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Images of 'Star Of David' found, 2,405

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Region near the Omega nebula (M17) in Sagittarius - Area near Omega nebula (M17) in Sagittarius - Region around the Omega nebula. Under the nebula, the cluster of stars M18, towards the middle, the group of stars M24, at the bottom of the picture the nebulae NGC 6589 - 90 and IC 1283 - 4. A little below the bright red emission nebula M17 is M18, a group of stars which is only conspicuous because, like M17, it is set in a relatively dark region of the Milky Way. The rich cloud of stars more or less in the middle of the photograph was listed by Messier as number 24 in his catalogue and it contains the open cluster NGC 6603, while towards the bottom of this field is a small group of nebulosities, the two blue reflection nebulae NGC 6589 - 90 and the emission nebulae IC 1283 - 4

Region near the Omega nebula (M17) in Sagittarius - Area near Omega nebula (M17) in Sagittarius - Region around the Omega nebula. Under the nebula, the cluster of stars M18, towards the middle, the group of stars M24, at the bottom of the picture the nebulae NGC 6589 - 90 and IC 1283 - 4. A little below the bright red emission nebula M17 is M18, a group of stars which is only conspicuous because, like M17, it is set in a relatively dark region of the Milky Way. The rich cloud of stars more or less in the middle of the photograph was listed by Messier as number 24 in his catalogue and it contains the open cluster NGC 6603, while towards the bottom of this field is a small group of nebulosities, the two blue reflection nebulae NGC 6589 - 90 and the emission nebulae IC 1283 - 4

PIX4620244

The Large Magellanic Cloud - The Large Magellanic Cloud - The Great Magellan Cloud galaxy is located about 160,000 light years away from Earth in the southern constellation of Dorado. Visible with the naked eye in the southern hemishere it is one of the closest galaxies to us. It contains large star-forming zones such as the Tarantula Nebula (30 Sea bream, visible to the left), the most active star-forming regions of the local group. Image obtained by the 1.2m UK Schmidt telescope from Siding Spring, Australia. The Large Magellanic Cloud (LMC) is the nearest galaxy to the Milky Way but less than one tenth as massive; even so it contains the equivalent of over ten billion solar masses of material in the form of stars, gas and dust. The LMC is at a distance of 160,000 light years and is visible to the unaided eye from southern latitudes, rather like a detached piece of the Milky Way. The nearness of the LMC ensures that it is well resolved into stars in quite a modest telescope, and deep

The Large Magellanic Cloud - The Large Magellanic Cloud - The Great Magellan Cloud galaxy is located about 160,000 light years away from Earth in the southern constellation of Dorado. Visible with the naked eye in the southern hemishere it is one of the closest galaxies to us. It contains large star-forming zones such as the Tarantula Nebula (30 Sea bream, visible to the left), the most active star-forming regions of the local group. Image obtained by the 1.2m UK Schmidt telescope from Siding Spring, Australia. The Large Magellanic Cloud (LMC) is the nearest galaxy to the Milky Way but less than one tenth as massive; even so it contains the equivalent of over ten billion solar masses of material in the form of stars, gas and dust. The LMC is at a distance of 160,000 light years and is visible to the unaided eye from southern latitudes, rather like a detached piece of the Milky Way. The nearness of the LMC ensures that it is well resolved into stars in quite a modest telescope, and deep

PIX4613427

Constellations of the Virgin, the Raven and the Cup - Constellations of Virgo, Corvus and Crate

Constellations of the Virgin, the Raven and the Cup - Constellations of Virgo, Corvus and Crate

PIX4594435

Constellations of Gemels and Little Dog - Constellations of Gemini and Canis Minor - Constellation of Gemels with bright stars Castor and Pollux. Below is the small constellation of the Little Dog, with the bright star Procyon. Canis Minor (the Lesser Dog) is sometimes regarded as the smaller of the two dogs of Orion the hunter. It is minor indeed, just 185 degrees square, and 71st in size of the 88 modern constellations. The most obvious and interesting object Canis Minor is its main star, the pale yellow Procyon. Its name is from the Greek, meaning 'before the dog', since it rises before the Sirius, the Dog Star. Gemini (the Twins) is a much more interesting collection of stars, easily visualised as two figures holding hands, their heads represented by the stars Castor and Pollux. The constellation is an ancient zodiacal construction, with a rich mythology vanishing in the mists of time. It is from the direction of Gemini (near Castor) that annual Geminid meteor showers radiate, arou

Constellations of Gemels and Little Dog - Constellations of Gemini and Canis Minor - Constellation of Gemels with bright stars Castor and Pollux. Below is the small constellation of the Little Dog, with the bright star Procyon. Canis Minor (the Lesser Dog) is sometimes regarded as the smaller of the two dogs of Orion the hunter. It is minor indeed, just 185 degrees square, and 71st in size of the 88 modern constellations. The most obvious and interesting object Canis Minor is its main star, the pale yellow Procyon. Its name is from the Greek, meaning 'before the dog', since it rises before the Sirius, the Dog Star. Gemini (the Twins) is a much more interesting collection of stars, easily visualised as two figures holding hands, their heads represented by the stars Castor and Pollux. The constellation is an ancient zodiacal construction, with a rich mythology vanishing in the mists of time. It is from the direction of Gemini (near Castor) that annual Geminid meteor showers radiate, arou

PIX4590692

Leo 1 dwarf galaxy in the Lion - Leo 1 dwarf galaxy - Leo 1 is located about 900,000 light years from Earth. It belongs to the local group, just like our galaxy or Andromede galaxy. It has only been known since the 1950s; it is difficult to observe due to the proximity of the Regulus star, thousands of times brighter. Image obtained from the 3.9m telescope of Siding Spring. The 'Local Group' of galaxies, to which the Milky Way belongs, contains more dwarf galaxies than any other type. The low surface brightness and lack of bright stars makes them difficult to study, even with a large telescope. Leo I presents particular problems because the galaxy appears only 20 arc minutes (less than the apparent diameter of the Moon) from the brilliant star Regulus and special precautions had to be taken to prevent scattered light from the star obliterating its feeble image. The plates from which this picture was made (the first in colour of a dwarf elliptical galaxy) will be used to learn more abou

Leo 1 dwarf galaxy in the Lion - Leo 1 dwarf galaxy - Leo 1 is located about 900,000 light years from Earth. It belongs to the local group, just like our galaxy or Andromede galaxy. It has only been known since the 1950s; it is difficult to observe due to the proximity of the Regulus star, thousands of times brighter. Image obtained from the 3.9m telescope of Siding Spring. The 'Local Group' of galaxies, to which the Milky Way belongs, contains more dwarf galaxies than any other type. The low surface brightness and lack of bright stars makes them difficult to study, even with a large telescope. Leo I presents particular problems because the galaxy appears only 20 arc minutes (less than the apparent diameter of the Moon) from the brilliant star Regulus and special precautions had to be taken to prevent scattered light from the star obliterating its feeble image. The plates from which this picture was made (the first in colour of a dwarf elliptical galaxy) will be used to learn more abou

PIX4613932

Spiral Galaxy M66 in the Lion - Spiral galaxy M66 in Leo - M 66 (NGC 3627) is a spiral galaxy located at a distance of about 35 million years - light. M66, with its neighbors M65 and NGC 3628, forms a remarkable triplet of galaxies, called the Lion Triplet or the M66 Group. Image obtained with Siding Spring's 3.9m telescope. M66 is a dusty spiral galaxy, and is a member of the same compact group of galaxies as M65 and NGC 3628. The striking symmetry of M65 is lacking, and the central bulge, though large, is less well defined. The spiral arms are very easy to see, but seem distorted and displaced above the plane of the galaxy, probably a result of interactions with its neighbours. Much more dust is visible here as well as a few pink nebulae, signs of star formation, near the end of one of the arms

Spiral Galaxy M66 in the Lion - Spiral galaxy M66 in Leo - M 66 (NGC 3627) is a spiral galaxy located at a distance of about 35 million years - light. M66, with its neighbors M65 and NGC 3628, forms a remarkable triplet of galaxies, called the Lion Triplet or the M66 Group. Image obtained with Siding Spring's 3.9m telescope. M66 is a dusty spiral galaxy, and is a member of the same compact group of galaxies as M65 and NGC 3628. The striking symmetry of M65 is lacking, and the central bulge, though large, is less well defined. The spiral arms are very easy to see, but seem distorted and displaced above the plane of the galaxy, probably a result of interactions with its neighbours. Much more dust is visible here as well as a few pink nebulae, signs of star formation, near the end of one of the arms

PIX4610845

Jupiter and Saturn in the Taurus 29/12/2000 - Jupiter and Saturn move into Taurus. 29 December 2000 - Winter sky with planets Jupiter and Saturn in the Taurus (middle right). Jupiter and Saturn move into Taurus, 1999-2000. 29 December 200

Jupiter and Saturn in the Taurus 29/12/2000 - Jupiter and Saturn move into Taurus. 29 December 2000 - Winter sky with planets Jupiter and Saturn in the Taurus (middle right). Jupiter and Saturn move into Taurus, 1999-2000. 29 December 200

PIX4587709

Dachau Concentration Camp. Jewish Memorial. Star of David. Germany.

Dachau Concentration Camp. Jewish Memorial. Star of David. Germany.

TRK832390

Constellations of Reticulum and Dorado - Constellations of Reticulum and Dorado - Constellations of Reticulum and Bream (top) near the galaxy of the Great Magellan Cloud. Reticulum is another small and insignificant southern constellation introduced by Lacaille in the 1750s. It commemorates a reticle, the cross hairs in an eyepiece used for measuring star positions, from the Latin for 'net' (hence reticulation, network). It is best found by looking for the Large Magellanic Cloud in the adjoining constellation of Dorado. Dorado, the Goldfish or Swordfish (Xiphias), is a constellation introduced by Johann Bayer, best known for his 1603 star atlas Uranometria, which was the first to cover the entire sky. It is notable mainly for containing most of the Large Magellanic Cloud (LMC), the nearest galaxy to the Milky Way

Constellations of Reticulum and Dorado - Constellations of Reticulum and Dorado - Constellations of Reticulum and Bream (top) near the galaxy of the Great Magellan Cloud. Reticulum is another small and insignificant southern constellation introduced by Lacaille in the 1750s. It commemorates a reticle, the cross hairs in an eyepiece used for measuring star positions, from the Latin for 'net' (hence reticulation, network). It is best found by looking for the Large Magellanic Cloud in the adjoining constellation of Dorado. Dorado, the Goldfish or Swordfish (Xiphias), is a constellation introduced by Johann Bayer, best known for his 1603 star atlas Uranometria, which was the first to cover the entire sky. It is notable mainly for containing most of the Large Magellanic Cloud (LMC), the nearest galaxy to the Milky Way

PIX4593553

Halley Comete and Lactee Way - Halley comet and milky way. April 1986 - View in April 1986 from the South Hemisphere

Halley Comete and Lactee Way - Halley comet and milky way. April 1986 - View in April 1986 from the South Hemisphere

PIX4569971

Constellations of Burin and Dove - Constellations of Caelum and Columba - Constellations of the southern hemisphere. Caelum (originally Caelum Sculptoris, the sculptor's chisel) is a small, rather obscure constallation hewn from rather thin pickings between Eridanus and Columba by Abbe de Lacaille in the 1750s. It is only 125 degrees square, making it 81st in area out of 88 constellations. Rather more interesting to the eye is Columba (originally Columba Noachi, Noah's dove) easily found between Sirius and Canopus. It is twice the area of Caelum and contans a few brighter stars. Best seen in the early evening in January

Constellations of Burin and Dove - Constellations of Caelum and Columba - Constellations of the southern hemisphere. Caelum (originally Caelum Sculptoris, the sculptor's chisel) is a small, rather obscure constallation hewn from rather thin pickings between Eridanus and Columba by Abbe de Lacaille in the 1750s. It is only 125 degrees square, making it 81st in area out of 88 constellations. Rather more interesting to the eye is Columba (originally Columba Noachi, Noah's dove) easily found between Sirius and Canopus. It is twice the area of Caelum and contans a few brighter stars. Best seen in the early evening in January

PIX4589365

Center of the Andromede Galaxy (M31) - Center of the Andromeda galaxy - The Andromede galaxy is located about 2 million years ago - light from Earth. Like the lactee path, the Andromede galaxy belongs to the local group. This image obtained from the 2.5m Isaac Newton telescope of La Palma shows the central region of the galaxy where a huge mass of stars is orbiting around the nucleus. This picture covers almost half a degree of sky (about the size of the full moon), but wide angle telescopes show the galaxy to be over three degrees long at its widest. Here we see only the central part of M31, the huge mass of stars that are in orbit around its nucleus. Silhouetted against this starry background are tangled sheets and curtains of dust, very reminiscent of dust clouds we see in our own galaxy. This picture was made from three black and white glass negatives. Some care has been taken to ensure that the colours seen here are realistic

Center of the Andromede Galaxy (M31) - Center of the Andromeda galaxy - The Andromede galaxy is located about 2 million years ago - light from Earth. Like the lactee path, the Andromede galaxy belongs to the local group. This image obtained from the 2.5m Isaac Newton telescope of La Palma shows the central region of the galaxy where a huge mass of stars is orbiting around the nucleus. This picture covers almost half a degree of sky (about the size of the full moon), but wide angle telescopes show the galaxy to be over three degrees long at its widest. Here we see only the central part of M31, the huge mass of stars that are in orbit around its nucleus. Silhouetted against this starry background are tangled sheets and curtains of dust, very reminiscent of dust clouds we see in our own galaxy. This picture was made from three black and white glass negatives. Some care has been taken to ensure that the colours seen here are realistic

PIX4608819

Stars Field in the Peacock - Random star field in Pavo, near NGC 6477 - Towards the middle of the picture, the cluster of galaxies IC 4765. Image obtained by Schmidt UK 1.2m Telescope from Siding Spring The brightest star visible here is the magnitude 4.2 variable blue star lambda Pav, visible to the unaided eye in a dark sky, while the scattering of stars in the lower part of the picture are about a magnitude fainter and would be hard to see in all but the darkest conditions. Near middle of the image, the cluster of galaxies IC 4765

Stars Field in the Peacock - Random star field in Pavo, near NGC 6477 - Towards the middle of the picture, the cluster of galaxies IC 4765. Image obtained by Schmidt UK 1.2m Telescope from Siding Spring The brightest star visible here is the magnitude 4.2 variable blue star lambda Pav, visible to the unaided eye in a dark sky, while the scattering of stars in the lower part of the picture are about a magnitude fainter and would be hard to see in all but the darkest conditions. Near middle of the image, the cluster of galaxies IC 4765

PIX4572367

Michael Bryant, Peter Wight and Richard Pasco

Michael Bryant, Peter Wight and Richard Pasco

John Haynes

HAS3795368

David Powell, Billie Burke, on-set of the Silent Film, "Gloria's Romance", 1916

David Powell, Billie Burke, on-set of the Silent Film, "Gloria's Romance", 1916

American Photographer, (20th century)

GLH1273490

Yom Kippur, illustration for “Lights on” by Bella Chagall, 1945

Yom Kippur, illustration for “Lights on” by Bella Chagall, 1945

Chagall, Marc (1887-1985)

IMJ408259

Comet Bennett - 1970 - Comet Bennett. 1970 - Comet Bennett, 1969Y1. 197

Comet Bennett - 1970 - Comet Bennett. 1970 - Comet Bennett, 1969Y1. 197

PIX4569580

Constellation of the Great Bear and Arcturus - Polaris, the Big Dipper, Arcturus and Spica - View of the Great Bear with on its left the star Arcturus du Bouvier. Also visible are the polar star and the Little Bear and the Spica star near the horizon

Constellation of the Great Bear and Arcturus - Polaris, the Big Dipper, Arcturus and Spica - View of the Great Bear with on its left the star Arcturus du Bouvier. Also visible are the polar star and the Little Bear and the Spica star near the horizon

PIX4591384

From Golus to Zion by E. M. Lilies, 1901 (b/w photo)

From Golus to Zion by E. M. Lilies, 1901 (b/w photo)

Lilien, Ephraim Moses (1874-1925)

SZT6362691

Peacock Constellation - Constellation of Pavo - Pavo, the Peacock, lies south of Sagittarius and Corona Australis, and is one of Johann Bayer's twelve constellations, introduced in 1603. It is one of several birds in the southern sky, including Apus, Grus, Phoenix and Tucanae. The legends say that the goddess of the heavens, Juno (the Greek Hera) ordered a hundred - eyed giant, Argos Panoptes, to keep his eyes on her wandering husband, Jupiter. He ordered Argos slain and Juno transformed the 100 eyes into the Peacock's tail. These eyes are also meant to represent the starry sky

Peacock Constellation - Constellation of Pavo - Pavo, the Peacock, lies south of Sagittarius and Corona Australis, and is one of Johann Bayer's twelve constellations, introduced in 1603. It is one of several birds in the southern sky, including Apus, Grus, Phoenix and Tucanae. The legends say that the goddess of the heavens, Juno (the Greek Hera) ordered a hundred - eyed giant, Argos Panoptes, to keep his eyes on her wandering husband, Jupiter. He ordered Argos slain and Juno transformed the 100 eyes into the Peacock's tail. These eyes are also meant to represent the starry sky

PIX4593107

Halley Comete - Halley's Comet on December 9, 1985 - Halley Comete December 9, 1985

Halley Comete - Halley's Comet on December 9, 1985 - Halley Comete December 9, 1985

PIX4569993

Constellation Scorpio - Constellation of Scorpiu

Constellation Scorpio - Constellation of Scorpiu

PIX4593725

The Milky Way, looking towards the Galactic Centre - The Milky Way, looking towards the Galactic Centre - The bright point at the bottom left is Jupiter Planet The Milky Way is best seen on winter nights (May to August) from the southern hemisphere. This wide-angle picture shows a broad span of the southern Milky Way and is a photograph made using colour film in a conventional camera. The camera which was pointed towards the centre of our Galaxy, in the direction of the constellation of Sagittarius. The Galactic centre itself is totally hidden at visible wavelengths by the band of dust which divides the Milky Way along much of its length. The dust lane is only visible because it blots out background stars. Embedded in the dust are many star-forming regions, seen as bright red emission nebulae. The brightest, left of the centre of the picture, is Messier 8, the Lagoon Nebula, which is visible to the unaided eye. The bright 'star' at lower left is the planet Jupiter

The Milky Way, looking towards the Galactic Centre - The Milky Way, looking towards the Galactic Centre - The bright point at the bottom left is Jupiter Planet The Milky Way is best seen on winter nights (May to August) from the southern hemisphere. This wide-angle picture shows a broad span of the southern Milky Way and is a photograph made using colour film in a conventional camera. The camera which was pointed towards the centre of our Galaxy, in the direction of the constellation of Sagittarius. The Galactic centre itself is totally hidden at visible wavelengths by the band of dust which divides the Milky Way along much of its length. The dust lane is only visible because it blots out background stars. Embedded in the dust are many star-forming regions, seen as bright red emission nebulae. The brightest, left of the centre of the picture, is Messier 8, the Lagoon Nebula, which is visible to the unaided eye. The bright 'star' at lower left is the planet Jupiter

PIX4637870

Constellation of the Dolphin - Constellation of Delphinus - Constellations of the Dolphin and Altair. On the top right, the constellation of the Fleche, on the left, the Dolphin; on the bottom right, the brilliant star Altair in the Eagle. Delphinus the Dolphin looks remarkably like the creature it represents. Delphinus is a small constellation of Greek origin, but despite its diminutive size it is quite easy to find. The bright star Altair in neighboring Aquila is probably the best guide. Delphinus' brightest star, Rotanev (ss Del) is of magnitude 4, and its name honors the astronomer Nicolaus Venator (Rotonov backwards). The next brightest star in Delphinus is Sualocin, which at first glance appears English, but is Nicolaus spelled backwards. He was assistant to the rather more famous Italian astronomer Giuseppe Piazzi. The main stars of Sagitta are also well seen here

Constellation of the Dolphin - Constellation of Delphinus - Constellations of the Dolphin and Altair. On the top right, the constellation of the Fleche, on the left, the Dolphin; on the bottom right, the brilliant star Altair in the Eagle. Delphinus the Dolphin looks remarkably like the creature it represents. Delphinus is a small constellation of Greek origin, but despite its diminutive size it is quite easy to find. The bright star Altair in neighboring Aquila is probably the best guide. Delphinus' brightest star, Rotanev (ss Del) is of magnitude 4, and its name honors the astronomer Nicolaus Venator (Rotonov backwards). The next brightest star in Delphinus is Sualocin, which at first glance appears English, but is Nicolaus spelled backwards. He was assistant to the rather more famous Italian astronomer Giuseppe Piazzi. The main stars of Sagitta are also well seen here

PIX4590467

Constellation Lizard - Constellation of Lacerta - Lacerta (the Lizard) was a constellation invented by the Polish astronomer Johannes Hevelius in 1687. It lies boxed in on all sides by the much more interesting groupings of Cygnus, Cephus, Pegasus and Andromeda. Lacerta had no bright stars or significant deep sky objects apart from 14th magnitude star - like object BL Lac, a prototype of an unusal kind of active galaxy whose nucleus varies in brightness by a few magnitudes over several days

Constellation Lizard - Constellation of Lacerta - Lacerta (the Lizard) was a constellation invented by the Polish astronomer Johannes Hevelius in 1687. It lies boxed in on all sides by the much more interesting groupings of Cygnus, Cephus, Pegasus and Andromeda. Lacerta had no bright stars or significant deep sky objects apart from 14th magnitude star - like object BL Lac, a prototype of an unusal kind of active galaxy whose nucleus varies in brightness by a few magnitudes over several days

PIX4591879

Planetary nebula NGC 6781 - A planetary nebula, NGC 6781 - This fairly inconspicuous planetary nebula is in Aquila and it marks the end of the long life of a sun - like star. Despite the longevity of their parent stars and the very brief lifetime of the nebula (typically less than 100,000 years) such sights are common because sun - like stars are common. The nebula has nothing to do with planet formation, indeed the formation of the nebula would effectively destroy any planets the parent star had, rather the name refers to the telescopic appearance of the nebula. Some planetaries are very bright and their discs look like solar system planets. A close look at this picture shows some structure in the expanding shell of gas around the star, reminiscent of the much more complex Helix nebula. The nebula we see is the ejected surface of the star expanding into material left from an earlier stage in its decline, when it briefly expanded as a 'red giant'. Irregularities in the earlier ejecta,

Planetary nebula NGC 6781 - A planetary nebula, NGC 6781 - This fairly inconspicuous planetary nebula is in Aquila and it marks the end of the long life of a sun - like star. Despite the longevity of their parent stars and the very brief lifetime of the nebula (typically less than 100,000 years) such sights are common because sun - like stars are common. The nebula has nothing to do with planet formation, indeed the formation of the nebula would effectively destroy any planets the parent star had, rather the name refers to the telescopic appearance of the nebula. Some planetaries are very bright and their discs look like solar system planets. A close look at this picture shows some structure in the expanding shell of gas around the star, reminiscent of the much more complex Helix nebula. The nebula we see is the ejected surface of the star expanding into material left from an earlier stage in its decline, when it briefly expanded as a 'red giant'. Irregularities in the earlier ejecta,

PIX4623396

Barree spiral galaxy NGC 1300 in Eridan - NGC 1300, barred spiral galaxy in Eridanus - The galaxy NGC 1300 is located about 60 million years ago - light and extends over about 85 000 years - light. Spiral galaxies appear in a variety of guises, but none are more intriguing than the barred variety. As their name suggests, these galaxies are distinguished by a bar, extending (in this case) like two more of less straight assemblies of stars either side of the bright nucleus. Caught up in the bar are two dust lanes, emerging on either side of the nuclear mass. At some distance from the nucleus, the straight, almost structurreless bar and dust lanes abruptly turn at a sharp angle. It is here that the delicately curved arms of the spiral begin, and it is here that star formation is at its most concentrated. Many spirals have such bars, including the Milky Way, where it is a subtle feature, very difficult to detect. NGC 1300, in the southern constellation of Eridanus is among the finest examp

Barree spiral galaxy NGC 1300 in Eridan - NGC 1300, barred spiral galaxy in Eridanus - The galaxy NGC 1300 is located about 60 million years ago - light and extends over about 85 000 years - light. Spiral galaxies appear in a variety of guises, but none are more intriguing than the barred variety. As their name suggests, these galaxies are distinguished by a bar, extending (in this case) like two more of less straight assemblies of stars either side of the bright nucleus. Caught up in the bar are two dust lanes, emerging on either side of the nuclear mass. At some distance from the nucleus, the straight, almost structurreless bar and dust lanes abruptly turn at a sharp angle. It is here that the delicately curved arms of the spiral begin, and it is here that star formation is at its most concentrated. Many spirals have such bars, including the Milky Way, where it is a subtle feature, very difficult to detect. NGC 1300, in the southern constellation of Eridanus is among the finest examp

PIX4609731

Halley Comete - Halley's Comet, March 12 1986 - Halley Comet, March 12, 1986

Halley Comete - Halley's Comet, March 12 1986 - Halley Comet, March 12, 1986

PIX4569994

Milky way and winter hexagon - The winter hexagon is an asterism formed by the stars Sirius, Procyon, Pollux, Capella, Aldebaran and Rigel. Winter hexagon is composed by bright stars Sirius, Procyon, Pollux, Capella, Aldebaran and Rigel

Milky way and winter hexagon - The winter hexagon is an asterism formed by the stars Sirius, Procyon, Pollux, Capella, Aldebaran and Rigel. Winter hexagon is composed by bright stars Sirius, Procyon, Pollux, Capella, Aldebaran and Rigel

PIX4593038

Milky way and winter hexagon - The winter hexagon is an asterism formed by the stars Sirius, Procyon, Pollux, Capella, Aldebaran and Rigel. Winter hexagon is composed by bright stars Sirius, Procyon, Pollux, Capella, Aldebaran and Rigel

Milky way and winter hexagon - The winter hexagon is an asterism formed by the stars Sirius, Procyon, Pollux, Capella, Aldebaran and Rigel. Winter hexagon is composed by bright stars Sirius, Procyon, Pollux, Capella, Aldebaran and Rigel

PIX4593062

Constellations of Gemels and Little Dog - Constellations of Gemini and Canis Minor - Constellation of Gemels with bright stars Castor and Pollux. Below is the small constellation of the Little Dog, with the bright star Procyon. Canis Minor (the Lesser Dog) is sometimes regarded as the smaller of the two dogs of Orion the hunter. It is minor indeed, just 185 degrees square, and 71st in size of the 88 modern constellations. The most obvious and interesting object Canis Minor is its main star, the pale yellow Procyon. Its name is from the Greek, meaning 'before the dog', since it rises before the Sirius, the Dog Star. Gemini (the Twins) is a much more interesting collection of stars, easily visualised as two figures holding hands, their heads represented by the stars Castor and Pollux. The constellation is an ancient zodiacal construction, with a rich mythology vanishing in the mists of time. It is from the direction of Gemini (near Castor) that annual Geminid meteor showers radiate, arou

Constellations of Gemels and Little Dog - Constellations of Gemini and Canis Minor - Constellation of Gemels with bright stars Castor and Pollux. Below is the small constellation of the Little Dog, with the bright star Procyon. Canis Minor (the Lesser Dog) is sometimes regarded as the smaller of the two dogs of Orion the hunter. It is minor indeed, just 185 degrees square, and 71st in size of the 88 modern constellations. The most obvious and interesting object Canis Minor is its main star, the pale yellow Procyon. Its name is from the Greek, meaning 'before the dog', since it rises before the Sirius, the Dog Star. Gemini (the Twins) is a much more interesting collection of stars, easily visualised as two figures holding hands, their heads represented by the stars Castor and Pollux. The constellation is an ancient zodiacal construction, with a rich mythology vanishing in the mists of time. It is from the direction of Gemini (near Castor) that annual Geminid meteor showers radiate, arou

PIX4590674

Remains of the supernova of the Sails - Detail - Vela supernova remnant. Detail - Detail of the rest of the supernova of the Sails. The supernova exploded 12,000 years ago. A supernova event marks the catastrophic end - point in the life of a massive star. The self - destruction of the star releases a huge amount of energy as radiation of all kinds, but a substantial fraction of the force of the explosion blasts the outer part of the supernova into an expanding shell of matter that travels through the almost empty space between the stars. As the rapidly moving blast wave encounters the relatively stationary interstellar medium it creates a very narrow, luminous shock front that appears as a faint nebula. Because the shock front is very convoluted the nebulosity appears to be highly structured and the various colours define different energy levels within the interaction. Although the star responsible for the Vela supernova remnant exploded 12,000 years ago, it is still affecting its env

Remains of the supernova of the Sails - Detail - Vela supernova remnant. Detail - Detail of the rest of the supernova of the Sails. The supernova exploded 12,000 years ago. A supernova event marks the catastrophic end - point in the life of a massive star. The self - destruction of the star releases a huge amount of energy as radiation of all kinds, but a substantial fraction of the force of the explosion blasts the outer part of the supernova into an expanding shell of matter that travels through the almost empty space between the stars. As the rapidly moving blast wave encounters the relatively stationary interstellar medium it creates a very narrow, luminous shock front that appears as a faint nebula. Because the shock front is very convoluted the nebulosity appears to be highly structured and the various colours define different energy levels within the interaction. Although the star responsible for the Vela supernova remnant exploded 12,000 years ago, it is still affecting its env

PIX4582820

Constellation of Circinus and southern constellations - Constellation of Circinus and southern constellations - The Southern Triangle constellations, the Fly, and the Southern Cross are also visible. Circinus (the drawing Comppass) is an inconspicuous constellation introduced by the French astronomer Nicolas Louis de Lacaille, who observed the southern sky from the Cape of Good Hope between 1750 and 1754. He named 14 constellations, many of them associated with science or navigation, such as Microscopium and Telescopium, Octans the Octant and Antlia Pneumatica, the air pump. Circinus contains no bright or named stars and covers 93 square degrees, making it the fourth - smallest. Triangulum Australe is the southern hemisphere counterpart of Triangulum. It is a bigger constellation and contains brighter stars than Triangulum and it never sets for most of Australia. Its brightest star is named Atria (for alpha Trianguli Australis), in the manner of Acrux in the Southern Cross. It is easil

Constellation of Circinus and southern constellations - Constellation of Circinus and southern constellations - The Southern Triangle constellations, the Fly, and the Southern Cross are also visible. Circinus (the drawing Comppass) is an inconspicuous constellation introduced by the French astronomer Nicolas Louis de Lacaille, who observed the southern sky from the Cape of Good Hope between 1750 and 1754. He named 14 constellations, many of them associated with science or navigation, such as Microscopium and Telescopium, Octans the Octant and Antlia Pneumatica, the air pump. Circinus contains no bright or named stars and covers 93 square degrees, making it the fourth - smallest. Triangulum Australe is the southern hemisphere counterpart of Triangulum. It is a bigger constellation and contains brighter stars than Triangulum and it never sets for most of Australia. Its brightest star is named Atria (for alpha Trianguli Australis), in the manner of Acrux in the Southern Cross. It is easil

PIX4590041

Galaxy NGC 891 in Andromede - Edge - on spiral galaxy NGC 891 in Andromeda - Spiral galaxy seen by the slice located at a distance of 10 million years - light.. This image obtained with the 2.5m Isaac Newton telescope of La Palma. If we could view the Milky Way from a distance of about 30 million light years it would look something like NGC 891. But galaxies that look like this are quite rare because the chance alignment of the thin disk of a spiral galaxy with our line of sight is unusual. A few degrees either side of its orientation and NGC 891 would be just another highly inclined spiral galaxy. From this unusual vantage point we can see in NGC 891 the surprising narrowness of the obscuring dust lane, a dark, slightly irregular band across the galaxy. We also see that it is yellowish, confirming that it is dust, which absorbs blue light, as in the Milky Way. Also similar to the Milky Way is the prominent central 'bulge' corresponding to the rich star clouds in Sagittarius. However,

Galaxy NGC 891 in Andromede - Edge - on spiral galaxy NGC 891 in Andromeda - Spiral galaxy seen by the slice located at a distance of 10 million years - light.. This image obtained with the 2.5m Isaac Newton telescope of La Palma. If we could view the Milky Way from a distance of about 30 million light years it would look something like NGC 891. But galaxies that look like this are quite rare because the chance alignment of the thin disk of a spiral galaxy with our line of sight is unusual. A few degrees either side of its orientation and NGC 891 would be just another highly inclined spiral galaxy. From this unusual vantage point we can see in NGC 891 the surprising narrowness of the obscuring dust lane, a dark, slightly irregular band across the galaxy. We also see that it is yellowish, confirming that it is dust, which absorbs blue light, as in the Milky Way. Also similar to the Milky Way is the prominent central 'bulge' corresponding to the rich star clouds in Sagittarius. However,

PIX4609481

Planetary nebula NGC 1360 in the Furnace - NGC 1360, the diffuse planetary nebula in Fornax - Image obtained by Siding Spring Planetary nebulae 3.9m telescope usually have well - defined boundaries, sometimes even a shell - like structure. For reasons that are not understood, NGC 1360 defies all these conventions, yet its colour still clearly identifies it as a planetary nebula. The green hue is oxygen, excited by the hot central star, and to the north - east of the nebula is a faint red smudge, probably traces of material ejected before the star became a true planetary nebula

Planetary nebula NGC 1360 in the Furnace - NGC 1360, the diffuse planetary nebula in Fornax - Image obtained by Siding Spring Planetary nebulae 3.9m telescope usually have well - defined boundaries, sometimes even a shell - like structure. For reasons that are not understood, NGC 1360 defies all these conventions, yet its colour still clearly identifies it as a planetary nebula. The green hue is oxygen, excited by the hot central star, and to the north - east of the nebula is a faint red smudge, probably traces of material ejected before the star became a true planetary nebula

PIX4622912

David Bowie, right hand panel of Diptych, 2000 (oil on canvas) (see 181145)

premium — David Bowie, right hand panel of Diptych, 2000 (oil on canvas) (see 181145)

David Bowie, right hand panel of Diptych, 2000 (oil on canvas) (see 181145)

SFI181146

Jews in France, 1942 (b/w photo)

Jews in France, 1942 (b/w photo)

SZT3010346

Constellation of the Dolphin - Constellation of Delphinus - Constellations of the Dolphin and Altair. On the top right, the constellation of the Fleche, on the left, the Dolphin; on the bottom right, the brilliant star Altair in the Eagle. Delphinus the Dolphin looks remarkably like the creature it represents. Delphinus is a small constellation of Greek origin, but despite its diminutive size it is quite easy to find. The bright star Altair in neighboring Aquila is probably the best guide. Delphinus' brightest star, Rotanev (ss Del) is of magnitude 4, and its name honors the astronomer Nicolaus Venator (Rotonov backwards). The next brightest star in Delphinus is Sualocin, which at first glance appears English, but is Nicolaus spelled backwards. He was assistant to the rather more famous Italian astronomer Giuseppe Piazzi. The main stars of Sagitta are also well seen here

Constellation of the Dolphin - Constellation of Delphinus - Constellations of the Dolphin and Altair. On the top right, the constellation of the Fleche, on the left, the Dolphin; on the bottom right, the brilliant star Altair in the Eagle. Delphinus the Dolphin looks remarkably like the creature it represents. Delphinus is a small constellation of Greek origin, but despite its diminutive size it is quite easy to find. The bright star Altair in neighboring Aquila is probably the best guide. Delphinus' brightest star, Rotanev (ss Del) is of magnitude 4, and its name honors the astronomer Nicolaus Venator (Rotonov backwards). The next brightest star in Delphinus is Sualocin, which at first glance appears English, but is Nicolaus spelled backwards. He was assistant to the rather more famous Italian astronomer Giuseppe Piazzi. The main stars of Sagitta are also well seen here

PIX4590492

Remnants of the Supernova of Sails - Part of the Vela Supernova Remnant - Rest of the Supernova of Sails. The supernova exploded 12,000 years ago and is approximately 815 light years away from Earth. Image obtained with the 1.2m Schmidt UK Telescope from Siding Spring. About 120 centuries ago an inconspicuous star in what is now the constellation of Vela brightened by about 100 million times to rival the Moon as the brightest object in the night sky. This photograph shows a portion of the north - western quadrant of an expanding nebulous shell, which now surrounds the site of the explosion. Near the centre of the nebula (and not seen here) is the Vela pulsar, a rapidly - spinning neutron star only a few kilometres in diameter, the remnant of the star that exploded. This tiny object spins about 11 times a second and until recently was among the faintest stars ever studied at optical wavelengths, a far cry from its brief glory as one of the brightest stars ever seen

Remnants of the Supernova of Sails - Part of the Vela Supernova Remnant - Rest of the Supernova of Sails. The supernova exploded 12,000 years ago and is approximately 815 light years away from Earth. Image obtained with the 1.2m Schmidt UK Telescope from Siding Spring. About 120 centuries ago an inconspicuous star in what is now the constellation of Vela brightened by about 100 million times to rival the Moon as the brightest object in the night sky. This photograph shows a portion of the north - western quadrant of an expanding nebulous shell, which now surrounds the site of the explosion. Near the centre of the nebula (and not seen here) is the Vela pulsar, a rapidly - spinning neutron star only a few kilometres in diameter, the remnant of the star that exploded. This tiny object spins about 11 times a second and until recently was among the faintest stars ever studied at optical wavelengths, a far cry from its brief glory as one of the brightest stars ever seen

PIX4582860

Comete Hale - Bopp et aurore boreale - April 1997 - Comet Hale - Bopp and aurora borealis 04/1997 - Comet Hale - Bopp 1996 O1 (1 April 1997) Comet Hale - Bopp aurorae and wooden house, photographed from Canada

Comete Hale - Bopp et aurore boreale - April 1997 - Comet Hale - Bopp and aurora borealis 04/1997 - Comet Hale - Bopp 1996 O1 (1 April 1997) Comet Hale - Bopp aurorae and wooden house, photographed from Canada

PIX4569839

Constellations of the Virgin, the Raven and the Cup - Constellations of Virgo, Corvus and Crate

Constellations of the Virgin, the Raven and the Cup - Constellations of Virgo, Corvus and Crate

PIX4594443

Constellation Constellation of Auriga - The brightest star in the constellation is Capella. Auriga (the Charioteer) is one of 48 constellations (out of the current 88) that were noted by Ptolemy (83 - 161 CE). It represents a chariot and its driver, a shepherd, with a goat or a sheep over his shoulder. The brightest star in Auriga is Capella, which is the ancient Greek word for little goat. It is a binary star 42 light years distant and is about 75 times more luminous than the Sun. Surprisingly, Capella is one of only two conspicuous stars whose combined light is similar to that of the Sun (the other is Alpha Centauri), so appears white on this photograph. Sun - like stars are common but are generally too faint to be seen at a distance which is why there are so few visible to the eye. Best seen in the early evening in February

Constellation Constellation of Auriga - The brightest star in the constellation is Capella. Auriga (the Charioteer) is one of 48 constellations (out of the current 88) that were noted by Ptolemy (83 - 161 CE). It represents a chariot and its driver, a shepherd, with a goat or a sheep over his shoulder. The brightest star in Auriga is Capella, which is the ancient Greek word for little goat. It is a binary star 42 light years distant and is about 75 times more luminous than the Sun. Surprisingly, Capella is one of only two conspicuous stars whose combined light is similar to that of the Sun (the other is Alpha Centauri), so appears white on this photograph. Sun - like stars are common but are generally too faint to be seen at a distance which is why there are so few visible to the eye. Best seen in the early evening in February

PIX4589985

Constellation Constellation of Auriga - The brightest star in the constellation is Capella. Auriga (the Charioteer) is one of 48 constellations (out of the current 88) that were noted by Ptolemy (83 - 161 CE). It represents a chariot and its driver, a shepherd, with a goat or a sheep over his shoulder. The brightest star in Auriga is Capella, which is the ancient Greek word for little goat. It is a binary star 42 light years distant and is about 75 times more luminous than the Sun. Surprisingly, Capella is one of only two conspicuous stars whose combined light is similar to that of the Sun (the other is Alpha Centauri), so appears white on this photograph. Sun - like stars are common but are generally too faint to be seen at a distance which is why there are so few visible to the eye. Best seen in the early evening in February

Constellation Constellation of Auriga - The brightest star in the constellation is Capella. Auriga (the Charioteer) is one of 48 constellations (out of the current 88) that were noted by Ptolemy (83 - 161 CE). It represents a chariot and its driver, a shepherd, with a goat or a sheep over his shoulder. The brightest star in Auriga is Capella, which is the ancient Greek word for little goat. It is a binary star 42 light years distant and is about 75 times more luminous than the Sun. Surprisingly, Capella is one of only two conspicuous stars whose combined light is similar to that of the Sun (the other is Alpha Centauri), so appears white on this photograph. Sun - like stars are common but are generally too faint to be seen at a distance which is why there are so few visible to the eye. Best seen in the early evening in February

PIX4589984

Spiral galaxy of Sombrero M104 in the Virgin - The Sombrero galaxy (M104) in Virgo - Image of the spiral galaxy M104 (Sombrero galaxy), located about 28 million years ago - light. Image obtained with the 3.9m Anglo - Australian Telescope from Siding Spring. The Sombrero, named after the broad - brimmed Mexican hat it superficially resembles, is probably the most famous galaxy in the sky. The light from this remarkable spiral system is dominated by the billions of old, faint stars that form the vast 'bulge' around its tiny hidden nucleus. Most spirals, including the Milky Way, have clouds of old, faint stars around their nuclei, but in M104 the galaxy's light is dominated by them. This effect is enhanced because disk of the galaxy is seen nearly edge - on and dust in its outer parts is in silhouette as it crosses the picture. The galaxy is about 28 million light years distant

Spiral galaxy of Sombrero M104 in the Virgin - The Sombrero galaxy (M104) in Virgo - Image of the spiral galaxy M104 (Sombrero galaxy), located about 28 million years ago - light. Image obtained with the 3.9m Anglo - Australian Telescope from Siding Spring. The Sombrero, named after the broad - brimmed Mexican hat it superficially resembles, is probably the most famous galaxy in the sky. The light from this remarkable spiral system is dominated by the billions of old, faint stars that form the vast 'bulge' around its tiny hidden nucleus. Most spirals, including the Milky Way, have clouds of old, faint stars around their nuclei, but in M104 the galaxy's light is dominated by them. This effect is enhanced because disk of the galaxy is seen nearly edge - on and dust in its outer parts is in silhouette as it crosses the picture. The galaxy is about 28 million light years distant

PIX4611600

Nebulae NGC 1973 - 1975 - 1977 in Orion - The reflection nebulae NGC 1973 - 75 - 77 in Orion - Reflection nebulae located just north of the Great Orion Nebula. This group of nebulous stars is just half a degree north of the much brighter Orion Nebula and has largely been ignored because of it. The group of stars here appear as a single star to the unaided eye, the northernmost 'star' in the sword of Orion. Most of the blue nebulosity is starlight scattered by dust, while some of the stars are sufficiently hot to excite the wisps of hydrogen that linger here and create a distinctive red glow

Nebulae NGC 1973 - 1975 - 1977 in Orion - The reflection nebulae NGC 1973 - 75 - 77 in Orion - Reflection nebulae located just north of the Great Orion Nebula. This group of nebulous stars is just half a degree north of the much brighter Orion Nebula and has largely been ignored because of it. The group of stars here appear as a single star to the unaided eye, the northernmost 'star' in the sword of Orion. Most of the blue nebulosity is starlight scattered by dust, while some of the stars are sufficiently hot to excite the wisps of hydrogen that linger here and create a distinctive red glow

PIX4618057

Constellations of Andromede and Cassiopee - Andromeda and Cassiopeia constellation

Constellations of Andromede and Cassiopee - Andromeda and Cassiopeia constellation

PIX4588892

Constellation of the Altar - Constellations of Ara, Norma and Telescopium - The Altar is a constellation of the southern hemisphere located between the Centaur and the Wolf. Also visible are the constellations of the Rule and the Telescope. Ara (the Altar) is an inconspicuous constellation in the southern sky. It was once considered part of Centaurus and Lupus but became separated when the 'modern' constellation Norma was created by Lacaille in the 1750s. It was recognised by the Greeks and Romans and was visualised as the altar on which the Centaur, Centaurus, was to sacrifice Lupus, the Wolf. This is reflected in its Latin name, Ara Centauri. The constellation is the 63rd largest in the sky and covers about 237 square degrees. The best - known objects in this field are some diffuse dusty nebulae and star clusters. The only named star in Ara is Karnot Mizbeach (ss Ara). Best seen in the early evening in July

Constellation of the Altar - Constellations of Ara, Norma and Telescopium - The Altar is a constellation of the southern hemisphere located between the Centaur and the Wolf. Also visible are the constellations of the Rule and the Telescope. Ara (the Altar) is an inconspicuous constellation in the southern sky. It was once considered part of Centaurus and Lupus but became separated when the 'modern' constellation Norma was created by Lacaille in the 1750s. It was recognised by the Greeks and Romans and was visualised as the altar on which the Centaur, Centaurus, was to sacrifice Lupus, the Wolf. This is reflected in its Latin name, Ara Centauri. The constellation is the 63rd largest in the sky and covers about 237 square degrees. The best - known objects in this field are some diffuse dusty nebulae and star clusters. The only named star in Ara is Karnot Mizbeach (ss Ara). Best seen in the early evening in July

PIX4589021

Planetary Nebula of the Red Rectangle in the Unicorn - The Red Rectangle, AFGL 915 - This planetary nebula is located about 2300 years ago - light. Image from Siding Spring 3.9m Telescope This surprising object is one of an unusual class of nebulae surrounding mature, sun - like stars that are about to turn into planetary nebulae. Not all pre - planetary nebulae have outbursts like this, and in those that do, the nebula lasts only a few thousand years, hence the rarity. The central star has a thick belt of dust like a girdle around its equator which restricts outflow in that direction. Instead, the star ejects material in a kind of cone from each of its poles. The spectrum of the nebula shows unusual, strong red lines from hydrogen bonded to grains of carbon, however there is sufficient light reflected from the embedded star to dilute the strong red spectrum to the deep yellow we see here

Planetary Nebula of the Red Rectangle in the Unicorn - The Red Rectangle, AFGL 915 - This planetary nebula is located about 2300 years ago - light. Image from Siding Spring 3.9m Telescope This surprising object is one of an unusual class of nebulae surrounding mature, sun - like stars that are about to turn into planetary nebulae. Not all pre - planetary nebulae have outbursts like this, and in those that do, the nebula lasts only a few thousand years, hence the rarity. The central star has a thick belt of dust like a girdle around its equator which restricts outflow in that direction. Instead, the star ejects material in a kind of cone from each of its poles. The spectrum of the nebula shows unusual, strong red lines from hydrogen bonded to grains of carbon, however there is sufficient light reflected from the embedded star to dilute the strong red spectrum to the deep yellow we see here

PIX4623779

Star worn by Jewish prisoners. Germany.

Star worn by Jewish prisoners. Germany.

DPA2487760

Orion Constellation - Constellation of Orion - Orion the Hunter is one of the most familar and best known constellations. There is extensive and varied mythology about this beautiful collection of stars, but the most common Greek legend has Orion as a giant huntsman, and he appears in this role in Homer's Odyssey. The most persistent legend seems to be that he died from the sting of a giant scorpion, which was placed in the sky so that Orion sets as the Scorpius rises, in an eternal chase across the sky. The momorable outline of the Hunter proudly bestrides the celestial equator and is equally visible from both hemispheres. The distinctive, equally spaced line of stars of Orion's Belt are more or less on the equator and are framed by quartet of bright and colourful stars. More subtle is Orions short sword, hanging from his belt. Under dark skies or in binoculars the central 'star' is distinctly misty. This is the famous Orion nebula, one of many well known telescopic objects that fill

Orion Constellation - Constellation of Orion - Orion the Hunter is one of the most familar and best known constellations. There is extensive and varied mythology about this beautiful collection of stars, but the most common Greek legend has Orion as a giant huntsman, and he appears in this role in Homer's Odyssey. The most persistent legend seems to be that he died from the sting of a giant scorpion, which was placed in the sky so that Orion sets as the Scorpius rises, in an eternal chase across the sky. The momorable outline of the Hunter proudly bestrides the celestial equator and is equally visible from both hemispheres. The distinctive, equally spaced line of stars of Orion's Belt are more or less on the equator and are framed by quartet of bright and colourful stars. More subtle is Orions short sword, hanging from his belt. Under dark skies or in binoculars the central 'star' is distinctly misty. This is the famous Orion nebula, one of many well known telescopic objects that fill

PIX4592404

Constellations of Ophiuchus and Snake - Ophiuchus and Serpens constellation

Constellations of Ophiuchus and Snake - Ophiuchus and Serpens constellation

PIX4592344

Michael Bryant & Richard Pasco

Michael Bryant & Richard Pasco

John Haynes

HAS3795371

Constellations of Reticulum and Dorado - Constellations of Reticulum and Dorado - Constellations of Reticulum and Bream (top) near the galaxy of the Great Magellan Cloud. Reticulum is another small and insignificant southern constellation introduced by Lacaille in the 1750s. It commemorates a reticle, the cross hairs in an eyepiece used for measuring star positions, from the Latin for 'net' (hence reticulation, network). It is best found by looking for the Large Magellanic Cloud in the adjoining constellation of Dorado. Dorado, the Goldfish or Swordfish (Xiphias), is a constellation introduced by Johann Bayer, best known for his 1603 star atlas Uranometria, which was the first to cover the entire sky. It is notable mainly for containing most of the Large Magellanic Cloud (LMC), the nearest galaxy to the Milky Way

Constellations of Reticulum and Dorado - Constellations of Reticulum and Dorado - Constellations of Reticulum and Bream (top) near the galaxy of the Great Magellan Cloud. Reticulum is another small and insignificant southern constellation introduced by Lacaille in the 1750s. It commemorates a reticle, the cross hairs in an eyepiece used for measuring star positions, from the Latin for 'net' (hence reticulation, network). It is best found by looking for the Large Magellanic Cloud in the adjoining constellation of Dorado. Dorado, the Goldfish or Swordfish (Xiphias), is a constellation introduced by Johann Bayer, best known for his 1603 star atlas Uranometria, which was the first to cover the entire sky. It is notable mainly for containing most of the Large Magellanic Cloud (LMC), the nearest galaxy to the Milky Way

PIX4593550

Comete McNaught 01/2007 - Comet McNaught 01/2007 - View of the McNaught comet obtained on January 19, 2007 from Australia. Chiro Observatory - Western Australia. Comet McNaught as seen from Chiro Observatory, W. Australia. Jan 19 2007

Comete McNaught 01/2007 - Comet McNaught 01/2007 - View of the McNaught comet obtained on January 19, 2007 from Australia. Chiro Observatory - Western Australia. Comet McNaught as seen from Chiro Observatory, W. Australia. Jan 19 2007

PIX4570772

Constellations of the Little Lion and the Lion - Constellations of Leo Minor and Leo - Leo Minor the lesser Lion, is a constellation of the northern Spring and was created by Johannes Hevelius (1611 - 1687), first published in his 1690 atlas Firmamentum Sobiescianum. He is believed to have named the star 46 Leonis Minoris 'Praecipua' because it was the principal star in his new and not very distictive constellation, which at 232 square degrees is 64th largest. Leo Minor is due north of the distinctive sickle shape in Leo, and south of the hind leg of Ursa Major, 'The Great Bear'

Constellations of the Little Lion and the Lion - Constellations of Leo Minor and Leo - Leo Minor the lesser Lion, is a constellation of the northern Spring and was created by Johannes Hevelius (1611 - 1687), first published in his 1690 atlas Firmamentum Sobiescianum. He is believed to have named the star 46 Leonis Minoris 'Praecipua' because it was the principal star in his new and not very distictive constellation, which at 232 square degrees is 64th largest. Leo Minor is due north of the distinctive sickle shape in Leo, and south of the hind leg of Ursa Major, 'The Great Bear'

PIX4593329

Crown Constellation Boreale - Constellation of Corona borealis - Corona Borealis, the Northern Crown, is a small but distinctive constellation in the northern sky, and was one of the 48 listed by Ptolemy that are still recognised today. In mythology it may have represented the crown given by Dionysus (or Bacchus) to Ariane, or belonged to Booetes

Crown Constellation Boreale - Constellation of Corona borealis - Corona Borealis, the Northern Crown, is a small but distinctive constellation in the northern sky, and was one of the 48 listed by Ptolemy that are still recognised today. In mythology it may have represented the crown given by Dionysus (or Bacchus) to Ariane, or belonged to Booetes

PIX4590139

Barree spiral galaxy M95 in the Lion - Barred spiral galaxy M95 in Leo - M95 (NGC 3351), is a barree spiral of type SBB. It belongs to the Leo I galaxy group, also known as the M96 group. It also contains M96, M105 and a number of weaker galaxies. This galaxy is located about 38 million light years away from Earth. The SBB barred spiral galaxy M95, is a member of the Leo I galaxy grouping, which includes M96 and M105 as well as various other galaxies, all at a distance of about 37 million light - years

Barree spiral galaxy M95 in the Lion - Barred spiral galaxy M95 in Leo - M95 (NGC 3351), is a barree spiral of type SBB. It belongs to the Leo I galaxy group, also known as the M96 group. It also contains M96, M105 and a number of weaker galaxies. This galaxy is located about 38 million light years away from Earth. The SBB barred spiral galaxy M95, is a member of the Leo I galaxy grouping, which includes M96 and M105 as well as various other galaxies, all at a distance of about 37 million light - years

PIX4610635

Constellation of the Great Dog - Constellation of Canis Major - Sirius, the bright star on this image is the brightest star in the sky. Canis Major (the Greater Dog) is one of two dogs accompanying Orion the hunter across the sky. The other is Canis Minor. The constellation figure is ancient, and was one of 48 constellations mentioned by Ptolemy (83 - 161 AD), no doubt reflecting earlier ideas. The modern stick figure joining the brightest stars (above) certainly has a very doggy appearance. The brightest star in the sky is here, Sirius, the Dog Star, so called because its emanations were thought to affect dogs in the heat of summer, the 'Dog Days' when the star is in the same part of the sky as the Sun. Sirius is bright because it is only 8.6 light years from the Sun and it is in any case it is an intrinsically bright star, 25 times more luminous than the Sun

Constellation of the Great Dog - Constellation of Canis Major - Sirius, the bright star on this image is the brightest star in the sky. Canis Major (the Greater Dog) is one of two dogs accompanying Orion the hunter across the sky. The other is Canis Minor. The constellation figure is ancient, and was one of 48 constellations mentioned by Ptolemy (83 - 161 AD), no doubt reflecting earlier ideas. The modern stick figure joining the brightest stars (above) certainly has a very doggy appearance. The brightest star in the sky is here, Sirius, the Dog Star, so called because its emanations were thought to affect dogs in the heat of summer, the 'Dog Days' when the star is in the same part of the sky as the Sun. Sirius is bright because it is only 8.6 light years from the Sun and it is in any case it is an intrinsically bright star, 25 times more luminous than the Sun

PIX4590972

Constellations of Grus and Piscis Austrinus - The Crane is a constellation in the southern hemisphere, located just below the Southern Fish. Grus (the Crane) is meant to represent a water bird, which may be a crane or perhaps a flamingo. This stellar grouping was introduced by Johann Bayer in his star atlas of 1603. Because of its location in the southern sky it is not visible from north latitudes above 40 degrees. Even if it were visible, it would hardly be remarked upon. Piscis Austrinus (the Southern Fish) once included Grus, and nowadays represents the Southern Fish, drinking from the water poured by Aquarius, adjoining it to the north. Piscis Austrinus was one of Ptolemy's 48 constellations and its brightest star is Fomalhaut, a name drived from the English for fish's mouth

Constellations of Grus and Piscis Austrinus - The Crane is a constellation in the southern hemisphere, located just below the Southern Fish. Grus (the Crane) is meant to represent a water bird, which may be a crane or perhaps a flamingo. This stellar grouping was introduced by Johann Bayer in his star atlas of 1603. Because of its location in the southern sky it is not visible from north latitudes above 40 degrees. Even if it were visible, it would hardly be remarked upon. Piscis Austrinus (the Southern Fish) once included Grus, and nowadays represents the Southern Fish, drinking from the water poured by Aquarius, adjoining it to the north. Piscis Austrinus was one of Ptolemy's 48 constellations and its brightest star is Fomalhaut, a name drived from the English for fish's mouth

PIX4591663

Orion Constellation - Constellation of Orion - Orion the Hunter is one of the most familar and best known constellations. There is extensive and varied mythology about this beautiful collection of stars, but the most common Greek legend has Orion as a giant huntsman, and he appears in this role in Homer's Odyssey. The most persistent legend seems to be that he died from the sting of a giant scorpion, which was placed in the sky so that Orion sets as the Scorpius rises, in an eternal chase across the sky. The momorable outline of the Hunter proudly bestrides the celestial equator and is equally visible from both hemispheres. The distinctive, equally spaced line of stars of Orion's Belt are more or less on the equator and are framed by quartet of bright and colourful stars. More subtle is Orions short sword, hanging from his belt. Under dark skies or in binoculars the central 'star' is distinctly misty. This is the famous Orion nebula, one of many well known telescopic objects that fill

Orion Constellation - Constellation of Orion - Orion the Hunter is one of the most familar and best known constellations. There is extensive and varied mythology about this beautiful collection of stars, but the most common Greek legend has Orion as a giant huntsman, and he appears in this role in Homer's Odyssey. The most persistent legend seems to be that he died from the sting of a giant scorpion, which was placed in the sky so that Orion sets as the Scorpius rises, in an eternal chase across the sky. The momorable outline of the Hunter proudly bestrides the celestial equator and is equally visible from both hemispheres. The distinctive, equally spaced line of stars of Orion's Belt are more or less on the equator and are framed by quartet of bright and colourful stars. More subtle is Orions short sword, hanging from his belt. Under dark skies or in binoculars the central 'star' is distinctly misty. This is the famous Orion nebula, one of many well known telescopic objects that fill

PIX4592500

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