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Images of 'Great Centre' found, 4,056

 
Andromede and Triangle Constellations - Constellations of Andromeda and Triangulum - The constellation of Andromede begins at the brilliant star Alpheratz, or Alpha Andromedae, one of the corners of the great square of Pegase. Alpheratz is the brightest star in the picture, on the right, and is located about 97 light years away from Earth. Mirach star, in the center of the image, is a giant red star situated about 200 years ago - light. The galaxy of Andromede, M31, is visible at the top of the picture. At the bottom of the mage, in the middle, the galaxy M33. The large open cluster NGC 752 is at the bottom left. The constellations of Andromeda, the Princess, and Triangulum, the Triangle, point the way to several deep - sky delights in the fall sky. Andromeda begins at the bright star Alpheratz, or Alpha Andromedae, one of the corners of the great square of Pegasus. Alpheratz is the brightest star in the image, near the right side of the frame and is located about 97 light years away f

Jerry Lodriguss

PIX4588973

Andromede and Triangle Constellations - Constellations of Andromeda and Triangulum - The constellation of Andromede begins at the brilliant star Alpheratz, or Alpha Andromedae, one of the corners of the great square of Pegase. Alpheratz is the brightest star in the picture, on the right, and is located about 97 light years away from Earth. Mirach star, in the center of the image, is a giant red star situated about 200 years ago - light. The galaxy of Andromede, M31, is visible at the top of the picture. At the bottom of the mage, in the middle, the galaxy M33. The large open cluster NGC 752 is at the bottom left. The constellations of Andromeda, the Princess, and Triangulum, the Triangle, point the way to several deep - sky delights in the fall sky. Andromeda begins at the bright star Alpheratz, or Alpha Andromedae, one of the corners of the great square of Pegasus. Alpheratz is the brightest star in the image, near the right side of the frame and is located about 97 light years away f

Jerry Lodriguss

PIX4588973

 
Visible Crab Nebula - Infrared and X - The Crab Nebula - M1, the Crab Nebula, is the rest of a supernova that exploded on July 4, 1054. It is located about 7000 light years from Earth in the constellation Taurus. At the heart of this nebula is a pulsar. To obtain this photo, three spatial observatories combined their observations: the Hubble telescope for the visible part (here in red and yellow), the Chandra telescope for the X-ray data (blue) and the Spitzer telescope for the infrared image (purple). The pulsar is the bright spot in the center of the image. The Crab Nebula (M1) is a supernova remnant at about 7,000 light - year from Earth in the constellation Taurus. The star explosion occured on July 04 1054. At the center of this nebula lies a pulsar. This composite image uses data from three of Nasa's Great Observatories. The Chandra X - ray image is shown in blue, the Hubble Space Telescope optical images are in red and yellow, and the Spitzer Space Telescope's infrared image is

PIX4583130

Visible Crab Nebula - Infrared and X - The Crab Nebula - M1, the Crab Nebula, is the rest of a supernova that exploded on July 4, 1054. It is located about 7000 light years from Earth in the constellation Taurus. At the heart of this nebula is a pulsar. To obtain this photo, three spatial observatories combined their observations: the Hubble telescope for the visible part (here in red and yellow), the Chandra telescope for the X-ray data (blue) and the Spitzer telescope for the infrared image (purple). The pulsar is the bright spot in the center of the image. The Crab Nebula (M1) is a supernova remnant at about 7,000 light - year from Earth in the constellation Taurus. The star explosion occured on July 04 1054. At the center of this nebula lies a pulsar. This composite image uses data from three of Nasa's Great Observatories. The Chandra X - ray image is shown in blue, the Hubble Space Telescope optical images are in red and yellow, and the Spitzer Space Telescope's infrared image is

PIX4583130

 
Spiral Galaxy M31 in Andromede - Spiral galaxy M31 in Andromeda - The galaxy of Andromede is located about 2 million years ago - light from Earth. Two satellite galaxies accompany it: M32 (NGC 221) at the top center, and M110 (NGC 205) at the bottom. Like the lactee path, the Andromede galaxy belongs to the local group, making up about thirty galaxies. Image obtained with an apochromatic bezel Televue 127is. 22 hours of laying. M31, the Great galaxy in Andromeda, is a gigantic collection of more than 300 billion stars and is located about 2 million light years from Earth. Companion dwarf elliptical galaxies M32 and M110 are also visible. M31 and its companions are part of our local group of galaxies, which includes the Milky Way and Magellanic Clouds, and M33. The Andromeda Galaxy is headed towards our Milky Way Galaxy and is expected to collide with it and possibly merge into a gigantic elliptical galaxy in about 3 billion years

PIX4608828

Spiral Galaxy M31 in Andromede - Spiral galaxy M31 in Andromeda - The galaxy of Andromede is located about 2 million years ago - light from Earth. Two satellite galaxies accompany it: M32 (NGC 221) at the top center, and M110 (NGC 205) at the bottom. Like the lactee path, the Andromede galaxy belongs to the local group, making up about thirty galaxies. Image obtained with an apochromatic bezel Televue 127is. 22 hours of laying. M31, the Great galaxy in Andromeda, is a gigantic collection of more than 300 billion stars and is located about 2 million light years from Earth. Companion dwarf elliptical galaxies M32 and M110 are also visible. M31 and its companions are part of our local group of galaxies, which includes the Milky Way and Magellanic Clouds, and M33. The Andromeda Galaxy is headed towards our Milky Way Galaxy and is expected to collide with it and possibly merge into a gigantic elliptical galaxy in about 3 billion years

PIX4608828

 
Andromede and Triangle Constellations - Constellations of Andromeda and Triangulum - The constellation of Andromede begins at the brilliant star Alpheratz, or Alpha Andromedae, one of the corners of the great square of Pegase. Alpheratz is the brightest star in the picture, on the right, and is located about 97 light years away from Earth. Mirach star, in the center of the image, is a giant red star situated about 200 years ago - light. The galaxy of Andromede, M31, is visible at the top of the picture. At the bottom of the mage, in the middle, the galaxy M33. The large open cluster NGC 752 is at the bottom left. The constellations of Andromeda, the Princess, and Triangulum, the Triangle, point the way to several deep - sky delights in the fall sky. Andromeda begins at the bright star Alpheratz, or Alpha Andromedae, one of the corners of the great square of Pegasus. Alpheratz is the brightest star in the image, near the right side of the frame and is located about 97 light years away f

Jerry Lodriguss

PIX4588980

Andromede and Triangle Constellations - Constellations of Andromeda and Triangulum - The constellation of Andromede begins at the brilliant star Alpheratz, or Alpha Andromedae, one of the corners of the great square of Pegase. Alpheratz is the brightest star in the picture, on the right, and is located about 97 light years away from Earth. Mirach star, in the center of the image, is a giant red star situated about 200 years ago - light. The galaxy of Andromede, M31, is visible at the top of the picture. At the bottom of the mage, in the middle, the galaxy M33. The large open cluster NGC 752 is at the bottom left. The constellations of Andromeda, the Princess, and Triangulum, the Triangle, point the way to several deep - sky delights in the fall sky. Andromeda begins at the bright star Alpheratz, or Alpha Andromedae, one of the corners of the great square of Pegasus. Alpheratz is the brightest star in the image, near the right side of the frame and is located about 97 light years away f

Jerry Lodriguss

PIX4588980

 
Spiral Galaxy M31 in Andromede - Spiral galaxy M31 in Andromeda - The galaxy of Andromede is located about 2 million years ago - light from Earth. Two satellite galaxies accompany it: M32 (NGC 221) in the center left, and M110 (NGC 205) below. Like the lactee path, the Andromede galaxy belongs to the local group, making up about thirty galaxies. Image made with an amateur instrument, a 130 mm bezel, several composite images. M31, the Great galaxy in Andromeda, is a gigantic collection of more than 300 billion stars and is located about 2 million light years from Earth. Companion dwarf elliptical galaxies M32 and M110 are also visible. M31 and its companions are part of our local group of galaxies, which includes the Milky Way and Magellanic Clouds, and M33. The Andromeda Galaxy is headed towards our Milky Way Galaxy and is expected to collide with it and possibly merge into a gigantic elliptical galaxy in about 3 billion years

Jerry Lodriguss

PIX4608685

Spiral Galaxy M31 in Andromede - Spiral galaxy M31 in Andromeda - The galaxy of Andromede is located about 2 million years ago - light from Earth. Two satellite galaxies accompany it: M32 (NGC 221) in the center left, and M110 (NGC 205) below. Like the lactee path, the Andromede galaxy belongs to the local group, making up about thirty galaxies. Image made with an amateur instrument, a 130 mm bezel, several composite images. M31, the Great galaxy in Andromeda, is a gigantic collection of more than 300 billion stars and is located about 2 million light years from Earth. Companion dwarf elliptical galaxies M32 and M110 are also visible. M31 and its companions are part of our local group of galaxies, which includes the Milky Way and Magellanic Clouds, and M33. The Andromeda Galaxy is headed towards our Milky Way Galaxy and is expected to collide with it and possibly merge into a gigantic elliptical galaxy in about 3 billion years

Jerry Lodriguss

PIX4608685

 
Barnard's loop and constellation Orion - Barnard's loop and Orion constellation - The constellation Orion and its nebulae. The main stars of this constellation are two supergeants, Betelgeuse (red) on the top left and Rigel (blue) on the bottom right. In the center of the constellation are the three stars forming Orion's Belt (or Baldrier) and the dark nebula of the horse's head (IC434 - B33). Further down, the large Orion nebula (M42) vast star-forming region. Wrapping these nebulae, Barnard's loop, a circle-arch nebula that would come from the explosion of a supernova more than two million years ago. The Orion constellation and its nebulae. The two Orion's bright stars are both supergiant stars: Betelgeuse (a red one) and Rigel (blue one). The center of this constellation is the Orion Belt with the Horsehead nebula (IC 434 - B33). Lower, the great Orion nebula, M42, a large star forming region. Also visible on this image, the Barnard's loop, a very faint nebula. This is composite mos

R. Gendler

PIX4617896

Barnard's loop and constellation Orion - Barnard's loop and Orion constellation - The constellation Orion and its nebulae. The main stars of this constellation are two supergeants, Betelgeuse (red) on the top left and Rigel (blue) on the bottom right. In the center of the constellation are the three stars forming Orion's Belt (or Baldrier) and the dark nebula of the horse's head (IC434 - B33). Further down, the large Orion nebula (M42) vast star-forming region. Wrapping these nebulae, Barnard's loop, a circle-arch nebula that would come from the explosion of a supernova more than two million years ago. The Orion constellation and its nebulae. The two Orion's bright stars are both supergiant stars: Betelgeuse (a red one) and Rigel (blue one). The center of this constellation is the Orion Belt with the Horsehead nebula (IC 434 - B33). Lower, the great Orion nebula, M42, a large star forming region. Also visible on this image, the Barnard's loop, a very faint nebula. This is composite mos

R. Gendler

PIX4617896

 
Galaxies Group: Stephan's Quintet in Pegase - Stephan's Quintet group of galaxies - Image obtained with the Hubble space telescope. This group of 5 galaxies is located about 270 million light years away from Earth. In this image three star-forming regions are visible: in the long arm of NGC 7319 (near the center); the gas debris of two galaxies, NGC 7318B and NGC 7318A (upper right); and in the upper left. Blue indicates that these stars are young. This NASA/ESA Hubble Space Telescope image is a close - up view of the central part of Stephan's Quintet, giving a magnificent view of a gigantic cosmic collision. Stephan's Quintet, as its name implies, is a group of five galaxies (NGC7317, 7318A, 7318B, 7319 and 7320) and lies about 270 million light - years away in the constellation of Pegasus (North - west of the Great Square of Pegasus). A sixth galaxy (NGC 7320C) lies south - east of the other five (upper left - hand corner of the overview image). The galaxy group was the first of its

PIX4565462

Galaxies Group: Stephan's Quintet in Pegase - Stephan's Quintet group of galaxies - Image obtained with the Hubble space telescope. This group of 5 galaxies is located about 270 million light years away from Earth. In this image three star-forming regions are visible: in the long arm of NGC 7319 (near the center); the gas debris of two galaxies, NGC 7318B and NGC 7318A (upper right); and in the upper left. Blue indicates that these stars are young. This NASA/ESA Hubble Space Telescope image is a close - up view of the central part of Stephan's Quintet, giving a magnificent view of a gigantic cosmic collision. Stephan's Quintet, as its name implies, is a group of five galaxies (NGC7317, 7318A, 7318B, 7319 and 7320) and lies about 270 million light - years away in the constellation of Pegasus (North - west of the Great Square of Pegasus). A sixth galaxy (NGC 7320C) lies south - east of the other five (upper left - hand corner of the overview image). The galaxy group was the first of its

PIX4565462

 
Nebula NGC 3372 in the Carene - NGC 3372 Carina nebula - The Carene Nebula (NGC 3372) is a very large region of star formation visible in the southern hemisphere. Image obtained through 3 different filters that highlight oxygen (blue), hydrogen (green), and sulfur (red). The bright star in the center of the image is Eta Carinae, a super massive star. The Carina Nebula (also known as the Great Nebula in Carina, the Eta Carinae Nebula, or NGC 3372) is a large bright nebula that surrounds several open clusters of stars. Eta Carinae and HD 93129A, two of the most massive and luminous stars in our Milky Way galaxy, are among them. The nebula lies at an estimated distance between 6,500 and 10,000 light years from Earth. It is located in the constellation of Carina. The nebula contains multiple O - type stars. This nebula is one of the largest H II regions in the Milky Way. It has a visual magnitude of 1.0. The nebula is one of the largest diffuse nebulae in our skies. Although it is some fou

Tom Davis

PIX4619112

Nebula NGC 3372 in the Carene - NGC 3372 Carina nebula - The Carene Nebula (NGC 3372) is a very large region of star formation visible in the southern hemisphere. Image obtained through 3 different filters that highlight oxygen (blue), hydrogen (green), and sulfur (red). The bright star in the center of the image is Eta Carinae, a super massive star. The Carina Nebula (also known as the Great Nebula in Carina, the Eta Carinae Nebula, or NGC 3372) is a large bright nebula that surrounds several open clusters of stars. Eta Carinae and HD 93129A, two of the most massive and luminous stars in our Milky Way galaxy, are among them. The nebula lies at an estimated distance between 6,500 and 10,000 light years from Earth. It is located in the constellation of Carina. The nebula contains multiple O - type stars. This nebula is one of the largest H II regions in the Milky Way. It has a visual magnitude of 1.0. The nebula is one of the largest diffuse nebulae in our skies. Although it is some fou

Tom Davis

PIX4619112

 
Basement of the Savoy Hotel, c.1904 (b/w photo)

CWA124896

Basement of the Savoy Hotel, c.1904 (b/w photo)

CWA124896

 
Antares star and the nebula Rho Ophiuchi - Antares and Rho Ophiuchi cloud - This coloree nebula represents the visible part of a very large molecule cloud, the cloud of Ophiuchus. This star-forming region is about 520 years old - light. The brightest star at the bottom left is the star Antares, from the Scorpio. The triple star Rho Ophiuchus is located in the middle of the blue cloud at the top of the picture. On the right, surrounded by a nebula, the star Sigma Scorpii. The globular clusters M4 (at the bottom of the image) and NGC 6144 (near Antares) are also visible on this image obtained with the UK Schmidt telescope of 1.2m. This photograph shows a portion of a great swath of obscuring gas and dust in the constellations Ophiuchus and Scorpius, and illustrates what is probably the most colourful region in the entire sky. The almost garish colours are due to the brilliance and contrasting colours of the stars, by whose reflected light we see the dust clouds. Dominating the picture is

PIX4621421

Antares star and the nebula Rho Ophiuchi - Antares and Rho Ophiuchi cloud - This coloree nebula represents the visible part of a very large molecule cloud, the cloud of Ophiuchus. This star-forming region is about 520 years old - light. The brightest star at the bottom left is the star Antares, from the Scorpio. The triple star Rho Ophiuchus is located in the middle of the blue cloud at the top of the picture. On the right, surrounded by a nebula, the star Sigma Scorpii. The globular clusters M4 (at the bottom of the image) and NGC 6144 (near Antares) are also visible on this image obtained with the UK Schmidt telescope of 1.2m. This photograph shows a portion of a great swath of obscuring gas and dust in the constellations Ophiuchus and Scorpius, and illustrates what is probably the most colourful region in the entire sky. The almost garish colours are due to the brilliance and contrasting colours of the stars, by whose reflected light we see the dust clouds. Dominating the picture is

PIX4621421

 
Pistol star - Massive star in the constellation Sagittarius - The massive star Pistol star in Sagittarius - Pistol star is one of the most massive stars in our galaxy. Located about 25,000 years ago - the light of the Earth in the constellation of Sagittarius, this star shines like 10 million Sun consuming in six seconds as much energy as our star in a year. This star is masked by the numerous interstellar dust present in the Sagittarius near the galactic center and appears only in infrared wavelengths, as in this image obtained with the NICMOS instrument embark on the Hubble space telescope. The nebula that surrounds it (in the shape of a gun), extends over 4 years - light. Image obtained in 1997. Astronomers using Nasa's Hubble Space Telescope have identified what may be the most luminous star known “” a celestial mammoth which releases up to 10 million times the power of the Sun and is big enough to fill the diameter of Earth's orbit. The star unleashes as much energy in six seconds

PIX4572084

Pistol star - Massive star in the constellation Sagittarius - The massive star Pistol star in Sagittarius - Pistol star is one of the most massive stars in our galaxy. Located about 25,000 years ago - the light of the Earth in the constellation of Sagittarius, this star shines like 10 million Sun consuming in six seconds as much energy as our star in a year. This star is masked by the numerous interstellar dust present in the Sagittarius near the galactic center and appears only in infrared wavelengths, as in this image obtained with the NICMOS instrument embark on the Hubble space telescope. The nebula that surrounds it (in the shape of a gun), extends over 4 years - light. Image obtained in 1997. Astronomers using Nasa's Hubble Space Telescope have identified what may be the most luminous star known “” a celestial mammoth which releases up to 10 million times the power of the Sun and is big enough to fill the diameter of Earth's orbit. The star unleashes as much energy in six seconds

PIX4572084

 
Corner of the forecourt of the Savoy Hotel, c.1904 (b/w photo)

CWA124895

Corner of the forecourt of the Savoy Hotel, c.1904 (b/w photo)

CWA124895

 
The Forecourt of the Savoy Hotel, c.1904 (b/w photo)

CWA124894

The Forecourt of the Savoy Hotel, c.1904 (b/w photo)

CWA124894

 
A Dining Room at the Savoy Hotel, c.1904 (b/w photo)

CWA124898

A Dining Room at the Savoy Hotel, c.1904 (b/w photo)

CWA124898

 
A Drawing Room in the Savoy Hotel, c.1904 (b/w photo)

CWA124897

A Drawing Room in the Savoy Hotel, c.1904 (b/w photo)

CWA124897

 
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Grimspound II, 1995 (w/c on paper)

Stevens, Philip (b.1953)

UEA420504

Grimspound II, 1995 (w/c on paper)

Stevens, Philip (b.1953)

UEA420504

 
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  • Copyright Applies
Dartmoor VI, Clearbrook, 1993 (oil on canvas)

Stevens, Philip (b.1953)

UEA420497

Dartmoor VI, Clearbrook, 1993 (oil on canvas)

Stevens, Philip (b.1953)

UEA420497

 
Copyright
  • Copyright Applies
Standing Stones I, Avebury, 1994 (oil on canvas)

Stevens, Philip (b.1953)

UEA420496

Standing Stones I, Avebury, 1994 (oil on canvas)

Stevens, Philip (b.1953)

UEA420496

 
Copyright
  • Copyright Applies
Postbridge, 1998 (oil on canvas)

Stevens, Philip (b.1953)

UEA420523

Postbridge, 1998 (oil on canvas)

Stevens, Philip (b.1953)

UEA420523

 
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HMS Polaris, used by Captain Charles Francis Hall (1821-1871) for shipment to Straits of Smith, between island of Ellesmere and Inglefield Land, May 31, 1871

DGA2583337

HMS Polaris, used by Captain Charles Francis Hall (1821-1871) for shipment to Straits of Smith, between island of Ellesmere and Inglefield Land, May 31, 1871

DGA2583337

 
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Burial of Captain Charles Francis Hall (1821-1871), who died on HMS Polaris during Polaris expedition to Smith's Strait, between island of Ellesmere and Inglefield Land, November 10, 1871

DGA2583338

Burial of Captain Charles Francis Hall (1821-1871), who died on HMS Polaris during Polaris expedition to Smith's Strait, between island of Ellesmere and Inglefield Land, November 10, 1871

DGA2583338

 
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Sir Winston Churchill's funeral, St. Paul's Cathedral, London, Jan 30, 1965 (photo)

Brian Seed

BRS880200

premium

premium
Sir Winston Churchill's funeral, St. Paul's Cathedral, London, Jan 30, 1965 (photo)

Brian Seed

BRS880200

 
Permissions
  • Permission required for non-editorial use (inc book and magazine covers). Please contact us
The Children of Charles I, 1637 (oil on canvas)

Dyck, Anthony van (1599-1641) (after)

NTE6424431

The Children of Charles I, 1637 (oil on canvas)

Dyck, Anthony van (1599-1641) (after)

NTE6424431

 
Interview between Marlborough and Charles XII of Sweden, Altranstadt (1707), c.1890 (engraving)

Ken Welsh

KWE7212151

Interview between Marlborough and Charles XII of Sweden, Altranstadt (1707), c.1890 (engraving)

Ken Welsh

KWE7212151

 
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Paradiso, Canto XVIII. Miniature shows Dante and Beatrice hovering before the half figure of Cacciaguida, who is on the periphery of the Heaven of Mars, which has the winged figure of Mars in its centre. Dante is shown the eight holy warriors who appear in the form of a cross. They are from the Old Testament, history, and medieval romance. Joshua and Judas Maccabaeus; Charlemagne, Godefroi de Bouillon and Robert Guiscard; Roland, William of Orange and Reynard

Paolo, Giovanni di (c.1389-1482)

BL6317734

Paradiso, Canto XVIII. Miniature shows Dante and Beatrice hovering before the half figure of Cacciaguida, who is on the periphery of the Heaven of Mars, which has the winged figure of Mars in its centre. Dante is shown the eight holy warriors who appear in the form of a cross. They are from the Old Testament, history, and medieval romance. Joshua and Judas Maccabaeus; Charlemagne, Godefroi de Bouillon and Robert Guiscard; Roland, William of Orange and Reynard

Paolo, Giovanni di (c.1389-1482)

BL6317734

 
Permissions
  • Permission required for non-editorial use (inc book and magazine covers). Please contact us
Paradiso, Canto XVIII. Miniature shows Dante and Beatrice hovering before the half figure of Cacciaguida, who is on the periphery of the Heaven of Mars, which has the winged figure of Mars in its centre. Dante is shown the eight holy warriors who appear in the form of a cross. They are from the Old Testament, history, and medieval romance. Joshua and Judas Maccabaeus; Charlemagne, Godefroi de Bouillon and Robert Guiscard; Roland, William of Orange and Reynard

Paolo, Giovanni di (c.1389-1482)

BL3286517

Paradiso, Canto XVIII. Miniature shows Dante and Beatrice hovering before the half figure of Cacciaguida, who is on the periphery of the Heaven of Mars, which has the winged figure of Mars in its centre. Dante is shown the eight holy warriors who appear in the form of a cross. They are from the Old Testament, history, and medieval romance. Joshua and Judas Maccabaeus; Charlemagne, Godefroi de Bouillon and Robert Guiscard; Roland, William of Orange and Reynard

Paolo, Giovanni di (c.1389-1482)

BL3286517

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