, and sulphur
Elephant tube nebula (VDB 142) in Cephee - The Elephant Trunk Nebula (VDB 142) in Cepheus - IC1396, VDB 142. Nebula located about 2700 years - light from Earth. The Elephant Trunk Nebula (IC 1396A) in Cepheus is part of the larger IC 1396 complex which spans a large area of the sky measuring 170 by 140 arc - minutes and is one of the brightest emission nebulae with a magnitude of 3.5. The western portion of IC 1396 contains the Elephant Trunk Nebula (IC 1396A) which is characterized with H - II emissions, dark lanes and globules as well as a small reflection nebula. The IC 1396 complex is technically a star cluster (aka Cr 439, Trumpler 37) owing to the presence of a developing open but loose cluster at the heart of this rich nebulosity. This open star cluster is comprised of 50 - 100 member stars which vary in brightness spanning an area of approximately 50 'in diameter and which are not very well detached from the background sky. This stellar nursery lies at a distance of 2,720 light - years away
Nebulae B175 and VDB 152 in Cephee - Dark nebula B175 and reflection nebula VDB 152 - Located about 1400 years ago - light in the constellation Cephee, a large dust trail leads to a bluish nebula. This is the dark nebula, Barnard 175, which faces the nebula by reflexion VDB 152 (Ced 201). The reflection nebula vdB 152 is really very faint. It lies about 1400 light - years away, along the northern Milky Way in the constellation Cepheus. Near the edge of a large molecular cloud, pockets of cosmic dust in the region block light from background stars or scatter light from the embedded bright star (top) giving parts of the nebula a characteristic blue color. Ultraviolet light from the star is also thought to cause a dim reddish luminescence in the nebular dust. Although stars do form in molecular clouds, this star seems to have only accidentally wandered into the area, as its measured velocity through interstellar space is very different from the cloud's velocity
Nebula NGC 7129 in Cephee - Grand Champ - Nebula NGC 7129 in Cepheus - Wide field - Nebula reflexion located 3300 years - light of the Earth. This nebula houses very young stars, aged less than a million years old. NGC 7129 is a young compact star forming region which displays an unusual patchwork of colorful nebulosity and bright stars contrasted against the dust clouds of the Milky Way. NGC 7129 contains several bright reflection nebulae including the large blue reflection cloud NGC 7133 and the unusual small yellow reflection cloud LBN 497. The dominant blue reflection nebula, NGC 7133 is illuminated by two young B - type stars BD+65* 1637 and BD+65* 1638. Both stars are less than one million years old and represent the core of NGC 7129, a small cluster of low mass stars which populate the 36 light year wide cavity
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
Perseus and Andromeda
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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
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
North celestial pole and circumpolar constellations - North celestial pole and circumpolar constellations - The northern celestial pole is marked by the polar star of the Little Bear. Around, the so-called circumpolar constellations with from top to bottom: The Great Bear on the left, the Dragon that encircles the Little Bear, Cephee below and the Swan on its right, then Cassiopee snaps everything against a big rock. May 20, 2007, Ploumanach (Cotes d'Armor - France). Pole star Polaris (near the center of the image) and circumpolar constellations; from left to right and top to bottom: Big Dipper, Draco with Little Dipper, Cygnus, Cepheus and Cassiopeia. May 20, 2007, Ploumanach (Cotes d'Armor - France)
North celestial pole and circumpolar constellations - North celestial pole and circumpolar constellations - The northern celestial pole is marked by the polar star of the Little Bear. Around, the so-called circumpolar constellations with from top to bottom: The Great Bear on the left, the Dragon that encircles the Little Bear, Cephee below and the Swan on its right, then Cassiopee snaps everything against a big rock. In overprint, the mythological forms of these constellations, extracted from the Uranographia of Hevelius. May 20, 2007, Ploumanach (Cotes d'Armor - France). Pole star Polaris (near the center of the image) and circumpolar constellations; from left to right and top to bottom: Big Dipper, Draco with Little Dipper, Cygnus, Cepheus and Cassiopeia. Constellation mythological forms from “” Uranographia”” star atlas by Hevelius (1690) have been added. May 20, 2007, Ploumanach (Cotes d'Armor - France)