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50,772 médias trouvés pour 'Star'

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Shooting star rain, Perseides - Perseid meteor shower - Shooting star rain. 12-13 August 2010. Perseid meteors on August 12, 2010

Shooting star rain, Perseides - Perseid meteor shower - Shooting star rain. 12-13 August 2010. Perseid meteors on August 12, 2010

Sebastian Voltmer

PIX4598956

Shooting star rain, Perseides - Perseid meteor shower - Shooting star rain seen from the top of Mount Omu (2507 metres) in Romania. Composite image of perseid meteors seen from the Omu summit (2507m) in Romania

Shooting star rain, Perseides - Perseid meteor shower - Shooting star rain seen from the top of Mount Omu (2507 metres) in Romania. Composite image of perseid meteors seen from the Omu summit (2507m) in Romania

Alex Tudorica

PIX4598903

The Star, or Dancer on the stage, c.1876-77 (pastel on paper)

The Star, or Dancer on the stage, c.1876-77 (pastel on paper)

Degas, Edgar (1834-1917)

BAL35845

Shooting Star Rain - Geminides - Geminid Meteor Shower: Shooting stars of the Geminides swarm cross the sky. 13 December 2017. Composite image. This is a composite of multiple Geminid meteors captured from Enisala, Dobrogea, Romania. A 15 mm lens was used

Shooting Star Rain - Geminides - Geminid Meteor Shower: Shooting stars of the Geminides swarm cross the sky. 13 December 2017. Composite image. This is a composite of multiple Geminid meteors captured from Enisala, Dobrogea, Romania. A 15 mm lens was used

Alex Conu

PIX4599214

Colliding neutron stars and gravitational waves - Colliding neutron stars and gravitational waves: Artist's view of two colliding neutron stars about to merge and explode in kilonova. This type of event produces gravitational waves and a gamma ray burst. This artist's impression shows two tiny but very dense neutron stars at the point at which they merge and explode as a kilonova. Such a very rare event is expected to produce both gravitational waves and a short gamma-ray burst, both of which were observed on 17 August 2017 by LIGO-Virgo and Fermi/INTEGRAL respectively. Subsequent detailed observations with many ESO telescopes confirmed that this object, seen in the galaxy NGC 4993 about 130 million light-years from the Earth, is indeed a kilonova. Such objects are the main source of very heavy chemical elements, such as gold and platinum, in the Universe

Colliding neutron stars and gravitational waves - Colliding neutron stars and gravitational waves: Artist's view of two colliding neutron stars about to merge and explode in kilonova. This type of event produces gravitational waves and a gamma ray burst. This artist's impression shows two tiny but very dense neutron stars at the point at which they merge and explode as a kilonova. Such a very rare event is expected to produce both gravitational waves and a short gamma-ray burst, both of which were observed on 17 August 2017 by LIGO-Virgo and Fermi/INTEGRAL respectively. Subsequent detailed observations with many ESO telescopes confirmed that this object, seen in the galaxy NGC 4993 about 130 million light-years from the Earth, is indeed a kilonova. Such objects are the main source of very heavy chemical elements, such as gold and platinum, in the Universe

PIX4607586

The Star, 1876-77 (pastel on paper)

The Star, 1876-77 (pastel on paper)

Degas, Edgar (1834-1917)

Photo Josse

JLJ4653424

Morning Star, 1902 (colour litho)

Morning Star, 1902 (colour litho)

Mucha, Alphonse Marie (1860-1939)

MCA176930

Shooting star rain -Leonides 11/2001 - Leonid meteor shower Nov 2001 - 15 minutes in the direction of the constellation Lion. A fifteen minute exposure captures the shower radiant in Leo along with dozens on meteor trails. Nov 19, 2001

Shooting star rain -Leonides 11/2001 - Leonid meteor shower Nov 2001 - 15 minutes in the direction of the constellation Lion. A fifteen minute exposure captures the shower radiant in Leo along with dozens on meteor trails. Nov 19, 2001

F.Espenak

PIX4598750

Shooting star rain - Leonid Meteor Storm - Leonides in front of the constellation Orion, November 2001. Leonid meteor storm. November 200

Shooting star rain - Leonid Meteor Storm - Leonides in front of the constellation Orion, November 2001. Leonid meteor storm. November 200

Sebastian Voltmer

PIX4598786

Shooting Star Rain - Night of the Falling Stars Nov.18 2001 - Leonid Rain. November 18, 2001, Joshua tree, California. Leonid Meteor Shower, on November 18, 2001. Joshua Tree national park, California

Shooting Star Rain - Night of the Falling Stars Nov.18 2001 - Leonid Rain. November 18, 2001, Joshua tree, California. Leonid Meteor Shower, on November 18, 2001. Joshua Tree national park, California

PIX4598821

Shooting star rain, Perseides - Perseid meteor shower - Shooting star rain seen from the top of Mount Omu (2507 metres) in Romania. Composite image of perseid meteors seen from the Omu summit (2507m) in Romania

Shooting star rain, Perseides - Perseid meteor shower - Shooting star rain seen from the top of Mount Omu (2507 metres) in Romania. Composite image of perseid meteors seen from the Omu summit (2507m) in Romania

Alex Tudorica

PIX4598894

Star Trek

Star Trek

DIL2724806

Falling Star

premium — Falling Star

Wright, H. David (b.1942)

DWT5675298

Night Star, 1889 (oil on canvas)

Night Star, 1889 (oil on canvas)

Gogh, Vincent van (1853-90)

Luisa Ricciarini

LRI4634367

Star of Asia (sapphire)

Star of Asia (sapphire)

XBP236613

The Polar Star, 1920

The Polar Star, 1920

Shackleton, William (1872-1933)

BRA37684

Double star 61 Cygni - Binary star 61 Cygni - 61 Cygni is a binary system of two stars comparable to the Sun. Located 11.4 years - light from the Earth, 61 Cygni is the first star (after the Sun) whose distance was measured thanks to its parallax. Image obtained by the Oschin telescope of Mount Palomar through several filters and composed. 61 Cygni is a binary star system in the Constellation Cygnus at approximately 11.4 light - years distance from Earth. Composite image obtained by the Oschin telescope refractor at the Palomar Observatory, USA

Double star 61 Cygni - Binary star 61 Cygni - 61 Cygni is a binary system of two stars comparable to the Sun. Located 11.4 years - light from the Earth, 61 Cygni is the first star (after the Sun) whose distance was measured thanks to its parallax. Image obtained by the Oschin telescope of Mount Palomar through several filters and composed. 61 Cygni is a binary star system in the Constellation Cygnus at approximately 11.4 light - years distance from Earth. Composite image obtained by the Oschin telescope refractor at the Palomar Observatory, USA

Vincent Toporenko

PIX4572201

Circumpolar, Pasargades, Iran - Pasargad and circumpolar - Long pose on the stars around the polar star. In the foreground, the ruins of the palace of Pasargades (Iran). Long exposure image of stars around the polaris star. Foreground is a 2500 - year old palace in Pasargad, Fars province, southen Iran

Circumpolar, Pasargades, Iran - Pasargad and circumpolar - Long pose on the stars around the polar star. In the foreground, the ruins of the palace of Pasargades (Iran). Long exposure image of stars around the polaris star. Foreground is a 2500 - year old palace in Pasargad, Fars province, southen Iran

Oshin Zakarian

PIX4580688

Telescope E-ELT -Artist's view - E-ELT concept: Artist's view of the E-ELT (European Extremely Large Telescope), a telescope project measuring 39 metres in diameter. Its main mirror will consist of 906 hexagonal mirrors assembled together, and its total surface will be equal to that of a football field. The Cerro Amazones mountain in the Chilean desert, near Eso's Paranal Observatory, will be the site for the European Extremely Large Telescope (E-ELT), which, with its 39-metre diameter mirror, will be the world's biggest eye on the sky. Here, an artist's rendering shows how the telescope will look on the mountain when it is complete in 2024

Telescope E-ELT -Artist's view - E-ELT concept: Artist's view of the E-ELT (European Extremely Large Telescope), a telescope project measuring 39 metres in diameter. Its main mirror will consist of 906 hexagonal mirrors assembled together, and its total surface will be equal to that of a football field. The Cerro Amazones mountain in the Chilean desert, near Eso's Paranal Observatory, will be the site for the European Extremely Large Telescope (E-ELT), which, with its 39-metre diameter mirror, will be the world's biggest eye on the sky. Here, an artist's rendering shows how the telescope will look on the mountain when it is complete in 2024

PIX4624162

Shooting Star - Quadrantides - Bright Quadrantid meteors - Two brilliant shooting stars of the Quadrantid swarm cross the star sky. Mojave Desert, California. January 5, 2012. Two bright meteors streak the sky above Mojave desert in California. The image is made during the peak of the 2012 Quadrantid meteor shower on january 5

Shooting Star - Quadrantides - Bright Quadrantid meteors - Two brilliant shooting stars of the Quadrantid swarm cross the star sky. Mojave Desert, California. January 5, 2012. Two bright meteors streak the sky above Mojave desert in California. The image is made during the peak of the 2012 Quadrantid meteor shower on january 5

PIX4599087

Star Vega in Lyra - Star Vega in Lyra - Vega (Alpha Lyrae) is the main star of the constellation Lyra, located only 25.4 light years from the Sun. It is the second brightest star in the northern hemisphere after Sirius. Due to the precession of the equinoxes, Vega will take the place of the polar star indicating the north in the year 14,000. Vega (Alpha Lyrae) is the brightest star of Lyra constellation, located at 25.4 light years from the Sun. It is the second most luminous star in northern hemisphere. Because of the precession of the equinoxes, Vega will point north celestial pole in year 14,000

Star Vega in Lyra - Star Vega in Lyra - Vega (Alpha Lyrae) is the main star of the constellation Lyra, located only 25.4 light years from the Sun. It is the second brightest star in the northern hemisphere after Sirius. Due to the precession of the equinoxes, Vega will take the place of the polar star indicating the north in the year 14,000. Vega (Alpha Lyrae) is the brightest star of Lyra constellation, located at 25.4 light years from the Sun. It is the second most luminous star in northern hemisphere. Because of the precession of the equinoxes, Vega will point north celestial pole in year 14,000

Jerry Lodriguss

PIX4571757

Circumpolar - Star trails around north celestial pole - Photographic pose around the polar star. Long exposure image; because the earth rotates on it's own axis, during the exposure the stars seem to revolve around a point in the sky very near to Polaris

Circumpolar - Star trails around north celestial pole - Photographic pose around the polar star. Long exposure image; because the earth rotates on it's own axis, during the exposure the stars seem to revolve around a point in the sky very near to Polaris

B&S.Fletcher

PIX4580204

Comete Hale - Bopp - 08/04/1997 - Comet Hale - Bopp in Perseus. April 8, 1997 - Comete Hale - Bopp in the constellation Persei

Comete Hale - Bopp - 08/04/1997 - Comet Hale - Bopp in Perseus. April 8, 1997 - Comete Hale - Bopp in the constellation Persei

Jerry Lodriguss

PIX4569698

Constellations of the Great Bear and Little Bear - Constellations of Ursa Major and Ursa Minor - On the right, the large trolley, asterism of the Great Bear; on the left, the small trolley, asterism of the Little Bear that houses the polar star, the star that currently indicates the position of the northern Celestial pole, at the end of the handle of the pan

Constellations of the Great Bear and Little Bear - Constellations of Ursa Major and Ursa Minor - On the right, the large trolley, asterism of the Great Bear; on the left, the small trolley, asterism of the Little Bear that houses the polar star, the star that currently indicates the position of the northern Celestial pole, at the end of the handle of the pan

PIX4591367

RMS Titanic of the White Star Line (litho)

RMS Titanic of the White Star Line (litho)

English Photographer, (20th century)

KWE270889

Star Trek: The Motion Picture by Robert Wise, 1979

Star Trek: The Motion Picture by Robert Wise, 1979

DIL4059245

Shooting star rain -Leonides 11/1999 - Leonid meteor shower Nov 1999 - Shooting star rain seen above the caravan of Deh Namak, Iran. Leonid meteor shower of Nov. 1999, Deh-Namak caravansary, Semnan, Iran

Shooting star rain -Leonides 11/1999 - Leonid meteor shower Nov 1999 - Shooting star rain seen above the caravan of Deh Namak, Iran. Leonid meteor shower of Nov. 1999, Deh-Namak caravansary, Semnan, Iran

Oshin Zakarian

PIX4598737

Orion Nebula - the trapeze - The Trapezium region in M42 - Located 1500 years - light, Orion Nebula is the closest region of formation of stars of the Sun. In the center of the picture, the Trapeze of Orion. The Trapeze is among the youngest known open clusters, it is made up of 4 massive stars that make the nebula shine. The central 'star' of the three groups forming the asterism of Orion's sword is in reality a nebula, and is clearly nebulous to the unaided eye. At the heart of the most luminous nebulosity shimmer a handful of stars known as the Trapezium cluster, visible in binoculars. These are the brightest members of a substantial cluster of stars, most of which are still hidden in the dusty recesses of the Orion nebula against which they are seen. The stars of the Trapezium provide much of the energy which makes the brilliant Orion Nebula visible and are at a distance of about 1500 light years

Orion Nebula - the trapeze - The Trapezium region in M42 - Located 1500 years - light, Orion Nebula is the closest region of formation of stars of the Sun. In the center of the picture, the Trapeze of Orion. The Trapeze is among the youngest known open clusters, it is made up of 4 massive stars that make the nebula shine. The central 'star' of the three groups forming the asterism of Orion's sword is in reality a nebula, and is clearly nebulous to the unaided eye. At the heart of the most luminous nebulosity shimmer a handful of stars known as the Trapezium cluster, visible in binoculars. These are the brightest members of a substantial cluster of stars, most of which are still hidden in the dusty recesses of the Orion nebula against which they are seen. The stars of the Trapezium provide much of the energy which makes the brilliant Orion Nebula visible and are at a distance of about 1500 light years

Sebastian Voltmer

PIX4617828

The evolution of stars - Illustration - The evolution of the stars - Illustration - All stars are born in interstellar clouds but according to their masses they will follow different destinies

The evolution of stars - Illustration - The evolution of the stars - Illustration - All stars are born in interstellar clouds but according to their masses they will follow different destinies

P. Carril

PIX4573022

Mars - Illustration - Mars - Illustration - Artist's view of the planet Mars. The three volcanoes of Tharsis and Olympus Mons are visible on the left. In the centre is the great canyon Valles Marineris. A “” full””” Mars. In this image the massive volcano Olympus Mons is clearly visible upper left of center, while near center are the three Tharsis Montes volcanoes. All these volcanoes are believed to be extinct. To the right of the Tharsis Montes are the deep canyons of Valles Marineris, a meandering network of channels as long as the United States is wide. Mars has been known historically as a bright, reddish “” star”” in Earth's sky. The ruddy hue is due to the presence of iron oxide (i.e., rust) on the martian surface. Mars is often host to white clouds of water - ice crystals (like the high - altitude cirrus clouds on Earth) and experiences seasonal dust storms that can cover the entire planet

Mars - Illustration - Mars - Illustration - Artist's view of the planet Mars. The three volcanoes of Tharsis and Olympus Mons are visible on the left. In the centre is the great canyon Valles Marineris. A “” full””” Mars. In this image the massive volcano Olympus Mons is clearly visible upper left of center, while near center are the three Tharsis Montes volcanoes. All these volcanoes are believed to be extinct. To the right of the Tharsis Montes are the deep canyons of Valles Marineris, a meandering network of channels as long as the United States is wide. Mars has been known historically as a bright, reddish “” star”” in Earth's sky. The ruddy hue is due to the presence of iron oxide (i.e., rust) on the martian surface. Mars is often host to white clouds of water - ice crystals (like the high - altitude cirrus clouds on Earth) and experiences seasonal dust storms that can cover the entire planet

Walter B Myers

PIX4616786

Ms Hunter 229 f.6v Capricorn, from the Hunterian Psalter, c.1170 (pen & ink and tempera on vellum) (detail)

Ms Hunter 229 f.6v Capricorn, from the Hunterian Psalter, c.1170 (pen & ink and tempera on vellum) (detail)

English School, (12th century)

GUL232032

Circumpolar above the dome of the 1.93 m of the Observatory of Haute - Provence - Haute - Provence Observatory, the 1.93 m telescope dome - Photographic pose showing the apparent rotation of stars around the polar star (circumpolar). Below, the dome of the 1.93 m telescope of the Observatory of Haute Provence. This is where the first exoplanet was discovered in 1995. The Observatory of Haute-Provence is located in the south-east of France, near the village of St. Michel l'Observatoire, a hundred kilometers north of Marseille, on a plateau with an average altitude of 650 meters. Long exposure image of starry sky around the pole star (circumpolar). Below, the 1.93 m telescope dome. Here has been discovered the first extrasolar planet (51 Peg b) in 1995. OHP is situated in the southeast of France, it lies at an altitude of about 650 m, near the village of Saint-Michel l'Observatoire

Circumpolar above the dome of the 1.93 m of the Observatory of Haute - Provence - Haute - Provence Observatory, the 1.93 m telescope dome - Photographic pose showing the apparent rotation of stars around the polar star (circumpolar). Below, the dome of the 1.93 m telescope of the Observatory of Haute Provence. This is where the first exoplanet was discovered in 1995. The Observatory of Haute-Provence is located in the south-east of France, near the village of St. Michel l'Observatoire, a hundred kilometers north of Marseille, on a plateau with an average altitude of 650 meters. Long exposure image of starry sky around the pole star (circumpolar). Below, the 1.93 m telescope dome. Here has been discovered the first extrasolar planet (51 Peg b) in 1995. OHP is situated in the southeast of France, it lies at an altitude of about 650 m, near the village of Saint-Michel l'Observatoire

Patrick Lécureuil

PIX4655293

Globular cluster M5 in Serpens - Globular cluster M5 in Serpens - This cluster of stars is located about 25,000 light years away from Earth. It is one of the most extensive (165 years - light) and one of the oldest known globular clusters. Globular clusters are generally peoples of very old stars, but here the Hubble space telescope has identified some young stars, blue stragglers. The globular cluster Messier 5, shown here in this NASA/ESA Hubble Space Telescope image, is one of the oldest belonging to the Milky Way. The majority of its stars formed more than 12 billion years ago, but there are some unexpected newcomers on the scene, adding some vitality to this aging population. Stars in globular clusters form in the same stellar nursery and grow old together. The most massive stars age quickly, exhausting their fuel supply in less than a million years, and end their lives in spectacular supernovae explosions. This process should have left the ancient cluster Messier 5 with only old, low - mass stars, which, as they have aged and cooled, have become red giants, while the oldest stars have evolved even further into blue horizontal branch stars. Yet astronomers have spotted many young, blue stars in this cluster, hiding among the much more luminous ancient stars. Astronomers think that these laggard youngsters, called blue stragglers, were created either by stellar collisions or by the transfer of mass between binary stars. Such events are easy to imagine in densely populated globular clusters, in which up to a few million stars are tightly packed together. Messier 5 lies at a distance of about 25 000 light - years in the constellation of Serpens (The Snake). This image was taken with Wide Field Channel of Hubble's Advanced Camera for Surveys — Globular cluster M5 in Serpens - Globular cluster M5 in Serpens - This cluster of stars is located about 25,000 light years away from Earth. It is one of the most extensive (165 years - light) and one of the oldest known globular clusters. Globular clusters are generally peoples of very old stars, but here the Hubble space telescope has identified some young stars, blue stragglers. The globular cluster Messier 5, shown here in this NASA/ESA Hubble Space Telescope image, is one of the oldest belonging to the Milky Way. The majority of its stars formed more than 12 billion years ago, but there are some unexpected newcomers on the scene, adding some vitality to this aging population. Stars in globular clusters form in the same stellar nursery and grow old together. The most massive stars age quickly, exhausting their fuel supply in less than a million years, and end their lives in spectacular supernovae explosions. This process should have left the ancient cluster Messier 5 with only old,

Globular cluster M5 in Serpens - Globular cluster M5 in Serpens - This cluster of stars is located about 25,000 light years away from Earth. It is one of the most extensive (165 years - light) and one of the oldest known globular clusters. Globular clusters are generally peoples of very old stars, but here the Hubble space telescope has identified some young stars, blue stragglers. The globular cluster Messier 5, shown here in this NASA/ESA Hubble Space Telescope image, is one of the oldest belonging to the Milky Way. The majority of its stars formed more than 12 billion years ago, but there are some unexpected newcomers on the scene, adding some vitality to this aging population. Stars in globular clusters form in the same stellar nursery and grow old together. The most massive stars age quickly, exhausting their fuel supply in less than a million years, and end their lives in spectacular supernovae explosions. This process should have left the ancient cluster Messier 5 with only old,

PIX4564490

Geminid Swim Car - Monster Geminid Fireball over Mojave Desert - A brilliant shooting star crosses the sky over Mojave Desert, California

Geminid Swim Car - Monster Geminid Fireball over Mojave Desert - A brilliant shooting star crosses the sky over Mojave Desert, California

PIX4599144

Shooting star rain on LAMOST telescope - China - Geminids over LAMOST telescope - China: Geminides shooting star rain above LAMOST telescope (Large Sky Area Multi-Object Fibre Spectroscopic Telescope), a 4-metre optical telescope, located on the site of the Xinglong Observatory in the Hebei region of China. December 2015. Space dust from asteroid 3200 Phaethon rained into the Earth's atmosphere, and burnt as meteors at about 100 km above Xinglong Station of National Astronomical Observatories of China, piercing the night sky over the Guoshoujing LAMOST telescope. All meteors seemed to radiate from the same point, which lies at Gemini, and that's how the meteor shower named Geminids.Over 100 meteors were captured in the composed image taken on the peak night of the 2015 Geminid meteor shower, and the brightest bolide even instantly lit up the landscape.

Shooting star rain on LAMOST telescope - China - Geminids over LAMOST telescope - China: Geminides shooting star rain above LAMOST telescope (Large Sky Area Multi-Object Fibre Spectroscopic Telescope), a 4-metre optical telescope, located on the site of the Xinglong Observatory in the Hebei region of China. December 2015. Space dust from asteroid 3200 Phaethon rained into the Earth's atmosphere, and burnt as meteors at about 100 km above Xinglong Station of National Astronomical Observatories of China, piercing the night sky over the Guoshoujing LAMOST telescope. All meteors seemed to radiate from the same point, which lies at Gemini, and that's how the meteor shower named Geminids.Over 100 meteors were captured in the composed image taken on the peak night of the 2015 Geminid meteor shower, and the brightest bolide even instantly lit up the landscape.

Yu Jun

PIX4657602

Star of David Badge, 1941 (textile)

Star of David Badge, 1941 (textile)

German School, (20th century)

GBW446687

The Evening Star, 1870 (gouache)

The Evening Star, 1870 (gouache)

Burne-Jones, Edward Coley (1833-98)

Martin Harrison

MH11891

Binary pulsar and gravitational waves - Binary pulsar and gravitational waves - Artist's view of a gravitational wave generated by a system of two stars a neutron, spreading over the fabric of space - time

Binary pulsar and gravitational waves - Binary pulsar and gravitational waves - Artist's view of a gravitational wave generated by a system of two stars a neutron, spreading over the fabric of space - time

L. Bret

PIX4572860

Comparison of Sun and Betelgeuse sizes - Size comparison: Betelgeuse and Sun - Betelgeuse star is a supergeant red star in the constellation Orion. It's one of the biggest stars known. It appears on this illustration at the scale next to the Sun (at the top). Betelgeuse is a red giant, one of the largest stars known. It forms the left shoulder of the constellation Orion. If Betelgeuse was placed at the center of our solar system, its fuzzy edge would extent out well beyond the orbit of Mars

Comparison of Sun and Betelgeuse sizes - Size comparison: Betelgeuse and Sun - Betelgeuse star is a supergeant red star in the constellation Orion. It's one of the biggest stars known. It appears on this illustration at the scale next to the Sun (at the top). Betelgeuse is a red giant, one of the largest stars known. It forms the left shoulder of the constellation Orion. If Betelgeuse was placed at the center of our solar system, its fuzzy edge would extent out well beyond the orbit of Mars

M. Carroll

PIX4571774

Fol.149va The Last Judgement: The stars fall and everything is turned upside down (vellum)

Fol.149va The Last Judgement: The stars fall and everything is turned upside down (vellum)

Italian School, (15th century)

FAF142844

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

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

Jerry Lodriguss

PIX4569599

Star (Etoile) 1939 (plaster)

Star (Etoile) 1939 (plaster)

Arp, Hans (Jean) (1887-1966)

IMJ424894

Halley's Comet Observed in 1759 by Cassini III (engraving)

Halley's Comet Observed in 1759 by Cassini III (engraving)

French School, (18th century)

XIR154683

Barree spiral galaxy M109 in the Great Bear - Barred spiral galaxy M109 in Ursa Major - The barree spiral galaxy M109 (NGC 3992) is located about 45 million years away - light from Earth. The barred spiral galaxy M109 (NGC 3992) is located at about 45 million light year from the Earth

Barree spiral galaxy M109 in the Great Bear - Barred spiral galaxy M109 in Ursa Major - The barree spiral galaxy M109 (NGC 3992) is located about 45 million years away - light from Earth. The barred spiral galaxy M109 (NGC 3992) is located at about 45 million light year from the Earth

Jim Misti

PIX4611025

Stephenson's 'North Star' Steam Engine, 1837

Stephenson's 'North Star' Steam Engine, 1837

English School, (19th century)

BAL1336

Etoile Merope in the Pleiades cluster - M45 - The Merope Nebulosity and IC 349 - Close up on the star Merope des Pleiades and its nebulosite. Image obtained with a telescope of 30 cm; 6h30 total installation. Star Merope in Pleiades star cluster seen on this 6 hours 30 minutes cumulative exposure

Etoile Merope in the Pleiades cluster - M45 - The Merope Nebulosity and IC 349 - Close up on the star Merope des Pleiades and its nebulosite. Image obtained with a telescope of 30 cm; 6h30 total installation. Star Merope in Pleiades star cluster seen on this 6 hours 30 minutes cumulative exposure

R. Gendler

PIX4568868

Polar ciricumpole above the dome of the GTC - La Palma Observatory: The GTC (Gran Telescopio Canarias) is a 10.4 m telescope

Polar ciricumpole above the dome of the GTC - La Palma Observatory: The GTC (Gran Telescopio Canarias) is a 10.4 m telescope

Patrick Lécureuil

PIX4624183

Star T - Tauri in Orion - Bow Shock around T - Tauri Star in the Orion Nebula - LL Ori is a star T - Tauri located about 1500 years ago - light from Earth in Orion's nebula. This young star emits a powerful stellar wind that hits the surrounding gas creating an arc-shaped shock wave Image obtained by the Hubble space telescope in February 1995. A bow shock can be created in space when two streams of gas collide. The star LL Ori emits a vigorous solar wind, a stream of charged particles moving rapidly outward from the star. Our own Sun has a less energetic version of this wind that is responsible for auroral displays on the Earth. The material in the fast wind from LL Ori collides with slow - moving gas evaporating away from the center of the Orion Nebula, which is located to the lower right in this Heritage image. The surface where the two winds collide is the crescent - shaped bow shock seen in the image. Unlike a water wave made by a ship, this interstellar bow shock is a three - dimensional structure. The filamentary emission has a very distinct boundary on the side facing away from LL Ori, but is diffuse on the side closest to the star, a characteristic common to many bow shocks. A second, fainter bow shock can be seen around a star near the upper right - hand corner of the image. Astronomers have identified numerous shock fronts in this complex star - forming region and are using this data to understand the many complex phenomena associated with the birth of stars. This image was taken in February 1995 as part of the Hubble Orion Nebula mosaic. A close visitor in our Milky Way galaxy, the nebula is only 1,500 light - years from Earth. The filters used in this color composite represent oxygen, nitrogen, and hydrogen emissions — Star T - Tauri in Orion - Bow Shock around T - Tauri Star in the Orion Nebula - LL Ori is a star T - Tauri located about 1500 years ago - light from Earth in Orion's nebula. This young star emits a powerful stellar wind that hits the surrounding gas creating an arc-shaped shock wave Image obtained by the Hubble space telescope in February 1995. A bow shock can be created in space when two streams of gas collide. The star LL Ori emits a vigorous solar wind, a stream of charged particles moving rapidly outward from the star. Our own Sun has a less energetic version of this wind that is responsible for auroral displays on the Earth. The material in the fast wind from LL Ori collides with slow - moving gas evaporating away from the center of the Orion Nebula, which is located to the lower right in this Heritage image. The surface where the two winds collide is the crescent - shaped bow shock seen in the image. Unlike a water wave made by a ship, this interstellar bow shock is a three - dim

Star T - Tauri in Orion - Bow Shock around T - Tauri Star in the Orion Nebula - LL Ori is a star T - Tauri located about 1500 years ago - light from Earth in Orion's nebula. This young star emits a powerful stellar wind that hits the surrounding gas creating an arc-shaped shock wave Image obtained by the Hubble space telescope in February 1995. A bow shock can be created in space when two streams of gas collide. The star LL Ori emits a vigorous solar wind, a stream of charged particles moving rapidly outward from the star. Our own Sun has a less energetic version of this wind that is responsible for auroral displays on the Earth. The material in the fast wind from LL Ori collides with slow - moving gas evaporating away from the center of the Orion Nebula, which is located to the lower right in this Heritage image. The surface where the two winds collide is the crescent - shaped bow shock seen in the image. Unlike a water wave made by a ship, this interstellar bow shock is a three - dim

PIX4572363

The Star of Bethlehem (engraving)

The Star of Bethlehem (engraving)

English School, (19th century)

LIP1046884

Chinese star chart (detail)

Chinese star chart (detail)

BL747653

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

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

PIX4589857

Open cluster Westerlund 2 in Carene - Open cluster Westerlund 2 in Carina - The open cluster Westerlund 2 is located about 20,000 years - light in the southern constellation of Carene, within the nebula Gum 29. About 3000 stars form this cluster. It contains a significant number of massive stars including one of the most massive stars known to date: WR 20a. Image obtained by the Hubble Space Telescope. The sparkling centerpiece of this image taken by the Hubble space telescope is a giant cluster of about 3,000 stars called Westerlund 2, named for Swedish astronomer Bengt Westerlund, who discovered the grouping in the 1960s. The cluster resides in a raucous stellar breeding ground known as Gum 29, located 20,000 light - years away from Earth in the constellation Carina. To capture this image, Hubble's near - infrared Wide Field Camera 3 near - infrared pierced through the dusty veil shrouding the stellar nursery, giving astronomers a clear view of the nebula and the dense concentration of stars in the central cluster. The cluster measures between 6 to 13 light - years across. The giant star cluster is only about 2 million years old and contains some of our galaxy's hottest, brightest, and most massive stars. Some of its heftiest stars unleash torrents of ultraviolet light and hurricane - force winds of charged particles that etch at the enveloping hydrogen gas cloud. The nebula reveals a fantasy landscape of pillars, ridges, and valleys. The pillars, composed of dense gas and thought to be incubators for new stars are a few light - years tall and point to the central star cluster. Other dense regions surround the pillars, including reddish - brown filaments of gas and dust. The brilliant stars sculpt the gaseous terrain of the nebula and help create a successive generation of baby stars. When the stellar winds hit dense walls of gas, the shockwaves may spark a new torrent of star birth along the wall of the cavity. The red dots scattered t — Open cluster Westerlund 2 in Carene - Open cluster Westerlund 2 in Carina - The open cluster Westerlund 2 is located about 20,000 years - light in the southern constellation of Carene, within the nebula Gum 29. About 3000 stars form this cluster. It contains a significant number of massive stars including one of the most massive stars known to date: WR 20a. Image obtained by the Hubble Space Telescope. The sparkling centerpiece of this image taken by the Hubble space telescope is a giant cluster of about 3,000 stars called Westerlund 2, named for Swedish astronomer Bengt Westerlund, who discovered the grouping in the 1960s. The cluster resides in a raucous stellar breeding ground known as Gum 29, located 20,000 light - years away from Earth in the constellation Carina. To capture this image, Hubble's near - infrared Wide Field Camera 3 near - infrared pierced through the dusty veil shrouding the stellar nursery, giving astronomers a clear view of the nebula and the dense concentration

Open cluster Westerlund 2 in Carene - Open cluster Westerlund 2 in Carina - The open cluster Westerlund 2 is located about 20,000 years - light in the southern constellation of Carene, within the nebula Gum 29. About 3000 stars form this cluster. It contains a significant number of massive stars including one of the most massive stars known to date: WR 20a. Image obtained by the Hubble Space Telescope. The sparkling centerpiece of this image taken by the Hubble space telescope is a giant cluster of about 3,000 stars called Westerlund 2, named for Swedish astronomer Bengt Westerlund, who discovered the grouping in the 1960s. The cluster resides in a raucous stellar breeding ground known as Gum 29, located 20,000 light - years away from Earth in the constellation Carina. To capture this image, Hubble's near - infrared Wide Field Camera 3 near - infrared pierced through the dusty veil shrouding the stellar nursery, giving astronomers a clear view of the nebula and the dense concentration

PIX4569094

Rock Star, 2014 (oil on canvas)

premium — Rock Star, 2014 (oil on canvas)

Rock Star, 2014 (oil on canvas)

Arsenault, David

AUT1272024

Zodiacal light - Zodiacal light - Zodiacal light. May 2004, Namibia. The zodiacal light comes from the reflection of the Sun's light on the countless interplanetary dust; it draws the plane of the Solar System. Zodiacal light, Namibia, May 2004. Zodiacal light comes from the reflexion of the sun's light off tiny interplanetary dust particles in the plane of the solar system

Zodiacal light - Zodiacal light - Zodiacal light. May 2004, Namibia. The zodiacal light comes from the reflection of the Sun's light on the countless interplanetary dust; it draws the plane of the Solar System. Zodiacal light, Namibia, May 2004. Zodiacal light comes from the reflexion of the sun's light off tiny interplanetary dust particles in the plane of the solar system

Sebastian Voltmer

PIX4581492

Pleiades open cluster - The Pleiades star cluster - The Pleiades star cluster contains about 500 stars formed 100 million years ago. It is located 440 light years from Earth, in the constellation Taurus. M45, the Pleiades, is a beautiful open cluster in Taurus surrounded by reflection nebulosity. The cluster has been known since ancient times and contains six bright stars that can easily be seen with the unaided eye, and 500 stars total, most too faint to be seen. The blue nebulosity is visible by starlight reflected off of dust in space. The cluster is located about 440 light years from the Earth and is estimated to be about 100 million years old

Pleiades open cluster - The Pleiades star cluster - The Pleiades star cluster contains about 500 stars formed 100 million years ago. It is located 440 light years from Earth, in the constellation Taurus. M45, the Pleiades, is a beautiful open cluster in Taurus surrounded by reflection nebulosity. The cluster has been known since ancient times and contains six bright stars that can easily be seen with the unaided eye, and 500 stars total, most too faint to be seen. The blue nebulosity is visible by starlight reflected off of dust in space. The cluster is located about 440 light years from the Earth and is estimated to be about 100 million years old

S. Numazawa

PIX4568812

Galactic Center Region - The Galactic Center - The Galactic Center Region of the center of our galaxy seen the Chandra, Spitzer and Hubble satellites. The galactic center (Sagittarius A*) is located in the white area in the middle to the right of the image. In yellow, near-infrared images obtained by the Hubble Space Telescope; in red, infrared images obtained by the Spitzer Space Telescope; in blue and purple, X-ray observations obtained by the Chandra Space Telescope. Nasa's Great Observatories - the Hubble Space Telescope, the Spitzer Space Telescope, and the Chandra X-ray Observatory - have collaborated to produce an unprecedented image of the central region of our Milky Way galaxy. In this spectacular image, observations using infrared light and X-ray light see through the obscuring dust and reveal the intense activity near the galactic core. Note that the center of the galaxy is located within the bright white region to the right of and just below the middle of the image. The entire image width covers about one-half a degree, about the same angular width as the full moon. Each telescope's contribution is presented in a different color: - Yellow represents the near-infrared observations of Hubble. These observations outline the energetic regions where stars are being born as well as reveal hundreds of thousands of stars. - Red represents the infrared observations of Spitzer. The radiation and winds from stars create glowing dust clouds that exhibit complex structures from compact, spherical globules to long, stringy filaments. - Blue and violet represent the X-ray observations of Chandra. X-rays are emitted by gas heated to millions of degrees by stellar explosions and by outflows from the supermassive black hole in the galaxy's center. The bright blue blob on the left side is emission from a double star system containing either a neutron star or a black hole. When these views are brought together, this composite image provides one of the most detailed — Galactic Center Region - The Galactic Center - The Galactic Center Region of the center of our galaxy seen the Chandra, Spitzer and Hubble satellites. The galactic center (Sagittarius A*) is located in the white area in the middle to the right of the image. In yellow, near-infrared images obtained by the Hubble Space Telescope; in red, infrared images obtained by the Spitzer Space Telescope; in blue and purple, X-ray observations obtained by the Chandra Space Telescope. Nasa's Great Observatories - the Hubble Space Telescope, the Spitzer Space Telescope, and the Chandra X-ray Observatory - have collaborated to produce an unprecedented image of the central region of our Milky Way galaxy. In this spectacular image, observations using infrared light and X-ray light see through the obscuring dust and reveal the intense activity near the galactic core. Note that the center of the galaxy is located within the bright white region to the right of and just below the middle of the image. The ent

Galactic Center Region - The Galactic Center - The Galactic Center Region of the center of our galaxy seen the Chandra, Spitzer and Hubble satellites. The galactic center (Sagittarius A*) is located in the white area in the middle to the right of the image. In yellow, near-infrared images obtained by the Hubble Space Telescope; in red, infrared images obtained by the Spitzer Space Telescope; in blue and purple, X-ray observations obtained by the Chandra Space Telescope. Nasa's Great Observatories - the Hubble Space Telescope, the Spitzer Space Telescope, and the Chandra X-ray Observatory - have collaborated to produce an unprecedented image of the central region of our Milky Way galaxy. In this spectacular image, observations using infrared light and X-ray light see through the obscuring dust and reveal the intense activity near the galactic core. Note that the center of the galaxy is located within the bright white region to the right of and just below the middle of the image. The ent

PIX4637984

October 16, 2012: Alpha Centauri A and B are located 4.36 light years from the Sun. These two stars are relatively similar to the Sun - This wide-field view of the sky around the bright star Alpha Centauri was created from photographic images forming part of the Digitized Sky Survey 2. The star appears so big just because of the scattering of light by the telescope's optics as well as in the photographic emulsion. Alpha Centauri is the closest star system to the Solar System

October 16, 2012: Alpha Centauri A and B are located 4.36 light years from the Sun. These two stars are relatively similar to the Sun - This wide-field view of the sky around the bright star Alpha Centauri was created from photographic images forming part of the Digitized Sky Survey 2. The star appears so big just because of the scattering of light by the telescope's optics as well as in the photographic emulsion. Alpha Centauri is the closest star system to the Solar System

PIX4650931

Constellation Persee - Perseus constellation

Constellation Persee - Perseus constellation

Alex Conu

PIX4571671

Star Sirius in the Great Dog - Sirius in Canis Major - Sirius is the main star in the constellation Big Dog. Seen from the Earth, Sirius is the brightest star in the sky after the Sun. Sirius, the Dog Star, is the brightest star in the night sky at mag - 1.44 and it dominates the constellation of Canis Major. Sirius is a binary star with a white dwarf companion named Sirius B, “” The Pup”. It is an eight - magnitude star that is separated from Sirius by only a couple of arc seconds making it difficult to observe in a telescope because of the primary's great brilliance

Star Sirius in the Great Dog - Sirius in Canis Major - Sirius is the main star in the constellation Big Dog. Seen from the Earth, Sirius is the brightest star in the sky after the Sun. Sirius, the Dog Star, is the brightest star in the night sky at mag - 1.44 and it dominates the constellation of Canis Major. Sirius is a binary star with a white dwarf companion named Sirius B, “” The Pup”. It is an eight - magnitude star that is separated from Sirius by only a couple of arc seconds making it difficult to observe in a telescope because of the primary's great brilliance

Jerry Lodriguss

PIX4571719

Constellations of the Great Bear and Little Bear - Constellations of Ursa Major and Ursa Minor - On the right, the large trolley, asterism of the Great Bear; on the left, the small trolley, asterism of the Little Bear that houses the polar star, the star that currently indicates the position of the northern Celestial pole, at the end of the handle of the pan

Constellations of the Great Bear and Little Bear - Constellations of Ursa Major and Ursa Minor - On the right, the large trolley, asterism of the Great Bear; on the left, the small trolley, asterism of the Little Bear that houses the polar star, the star that currently indicates the position of the northern Celestial pole, at the end of the handle of the pan

PIX4591377

Illicium verum/Badian/Anise star/Star Anise

Illicium verum/Badian/Anise star/Star Anise

Descamps

HFE4447938

Galaxy of the Wheel of the Charette in the Sculptor - The Cartwheel Galaxy - The ring galaxy of the Wheel of the Charette is about 500 million years away - light from the Earth. It is surrounded by a ring of 150,000 years - light of diameter composed of young and very bright stars. This particular form is the result of a collision, probably with one of the two galaxies on the right. Image obtained by the Hubble Space Telescope in October 1994. A rare and spectacular head - on collision between two galaxies appears in this NASA Hubble Space Telescope true - color image of the Cartwheel Galaxy, located 500 million light - years away in the constellation Sculptor. The details of star birth resolved by Hubble provide an opportunity to study how extremely massive stars are born in large fragmented gas clouds. The striking ring - like feature is a direct result of a smaller intruder galaxy - - possibly one of two objects to the right of the ring - - that careened through the core of the host galaxy. Like a rock tossed into a lake, the collision sent a ripple of energy into space, plowing gas and dust in front of it. Expanding at 200,000 miles per hour, this cosmic tsunami leaves in its wake a firestorm of new star creation. Hubble resolves bright blue knots that are gigantic clusters of newborn stars and immense loops and bubbles blown into space by exploding stars (supernovae) going off like a string of firecrackers. The Cartwheel Galaxy presumably was a normal spiral galaxy like our Milky Way before the collision. This spiral structure is beginning to re - emerge, as seen in the faint arms or spokes between the outer ring and bulls - eye shaped nucleus. The ring contains at least several billion new stars that would not normally have been created in such a short time span and is so large (150,000 light - years across) our entire Milky Way Galaxy would fit inside. Hubble's new view does not solve the mystery as to which of the two small galaxies m — Galaxy of the Wheel of the Charette in the Sculptor - The Cartwheel Galaxy - The ring galaxy of the Wheel of the Charette is about 500 million years away - light from the Earth. It is surrounded by a ring of 150,000 years - light of diameter composed of young and very bright stars. This particular form is the result of a collision, probably with one of the two galaxies on the right. Image obtained by the Hubble Space Telescope in October 1994. A rare and spectacular head - on collision between two galaxies appears in this NASA Hubble Space Telescope true - color image of the Cartwheel Galaxy, located 500 million light - years away in the constellation Sculptor. The details of star birth resolved by Hubble provide an opportunity to study how extremely massive stars are born in large fragmented gas clouds. The striking ring - like feature is a direct result of a smaller intruder galaxy - - possibly one of two objects to the right of the ring - - that careened through the core of the host

Galaxy of the Wheel of the Charette in the Sculptor - The Cartwheel Galaxy - The ring galaxy of the Wheel of the Charette is about 500 million years away - light from the Earth. It is surrounded by a ring of 150,000 years - light of diameter composed of young and very bright stars. This particular form is the result of a collision, probably with one of the two galaxies on the right. Image obtained by the Hubble Space Telescope in October 1994. A rare and spectacular head - on collision between two galaxies appears in this NASA Hubble Space Telescope true - color image of the Cartwheel Galaxy, located 500 million light - years away in the constellation Sculptor. The details of star birth resolved by Hubble provide an opportunity to study how extremely massive stars are born in large fragmented gas clouds. The striking ring - like feature is a direct result of a smaller intruder galaxy - - possibly one of two objects to the right of the ring - - that careened through the core of the host

PIX4613594

Shooting star rain - Leonid Meteor Storm - Leonides, in the constellation Orion, November 18, 2001. Leonid meteors rain down through the constellations of Canis Major, Orion, Eridanus and Taurus. Falling at a rate of about one per second, dozens of meteors are recorded in this composite image

Shooting star rain - Leonid Meteor Storm - Leonides, in the constellation Orion, November 18, 2001. Leonid meteors rain down through the constellations of Canis Major, Orion, Eridanus and Taurus. Falling at a rate of about one per second, dozens of meteors are recorded in this composite image

Jerry Lodriguss

PIX4598818

The Rosette Nebula in the Unicorn - The Rosette Nebula and NGC 2244 cluster - The Rosette Nebula is a vast cloud of dust and gas located about 5500 years from Earth. Towards the center of the nebula, a cluster of blue stars, NGC 2244 formed less than a million years ago. Image obtained by Siding Spring's 3.9m telescope. In the hollowed - out centre of the Rosette nebula lies NGC 2244, the cluster of young stars recently formed there. The cluster has itself created the cavity, radiation pressure and stellar winds from the stars blowing the gas and dust away from the young cluster. The hottest (and brightest) members of the group are seen as distinctly blue on this photograph, a colour corresponding to a surface temperature around 20,000K which may be compared with the Sun's 5500K. The nebula and its cluster is at a distance of about 4500 light years and shows many streaks and globules of dust, remnants of the cloud from which the stars formed

The Rosette Nebula in the Unicorn - The Rosette Nebula and NGC 2244 cluster - The Rosette Nebula is a vast cloud of dust and gas located about 5500 years from Earth. Towards the center of the nebula, a cluster of blue stars, NGC 2244 formed less than a million years ago. Image obtained by Siding Spring's 3.9m telescope. In the hollowed - out centre of the Rosette nebula lies NGC 2244, the cluster of young stars recently formed there. The cluster has itself created the cavity, radiation pressure and stellar winds from the stars blowing the gas and dust away from the young cluster. The hottest (and brightest) members of the group are seen as distinctly blue on this photograph, a colour corresponding to a surface temperature around 20,000K which may be compared with the Sun's 5500K. The nebula and its cluster is at a distance of about 4500 light years and shows many streaks and globules of dust, remnants of the cloud from which the stars formed

PIX4618457

Shooting star, Orionide - Orionid Meteor in Ursa Major - An Orionid swarm car near the Great Bear seen on October 21, 2017. An Orionid meteor passes by the constellation Ursa Major

Shooting star, Orionide - Orionid Meteor in Ursa Major - An Orionid swarm car near the Great Bear seen on October 21, 2017. An Orionid meteor passes by the constellation Ursa Major

Alex Conu

PIX4599240

A Star Masquer (w/c on paper)

A Star Masquer (w/c on paper)

Jones, Inigo (1573-1652)

CTS407539

IC 348 in Persee - IC 348 in Perseus - IC 348, near the star Omicron Persei; is a cluster of 300 stars associated with a relatively bright nebula. The nebula is located 1043 years of light from Earth. IC 348, near Omicron Persei, is a star cluster which contains more than 300 young stars. The Perseus Nebula is located about 1,043 light - years away in the Perseus constellation

IC 348 in Persee - IC 348 in Perseus - IC 348, near the star Omicron Persei; is a cluster of 300 stars associated with a relatively bright nebula. The nebula is located 1043 years of light from Earth. IC 348, near Omicron Persei, is a star cluster which contains more than 300 young stars. The Perseus Nebula is located about 1,043 light - years away in the Perseus constellation

Tom Davis

PIX4568953

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

Three Kings and Camel (gouache on paper)

premium — Three Kings and Camel (gouache on paper)

Three Kings and Camel (gouache on paper)

LB149359

Open Cluster of Pleiades - The Pleiades star cluster - The Pleiades cluster (M45) is a cluster of about 500 young stars nees 150 million years ago. Visible in the constellation Taurus, this cluster is 440 years from the Earth. Brown dwarfs have been observed in this cluster. The Pleiades star cluster, also known as the Seven Sisters and Messier 45 (M45), is one of the brightest and famous star clusters visible in the northern hemisphere. It consists of about 500 bright, hot, young stars that were all born at the same time between 75 and 150 million years ago within a large cloud of dust and gas. This star cluster lie some 440 light years away from the Earth, in the constellation of Taurus

Open Cluster of Pleiades - The Pleiades star cluster - The Pleiades cluster (M45) is a cluster of about 500 young stars nees 150 million years ago. Visible in the constellation Taurus, this cluster is 440 years from the Earth. Brown dwarfs have been observed in this cluster. The Pleiades star cluster, also known as the Seven Sisters and Messier 45 (M45), is one of the brightest and famous star clusters visible in the northern hemisphere. It consists of about 500 bright, hot, young stars that were all born at the same time between 75 and 150 million years ago within a large cloud of dust and gas. This star cluster lie some 440 light years away from the Earth, in the constellation of Taurus

Sebastian Voltmer

PIX4568871

Constellations of the Great Bear and Little Bear - Constellations of Ursa Major and Ursa Mino

Constellations of the Great Bear and Little Bear - Constellations of Ursa Major and Ursa Mino

B&S.Fletcher

PIX4591297

Shooting star above Niasar - Geminid meteor above Niasar - A shooting star of the geminid swarm passes over a zoroastrist temple in Niasar, Iran. A bright meteor from Gemenid shower grazes sky above the 1600-year old fire temple of Niasar in Iran, used for centuries by Zoroastrians

Shooting star above Niasar - Geminid meteor above Niasar - A shooting star of the geminid swarm passes over a zoroastrist temple in Niasar, Iran. A bright meteor from Gemenid shower grazes sky above the 1600-year old fire temple of Niasar in Iran, used for centuries by Zoroastrians

Oshin Zakarian

PIX4598709

Winter hexagon and March - Winter hexagon - The winter hexagon is an asterism formed by the stars Sirius, Procyon, Pollux, Capella, Aldebaran and Rigel. The image also shows the planet Mars (the brightest spot) and the comet Holmes (scattered spot on the right. 19 December 2007. Winter hexagon is composed by bright stars Sirius, Procyon, Pollux, Capella, Aldebaran and Rigel. The image shows also the comet 17P/Holmes. But very prominent inside the Hexagon is Mars. December 19, 2007

Winter hexagon and March - Winter hexagon - The winter hexagon is an asterism formed by the stars Sirius, Procyon, Pollux, Capella, Aldebaran and Rigel. The image also shows the planet Mars (the brightest spot) and the comet Holmes (scattered spot on the right. 19 December 2007. Winter hexagon is composed by bright stars Sirius, Procyon, Pollux, Capella, Aldebaran and Rigel. The image shows also the comet 17P/Holmes. But very prominent inside the Hexagon is Mars. December 19, 2007

Stefan Seip

PIX4593026

Halley Comete - 1986 - Halley's comet March 21 1986 - March 21 1986

Halley Comete - 1986 - Halley's comet March 21 1986 - March 21 1986

Jerry Lodriguss

PIX4569897

The Polar Star (diamond)

The Polar Star (diamond)

CH408870

Persee Constellation - Constellation of Persia

Persee Constellation - Constellation of Persia

PIX4593202

Shooting star -Perseide - Perseid Meteor - Rain des Perseides. August 10, 2013, Mojave desert, California. Bright and colorful meteor captured from the Mojave desert in California. August 10 2013

Shooting star -Perseide - Perseid Meteor - Rain des Perseides. August 10, 2013, Mojave desert, California. Bright and colorful meteor captured from the Mojave desert in California. August 10 2013

PIX4599015

Comparison of Sun Sizes and VY Canis Majoris: VY Canis Majoris (VY CMa) is a red hypergeant star located about 4,890 light years from Earth in the constellation Big Dog. She's one of the biggest stars known

Comparison of Sun Sizes and VY Canis Majoris: VY Canis Majoris (VY CMa) is a red hypergeant star located about 4,890 light years from Earth in the constellation Big Dog. She's one of the biggest stars known

Miller, Ron (b.1947)

PIX4573073

Comparison of the sizes of the Sun, Rigel, Betelgeuse and Antares - Size comparison: Sun, Rigel, Betelgeuse and Antares - The Sun (small dot on the right), and the blue supergiant star Rigel, are here compared to the supergiant red stars Betelgeuse (left), and Antares (in the background). The Sun (little dot at right) and Rigel are dwarfed by the red supergiants Betelgeuse (at left) and Antares (in background). Antares (alpha Scorpii) is the brightest star in the constellation Scorpius

Comparison of the sizes of the Sun, Rigel, Betelgeuse and Antares - Size comparison: Sun, Rigel, Betelgeuse and Antares - The Sun (small dot on the right), and the blue supergiant star Rigel, are here compared to the supergiant red stars Betelgeuse (left), and Antares (in the background). The Sun (little dot at right) and Rigel are dwarfed by the red supergiants Betelgeuse (at left) and Antares (in background). Antares (alpha Scorpii) is the brightest star in the constellation Scorpius

M. Carroll

PIX4571710

The double star Albireo - The double star Albireo - The double star Albireo (Beta Cygni) is located about 380 years from Earth in the constellation Swan. The double star Albireo (Beta Cygni) is approximately 380 light - years away from Earth in the constellation of Cygnus

The double star Albireo - The double star Albireo - The double star Albireo (Beta Cygni) is located about 380 years from Earth in the constellation Swan. The double star Albireo (Beta Cygni) is approximately 380 light - years away from Earth in the constellation of Cygnus

Stefan Seip

PIX4571868

The Star (pastel)

The Star (pastel)

Degas, Edgar (1834-1917)

BRM280024

Laguna Verde - Desert d'Atacama - Chile: Star line above Laguna Verde, a dirty lake located at 4200 metres above sea level. August 2014. Laguna Verde, a salt lake at 4350m in Chile. It's quite close to the highest volcano in the world, Ojos del Salado. The color of the lake comes from algae that live in it.

Laguna Verde - Desert d'Atacama - Chile: Star line above Laguna Verde, a dirty lake located at 4200 metres above sea level. August 2014. Laguna Verde, a salt lake at 4350m in Chile. It's quite close to the highest volcano in the world, Ojos del Salado. The color of the lake comes from algae that live in it.

Alex Tudorica

PIX4676154

Poster advertising the White Star Line, 1911 (litho)

Poster advertising the White Star Line, 1911 (litho)

English School, (20th century)

SFP409459

Constellations of the Great Bear and Little Bear - Constellations of Ursa Major and Ursa Minor - At the top, the large carriage, asterism of the Great Bear; at the bottom, the small carriage, asterism of the Little Bear that houses the polar star, the star that currently indicates the position of the northern Celestial pole, at the end of the handle of the pan

Constellations of the Great Bear and Little Bear - Constellations of Ursa Major and Ursa Minor - At the top, the large carriage, asterism of the Great Bear; at the bottom, the small carriage, asterism of the Little Bear that houses the polar star, the star that currently indicates the position of the northern Celestial pole, at the end of the handle of the pan

Jerry Lodriguss

PIX4591315

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

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

PIX4589859

The Star of Bethlehem

The Star of Bethlehem

Burne-Jones, Edward Coley (1833-98)

IL931045

Artist's view of a magnetar and its magnetic field - A magnetar with its magnetic field. Artwork - Illustration showing the magnetic field lines of a magnetar that intertwine causing tensions on the surface of the neutron star that partially breaks causing an emission of X-rays and gamma rays. A magnetar is a neutron star with an extremely powerful magnetic field. This artwork shows magnetic field lines of the star causing X and gamma rays burst when they mix

Artist's view of a magnetar and its magnetic field - A magnetar with its magnetic field. Artwork - Illustration showing the magnetic field lines of a magnetar that intertwine causing tensions on the surface of the neutron star that partially breaks causing an emission of X-rays and gamma rays. A magnetar is a neutron star with an extremely powerful magnetic field. This artwork shows magnetic field lines of the star causing X and gamma rays burst when they mix

P. Carril

PIX4572872

MS Hunter 229 f.4v Virgo, from the Hunterian Psalter, c.1170 (pen & ink and tempera on vellum) (detail)

MS Hunter 229 f.4v Virgo, from the Hunterian Psalter, c.1170 (pen & ink and tempera on vellum) (detail)

English School, (12th century)

GUL232030

Southern Crown Nebula - The CRA reflection nebula - R Coronae Australis is a region of star formations visible in the southern hemisphere. It is located about 500 light years away from Earth. On the right, the globular cluster NGC 6723, located 30 000 light years from Earth in Sagittarius. Image made with the 1.2m Telescope of Schmidt UK from Siding Spring. Corona Australis (the southern crown, CRA) is in the far southern sky but visible from the southern states of the USA. The constellation is small but distinctive. The conspicuous globular cluster NGC 6723 is at the western (right) edge of the photograph, but it is in Sagittarius, and is about 30,000 light years distant. Almost all the nebulosity here is starlight, reflected from minute grains of dust, some of which gather into darker condensations ('molecular clouds'), blotting out the background stars. Fainter features can be seen here. Shiny NGC 6726 - 27 near middle of image contains both a visual binary and a variable star. Other wispy nebulae in the western part of the dark cloud betray the presence of young, hidden stars — Southern Crown Nebula - The CRA reflection nebula - R Coronae Australis is a region of star formations visible in the southern hemisphere. It is located about 500 light years away from Earth. On the right, the globular cluster NGC 6723, located 30 000 light years from Earth in Sagittarius. Image made with the 1.2m Telescope of Schmidt UK from Siding Spring. Corona Australis (the southern crown, CRA) is in the far southern sky but visible from the southern states of the USA. The constellation is small but distinctive. The conspicuous globular cluster NGC 6723 is at the western (right) edge of the photograph, but it is in Sagittarius, and is about 30,000 light years distant. Almost all the nebulosity here is starlight, reflected from minute grains of dust, some of which gather into darker condensations ('molecular clouds'), blotting out the background stars. Fainter features can be seen here. Shiny NGC 6726 - 27 near middle of image contains both a visual binary and a variable star. Othe

Southern Crown Nebula - The CRA reflection nebula - R Coronae Australis is a region of star formations visible in the southern hemisphere. It is located about 500 light years away from Earth. On the right, the globular cluster NGC 6723, located 30 000 light years from Earth in Sagittarius. Image made with the 1.2m Telescope of Schmidt UK from Siding Spring. Corona Australis (the southern crown, CRA) is in the far southern sky but visible from the southern states of the USA. The constellation is small but distinctive. The conspicuous globular cluster NGC 6723 is at the western (right) edge of the photograph, but it is in Sagittarius, and is about 30,000 light years distant. Almost all the nebulosity here is starlight, reflected from minute grains of dust, some of which gather into darker condensations ('molecular clouds'), blotting out the background stars. Fainter features can be seen here. Shiny NGC 6726 - 27 near middle of image contains both a visual binary and a variable star. Othe

PIX4620295

Winter sky in english Alps - Sky star above the Alps (La Rosiere). In the sky, the constellation of Orion and the lactee path. 27 December 2011. Starry sky above english Alps. December 27, 2011

Winter sky in english Alps - Sky star above the Alps (La Rosiere). In the sky, the constellation of Orion and the lactee path. 27 December 2011. Starry sky above english Alps. December 27, 2011

Sebastian Voltmer

PIX4592898

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