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Immagini di 'L'età' trovate, 76,308

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Pastel portrait by Renoir titled Jeune fille (L'EtÃ©) rests next to rococo fire surro…, 2021 (photo)

premium — Pastel portrait by Renoir titled Jeune fille (L'EtÃ©) rests next to rococo fire surro…, 2021 (photo)

Pastel portrait by Renoir titled Jeune fille (L'EtÃ©) rests next to rococo fire surro…, 2021 (photo)

Hatfield, Visko

HAF8776191

Gigliola Cinquetti performing on the stage of the Ariston theatre

Gigliola Cinquetti performing on the stage of the Ariston theatre

Sergio del Grande

MEP2370632

Gigliola Cinquetti and Patricia Carli with Mike Bongiorno on the stage of Sanremo

Gigliola Cinquetti and Patricia Carli with Mike Bongiorno on the stage of Sanremo

Sergio del Grande

MEP2370371

Gigliola Cinquetti and Patricia Carli prize winners at the 14th Sanremo Music Festival

Gigliola Cinquetti and Patricia Carli prize winners at the 14th Sanremo Music Festival

Archivio TV Sorrisi e Canzoni

MEP2389877

Close-up of Gigliola Cinquetti while she is looking out of a window

Close-up of Gigliola Cinquetti while she is looking out of a window

Angelo Cozzi

MEP2371989

Gigliola Cinquetti chatting with a person in the back

Gigliola Cinquetti chatting with a person in the back

Giorgio Lotti

MEP2372061

Gigliola Cinquetta is signing her autograph for one of her fans

Gigliola Cinquetta is signing her autograph for one of her fans

Giorgio Lotti

MEP2372057

Gigliola Cinquetti is signing her autograph for some very young fans

Gigliola Cinquetti is signing her autograph for some very young fans

Angelo Cozzi

MEP2372019

Age of Silver, 1587 (oil on board)

Age of Silver, 1587 (oil on board)

Zucchi, Jacopo (c.1540-96)

Antonio Quattrone

MEP2627516

Gigliola Cinquetti looking upwards with a thoughtful expression

Gigliola Cinquetti looking upwards with a thoughtful expression

Giorgio Lotti

MEP2372071

Italy, Florence, Palazzo Pitti, Stove Room in Palatine Gallery, Iron Age, detail of Four Ages of Man, 1637, by Pietro da Cortona (1596-1669), fresco

Italy, Florence, Palazzo Pitti, Stove Room in Palatine Gallery, Iron Age, detail of Four Ages of Man, 1637, by Pietro da Cortona (1596-1669), fresco

DGA569841

Martin Scorsese

Martin Scorsese

Mencarini, Marcello

MME3832933

Close-up of Gigliola Cinquetti looking at fish in an aquarium

Close-up of Gigliola Cinquetti looking at fish in an aquarium

Giorgio Lotti

MEP2372059

Gigliola Cinquetti in a graceful pose in Piazza delle Erbe

Gigliola Cinquetti in a graceful pose in Piazza delle Erbe

Giorgio Lotti

MEP2372052

Italy, Florence, Palazzo Pitti, Stove Room in Palatine Gallery, Copper Age, detail of Four Ages of Man, 1637, by Pietro da Cortona (1596-1669), fresco

Italy, Florence, Palazzo Pitti, Stove Room in Palatine Gallery, Copper Age, detail of Four Ages of Man, 1637, by Pietro da Cortona (1596-1669), fresco

DGA569836

Italy, Florence, Palazzo Pitti, Stove Room in Palatine Gallery, Copper Age, detail of Four Ages of Man, 1637, by Pietro da Cortona (1596-1669), fresco

Italy, Florence, Palazzo Pitti, Stove Room in Palatine Gallery, Copper Age, detail of Four Ages of Man, 1637, by Pietro da Cortona (1596-1669), fresco

DGA569837

The Golden Age, detail from Four Ages of Man, by Pietro da Cortona (1596-1669), fresco, Detail, Stove Room in Palatine Gallery, Palazzo Pitti, Florence, 1637-1640

The Golden Age, detail from Four Ages of Man, by Pietro da Cortona (1596-1669), fresco, Detail, Stove Room in Palatine Gallery, Palazzo Pitti, Florence, 1637-1640

DGA576606

Italy, Florence, Palazzo Pitti, Stove Room in Palatine Gallery, Iron Age or rather uncontrolled soldiery hunts and kills, detail from Four Ages of Man, 1637-1640, by Pietro da Cortona (1596-1669), fresco

Italy, Florence, Palazzo Pitti, Stove Room in Palatine Gallery, Iron Age or rather uncontrolled soldiery hunts and kills, detail from Four Ages of Man, 1637-1640, by Pietro da Cortona (1596-1669), fresco

DGA569839

Italy, Florence, Palazzo Pitti, Stove Room in Palatine Gallery, Golden Age, detail from Four Ages of Man, 1637-1640, by Pietro da Cortona (1596-1669), fresco, Detail

Italy, Florence, Palazzo Pitti, Stove Room in Palatine Gallery, Golden Age, detail from Four Ages of Man, 1637-1640, by Pietro da Cortona (1596-1669), fresco, Detail

DGA569833

Italy, Florence, Palazzo Pitti, Stove Room in Palatine Gallery, Iron Age or rather uncontrolled soldiery hunts and kills, detail from Four Ages of Man, 1637-1640, by Pietro da Cortona (1596-1669), fresco

Italy, Florence, Palazzo Pitti, Stove Room in Palatine Gallery, Iron Age or rather uncontrolled soldiery hunts and kills, detail from Four Ages of Man, 1637-1640, by Pietro da Cortona (1596-1669), fresco

DGA569840

Golden Age, 1886 (bronze)

Golden Age, 1886 (bronze)

Rosso, Medardo (1858-1928)

Alessandro Vasari

MEP2646489

The Iron Age or rather uncontrolled soldiery hunts and kills, detail from Four Ages of Man, by Pietro da Cortona (1596-1669), fresco, Stove Room, Palatine Gallery, Palazzo Pitti, Florence, 1637-1640

The Iron Age or rather uncontrolled soldiery hunts and kills, detail from Four Ages of Man, by Pietro da Cortona (1596-1669), fresco, Stove Room, Palatine Gallery, Palazzo Pitti, Florence, 1637-1640

DGA576601

The Iron Age or rather uncontrolled soldiery hunts and kills, detail from Four Ages of Man, by Pietro da Cortona (1596-1669), fresco, Stove Room, Palatine Gallery, Palazzo Pitti, Florence, 1637-1640

The Iron Age or rather uncontrolled soldiery hunts and kills, detail from Four Ages of Man, by Pietro da Cortona (1596-1669), fresco, Stove Room, Palatine Gallery, Palazzo Pitti, Florence, 1637-1640

DGA576600

Italy, Florence, Palazzo Pitti, Stove Room in Palatine Gallery, Silver Age or rather quiet life devoted to sheep farming and agriculture, detail from Four Ages of Man, 1637-1640, by Pietro da Cortona (1596-1669), fresco, Detail

Italy, Florence, Palazzo Pitti, Stove Room in Palatine Gallery, Silver Age or rather quiet life devoted to sheep farming and agriculture, detail from Four Ages of Man, 1637-1640, by Pietro da Cortona (1596-1669), fresco, Detail

DGA569835

Italy, Florence, Palazzo Pitti, Stove Room in Palatine Gallery, Golden Age or rather peaceful life of young man in flourishing nature, detail from Four Ages of Man, 1637-1640, by Pietro da Cortona (1596-1669), fresco

Italy, Florence, Palazzo Pitti, Stove Room in Palatine Gallery, Golden Age or rather peaceful life of young man in flourishing nature, detail from Four Ages of Man, 1637-1640, by Pietro da Cortona (1596-1669), fresco

DGA569832

The Silver Age or rather quiet life devoted to sheep farming and agriculture, detail from Four Ages of Man, by Pietro da Cortona (1596-1669), fresco, Stove Room in Palatine Gallery, Palazzo Pitti, Florence, 1637-1640

The Silver Age or rather quiet life devoted to sheep farming and agriculture, detail from Four Ages of Man, by Pietro da Cortona (1596-1669), fresco, Stove Room in Palatine Gallery, Palazzo Pitti, Florence, 1637-1640

DGA576603

Italy, Florence, Palazzo Pitti, Stove Room in Palatine Gallery, Silver Age or rather quiet life devoted to sheep farming and agriculture, detail from Four Ages of Man, 1637-1640, by Pietro da Cortona (1596-1669), fresco, Detail

Italy, Florence, Palazzo Pitti, Stove Room in Palatine Gallery, Silver Age or rather quiet life devoted to sheep farming and agriculture, detail from Four Ages of Man, 1637-1640, by Pietro da Cortona (1596-1669), fresco, Detail

DGA569834

Italy, Florence, Palazzo Pitti, Stove Room in Palatine Gallery, Copper Age or rather soldiers receiving award for capturing prisoners, detail from Four Ages of Man, 1637-1640, by Pietro da Cortona (1596-1669), fresco, Detail

Italy, Florence, Palazzo Pitti, Stove Room in Palatine Gallery, Copper Age or rather soldiers receiving award for capturing prisoners, detail from Four Ages of Man, 1637-1640, by Pietro da Cortona (1596-1669), fresco, Detail

DGA569838

The Silver Age or rather quiet life devoted to sheep farming and agriculture, detail from Four Ages of Man, by Pietro da Cortona (1596-1669), fresco, Detail, Stove Room in Palatine Gallery, Palazzo Pitti, Florence, 1637-1640

The Silver Age or rather quiet life devoted to sheep farming and agriculture, detail from Four Ages of Man, by Pietro da Cortona (1596-1669), fresco, Detail, Stove Room in Palatine Gallery, Palazzo Pitti, Florence, 1637-1640

DGA576605

The Copper Age or rather soldiers receiving award for capturing prisoners, detail from Four Ages of Man, by Pietro da Cortona (1596-1669), fresco, Detail, Stove Room in Palatine Gallery, Palazzo Pitti, Florence, 1637-1640

The Copper Age or rather soldiers receiving award for capturing prisoners, detail from Four Ages of Man, by Pietro da Cortona (1596-1669), fresco, Detail, Stove Room in Palatine Gallery, Palazzo Pitti, Florence, 1637-1640

DGA576602

Hoffmann ETA

Hoffmann, Ernst Theodor Amadeus (1776-1822)

XLE3747850

ETA Hoffmann - Self-portrait

ETA Hoffmann - Self-portrait

Hoffmann, Ernst Theodor Amadeus (1776-1822)

XLE3776980

Hoffmann ETA

Hoffmann, Ernst Theodor Amadeus (1776-1822)

XLE3772392

Hoffmann ETA (Ernest

Hoffmann ETA (Ernest

XLE3754584

ETA Hoffmann self-portrait

ETA Hoffmann self-portrait

Hoffmann, Ernst Theodor Amadeus (1776-1822)

XLE3754583

ETA HOFFMANN

ETA HOFFMANN

EPL6802899

Hoffmann ETA

Hoffmann, Ernst Theodor Amadeus (1776-1822)

XLE3764149

Illustration par ETA Hoffmann

Illustration par ETA Hoffmann

Hoffmann, Ernst Theodor Amadeus (1776-1822)

XLE3768340

ETA Hoffmann's character Kapellmeister

ETA Hoffmann's character Kapellmeister

XLA3768168

ETA Hoffmann's character Kapellmeister

ETA Hoffmann's character Kapellmeister

XLA3761157

ETA Hoffmann - Self-portrait

ETA Hoffmann - Self-portrait

Hoffmann, Ernst Theodor Amadeus (1776-1822)

XLE3750672

ETA Hoffmann self-portrait

ETA Hoffmann self-portrait

Hoffmann, Ernst Theodor Amadeus (1776-1822)

XLE3751789

ETA Hoffmann - Self-portrait

ETA Hoffmann - Self-portrait

Hoffmann, Ernst Theodor Amadeus (1776-1822)

XLE3747939

Constellation of the Southern Cross - The Southern Cross - The Southern Cross and the Alpha and Beta stars of Centaurus. Crux, the Southern Cross, is the smallest constellation in the sky yet one of the most distinctive, at least to those of us who live in the southern hemisphere. It was once part of Centaurus, where the bright stars Acrux and Mimosa could easly be imagined as the rear hooves of the rearing mythical centaur. However, when Christian sailors began to explore southwards in the 16th century, this memorable asterism took on a new significance. The cross appears on the national flags of several southern hemisphere countries, including Australia, though it can be seen on the southern horizon from the tropic of Cancer, 23.5 degrees north of the equator. Along with the Southern Cross is a very distinctive dark shape known as the Coalsack, much used by southern hemisphere astronomers as an indicator of a dark sky, especially if the sixth magnitude star embedded in it is visible. The long axis of the southern cross points towards the south celestial pole, so the cross itself acts as a very convenient circumpolar clock, compasset and calendar — Constellation of the Southern Cross - The Southern Cross - The Southern Cross and the Alpha and Beta stars of Centaurus. Crux, the Southern Cross, is the smallest constellation in the sky yet one of the most distinctive, at least to those of us who live in the southern hemisphere. It was once part of Centaurus, where the bright stars Acrux and Mimosa could easly be imagined as the rear hooves of the rearing mythical centaur. However, when Christian sailors began to explore southwards in the 16th century, this memorable asterism took on a new significance. The cross appears on the national flags of several southern hemisphere countries, including Australia, though it can be seen on the southern horizon from the tropic of Cancer, 23.5 degrees north of the equator. Along with the Southern Cross is a very distinctive dark shape known as the Coalsack, much used by southern hemisphere astronomers as an indicator of a dark sky, especially if the sixth magnitude star embedded in it is visible.

Constellation of the Southern Cross - The Southern Cross - The Southern Cross and the Alpha and Beta stars of Centaurus. Crux, the Southern Cross, is the smallest constellation in the sky yet one of the most distinctive, at least to those of us who live in the southern hemisphere. It was once part of Centaurus, where the bright stars Acrux and Mimosa could easly be imagined as the rear hooves of the rearing mythical centaur. However, when Christian sailors began to explore southwards in the 16th century, this memorable asterism took on a new significance. The cross appears on the national flags of several southern hemisphere countries, including Australia, though it can be seen on the southern horizon from the tropic of Cancer, 23.5 degrees north of the equator. Along with the Southern Cross is a very distinctive dark shape known as the Coalsack, much used by southern hemisphere astronomers as an indicator of a dark sky, especially if the sixth magnitude star embedded in it is visible.

PIX4590268

Chief of Eta, Drummond's island

Chief of Eta, Drummond's island

BL3268628

The Artemis of Ephesus

The Artemis of Ephesus

GRL1630018

Three ages (etching and aquatint on paper, plate)

Three ages (etching and aquatint on paper, plate)

Magnavacca, Ubaldo (1885-1957)

GRL3713116

Amori: Eta d'Oro (painting)

Amori: Eta d'Oro (painting)

Fiammingo, Paolo (Franck, Pauwels) (1540-96)

Lessing, Erich

ELS9191356

Hoffmann ETA (German novelist

Hoffmann ETA (German novelist

XLE3771350

Constellations of Centaur and Southern Cross - Constellations Centaurus and Crux - Visible also, the constellations of the Compas, Southern Triangle, Southern Cross and Fly. Image obtained from New Zealand. Constellations also visible in this image: Circinus, Southern Triangulum, Crux and Musca. Image obtained from New Zealand

Constellations of Centaur and Southern Cross - Constellations Centaurus and Crux - Visible also, the constellations of the Compas, Southern Triangle, Southern Cross and Fly. Image obtained from New Zealand. Constellations also visible in this image: Circinus, Southern Triangulum, Crux and Musca. Image obtained from New Zealand

Minoru Yoneto

PIX4589735

The Greek theatre, The Archaeological Park of the Neapolis, Syracuse, Sicily, Italy (photo)

The Greek theatre, The Archaeological Park of the Neapolis, Syracuse, Sicily, Italy (photo)

GRL3961088

Constellation of the Southern Cross - The Southern Cross - The Southern Cross and Coalsack and the Great Carina nebula. Centred on lamda Ce

Constellation of the Southern Cross - The Southern Cross - The Southern Cross and Coalsack and the Great Carina nebula. Centred on lamda Ce

PIX4590245

Constellation of the Southern Cross - Constellation Crux. The Southern Cross - With the lack of a significant pole star in the southern sky (Sigma Octantis is closest to the pole, but is so faint as to be useless for the purpose), two of the stars of Crux (Alpha and Gamma, Acrux and Gacrux respectively) are commonly used to mark south. Following the line defined by the two stars for approximately 4.5 times the distance between them leads to a point close to the Southern Celestial Pole

Constellation of the Southern Cross - Constellation Crux. The Southern Cross - With the lack of a significant pole star in the southern sky (Sigma Octantis is closest to the pole, but is so faint as to be useless for the purpose), two of the stars of Crux (Alpha and Gamma, Acrux and Gacrux respectively) are commonly used to mark south. Following the line defined by the two stars for approximately 4.5 times the distance between them leads to a point close to the Southern Celestial Pole

Christopher Picking

PIX4590169

Nebula NGC 3372 in Carene - Nebula NGC 3372 in Carina - The nebula of the Carene is located about 7000 years - light from Earth. It is home to many hot stars, including the star Eta Carinae (on the left, the brightest star in the picture). In the right center, a cluster of young stars, Trumpler 14. This image shows a giant star - forming region in the southern sky known as the Carina Nebula (NGC 3372). The bright star on the left of the image is Eta Carinae, which is one of the most massive and luminous stars known

Nebula NGC 3372 in Carene - Nebula NGC 3372 in Carina - The nebula of the Carene is located about 7000 years - light from Earth. It is home to many hot stars, including the star Eta Carinae (on the left, the brightest star in the picture). In the right center, a cluster of young stars, Trumpler 14. This image shows a giant star - forming region in the southern sky known as the Carina Nebula (NGC 3372). The bright star on the left of the image is Eta Carinae, which is one of the most massive and luminous stars known

R. Gendler

PIX4619048

Super massive star Eta Carinae - Super massive star Eta Carinae - Eta Carinae is one of the most massive stars in our galaxy. Its mass would be about 120 times that of the Sun with a diameter 1000 times larger than our star. The image obtained by the Hubble space telescope reveals two expanding gas lobes; it is the nebula called the Homuncule, vestige of a huge explosion that the star experienced 150 years ago. The star blows its exterior atmosphere and will eventually explode in a supernova. Eta Carinae is located approximately 8000 light years from Earth in the southern constellation of Carene. A huge, billowing pair of gas and dust clouds is captured in this stunning Hubble telescope picture of the super - massive star Eta Carinae. Even though Eta Carinae is more than 8,000 light - years away, features 10 billion miles across (about the diameter of our solar system) can be distinguished. Eta Carinae suffered giant outburst about 150 years ago, when it became one of the brightest stars in the southern sky. Although the star released as much visible light as a supernova explosion, it survived the outburst. Somehow, the explosion produced two lobes and a large, thin equatorial disk, all moving outward at about 1.5 million miles per hour. Estimated to be 100 times heftier than our Sun, Eta Carinae may be one of the most massive stars in our galaxy — Super massive star Eta Carinae - Super massive star Eta Carinae - Eta Carinae is one of the most massive stars in our galaxy. Its mass would be about 120 times that of the Sun with a diameter 1000 times larger than our star. The image obtained by the Hubble space telescope reveals two expanding gas lobes; it is the nebula called the Homuncule, vestige of a huge explosion that the star experienced 150 years ago. The star blows its exterior atmosphere and will eventually explode in a supernova. Eta Carinae is located approximately 8000 light years from Earth in the southern constellation of Carene. A huge, billowing pair of gas and dust clouds is captured in this stunning Hubble telescope picture of the super - massive star Eta Carinae. Even though Eta Carinae is more than 8,000 light - years away, features 10 billion miles across (about the diameter of our solar system) can be distinguished. Eta Carinae suffered giant outburst about 150 years ago, when it became one of the brightest sta

Super massive star Eta Carinae - Super massive star Eta Carinae - Eta Carinae is one of the most massive stars in our galaxy. Its mass would be about 120 times that of the Sun with a diameter 1000 times larger than our star. The image obtained by the Hubble space telescope reveals two expanding gas lobes; it is the nebula called the Homuncule, vestige of a huge explosion that the star experienced 150 years ago. The star blows its exterior atmosphere and will eventually explode in a supernova. Eta Carinae is located approximately 8000 light years from Earth in the southern constellation of Carene. A huge, billowing pair of gas and dust clouds is captured in this stunning Hubble telescope picture of the super - massive star Eta Carinae. Even though Eta Carinae is more than 8,000 light - years away, features 10 billion miles across (about the diameter of our solar system) can be distinguished. Eta Carinae suffered giant outburst about 150 years ago, when it became one of the brightest sta

PIX4572090

The Greek theatre, The Archaeological Park of the Neapolis, Syracuse, Sicily, Italy (photo)

The Greek theatre, The Archaeological Park of the Neapolis, Syracuse, Sicily, Italy (photo)

GRL3961082

Constellations of the Fly and the Southern Cross - Constellations of Musca and the Southern cross - The Southern Cross and the Alpha and Beta Stars of Centaur. Below, the constellation of the Fly. In contrast to adjacent Crux, Musca (The Fly) is a much less obvious, less distinguished and less useful constellation that first appeared in Johann Bayer's 1603 Uranometria. It is one of a dozen created by the Dutch explorers/navigators Pieter Dirkszoon Keyser and Frederick de Houtman on their voyages into the south seas in the late 16th century

Constellations of the Fly and the Southern Cross - Constellations of Musca and the Southern cross - The Southern Cross and the Alpha and Beta Stars of Centaur. Below, the constellation of the Fly. In contrast to adjacent Crux, Musca (The Fly) is a much less obvious, less distinguished and less useful constellation that first appeared in Johann Bayer's 1603 Uranometria. It is one of a dozen created by the Dutch explorers/navigators Pieter Dirkszoon Keyser and Frederick de Houtman on their voyages into the south seas in the late 16th century

PIX4592323

Super massive star Eta Carinae - Super massive star Eta Carinae - Eta Carinae is one of the most massive stars in our galaxy. Its mass would be about 120 times that of the Sun with a diameter 1000 times larger than our star. The image obtained by the Hubble space telescope reveals two expanding gas lobes; it is the nebula called the Homuncule, vestige of a huge explosion that the star experienced 150 years ago. The star blows its exterior atmosphere and will eventually explode in a supernova. Eta Carinae is located approximately 8000 light years from Earth in the southern constellation of Carene. A huge, billowing pair of gas and dust clouds is captured in this stunning Hubble telescope picture of the super - massive star Eta Carinae. Even though Eta Carinae is more than 8,000 light - years away, features 10 billion miles across (about the diameter of our solar system) can be distinguished. Eta Carinae suffered giant outburst about 150 years ago, when it became one of the brightest stars in the southern sky. Although the star released as much visible light as a supernova explosion, it survived the outburst. Somehow, the explosion produced two lobes and a large, thin equatorial disk, all moving outward at about 1.5 million miles per hour. Estimated to be 100 times heftier than our Sun, Eta Carinae may be one of the most massive stars in our galaxy — Super massive star Eta Carinae - Super massive star Eta Carinae - Eta Carinae is one of the most massive stars in our galaxy. Its mass would be about 120 times that of the Sun with a diameter 1000 times larger than our star. The image obtained by the Hubble space telescope reveals two expanding gas lobes; it is the nebula called the Homuncule, vestige of a huge explosion that the star experienced 150 years ago. The star blows its exterior atmosphere and will eventually explode in a supernova. Eta Carinae is located approximately 8000 light years from Earth in the southern constellation of Carene. A huge, billowing pair of gas and dust clouds is captured in this stunning Hubble telescope picture of the super - massive star Eta Carinae. Even though Eta Carinae is more than 8,000 light - years away, features 10 billion miles across (about the diameter of our solar system) can be distinguished. Eta Carinae suffered giant outburst about 150 years ago, when it became one of the brightest sta

Super massive star Eta Carinae - Super massive star Eta Carinae - Eta Carinae is one of the most massive stars in our galaxy. Its mass would be about 120 times that of the Sun with a diameter 1000 times larger than our star. The image obtained by the Hubble space telescope reveals two expanding gas lobes; it is the nebula called the Homuncule, vestige of a huge explosion that the star experienced 150 years ago. The star blows its exterior atmosphere and will eventually explode in a supernova. Eta Carinae is located approximately 8000 light years from Earth in the southern constellation of Carene. A huge, billowing pair of gas and dust clouds is captured in this stunning Hubble telescope picture of the super - massive star Eta Carinae. Even though Eta Carinae is more than 8,000 light - years away, features 10 billion miles across (about the diameter of our solar system) can be distinguished. Eta Carinae suffered giant outburst about 150 years ago, when it became one of the brightest sta

PIX4572109

Constellation of the Southern Cross - Constellation Crux. The Southern Cross - The Southern Cross with Beta and Alpha Centaurus left. Image obtained from New Zealand. 'Crux', being Latin for 'cross', commonly known as the' Southern Cross' (in contrast to the Cygnus (constellation) Northern Cross), is the smallest of the 88 modern constellations, but nevertheless one of the most distinctive. It is surrounded on three sides by the constellation Centaurus while to the south lies the 'Fly' (Musca). Crux was originally thought of by ancient Greeks as part of Centaurus, but was defined as a separate asterism in the 16th Century after Amerigo Vespucci's expedition to South America in 1501. Vespucci mapped the two stars, Alpha Centauri and Beta Centauri as well as the stars of the Crux. Although these stars were known to the ancient Greeks, gradual precession had lowered them below the European skyline so that they were forgotten

Constellation of the Southern Cross - Constellation Crux. The Southern Cross - The Southern Cross with Beta and Alpha Centaurus left. Image obtained from New Zealand. 'Crux', being Latin for 'cross', commonly known as the' Southern Cross' (in contrast to the Cygnus (constellation) Northern Cross), is the smallest of the 88 modern constellations, but nevertheless one of the most distinctive. It is surrounded on three sides by the constellation Centaurus while to the south lies the 'Fly' (Musca). Crux was originally thought of by ancient Greeks as part of Centaurus, but was defined as a separate asterism in the 16th Century after Amerigo Vespucci's expedition to South America in 1501. Vespucci mapped the two stars, Alpha Centauri and Beta Centauri as well as the stars of the Crux. Although these stars were known to the ancient Greeks, gradual precession had lowered them below the European skyline so that they were forgotten

Christopher Picking

PIX4590166

Nebula NGC 3372 in the Carene - The Carina nebula - The Carene nebula is located about 8000 years from the Earth. It is home to many hot stars, including the massive star Eta Carinae in the centre of the nebula. Image obtained from the 1.2m Schmidt UK telescope of Siding Spring. Although no bright naked - eye stars are associated with the Carina nebula now, 150 years ago there blazed forth here one of the most unusual and peculiar stars ever seen. The star is known as Eta Carinae and for a few months in 1843 it was the second or third brightest star in the sky. Since then it has faded and is today about 1000 times fainter than it was at its brightest as the nebula it created during its outburst has cooled and become opaque. The whole region around Eta Carinae is rich in hot stars of which Eta is an extreme example and it is their combined radiation that produces the spectacular Carina nebula that dominates this picture. The nebula and its peculiar star are about 8000 light years away

Nebula NGC 3372 in the Carene - The Carina nebula - The Carene nebula is located about 8000 years from the Earth. It is home to many hot stars, including the massive star Eta Carinae in the centre of the nebula. Image obtained from the 1.2m Schmidt UK telescope of Siding Spring. Although no bright naked - eye stars are associated with the Carina nebula now, 150 years ago there blazed forth here one of the most unusual and peculiar stars ever seen. The star is known as Eta Carinae and for a few months in 1843 it was the second or third brightest star in the sky. Since then it has faded and is today about 1000 times fainter than it was at its brightest as the nebula it created during its outburst has cooled and become opaque. The whole region around Eta Carinae is rich in hot stars of which Eta is an extreme example and it is their combined radiation that produces the spectacular Carina nebula that dominates this picture. The nebula and its peculiar star are about 8000 light years away

PIX4618987

Marble End Paper (paper)

Marble End Paper (paper)

Kilburn, William (1745-1818)

STC312698

ETA (Ernst Theodor Amadeus) Hoffmann (hand-coloured etching)

ETA (Ernst Theodor Amadeus) Hoffmann (hand-coloured etching)

Hensel, Wilhelm (1794-1861)

SZT3025255

Constellation of the Southern Cross and False Cross - The southern cross and the false cross - The southern cross on the left can sometimes be confused with a near asterism, the false cross on the right. Image obtained from New Zealand. The Southern Cross constellation (left) is sometimes confused with to other nearby asterisms which also resemble a cross, these are the 'Diamond' cross and the 'False' cross (right)

Constellation of the Southern Cross and False Cross - The southern cross and the false cross - The southern cross on the left can sometimes be confused with a near asterism, the false cross on the right. Image obtained from New Zealand. The Southern Cross constellation (left) is sometimes confused with to other nearby asterisms which also resemble a cross, these are the 'Diamond' cross and the 'False' cross (right)

Christopher Picking

PIX4590168

Constellation of the Southern Cross - The Southern cross. Panorama - The cross of the South, in the center, with Beta and Alpha of the Centaurus. Image obtained from New Zealand. The Southern Cross (center) seen from New Zealand

Constellation of the Southern Cross - The Southern cross. Panorama - The cross of the South, in the center, with Beta and Alpha of the Centaurus. Image obtained from New Zealand. The Southern Cross (center) seen from New Zealand

Christopher Picking

PIX4590185

Nebula NGC 3372 in the Carene - NGC 3372, Eta Carinae nebula - The nebula of the Carene is located about 8000 years - light from the Earth. It is home to many hot massive stars, including the star Eta Carinae in the centre of the nebula. This nebula is larger than the Great Nebula in Orion, but is not visible from most northern latitudes. It is a giant complex of emission and dark nebulae surrounding the unique variable star Eta Carinae, which scientists believe is the most massive and energetic star in the Milky Way galaxy. Located about 8,500 light years from the Earth, the star is about 100 times as massive as our own Sun, but produces 6 million times the light output. It was observed producing a remarkable burst of X - ray emissions that doubled its X - ray output in only four months. In the 1840's, Eta Carinae erupted visibly and was the second brightest star in the sky during this time

Nebula NGC 3372 in the Carene - NGC 3372, Eta Carinae nebula - The nebula of the Carene is located about 8000 years - light from the Earth. It is home to many hot massive stars, including the star Eta Carinae in the centre of the nebula. This nebula is larger than the Great Nebula in Orion, but is not visible from most northern latitudes. It is a giant complex of emission and dark nebulae surrounding the unique variable star Eta Carinae, which scientists believe is the most massive and energetic star in the Milky Way galaxy. Located about 8,500 light years from the Earth, the star is about 100 times as massive as our own Sun, but produces 6 million times the light output. It was observed producing a remarkable burst of X - ray emissions that doubled its X - ray output in only four months. In the 1840's, Eta Carinae erupted visibly and was the second brightest star in the sky during this time

Jerry Lodriguss

PIX4618875

The Greek theatre, The Archaeological Park of the Neapolis, Syracuse, Sicily, Italy (photo)

The Greek theatre, The Archaeological Park of the Neapolis, Syracuse, Sicily, Italy (photo)

GRL3961085

Nebula NGC 3372 in the Carene - The Carina nebula, NGC 3372 - The Carene nebula is located about 7000 years from the Earth. It is home to many hot stars, including the star Eta Carinae in the centre of the nebula. Image obtained by Siding Spring's 3.9m telescope. The brightest part of the Milky Way, as seen by the unaided eye, lies in the southern constellation Carina. Here there are an unusually large number of young, hot stars. Their radiation is rich in energetic ultraviolet light. Many of these stars were born within the spectacular Carinae nebula, seen here. The nebula is a cloud of glowing gas composed mostly of hydrogen. It excited by ultrviolet light from the embedded stars. This dostictive emission radiation is responsible for the red colour. About a quarter of the nebula is made of helium gas, the second most abundant element in the universe after hydrogen, and all the other chemical elements account for only a few percent of the total mass. The brightest star in the nebula is known as eta Carinae. This remarkable object is one of the most luminous and most massive stars known — Nebula NGC 3372 in the Carene - The Carina nebula, NGC 3372 - The Carene nebula is located about 7000 years from the Earth. It is home to many hot stars, including the star Eta Carinae in the centre of the nebula. Image obtained by Siding Spring's 3.9m telescope. The brightest part of the Milky Way, as seen by the unaided eye, lies in the southern constellation Carina. Here there are an unusually large number of young, hot stars. Their radiation is rich in energetic ultraviolet light. Many of these stars were born within the spectacular Carinae nebula, seen here. The nebula is a cloud of glowing gas composed mostly of hydrogen. It excited by ultrviolet light from the embedded stars. This dostictive emission radiation is responsible for the red colour. About a quarter of the nebula is made of helium gas, the second most abundant element in the universe after hydrogen, and all the other chemical elements account for only a few percent of the total mass. The brightest star in the nebula i

Nebula NGC 3372 in the Carene - The Carina nebula, NGC 3372 - The Carene nebula is located about 7000 years from the Earth. It is home to many hot stars, including the star Eta Carinae in the centre of the nebula. Image obtained by Siding Spring's 3.9m telescope. The brightest part of the Milky Way, as seen by the unaided eye, lies in the southern constellation Carina. Here there are an unusually large number of young, hot stars. Their radiation is rich in energetic ultraviolet light. Many of these stars were born within the spectacular Carinae nebula, seen here. The nebula is a cloud of glowing gas composed mostly of hydrogen. It excited by ultrviolet light from the embedded stars. This dostictive emission radiation is responsible for the red colour. About a quarter of the nebula is made of helium gas, the second most abundant element in the universe after hydrogen, and all the other chemical elements account for only a few percent of the total mass. The brightest star in the nebula i

PIX4618887

Super Massive Star Eta Carinae - Illustration

Super Massive Star Eta Carinae - Illustration

Miller, Ron (b.1947)

PIX7223355

Eta Carina Nebula, 2009 (digital photo)

Eta Carina Nebula, 2009 (digital photo)

Davis, Thomas (21st century)

MMM7342752

Birth of stars in the nebula NGC 3372 - Star formation in the Carina Nebula - Detail of the Carene nebula (NGC 3372) obtained by the Hubble space telescope. The image shows a column of gas eroded by ultraviolet radiation emitted by young stars. Jets are also visible, showing the presence of emerging stars. NGC 3372 is located about 7500 light years away from Earth. The colors used in this image correspond to the emissions of different gases: sulfur in red, hydrogen in green and oxygen in blue. The NASA Hubble Space Telescope photograph captures the chaotic activity atop a three - light - year - tall pillar of gas and dust that is being eaten away by the brilliant light from nearby bright stars. The pillar is also being assaulted from within, as infant stars buried inside it fire off jets of gas that can be seen streaming from towering peaks. This turbulent cosmic pinnacle lies within a tempestuous stellar nursery called the Carina Nebula, located 7,500 light - years away in the southern constellation Carina. The image marks the 20th anniversary of Hubble's launch and deployment into Earth orbit. Nestled inside this dense mountain are fledgling stars. Long streamers of gas can be seen shooting in opposite directions off the pedestal at the top of the image. Another pair of jets is visible at another peak near the center of the image. These jets are the signpost for new star birth. The jets are launched by swirling disks around the stars, as these disks allow material to slowly accrete onto the stars' surfaces. Hubble's Wide Field Camera 3 observed the pillar on Feb. 1 - 2, 2010. The colors in this composite image correspond to the glow of oxygen (blue), hydrogen and nitrogen (green), and sulfur (red) — Birth of stars in the nebula NGC 3372 - Star formation in the Carina Nebula - Detail of the Carene nebula (NGC 3372) obtained by the Hubble space telescope. The image shows a column of gas eroded by ultraviolet radiation emitted by young stars. Jets are also visible, showing the presence of emerging stars. NGC 3372 is located about 7500 light years away from Earth. The colors used in this image correspond to the emissions of different gases: sulfur in red, hydrogen in green and oxygen in blue. The NASA Hubble Space Telescope photograph captures the chaotic activity atop a three - light - year - tall pillar of gas and dust that is being eaten away by the brilliant light from nearby bright stars. The pillar is also being assaulted from within, as infant stars buried inside it fire off jets of gas that can be seen streaming from towering peaks. This turbulent cosmic pinnacle lies within a tempestuous stellar nursery called the Carina Nebula, located 7,500 light - years away in the souther

Birth of stars in the nebula NGC 3372 - Star formation in the Carina Nebula - Detail of the Carene nebula (NGC 3372) obtained by the Hubble space telescope. The image shows a column of gas eroded by ultraviolet radiation emitted by young stars. Jets are also visible, showing the presence of emerging stars. NGC 3372 is located about 7500 light years away from Earth. The colors used in this image correspond to the emissions of different gases: sulfur in red, hydrogen in green and oxygen in blue. The NASA Hubble Space Telescope photograph captures the chaotic activity atop a three - light - year - tall pillar of gas and dust that is being eaten away by the brilliant light from nearby bright stars. The pillar is also being assaulted from within, as infant stars buried inside it fire off jets of gas that can be seen streaming from towering peaks. This turbulent cosmic pinnacle lies within a tempestuous stellar nursery called the Carina Nebula, located 7,500 light - years away in the souther

PIX4619129

Birth of stars in the nebula NGC 3372 - Star formation in the Carina Nebula - Detail of the Carene nebula (NGC 3372) obtained by the Hubble space telescope. The image shows a column of gas eroded by ultraviolet radiation emitted by young stars. Jets are also visible, showing the presence of emerging stars. NGC 3372 is located about 7500 light years away from Earth. The colors used in this image correspond to the emissions of different gases: sulfur in red, hydrogen in green and oxygen in blue. The NASA Hubble Space Telescope photograph captures the chaotic activity atop a three - light - year - tall pillar of gas and dust that is being eaten away by the brilliant light from nearby bright stars. The pillar is also being assaulted from within, as infant stars buried inside it fire off jets of gas that can be seen streaming from towering peaks. This turbulent cosmic pinnacle lies within a tempestuous stellar nursery called the Carina Nebula, located 7,500 light - years away in the southern constellation Carina. Hubble's Wide Field Camera 3 observed the pillar on Feb. 1 - 2, 2010. The colors in this composite image correspond to the glow of oxygen (blue), hydrogen and nitrogen (green), and sulfur (red) — Birth of stars in the nebula NGC 3372 - Star formation in the Carina Nebula - Detail of the Carene nebula (NGC 3372) obtained by the Hubble space telescope. The image shows a column of gas eroded by ultraviolet radiation emitted by young stars. Jets are also visible, showing the presence of emerging stars. NGC 3372 is located about 7500 light years away from Earth. The colors used in this image correspond to the emissions of different gases: sulfur in red, hydrogen in green and oxygen in blue. The NASA Hubble Space Telescope photograph captures the chaotic activity atop a three - light - year - tall pillar of gas and dust that is being eaten away by the brilliant light from nearby bright stars. The pillar is also being assaulted from within, as infant stars buried inside it fire off jets of gas that can be seen streaming from towering peaks. This turbulent cosmic pinnacle lies within a tempestuous stellar nursery called the Carina Nebula, located 7,500 light - years away in the souther

Birth of stars in the nebula NGC 3372 - Star formation in the Carina Nebula - Detail of the Carene nebula (NGC 3372) obtained by the Hubble space telescope. The image shows a column of gas eroded by ultraviolet radiation emitted by young stars. Jets are also visible, showing the presence of emerging stars. NGC 3372 is located about 7500 light years away from Earth. The colors used in this image correspond to the emissions of different gases: sulfur in red, hydrogen in green and oxygen in blue. The NASA Hubble Space Telescope photograph captures the chaotic activity atop a three - light - year - tall pillar of gas and dust that is being eaten away by the brilliant light from nearby bright stars. The pillar is also being assaulted from within, as infant stars buried inside it fire off jets of gas that can be seen streaming from towering peaks. This turbulent cosmic pinnacle lies within a tempestuous stellar nursery called the Carina Nebula, located 7,500 light - years away in the souther

PIX4619114

Constellation of the Southern Cross - The Southern cross - Image obtained from Kangaroo Island, Australia. The Southern Cross and Carina from Kangaroo Island, Australia

Constellation of the Southern Cross - The Southern cross - Image obtained from Kangaroo Island, Australia. The Southern Cross and Carina from Kangaroo Island, Australia

David Miller

PIX4590228

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 four times as large and even brighter than the famous Orion Nebula, the Carina Nebula is much less well known, due to its location far in the Southern Hemisphere. It was discovered by Nicolas Louis de Lacaille in 1751 - 52 from the Cape of Good Hope. This is an amazingly bright nebula. This image is in the classic “” Hubble palette”” where SII is assigned to red, H - alpha to green, and OIII to blue. RGB frames were taken for star colors — 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

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

Most of the area of the southern Milky Way covered by this picture never sets for those of us who live at southern latitudes south on -30 degrees. The main constellations here are Centaurus, Crux and Carina, containing some of the most interesting, beautiful and bizzare astronomical objects, including the nearest stars. Alpha Centauri is at lower left and with its companion, beta points (more or less) to the Southern Cross, which in turn lies alongside the Coalsack, one of the nearest dust clouds. Further along the Milky Way is the astonishing Carina nebula, which is home to eta Carinae, probably the most massive star known, and a prime candidate for the next Galactic supernova. It is in Carina that the Sagittarius arm of our galaxy curves sharply away from us, so we see deep into a rich star-forming region.: The Lactee Way from Centaur to Carene - Souther Milky Way form Centaurus to Carina

Most of the area of the southern Milky Way covered by this picture never sets for those of us who live at southern latitudes south on -30 degrees. The main constellations here are Centaurus, Crux and Carina, containing some of the most interesting, beautiful and bizzare astronomical objects, including the nearest stars. Alpha Centauri is at lower left and with its companion, beta points (more or less) to the Southern Cross, which in turn lies alongside the Coalsack, one of the nearest dust clouds. Further along the Milky Way is the astonishing Carina nebula, which is home to eta Carinae, probably the most massive star known, and a prime candidate for the next Galactic supernova. It is in Carina that the Sagittarius arm of our galaxy curves sharply away from us, so we see deep into a rich star-forming region.: The Lactee Way from Centaur to Carene - Souther Milky Way form Centaurus to Carina

PIX4635895

Constellation of the Southern Cross and False Cross - The Southern Cross and the False Cross - The Southern Cross on the left can sometimes be confused with a near asterism, the false cross on the bottom right. The Southern Cross and the False Cross, from the Coal Sack to the Vel, centred on the theta Car cluste

Constellation of the Southern Cross and False Cross - The Southern Cross and the False Cross - The Southern Cross on the left can sometimes be confused with a near asterism, the false cross on the bottom right. The Southern Cross and the False Cross, from the Coal Sack to the Vel, centred on the theta Car cluste

PIX4590243

Nebula NGC 3372 in the Carene in fake colors - NGC 3372 Carina nebula in narrow band - The nebula of the Carene is located about 8000 years - light from Earth. It is home to many hot stars, including the massive star Eta Carinae in the centre of the nebula. Image obtained by the 1.2m Schmidt UK Telescope of Siding Spring through 3 different filters that highlight oxygen, hydrogen, and sulfur. Although no bright naked - eye stars are associated with the Carina nebula now, 150 years ago there blazed forth here one of the most unusual and peculiar stars ever seen. The star is known as Eta Carinae and for a few months in 1843 it was the second or third brightest star in the sky. Since then it has faded and is today about 1000 times fainter than it was at its brightest as the nebula it created during its outburst has cooled and become opaque. The whole region around Eta Carinae is rich in hot stars of which Eta is an extreme example and it is their combined radiation that produces the spectacular Carina nebula that dominates this picture. The nebula and its peculiar star are about 8000 light years away — Nebula NGC 3372 in the Carene in fake colors - NGC 3372 Carina nebula in narrow band - The nebula of the Carene is located about 8000 years - light from Earth. It is home to many hot stars, including the massive star Eta Carinae in the centre of the nebula. Image obtained by the 1.2m Schmidt UK Telescope of Siding Spring through 3 different filters that highlight oxygen, hydrogen, and sulfur. Although no bright naked - eye stars are associated with the Carina nebula now, 150 years ago there blazed forth here one of the most unusual and peculiar stars ever seen. The star is known as Eta Carinae and for a few months in 1843 it was the second or third brightest star in the sky. Since then it has faded and is today about 1000 times fainter than it was at its brightest as the nebula it created during its outburst has cooled and become opaque. The whole region around Eta Carinae is rich in hot stars of which Eta is an extreme example and it is their combined radiation that produces the spect

Nebula NGC 3372 in the Carene in fake colors - NGC 3372 Carina nebula in narrow band - The nebula of the Carene is located about 8000 years - light from Earth. It is home to many hot stars, including the massive star Eta Carinae in the centre of the nebula. Image obtained by the 1.2m Schmidt UK Telescope of Siding Spring through 3 different filters that highlight oxygen, hydrogen, and sulfur. Although no bright naked - eye stars are associated with the Carina nebula now, 150 years ago there blazed forth here one of the most unusual and peculiar stars ever seen. The star is known as Eta Carinae and for a few months in 1843 it was the second or third brightest star in the sky. Since then it has faded and is today about 1000 times fainter than it was at its brightest as the nebula it created during its outburst has cooled and become opaque. The whole region around Eta Carinae is rich in hot stars of which Eta is an extreme example and it is their combined radiation that produces the spect

PIX4619010

Constellations of Centaur and Southern Cross - Constellations Centaurus and Crux - Visible also, the constellations of the Compas, Southern Triangle, Fly. Image obtained from New Zealand. Constellations also visible in this image: Circinus, Triangulum Australe and Musca. Image obtained from New Zealand

Constellations of Centaur and Southern Cross - Constellations Centaurus and Crux - Visible also, the constellations of the Compas, Southern Triangle, Fly. Image obtained from New Zealand. Constellations also visible in this image: Circinus, Triangulum Australe and Musca. Image obtained from New Zealand

Minoru Yoneto

PIX4589724

Detail of the nebula NGC 3372 in the Carene - Eta Carinae nebula detail - Detail of the nebula NGC 3372 near the star Eta Carinae (off field). Region of star formation. Image obtained by the Hubble Space Telescope in April 1999. The Hubble Space Telescope image reveals complex structure in the Carina Nebula (NGC 3372). The picture is dominated by a large, approximately circular feature, which is part of the Keyhole Nebula. This region, about 8000 light - years from Earth, is located adjacent to the famous explosive variable star Eta Carinae, which lies just outside the field of view towards the upper right. The Carina Nebula also contains several other stars that are among the hottest and most massive known, each about 10 times as hot, and 100 times as massive, as our Sun

Detail of the nebula NGC 3372 in the Carene - Eta Carinae nebula detail - Detail of the nebula NGC 3372 near the star Eta Carinae (off field). Region of star formation. Image obtained by the Hubble Space Telescope in April 1999. The Hubble Space Telescope image reveals complex structure in the Carina Nebula (NGC 3372). The picture is dominated by a large, approximately circular feature, which is part of the Keyhole Nebula. This region, about 8000 light - years from Earth, is located adjacent to the famous explosive variable star Eta Carinae, which lies just outside the field of view towards the upper right. The Carina Nebula also contains several other stars that are among the hottest and most massive known, each about 10 times as hot, and 100 times as massive, as our Sun

PIX4618927

Lactee Way and Constellation of the Southern Cross - The Southern Cross and Carina from Australia

Lactee Way and Constellation of the Southern Cross - The Southern Cross and Carina from Australia

Sebastian Voltmer

PIX4590299

Heart of the nebula NGC 3372 in the Carene - Eta Carinae and the Keyhole Nebula - The nebula of the Carene is located about 7000 years - light from the Earth. It is home to many hot stars, including the star Eta Carinae visible in the centre left of the image. Eta Carinae is a supermassive star (100 to 150 times the mass of the Sun). Image obtained by Siding Spring's 3.9m telescope. This wonderfully complex region at the heart of the NGC 3372 nebula was first described in detail by Sir John Herschel in 1838. He saw the bright circular shell visible in the upper part of the picture extending to the south to form a keyhole - shaped nebula. This luminous outline is no longer seen and the southern extension appears only as a dark dust cloud. It seems that the curious, explosively variable star Eta Carinae has enveloped itself in a cocoon of obscuring matter in the years since Herschel's observations and light from the star is no longer able to illuminate the rim of the dust cloud. The nebula thrown off by eta Car in Herschel's time has grown to the tiny orange nebula seen to the left of the dust cloud and is known as the Homunculus nebula — Heart of the nebula NGC 3372 in the Carene - Eta Carinae and the Keyhole Nebula - The nebula of the Carene is located about 7000 years - light from the Earth. It is home to many hot stars, including the star Eta Carinae visible in the centre left of the image. Eta Carinae is a supermassive star (100 to 150 times the mass of the Sun). Image obtained by Siding Spring's 3.9m telescope. This wonderfully complex region at the heart of the NGC 3372 nebula was first described in detail by Sir John Herschel in 1838. He saw the bright circular shell visible in the upper part of the picture extending to the south to form a keyhole - shaped nebula. This luminous outline is no longer seen and the southern extension appears only as a dark dust cloud. It seems that the curious, explosively variable star Eta Carinae has enveloped itself in a cocoon of obscuring matter in the years since Herschel's observations and light from the star is no longer able to illuminate the rim of the dust cloud. The nebu

Heart of the nebula NGC 3372 in the Carene - Eta Carinae and the Keyhole Nebula - The nebula of the Carene is located about 7000 years - light from the Earth. It is home to many hot stars, including the star Eta Carinae visible in the centre left of the image. Eta Carinae is a supermassive star (100 to 150 times the mass of the Sun). Image obtained by Siding Spring's 3.9m telescope. This wonderfully complex region at the heart of the NGC 3372 nebula was first described in detail by Sir John Herschel in 1838. He saw the bright circular shell visible in the upper part of the picture extending to the south to form a keyhole - shaped nebula. This luminous outline is no longer seen and the southern extension appears only as a dark dust cloud. It seems that the curious, explosively variable star Eta Carinae has enveloped itself in a cocoon of obscuring matter in the years since Herschel's observations and light from the star is no longer able to illuminate the rim of the dust cloud. The nebu

PIX4618913

Nebula NGC 3372 in the Carene - The Eta Carinae Nebula and Trumpler 14 - The Carene nebula is located about 7000 years from the Earth. It is home to many hot stars, including the star Eta Carinae (lower left, the brightest star in the picture). Top right is a cluster of young stars, Trumpler 14. Image obtained by Siding Spring's 3.9m telescope. In the small region pictured here are three of the brightest stars known in our Galaxy, each a million times more luminous than the Sun. To the left of the picture is an even more extreme star, Eta Carinae itself, shrouded in a small bright irregular nebula of its own making. In the upper right of the photograph is Trumpler 14, a cluster of very young stars which appears to be associated with a number of bright - edged 'elephant trunk' dust lanes, typical of star - forming regions. All these objects and most of the bright stars scattered across the face of the nebula are together in space at a distance of about 7000 light years. Despite this distance, the Carina nebula is clearly visible to the unaided eye to those of us who live in the southern hemisphere — Nebula NGC 3372 in the Carene - The Eta Carinae Nebula and Trumpler 14 - The Carene nebula is located about 7000 years from the Earth. It is home to many hot stars, including the star Eta Carinae (lower left, the brightest star in the picture). Top right is a cluster of young stars, Trumpler 14. Image obtained by Siding Spring's 3.9m telescope. In the small region pictured here are three of the brightest stars known in our Galaxy, each a million times more luminous than the Sun. To the left of the picture is an even more extreme star, Eta Carinae itself, shrouded in a small bright irregular nebula of its own making. In the upper right of the photograph is Trumpler 14, a cluster of very young stars which appears to be associated with a number of bright - edged 'elephant trunk' dust lanes, typical of star - forming regions. All these objects and most of the bright stars scattered across the face of the nebula are together in space at a distance of about 7000 light years. Despite this dis

Nebula NGC 3372 in the Carene - The Eta Carinae Nebula and Trumpler 14 - The Carene nebula is located about 7000 years from the Earth. It is home to many hot stars, including the star Eta Carinae (lower left, the brightest star in the picture). Top right is a cluster of young stars, Trumpler 14. Image obtained by Siding Spring's 3.9m telescope. In the small region pictured here are three of the brightest stars known in our Galaxy, each a million times more luminous than the Sun. To the left of the picture is an even more extreme star, Eta Carinae itself, shrouded in a small bright irregular nebula of its own making. In the upper right of the photograph is Trumpler 14, a cluster of very young stars which appears to be associated with a number of bright - edged 'elephant trunk' dust lanes, typical of star - forming regions. All these objects and most of the bright stars scattered across the face of the nebula are together in space at a distance of about 7000 light years. Despite this dis

PIX4618903

View of the latomie (prisons in quarries), The Archaeological Park of the Neapolis, Syracuse, Sicily, Italy (photo)

View of the latomie (prisons in quarries), The Archaeological Park of the Neapolis, Syracuse, Sicily, Italy (photo)

GRL3961091

Nebula NGC 3372 in the Carene in false colours - NGC 3372 Carina nebula - Image of the nebula of the Carene (NGC 3372), a very vast region of star formation, obtained by combining light through 3 different filters that highlight oxygen in blue, hydrogen in green, and sulfur in red. The colors also represent different gas temperatures, warm, blue, colder in red. The bright star in the center of the image is Eta Carinae, a super massive star. Image obtained with the Curtis - Schmidt telescope of the Cerro Tololo Observatory. This image shows a giant star - forming region in the southern sky known as the Carina Nebula (NGC 3372), combining the light from 3 different filters tracing emission from oxygen (blue), hydrogen (green), and sulphur (red). The color is also representative of the temperature in the ionized gas: blue is relatively hot and red is cooler. The Carina Nebula is a good example of how very massive stars rip apart the molecular clouds that give birth to them. The bright star near the center of the image is Eta Carinae, which is one of the most massive and luminous stars known. This picture is a composite of several exposures made with the Curtis - Schmidt telescope at the Cerro Tololo Interamerican Observatory — Nebula NGC 3372 in the Carene in false colours - NGC 3372 Carina nebula - Image of the nebula of the Carene (NGC 3372), a very vast region of star formation, obtained by combining light through 3 different filters that highlight oxygen in blue, hydrogen in green, and sulfur in red. The colors also represent different gas temperatures, warm, blue, colder in red. The bright star in the center of the image is Eta Carinae, a super massive star. Image obtained with the Curtis - Schmidt telescope of the Cerro Tololo Observatory. This image shows a giant star - forming region in the southern sky known as the Carina Nebula (NGC 3372), combining the light from 3 different filters tracing emission from oxygen (blue), hydrogen (green), and sulphur (red). The color is also representative of the temperature in the ionized gas: blue is relatively hot and red is cooler. The Carina Nebula is a good example of how very massive stars rip apart the molecular clouds that give birth to them. The bright sta

Nebula NGC 3372 in the Carene in false colours - NGC 3372 Carina nebula - Image of the nebula of the Carene (NGC 3372), a very vast region of star formation, obtained by combining light through 3 different filters that highlight oxygen in blue, hydrogen in green, and sulfur in red. The colors also represent different gas temperatures, warm, blue, colder in red. The bright star in the center of the image is Eta Carinae, a super massive star. Image obtained with the Curtis - Schmidt telescope of the Cerro Tololo Observatory. This image shows a giant star - forming region in the southern sky known as the Carina Nebula (NGC 3372), combining the light from 3 different filters tracing emission from oxygen (blue), hydrogen (green), and sulphur (red). The color is also representative of the temperature in the ionized gas: blue is relatively hot and red is cooler. The Carina Nebula is a good example of how very massive stars rip apart the molecular clouds that give birth to them. The bright sta

PIX4618865

Terrassa's citizens show their anti-ETA banners (Peace yes, ETA no) during the silent protest agains.., 2000 (photo)

Terrassa's citizens show their anti-ETA banners (Peace yes, ETA no) during the silent protest agains.., 2000 (photo)

Gustau Nacarino

REU7471736

Etw or Eta Hoffmann - German Romantic writer and composer

Etw or Eta Hoffmann - German Romantic writer and composer

EPL6802893

Constellations of the Fly and the Southern Cross - Constellations of Musca and the Southern cross - The Southern Cross and the Alpha and Beta Stars of Centaur. Below, the constellation of the Fly. In contrast to adjacent Crux, Musca (The Fly) is a much less obvious, less distinguished and less useful constellation that first appeared in Johann Bayer's 1603 Uranometria. It is one of a dozen created by the Dutch explorers/navigators Pieter Dirkszoon Keyser and Frederick de Houtman on their voyages into the south seas in the late 16th century

Constellations of the Fly and the Southern Cross - Constellations of Musca and the Southern cross - The Southern Cross and the Alpha and Beta Stars of Centaur. Below, the constellation of the Fly. In contrast to adjacent Crux, Musca (The Fly) is a much less obvious, less distinguished and less useful constellation that first appeared in Johann Bayer's 1603 Uranometria. It is one of a dozen created by the Dutch explorers/navigators Pieter Dirkszoon Keyser and Frederick de Houtman on their voyages into the south seas in the late 16th century

PIX4592314

Nebula NGC 3372 in the Carene - Carina nebula NGC 3372 - The Carene nebula is located about 7500 years from the Earth. It is home to many hot stars, including the massive star Eta Carinae at the bottom left of the image, the clusters of young stars Trumpler 14 (above the right of eta carinae) and Collinder 228 (below eta carinae). Image obtained by the 2.2m ESO/MPG telescope of the La Silla Observatory in Chile. Colour - composite image of the Carina Nebula, revealing exquisite details in the stars and dust of the region. Several well known astronomical objects can be seen in this wide field image: to the bottom left of the image is one of the most impressive binary stars in the Universe, Eta Carinae, with the famous Keyhole Nebula just adjacent to the star. The collection of very bright, young stars above and to the right of Eta Carinae is the open star cluster Trumpler 14. A second open star cluster, Collinder 228 is also seen in the image, just below Eta Carinae. North is up and East is to the left. The field of view is 0.55 x 0.55 degrees, covering a 144 x 144 light - year region at the distance of the nebula. This image was produced by combining exposures through six different filters from the Wide Field Imager (WFI), attached to the 2.2 m ESO/MPG telescope at Eso's La Silla Observatory, in Chile — Nebula NGC 3372 in the Carene - Carina nebula NGC 3372 - The Carene nebula is located about 7500 years from the Earth. It is home to many hot stars, including the massive star Eta Carinae at the bottom left of the image, the clusters of young stars Trumpler 14 (above the right of eta carinae) and Collinder 228 (below eta carinae). Image obtained by the 2.2m ESO/MPG telescope of the La Silla Observatory in Chile. Colour - composite image of the Carina Nebula, revealing exquisite details in the stars and dust of the region. Several well known astronomical objects can be seen in this wide field image: to the bottom left of the image is one of the most impressive binary stars in the Universe, Eta Carinae, with the famous Keyhole Nebula just adjacent to the star. The collection of very bright, young stars above and to the right of Eta Carinae is the open star cluster Trumpler 14. A second open star cluster, Collinder 228 is also seen in the image, just below Eta Carinae. North is up and Eas

Nebula NGC 3372 in the Carene - Carina nebula NGC 3372 - The Carene nebula is located about 7500 years from the Earth. It is home to many hot stars, including the massive star Eta Carinae at the bottom left of the image, the clusters of young stars Trumpler 14 (above the right of eta carinae) and Collinder 228 (below eta carinae). Image obtained by the 2.2m ESO/MPG telescope of the La Silla Observatory in Chile. Colour - composite image of the Carina Nebula, revealing exquisite details in the stars and dust of the region. Several well known astronomical objects can be seen in this wide field image: to the bottom left of the image is one of the most impressive binary stars in the Universe, Eta Carinae, with the famous Keyhole Nebula just adjacent to the star. The collection of very bright, young stars above and to the right of Eta Carinae is the open star cluster Trumpler 14. A second open star cluster, Collinder 228 is also seen in the image, just below Eta Carinae. North is up and Eas

PIX4619045

Portrait of Mrs Margaret Gainsborough, c.1778 (oil on canvas)

Portrait of Mrs Margaret Gainsborough, c.1778 (oil on canvas)

Gainsborough, Thomas (1727-88)

COU29613

E.T.A. Hoffmann

E.T.A. Hoffmann

XLA3752899

Early light bulbs by Thomas Alva Edison (1847-1931) (glass & wood)

Early light bulbs by Thomas Alva Edison (1847-1931) (glass & wood)

NRM3197

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