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Ball at the Court of Henri III on the Occasion of the Marriage of Anne, Duke of Joyeuse, to Marguerite de Vaudemont, 24th September 1581, c.1581 (oil on panel)

Ball at the Court of Henri III on the Occasion of the Marriage of Anne, Duke of Joyeuse, to Marguerite de Vaudemont, 24th September 1581, c.1581 (oil on panel)

French School, (16th century)

XIR139884

Ball at the Court of King Henri III of France, or Ball of the Duke of Alencon, 2nd half of the 16th century (panel)

Ball at the Court of King Henri III of France, or Ball of the Duke of Alencon, 2nd half of the 16th century (panel)

French School, (16th century)

XIR70319

Portrait of Countee Cullen, c.1931 (engraving)

Portrait of Countee Cullen, c.1931 (engraving)

Unknown Artist, (20th century)

XLA3776037

Tungurahua - Ecuador - Volcano Tungurahua - Ecuador - Tungurahua is an active stratovolcano located in the Andes of Ecuador. It peaks at 5023 meters. Tungurahua is an active stratovolcano located in Cordillera Central of the Andes in Ecuador. Eruption feather seen in march 2008

Tungurahua - Ecuador - Volcano Tungurahua - Ecuador - Tungurahua is an active stratovolcano located in the Andes of Ecuador. It peaks at 5023 meters. Tungurahua is an active stratovolcano located in Cordillera Central of the Andes in Ecuador. Eruption feather seen in march 2008

Martin Rietze

PIX4677585

Portrait of a Boy, c.1711-1716 (oil on canvas)

Portrait of a Boy, c.1711-1716 (oil on canvas)

Limner, Pierpont (fl.c.1710-16)

HST861989

Volcano Sangay - Ecuador - Volcano Sangay - Ecuador - Sangay is an active stratovolcano located in Ecuador. It peaks at 5230 meters. Sangay is a stratovolcano in Ecuador

Volcano Sangay - Ecuador - Volcano Sangay - Ecuador - Sangay is an active stratovolcano located in Ecuador. It peaks at 5230 meters. Sangay is a stratovolcano in Ecuador

Martin Rietze

PIX4677537

Advertisement for Peugeot, c.1910 (colour litho)

Advertisement for Peugeot, c.1910 (colour litho)

Liebeaux, Michel, called Mich (1881-1923)

SIT394582

King George VI at Y.M.C.A. Sports Carnival, 1919

King George VI at Y.M.C.A. Sports Carnival, 1919

XLF3783323

Mission ExoMars 2016 - Artist view - ExoMars Mission - Artist view - Artist view of the European mission ExoMars 2016 with the Shiaparelli landing module embarks on the TGO (Trace Gas Orbiter) probe. Artist's impression depicting the ExoMars 2016 entry, descent and landing demonstrator module, named Schiaparelli, on the Trace Gas Orbiter, and heading for Mars. TGO will be launched in 2016 with Schiaparelli, the entry, descent and landing demonstrator module. It will search for evidence of methane and other atmospheric gases that could be signatures of active biological or geological processes on Mars. TGO will also serve as a communications relay for the rover and surface science platform that will be launched in 2018

Mission ExoMars 2016 - Artist view - ExoMars Mission - Artist view - Artist view of the European mission ExoMars 2016 with the Shiaparelli landing module embarks on the TGO (Trace Gas Orbiter) probe. Artist's impression depicting the ExoMars 2016 entry, descent and landing demonstrator module, named Schiaparelli, on the Trace Gas Orbiter, and heading for Mars. TGO will be launched in 2016 with Schiaparelli, the entry, descent and landing demonstrator module. It will search for evidence of methane and other atmospheric gases that could be signatures of active biological or geological processes on Mars. TGO will also serve as a communications relay for the rover and surface science platform that will be launched in 2018

D. Ducros

PIX4606969

E.DEORBIT: a satellite to clean up space - E.Deorbit grabbing debris - Artist view of the satellite e.deorbit (right) catching a satellite with a net to take it to consume in the Earth's atmosphere. e.Deorbit is a European mission project that if approved in 2019 will start in 2024. This satellite will be the first to clean up space debris. He would recapture the larger objects with his articulated arm or a net, before discharging them into the atmosphere, or they would be destroyed. ESA's proposed e.Deorbit mission, shown right, using a net to catch a derelict satellite - the baseline capture method for what would be the world's first active space debris removal mission, in 2024. The mission would first rendezvous with a large, drifting ESA satellite, then capture and secure it safely ahead of steering the combination down for a controlled burn-up in the atmosphere. As well as the baselined robot arm, additional capture technologies are being investigated, including a net and harpon.

E.DEORBIT: a satellite to clean up space - E.Deorbit grabbing debris - Artist view of the satellite e.deorbit (right) catching a satellite with a net to take it to consume in the Earth's atmosphere. e.Deorbit is a European mission project that if approved in 2019 will start in 2024. This satellite will be the first to clean up space debris. He would recapture the larger objects with his articulated arm or a net, before discharging them into the atmosphere, or they would be destroyed. ESA's proposed e.Deorbit mission, shown right, using a net to catch a derelict satellite - the baseline capture method for what would be the world's first active space debris removal mission, in 2024. The mission would first rendezvous with a large, drifting ESA satellite, then capture and secure it safely ahead of steering the combination down for a controlled burn-up in the atmosphere. As well as the baselined robot arm, additional capture technologies are being investigated, including a net and harpon.

D. Ducros

PIX4605506

Central region of the elliptical galaxy Centaurus A (NGC 5128) - Central part of the galaxy Centaurus A (NGC 5128) - The galaxy NGC 5128 is located about 13 million years away from Earth in the southern constellation of Centaurus. A broad dark band crosses it in the middle, a probable vestige of a collision with a spiral galaxy. This giant galaxy is a powerful radio source known as Centaurus A. It is an active galaxy whose energy comes from a supermassive black hole. The green dot visible in the dust strip is a supernova, the supernova 1986g. It appears green because the red filter image that made this trichromy image was only taken a year after the event and the supernova had weakened. Image obtained from the 3.9m telescope of Siding Spring, Australia. The nearby radio source Centaurus A (NGC 5128) looks like an elliptical galaxy, crossed by a broad, irregular dust lane. The dark band is probably the remains of a dusty spiral galaxy which is being absorbed by the giant elliptical. One

Central region of the elliptical galaxy Centaurus A (NGC 5128) - Central part of the galaxy Centaurus A (NGC 5128) - The galaxy NGC 5128 is located about 13 million years away from Earth in the southern constellation of Centaurus. A broad dark band crosses it in the middle, a probable vestige of a collision with a spiral galaxy. This giant galaxy is a powerful radio source known as Centaurus A. It is an active galaxy whose energy comes from a supermassive black hole. The green dot visible in the dust strip is a supernova, the supernova 1986g. It appears green because the red filter image that made this trichromy image was only taken a year after the event and the supernova had weakened. Image obtained from the 3.9m telescope of Siding Spring, Australia. The nearby radio source Centaurus A (NGC 5128) looks like an elliptical galaxy, crossed by a broad, irregular dust lane. The dark band is probably the remains of a dusty spiral galaxy which is being absorbed by the giant elliptical. One

PIX4612262

Summit cone of Sangay, October 2002 (photo)

Summit cone of Sangay, October 2002 (photo)

Doug Allan

TDR408151

Grace Greenwood (1823-1904) 1845-61 (daguerreotype)

Grace Greenwood (1823-1904) 1845-61 (daguerreotype)

Southworth, Albert S. (1811-94) & Hawes, Josiah (1808-1901)

BST261797

Napoleon III and the Empress Eugenie of France, c 1865

Napoleon III and the Empress Eugenie of France, c 1865

UIS5072140

M87 elliptical galaxy in Virgo - M87 elliptical galaxy in Virgo - The M87 galaxy (NGC 4486) is located about 52 million years away - light from Earth, in the heart of the Virgin's cluster. M87 is the brightest radio source of the constellation, it is also called Virgo A. NGC 4486 (M87) is the largest and brightest elliptical galaxy within the northern Virgo Cluster at about 52 million light years from Earth. The galaxy also called Virgo A contains a notable active galactic nucleus that is a strong source of multiwavelength radiation, particularly radio waves. In 1918 astronomer Heber Curtis discovered a jet of matter coming from M87 which extends at least 5000 light - years from the nucleus of M87 and is made up of matter ejected from the galaxy, most likely by a supermassive black hole

M87 elliptical galaxy in Virgo - M87 elliptical galaxy in Virgo - The M87 galaxy (NGC 4486) is located about 52 million years away - light from Earth, in the heart of the Virgin's cluster. M87 is the brightest radio source of the constellation, it is also called Virgo A. NGC 4486 (M87) is the largest and brightest elliptical galaxy within the northern Virgo Cluster at about 52 million light years from Earth. The galaxy also called Virgo A contains a notable active galactic nucleus that is a strong source of multiwavelength radiation, particularly radio waves. In 1918 astronomer Heber Curtis discovered a jet of matter coming from M87 which extends at least 5000 light - years from the nucleus of M87 and is made up of matter ejected from the galaxy, most likely by a supermassive black hole

R. Gendler

PIX4611406

Barree spiral galaxy NGC 1365 in the Furnace - Barred spiral galaxy NGC 1365 in Fornax - NGC 1365 is a barree spiral galaxy that extends over 200,000 years - light. Located 60 million years ago - light, it belongs to the cluster of galaxies of the Furnace. Image obtained by Siding Spring's 3.9m telescope. NGC 1365, the largest spiral in the southern constellation of Fornax, is located at a distance of about 60 million light years. This beautiful galaxy is about as massive as the Milky Way, itself a substantial galaxy. Not much is known about how galaxies take on their beautiful forms, but a good deal is known about their internal organisation. The obvious 'bar' has the nucleus of the galaxy at its hub and is surrounded by masses of cooler stars that appear yellow on colour photographs. The bar itself is also yellowish, and has distinct dust lanes but it terminates abruptly in slender, curved arms that are lit by blue stars and the pink star - forming regions from which they spring

Barree spiral galaxy NGC 1365 in the Furnace - Barred spiral galaxy NGC 1365 in Fornax - NGC 1365 is a barree spiral galaxy that extends over 200,000 years - light. Located 60 million years ago - light, it belongs to the cluster of galaxies of the Furnace. Image obtained by Siding Spring's 3.9m telescope. NGC 1365, the largest spiral in the southern constellation of Fornax, is located at a distance of about 60 million light years. This beautiful galaxy is about as massive as the Milky Way, itself a substantial galaxy. Not much is known about how galaxies take on their beautiful forms, but a good deal is known about their internal organisation. The obvious 'bar' has the nucleus of the galaxy at its hub and is surrounded by masses of cooler stars that appear yellow on colour photographs. The bar itself is also yellowish, and has distinct dust lanes but it terminates abruptly in slender, curved arms that are lit by blue stars and the pink star - forming regions from which they spring

PIX4609870

Spiral galaxy M81 in the Great Bear - Spiral galaxy M81 in Ursa Major - The spiral galaxy M81 is located 12 million years ago - light from Earth. Its arms are home to star-forming regions while its core is surrounded by much older yellow stars. In the background at the top, an irregular dwarf galaxy, Holmberg IX. This image obtained by a 50 cm amateur telescope, in February 2010 for 23 hours of poses, shows gas filaments whose origin is uncertain. Located about 12 million light - years from our planet, M81 (NGC 3031) together with M82 (NGC 3034), NGC 3077 and NGC 2976 forms one of the most iconic groups of interacting galaxies. The M81 group has also been the subject of many studies searching for and analyzing evidence of strong interactions among its components. In 1965, Halton Arp detected an unusual looping feature near M81 while examining photographic plates produced with the 48 - inch Schmidt on Mount Palomar. Traditionally, ARP's loop has been interpreted as a tail resulting from

Spiral galaxy M81 in the Great Bear - Spiral galaxy M81 in Ursa Major - The spiral galaxy M81 is located 12 million years ago - light from Earth. Its arms are home to star-forming regions while its core is surrounded by much older yellow stars. In the background at the top, an irregular dwarf galaxy, Holmberg IX. This image obtained by a 50 cm amateur telescope, in February 2010 for 23 hours of poses, shows gas filaments whose origin is uncertain. Located about 12 million light - years from our planet, M81 (NGC 3031) together with M82 (NGC 3034), NGC 3077 and NGC 2976 forms one of the most iconic groups of interacting galaxies. The M81 group has also been the subject of many studies searching for and analyzing evidence of strong interactions among its components. In 1965, Halton Arp detected an unusual looping feature near M81 while examining photographic plates produced with the 48 - inch Schmidt on Mount Palomar. Traditionally, ARP's loop has been interpreted as a tail resulting from

R. Jay GaBany

PIX4610376

M87 elliptical galaxy in Virgo - M87 elliptical galaxy in Virgo - The M87 galaxy (NGC 4486) is located about 60 million years ago - light from Earth, in the heart of the Virgin's cluster. M87 is the brightest radio source in the constellation, it is also called Virgo A. Image made with Siding Spring's 3.9m telescope. Messier 87 (NGC 4486) lies near the centre of the nearby cluster of galaxies in Virgo at a distance of about 60 million light years. Although the physical boundaries of elliptical galaxies are not well defined, their mass can be, and by any standards M87 is enormous. It contains several thousand billion stars. Associated with this giant galaxy are large numbers of globular clusters, visible in this photograph as the cloud of slightly fuzzy objects around it. Like all ellipticals, M 87 is composed mainly of old stars and is largely devoid of the materials needed to make new ones. The galaxy is not inert however; high energy X - rays have been detected from an extensive oute

M87 elliptical galaxy in Virgo - M87 elliptical galaxy in Virgo - The M87 galaxy (NGC 4486) is located about 60 million years ago - light from Earth, in the heart of the Virgin's cluster. M87 is the brightest radio source in the constellation, it is also called Virgo A. Image made with Siding Spring's 3.9m telescope. Messier 87 (NGC 4486) lies near the centre of the nearby cluster of galaxies in Virgo at a distance of about 60 million light years. Although the physical boundaries of elliptical galaxies are not well defined, their mass can be, and by any standards M87 is enormous. It contains several thousand billion stars. Associated with this giant galaxy are large numbers of globular clusters, visible in this photograph as the cloud of slightly fuzzy objects around it. Like all ellipticals, M 87 is composed mainly of old stars and is largely devoid of the materials needed to make new ones. The galaxy is not inert however; high energy X - rays have been detected from an extensive oute

PIX4611461

View of Naples (gouache on panel) (see also 207963, 207965, 207966)

View of Naples (gouache on panel) (see also 207963, 207965, 207966)

Italian School, (19th century)

BON207964

Jet of the Galaxy Centaurus A (NGC 5128) seen in X-rays - Galaxy Centaurus A X - ray jet - View in false colours of a 30 000-year long jet - light that escapes from the nucleus of the Galaxy Centaurus A where a massive black hole is suspected. The galaxy NGC 5128 is located about 13 million light years away from Earth. Image obtained by the Chandra Space Telescope in May 2000. Chandra space telescope detects a jet emanating from the NGC 5128 core and numerous point - like X - ray sources, all bathed in diffuse X - rays produced by several - million - degree gas that fills the galaxy. It is believed that most of these sources are X - ray binaries in which a neutron star or stellar - sized black hole is accreting matter from a nearby companion star. The Cen A image was created from Chandra observations taken on December 5, 1999 and May 17, 2000

Jet of the Galaxy Centaurus A (NGC 5128) seen in X-rays - Galaxy Centaurus A X - ray jet - View in false colours of a 30 000-year long jet - light that escapes from the nucleus of the Galaxy Centaurus A where a massive black hole is suspected. The galaxy NGC 5128 is located about 13 million light years away from Earth. Image obtained by the Chandra Space Telescope in May 2000. Chandra space telescope detects a jet emanating from the NGC 5128 core and numerous point - like X - ray sources, all bathed in diffuse X - rays produced by several - million - degree gas that fills the galaxy. It is believed that most of these sources are X - ray binaries in which a neutron star or stellar - sized black hole is accreting matter from a nearby companion star. The Cen A image was created from Chandra observations taken on December 5, 1999 and May 17, 2000

PIX4612176

Centaurus A elliptical galaxy (NGC 5128) in Centaurus - The radio galaxy Centaurus A (NGC 5128): The galaxy NGC 5128 is located about 13 million light years away from Earth in the southern constellation of Centaurus. A broad dark band crosses it in the middle, a probable vestige of a collision with a spiral galaxy. This giant galaxy is a powerful radio source known as Centaurus A. It is an active galaxy whose energy comes from a supermassive black hole. - NGC 5128 is the nearest large elliptical galaxies to our sun at about 13 million light years. It is also the nearest of the giant radio galaxies, possessing an active galactic nucleus (AGN) and optically one of the most luminous galaxies in the sky. In 1949, NGC 5128 was found to be a loud source of radio energy, in fact the loudest radio source in its region of the sky (second overall to Cygnus A), earning it the designation Centarus A. As a radio galaxy it releases 1000 times the radio energy of the Milky Way in the form of large bi

Centaurus A elliptical galaxy (NGC 5128) in Centaurus - The radio galaxy Centaurus A (NGC 5128): The galaxy NGC 5128 is located about 13 million light years away from Earth in the southern constellation of Centaurus. A broad dark band crosses it in the middle, a probable vestige of a collision with a spiral galaxy. This giant galaxy is a powerful radio source known as Centaurus A. It is an active galaxy whose energy comes from a supermassive black hole. - NGC 5128 is the nearest large elliptical galaxies to our sun at about 13 million light years. It is also the nearest of the giant radio galaxies, possessing an active galactic nucleus (AGN) and optically one of the most luminous galaxies in the sky. In 1949, NGC 5128 was found to be a loud source of radio energy, in fact the loudest radio source in its region of the sky (second overall to Cygnus A), earning it the designation Centarus A. As a radio galaxy it releases 1000 times the radio energy of the Milky Way in the form of large bi

PIX4612309

Paricutin, Lava Flow, 1947 (oil on masonite)

Paricutin, Lava Flow, 1947 (oil on masonite)

Atl, Dr. (Gerardo Murillo) (1875-1964)

CH987983

Self-Portrait with Popocatépetl, 1928 (Atl colour: oil, wax, dry resin & gasoline)

Self-Portrait with Popocatépetl, 1928 (Atl colour: oil, wax, dry resin & gasoline)

Atl, Dr. (Gerardo Murillo) (1875-1964)

PHL2641451

Charles V the Wise (1338-80) King of France, from 'Les Augustes Representations de tous les Rois de France depuis Pharamond jusqu'a Louis XIV', Paris, 1679 (engraving) (b/w photo)

Charles V the Wise (1338-80) King of France, from 'Les Augustes Representations de tous les Rois de France depuis Pharamond jusqu'a Louis XIV', Paris, 1679 (engraving) (b/w photo)

de Larmessin (family of engravers) (1600-1799)

CHT163782

Hawaii, Big Island. Active Lava Flow As Lava Reaches Ocean In Volcano National Park. Kilauea Volcano.

Hawaii, Big Island. Active Lava Flow As Lava Reaches Ocean In Volcano National Park. Kilauea Volcano.

UIG545363

"Laila and Majnun at School", Folio from a Khamsa (Quintet) of Nizami, 1431-32 (ink, opaque w/c and gold on paper)

"Laila and Majnun at School", Folio from a Khamsa (Quintet) of Nizami, 1431-32 (ink, opaque w/c and gold on paper)

Persian School, (15th century)

XOS6366239

Triumph of Death, by Buonamico di Cristofano known as Buffalmacco (active beginning of 14th century), sinopia.

Triumph of Death, by Buonamico di Cristofano known as Buffalmacco (active beginning of 14th century), sinopia.

Buffalmacco, Buonamico (fl.1315-36)

DGA771798

Ilhas de Maluco', a map of the Moluccas, Indonesia, 1646. Settlements on the islands are shown, as well as an active volcano.

Ilhas de Maluco', a map of the Moluccas, Indonesia, 1646. Settlements on the islands are shown, as well as an active volcano.

BL5342369

Volcano Sangay - Ecuador - Volcano Sangay - Ecuador - Sangay is an active stratovolcano located in Ecuador. It peaks at 5230 meters. Sangay is a stratovolcano in Ecuador

Volcano Sangay - Ecuador - Volcano Sangay - Ecuador - Sangay is an active stratovolcano located in Ecuador. It peaks at 5230 meters. Sangay is a stratovolcano in Ecuador

Martin Rietze

PIX4677539

Anne, Duke of Joyeuse (engraving)

Anne, Duke of Joyeuse (engraving)

French School, (16th century)

XIR1272776

Belle Starr (1848-1889), photographed holding a revolver, was an active Western outlaw in Indian Territory (Oklahoma) the 1870s and 1880s. Gene Tierney starred in the 1941 film, BELLE STARR

Belle Starr (1848-1889), photographed holding a revolver, was an active Western outlaw in Indian Territory (Oklahoma) the 1870s and 1880s. Gene Tierney starred in the 1941 film, BELLE STARR

EVB2937176

Early issues of the Russian Bolshevik newspaper Pravda, 1912 (b/w photo)

Early issues of the Russian Bolshevik newspaper Pravda, 1912 (b/w photo)

Russian Photographer (20th century)

LLE5231615

View of the Vittoria lighthouse in Trieste, Italy (b/w photo)

View of the Vittoria lighthouse in Trieste, Italy (b/w photo)

FAF494597

The Vittoria lighthouse in Trieste, Italy (b/w photo)

The Vittoria lighthouse in Trieste, Italy (b/w photo)

FAF494600

Mission ExoMars 2016 - Artist view - ExoMars Mission - Artist view - Artist view of the TGO probe (Trace Gas Orbiter) of the European mission ExoMars 2016. ExoMars Trace Gas Orbiter at Mars. TGO will be launched in 2016 with Schiaparelli, the entry, descent and landing demonstrator module. It will search for evidence of methane and other atmospheric gases that could be signatures of active biological or geological processes on Mars. TGO will also serve as a communications relay for the rover and surface science platform that will be launched in 2018

Mission ExoMars 2016 - Artist view - ExoMars Mission - Artist view - Artist view of the TGO probe (Trace Gas Orbiter) of the European mission ExoMars 2016. ExoMars Trace Gas Orbiter at Mars. TGO will be launched in 2016 with Schiaparelli, the entry, descent and landing demonstrator module. It will search for evidence of methane and other atmospheric gases that could be signatures of active biological or geological processes on Mars. TGO will also serve as a communications relay for the rover and surface science platform that will be launched in 2018

D. Ducros

PIX4606979

Volcano Llullaillaco - Volcano Llullaillaco - Llullaillaco or Llullay - Yacu is an active stratovolcano located in the Andes on the border between Argentina and Chile. This image obtained from the International Space Station on 9 December 2009 shows a vast flow of lava that extends from the volcanic cone. The summit of South America's Llullaillaco Volcano has an elevation of 6,739 meters (22,110 feet) above sea level, making it the highest historically active volcano in the world. The current stratovolcano - - a cone - shaped volcano built from successive layers of thick lava flows and eruption products like ash and rock fragments - - is built on top of an older stratovolcano. This detailed astronaut photograph of Llullaillaco illustrates an interesting volcanic feature known as a coulee (image top right). Coulees are formed from highly viscous, thick lavas that flow onto a steep surface. Image taken on December 9, 2009 from the International space station (ISS)

Volcano Llullaillaco - Volcano Llullaillaco - Llullaillaco or Llullay - Yacu is an active stratovolcano located in the Andes on the border between Argentina and Chile. This image obtained from the International Space Station on 9 December 2009 shows a vast flow of lava that extends from the volcanic cone. The summit of South America's Llullaillaco Volcano has an elevation of 6,739 meters (22,110 feet) above sea level, making it the highest historically active volcano in the world. The current stratovolcano - - a cone - shaped volcano built from successive layers of thick lava flows and eruption products like ash and rock fragments - - is built on top of an older stratovolcano. This detailed astronaut photograph of Llullaillaco illustrates an interesting volcanic feature known as a coulee (image top right). Coulees are formed from highly viscous, thick lavas that flow onto a steep surface. Image taken on December 9, 2009 from the International space station (ISS)

PIX4675790

Mission ExoMars 2016 - Artist view - ExoMars Mission - Artist view: Artist view of the European mission ExoMars 2016 with the separation of the Shiaparelli landing module from the TGO probe (Trace Gas Orbiter). TGO has been in orbit around Mars since October 19, 2016. The Schiaparelli module was lost after separation. Artist's impression depicting the separation of the ExoMars 2016 entry, descent and landing demonstrator module, named Schiaparelli, from the Trace Gas Orbiter, and heading for Mars. TGO was launched on March 14 2016 with Schiaparelli. TGO orbits March since October 19 2016. Schiaparelli was lost after separation. TGO searches for evidence of methane and other atmospheric gases that could be signatures of active biological or geological processes on Mars. TGO will also serve as a communications relay for the rover and surface science platform that will be launched in 2020

Mission ExoMars 2016 - Artist view - ExoMars Mission - Artist view: Artist view of the European mission ExoMars 2016 with the separation of the Shiaparelli landing module from the TGO probe (Trace Gas Orbiter). TGO has been in orbit around Mars since October 19, 2016. The Schiaparelli module was lost after separation. Artist's impression depicting the separation of the ExoMars 2016 entry, descent and landing demonstrator module, named Schiaparelli, from the Trace Gas Orbiter, and heading for Mars. TGO was launched on March 14 2016 with Schiaparelli. TGO orbits March since October 19 2016. Schiaparelli was lost after separation. TGO searches for evidence of methane and other atmospheric gases that could be signatures of active biological or geological processes on Mars. TGO will also serve as a communications relay for the rover and surface science platform that will be launched in 2020

PIX4643703

E.DEORBIT: a satellite to clean space - E.Deorbit grabbing debris - An artist's view of the e.deorbit satellite (left) catching a satellite with a robotic arm to take it to consume itself in the Earth's atmosphere. e.Deorbit is a European mission project that if approved in 2019 will start in 2024. This satellite will be the first to clean up space debris. He would remove the larger objects with his arm or a net, before discharging them into the atmosphere, or they would be destroyed. ESA's proposed e.Deorbit mission, shown left, using a robotic arm to catch a derelict satellite - the baseline capture method for what would be the world's first active space debris removal mission, in 2024. The mission would first rendezvous with a large, drifting ESA satellite, then capture and secure it safely ahead of steering the combination down for a controlled burn-up in the atmosphere. As well as the baselined robot arm, additional capture technologies are being investigated, including a net and

E.DEORBIT: a satellite to clean space - E.Deorbit grabbing debris - An artist's view of the e.deorbit satellite (left) catching a satellite with a robotic arm to take it to consume itself in the Earth's atmosphere. e.Deorbit is a European mission project that if approved in 2019 will start in 2024. This satellite will be the first to clean up space debris. He would remove the larger objects with his arm or a net, before discharging them into the atmosphere, or they would be destroyed. ESA's proposed e.Deorbit mission, shown left, using a robotic arm to catch a derelict satellite - the baseline capture method for what would be the world's first active space debris removal mission, in 2024. The mission would first rendezvous with a large, drifting ESA satellite, then capture and secure it safely ahead of steering the combination down for a controlled burn-up in the atmosphere. As well as the baselined robot arm, additional capture technologies are being investigated, including a net and

D. Ducros

PIX4605477

E.DEORBIT: a satellite to clean space - E.Deorbit grabbing debris - An artist's view of the e.deorbit satellite (left) catching a satellite with a robotic arm to take it to consume itself in the Earth's atmosphere. e.Deorbit is a European mission project that if approved in 2019 will start in 2024. This satellite will be the first to clean up space debris. He would remove the larger objects with his arm or a net, before discharging them into the atmosphere, or they would be destroyed. ESA's proposed e.Deorbit mission, shown left, using a robotic arm to catch a derelict satellite - the baseline capture method for what would be the world's first active space debris removal mission, in 2024. The mission would first rendezvous with a large, drifting ESA satellite, then capture and secure it safely ahead of steering the combination down for a controlled burn-up in the atmosphere. As well as the baselined robot arm, additional capture technologies are being investigated, including a net and

E.DEORBIT: a satellite to clean space - E.Deorbit grabbing debris - An artist's view of the e.deorbit satellite (left) catching a satellite with a robotic arm to take it to consume itself in the Earth's atmosphere. e.Deorbit is a European mission project that if approved in 2019 will start in 2024. This satellite will be the first to clean up space debris. He would remove the larger objects with his arm or a net, before discharging them into the atmosphere, or they would be destroyed. ESA's proposed e.Deorbit mission, shown left, using a robotic arm to catch a derelict satellite - the baseline capture method for what would be the world's first active space debris removal mission, in 2024. The mission would first rendezvous with a large, drifting ESA satellite, then capture and secure it safely ahead of steering the combination down for a controlled burn-up in the atmosphere. As well as the baselined robot arm, additional capture technologies are being investigated, including a net and

D. Ducros

PIX4605498

Disabled handbike competitor participant of the Berlin Marathon at kilometer 40, Berlin, Germany, Europe (photo)

Disabled handbike competitor participant of the Berlin Marathon at kilometer 40, Berlin, Germany, Europe (photo)

Sergi Reboredo

SRB6177482

Disabled handbike competitor participant of the Berlin Marathon at kilometer 40, Berlin, Germany, Europe (photo)

Disabled handbike competitor participant of the Berlin Marathon at kilometer 40, Berlin, Germany, Europe (photo)

Sergi Reboredo

SRB6177492

Disabled handbike competitor participant of the Berlin Marathon at kilometer 40, Berlin, Germany, Europe (photo)

Disabled handbike competitor participant of the Berlin Marathon at kilometer 40, Berlin, Germany, Europe (photo)

Sergi Reboredo

SRB6177481

Disabled handbike competitor participant of the Berlin Marathon at kilometer 40, Berlin, Germany, Europe (photo)

Disabled handbike competitor participant of the Berlin Marathon at kilometer 40, Berlin, Germany, Europe (photo)

Sergi Reboredo

SRB6177483

Disabled handbike competitor participant of the Berlin Marathon at kilometer 40, Berlin, Germany, Europe (photo)

Disabled handbike competitor participant of the Berlin Marathon at kilometer 40, Berlin, Germany, Europe (photo)

Sergi Reboredo

SRB6177484

Festina girls bike support of Disabled handbike competitor participant of the Berlin Marathon at kilometer 40, Berlin, Germany, Europe (photo)

Festina girls bike support of Disabled handbike competitor participant of the Berlin Marathon at kilometer 40, Berlin, Germany, Europe (photo)

Sergi Reboredo

SRB6177487

Home Again, 1858 (see also 68094)

Home Again, 1858 (see also 68094)

O'Neil, Henry Nelson (1817-80)

FC68095

The 10th (Prince of Wales's Own Royal) Hussars (litho)

The 10th (Prince of Wales's Own Royal) Hussars (litho)

English School, (19th century)

LIP1592716

Summoned for Active Service (engraving)

Summoned for Active Service (engraving)

Holl, Frank (1845-88) (after)

LIP1058999

The Montgomeryshire Yeomanry, with "Pom-Pom," returned from Active Service (b/w photo)

The Montgomeryshire Yeomanry, with "Pom-Pom," returned from Active Service (b/w photo)

English Photographer, (20th century)

LIP1600429

The Crisis in the Transvaal (engraving)

The Crisis in the Transvaal (engraving)

Charlton, John (1849-1917) (after)

LIP1041857

Active Galaxy - Illustration - An active galaxy. Artwor

Active Galaxy - Illustration - An active galaxy. Artwor

S. Numazawa

PIX4613914

The First (Royal) Regiment of Dragoons, held in Readiness for South African Service (litho)

The First (Royal) Regiment of Dragoons, held in Readiness for South African Service (litho)

English School, (19th century)

LIP1592634

In the Niger Country, our Native Troops in Peace Time and on Active Service (litho)

In the Niger Country, our Native Troops in Peace Time and on Active Service (litho)

Dadd, Frank (1851-1929) (after)

LIP1043237

The Cheshire Regiment leaving its Colours with the Mayor of Chester for Safe Custody, the Regiment goes on Active Service to South Africa (b/w photo)

The Cheshire Regiment leaving its Colours with the Mayor of Chester for Safe Custody, the Regiment goes on Active Service to South Africa (b/w photo)

English Photographer, (20th century)

LIP1599210

Mexico's active Popocatepetl volcano spewing water vapor, gas, ashes and glowing rocks since its most recent eruption period began in April 2012. April 23, 2012.

Mexico's active Popocatepetl volcano spewing water vapor, gas, ashes and glowing rocks since its most recent eruption period began in April 2012. April 23, 2012.

UIG866958

Mexico's active Popocatepetl volcano spewing water vapor, gas, ashes and glowing rocks since its most recent eruption period began in April 2012. April 23, 2012.

Mexico's active Popocatepetl volcano spewing water vapor, gas, ashes and glowing rocks since its most recent eruption period began in April 2012. April 23, 2012.

UIG866959

The active crater of Rincon de la Vieja an andesitic complex volcano in the north-western Costa Rica, in the province of Guanacaste. April 27, 2007. (photo)

The active crater of Rincon de la Vieja an andesitic complex volcano in the north-western Costa Rica, in the province of Guanacaste. April 27, 2007. (photo)

UIG800400

active crater lake of Rincon de la Vieja volcano, Guanacaste Province, Costa Rica. 04-27-2006. (photo)

active crater lake of Rincon de la Vieja volcano, Guanacaste Province, Costa Rica. 04-27-2006. (photo)

UIG800401

Active Spirit, Vigour and Importance (engraving)

Active Spirit, Vigour and Importance (engraving)

English School, (19th century)

LLM666916

Planet near an active galaxy - Illustration - Planet and Active Galaxy - Illustration

Planet near an active galaxy - Illustration - Planet and Active Galaxy - Illustration

Miller, Ron (b.1947)

PIX4574362

The Modern "Tommy Atkins" (engraving)

The Modern "Tommy Atkins" (engraving)

Ralston, William (1848-1911) (after)

LIP1054858

Mount Erebus, Antarctica, Natural Colour Satellite Image (photo)

Mount Erebus, Antarctica, Natural Colour Satellite Image (photo)

UIG3274971

Mount Raung, Java, Indonesia, Natural Colour Satellite Image (photo)

Mount Raung, Java, Indonesia, Natural Colour Satellite Image (photo)

UIG3274974

Group of galaxies HCG 87 in Capricorn - Hickson Compact Group 87 in Capricornus - Group of galaxies in interaction situated 400 million years ago - light from Earth. The largest of these galaxies (HCG 87a) is a spiral galaxy seen by the slice; it and its neighbor the elliptical galaxy HCG 87b probably have a central black hole. The third member of this group, the spiral galaxy HCG 87c appears to be in an active phase of star formation. Group of interacting galaxies located at about 400 million light - years. The largest galaxy member (HCG 87a), which is actually disk - shaped, but tilted so that we see it nearly edge - on and its elliptically shaped nearest neighbor (87b) have active galactic nuclei which are believed to harbor black holes that are consuming gas. A third group member, the nearby spiral galaxy 87c, may be undergoing a burst of active star formation. These three galaxies are so close to each other that gravitational forces disrupt their structure and alter their evolutio

Group of galaxies HCG 87 in Capricorn - Hickson Compact Group 87 in Capricornus - Group of galaxies in interaction situated 400 million years ago - light from Earth. The largest of these galaxies (HCG 87a) is a spiral galaxy seen by the slice; it and its neighbor the elliptical galaxy HCG 87b probably have a central black hole. The third member of this group, the spiral galaxy HCG 87c appears to be in an active phase of star formation. Group of interacting galaxies located at about 400 million light - years. The largest galaxy member (HCG 87a), which is actually disk - shaped, but tilted so that we see it nearly edge - on and its elliptically shaped nearest neighbor (87b) have active galactic nuclei which are believed to harbor black holes that are consuming gas. A third group member, the nearby spiral galaxy 87c, may be undergoing a burst of active star formation. These three galaxies are so close to each other that gravitational forces disrupt their structure and alter their evolutio

PIX4565539

Galaxies NGC 3718 and NGC 3729 in the Great Bear

Galaxies NGC 3718 and NGC 3729 in the Great Bear

Adam Block

PIX4611005

Centaurus A elliptical galaxy (NGC 5128) in Centaurus - Elliptical galaxy Centaurus A (NGC 5128) - The galaxy NGC 5128 is located about 13 million years away from Earth in the southern constellation of Centaurus. A broad dark band crosses it in the middle, a probable vestige of a collision with a spiral galaxy. This giant galaxy is a powerful radio source known as Centaurus A. NGC 5128 is the nearest large elliptical galaxies to our sun located at about 13 million light years. It is also the nearest of the giant radio galaxies, possessing an active galactic nucleus (AGN) and optically one of the most luminous galaxies in the sky

Centaurus A elliptical galaxy (NGC 5128) in Centaurus - Elliptical galaxy Centaurus A (NGC 5128) - The galaxy NGC 5128 is located about 13 million years away from Earth in the southern constellation of Centaurus. A broad dark band crosses it in the middle, a probable vestige of a collision with a spiral galaxy. This giant galaxy is a powerful radio source known as Centaurus A. NGC 5128 is the nearest large elliptical galaxies to our sun located at about 13 million light years. It is also the nearest of the giant radio galaxies, possessing an active galactic nucleus (AGN) and optically one of the most luminous galaxies in the sky

Stephane Guisard

PIX4612265

Galaxies NGC 3718 in the Great Bear - Galaxy NGC 3718 in Ursa Major - NGC 3718 (Arp 214) is a special galaxy located about 42 million years ago - light from the Earth in the constellation Big Bear. It's an active nucleus galaxy. Its tormented form is probably due to the attraction exerted by another galaxy, NGC 3729 (off-field). On the right, Arp 322 (or Hickson 56), is a group of 5 galaxies far farther away, located about 300 million years from Earth. NGC 3718 (Arp 214) seems to have a rudimentary bar and spiral structure although it is recognized as a peculiar galaxy and as such is listed within ARP's Atlas of Peculiar Galaxies. NGC 3718 contains an active galactic nucleus (AGN) and is known as a Seyfert type 1.9 galaxy. Its strange shape is probably due to a gravitational interaction with its companion NGC 3729 (out of field). A grouping of 5 background galaxies 300 million light years distant are projected at right of NGC 3718 and are designated Arp 322 (also Hickson 56). Several m

Galaxies NGC 3718 in the Great Bear - Galaxy NGC 3718 in Ursa Major - NGC 3718 (Arp 214) is a special galaxy located about 42 million years ago - light from the Earth in the constellation Big Bear. It's an active nucleus galaxy. Its tormented form is probably due to the attraction exerted by another galaxy, NGC 3729 (off-field). On the right, Arp 322 (or Hickson 56), is a group of 5 galaxies far farther away, located about 300 million years from Earth. NGC 3718 (Arp 214) seems to have a rudimentary bar and spiral structure although it is recognized as a peculiar galaxy and as such is listed within ARP's Atlas of Peculiar Galaxies. NGC 3718 contains an active galactic nucleus (AGN) and is known as a Seyfert type 1.9 galaxy. Its strange shape is probably due to a gravitational interaction with its companion NGC 3729 (out of field). A grouping of 5 background galaxies 300 million light years distant are projected at right of NGC 3718 and are designated Arp 322 (also Hickson 56). Several m

Jim Misti

PIX4610955

Barree spiral galaxy NGC 1365 in the Furnace - NGC 1365, barred spiral galaxy in Fornax - NGC 1365 is a barree spiral galaxy that extends over 200,000 years - light. Located 60 million years ago - light, it belongs to the cluster of galaxies of the Furnace. Image obtained with a telescope of 30 cm, cumulative poses of 14 hours. NGC 1365 is a giant barred spiral galaxy who spans 200 000 light years across. It is located 60 million years away in the Fornax constellation. Image made from Australia with a 14.5 inches telescope; total Exposure 14 Hours

Barree spiral galaxy NGC 1365 in the Furnace - NGC 1365, barred spiral galaxy in Fornax - NGC 1365 is a barree spiral galaxy that extends over 200,000 years - light. Located 60 million years ago - light, it belongs to the cluster of galaxies of the Furnace. Image obtained with a telescope of 30 cm, cumulative poses of 14 hours. NGC 1365 is a giant barred spiral galaxy who spans 200 000 light years across. It is located 60 million years away in the Fornax constellation. Image made from Australia with a 14.5 inches telescope; total Exposure 14 Hours

R. Gendler

PIX4609876

Galaxies NGC 3718 and NGC 3729 in Ursa Major

Galaxies NGC 3718 and NGC 3729 in Ursa Major

Adam Block

PIX4610936

M87 elliptical galaxy in Virgo - M87 elliptical galaxy in Virgo - The M87 galaxy (NGC 4486) is located about 60 million years ago - light from Earth, in the heart of the Virgin's cluster. M87 is the brightest radio source in the constellation, it is also called Virgo A. Image made with Siding Spring's 3.9m telescope. Messier 87 (NGC 4486) is at the heart of the Virgo cluster and has a mass many times that of the Milky Way, itself no lightweight. Unlike our galaxy however, M87 is an elliptical galaxy. Though it appears more - or - less spherical on this photograph, a deep image shows it to be markedly elongated. Also unlike the Milky Way, M87 contains relatively little gas and dust. It is composed mainly of cool stars, which gives it a yellowish colour, in contrast to the blue of spiral galaxies. Despite the lack of star - forming materials, M87 is not a quiescent backwater. It is a powerful source of radio waves and the orbits of stars near its nucleus suggest they are held by a very m

M87 elliptical galaxy in Virgo - M87 elliptical galaxy in Virgo - The M87 galaxy (NGC 4486) is located about 60 million years ago - light from Earth, in the heart of the Virgin's cluster. M87 is the brightest radio source in the constellation, it is also called Virgo A. Image made with Siding Spring's 3.9m telescope. Messier 87 (NGC 4486) is at the heart of the Virgo cluster and has a mass many times that of the Milky Way, itself no lightweight. Unlike our galaxy however, M87 is an elliptical galaxy. Though it appears more - or - less spherical on this photograph, a deep image shows it to be markedly elongated. Also unlike the Milky Way, M87 contains relatively little gas and dust. It is composed mainly of cool stars, which gives it a yellowish colour, in contrast to the blue of spiral galaxies. Despite the lack of star - forming materials, M87 is not a quiescent backwater. It is a powerful source of radio waves and the orbits of stars near its nucleus suggest they are held by a very m

PIX4611429

Centaurus A elliptical galaxy (NGC 5128) in the Centaurus - Galaxy Centaurus A (NGC 5128) - The galaxy NGC 5128 is located about 13 million years away from Earth. This Giant Galaxy is a powerful radio source known as Centaurus A. It is an active galaxy whose energy comes from a supermassive black hole. Image obtained from the 3.9m telescope of Siding Spring, Australia. Centaurus A is a most unusual galaxy. The circular, uniformly bright portion is composed of several thousand million stars, most of them old and yellowish. The galaxy is girded by a dense dust lane which obscures and reddens the light of stars behind it. Some younger, blue stars can be seen at the edges of the dust cloud. One of the nearer galaxies, 13 million light years away, Centaurus A is the most powerful nearby radio source and is also a copious source of X - and gamma rays as well as visible and infrared radiation

Centaurus A elliptical galaxy (NGC 5128) in the Centaurus - Galaxy Centaurus A (NGC 5128) - The galaxy NGC 5128 is located about 13 million years away from Earth. This Giant Galaxy is a powerful radio source known as Centaurus A. It is an active galaxy whose energy comes from a supermassive black hole. Image obtained from the 3.9m telescope of Siding Spring, Australia. Centaurus A is a most unusual galaxy. The circular, uniformly bright portion is composed of several thousand million stars, most of them old and yellowish. The galaxy is girded by a dense dust lane which obscures and reddens the light of stars behind it. Some younger, blue stars can be seen at the edges of the dust cloud. One of the nearer galaxies, 13 million light years away, Centaurus A is the most powerful nearby radio source and is also a copious source of X - and gamma rays as well as visible and infrared radiation

PIX4612201

George II at the battle of Dettingen

George II at the battle of Dettingen

Doughty, C.L. (1913-85)

LAL337471

Vesuvius in Winter, 1893 (oil on board)

Vesuvius in Winter, 1893 (oil on board)

Richards, William Trost (1833-1905)

PNY155803

Indian Troops in China (b/w photo)

Indian Troops in China (b/w photo)

English Photographer, (20th century)

LIP1599817

Experiences of a British Officer of the Gendarmerie in Egypt (engraving)

Experiences of a British Officer of the Gendarmerie in Egypt (engraving)

Marie, Adrien Emmanuel (1848-91) (after)

LIP1045667

Spiral galaxy M81 in the Great Bear - Spiral galaxy M81 in Ursa Major - The spiral galaxy M81 is located 12 million years ago - light from Earth. Its arms are home to star-forming regions while its core is surrounded by much older yellow stars. In the background at the top, an irregular dwarf galaxy, Holmberg IX. Image obtained by an amateur telescope of 50 cm, composting different poses. M81 is the brightest member of the nearby galactic group called the M81 group. This group contains at least 25 other members including the peculiar starburst galaxy M82, the peculiar galaxy NGC 3077 and many dwarfs galaxies. The core galaxies of the group (M81, M82, NGC 3077, NGC 2976) are strongly interacting and are all imbedded within a large and extended molecular gas cloud. The Dwarf irregular Holmberg IX (seen above M81 in the image) most likely condensed from tidal debri existing between M81 and M82. M81 has the distinction of being the nearest spiral galaxy to have an active galactic nucleus (

Spiral galaxy M81 in the Great Bear - Spiral galaxy M81 in Ursa Major - The spiral galaxy M81 is located 12 million years ago - light from Earth. Its arms are home to star-forming regions while its core is surrounded by much older yellow stars. In the background at the top, an irregular dwarf galaxy, Holmberg IX. Image obtained by an amateur telescope of 50 cm, composting different poses. M81 is the brightest member of the nearby galactic group called the M81 group. This group contains at least 25 other members including the peculiar starburst galaxy M82, the peculiar galaxy NGC 3077 and many dwarfs galaxies. The core galaxies of the group (M81, M82, NGC 3077, NGC 2976) are strongly interacting and are all imbedded within a large and extended molecular gas cloud. The Dwarf irregular Holmberg IX (seen above M81 in the image) most likely condensed from tidal debri existing between M81 and M82. M81 has the distinction of being the nearest spiral galaxy to have an active galactic nucleus (

R. Jay GaBany

PIX4610325

Galaxies NGC 3718 and NGC 3729 in the Great Bear - Galaxies NGC 3718 and NGC 3729 in Ursa Major - NGC 3718 is a special galaxy located about 42 million years ago - light from Earth in the constellation of the Great Bear. It's an active nucleus galaxy. Its tormented shape is probably due to the attraction exerted by another galaxy, NGC 3729, visible to its left. To the south, Arp 322 (or Hickson 56), is a group of 5 galaxies far farther away, located about 300 million light years away from Earth. NGC 3718 and its companion NGC 3729 (left) are physically related members of the Ursa Major galaxy cluster. The two galaxies appear to orbit each other at a projected separation of 147,000 light years. NGC 3718 (Arp 214) seems to have a rudimentary bar and spiral structure although it is recognized as a peculiar galaxy and as such is listed within ARP's Atlas of Peculiar Galaxies. NGC 3718 contains an active galactic nucleus (AGN) and is known as a Seyfert type 1.9 galaxy. Its strange shape is

Galaxies NGC 3718 and NGC 3729 in the Great Bear - Galaxies NGC 3718 and NGC 3729 in Ursa Major - NGC 3718 is a special galaxy located about 42 million years ago - light from Earth in the constellation of the Great Bear. It's an active nucleus galaxy. Its tormented shape is probably due to the attraction exerted by another galaxy, NGC 3729, visible to its left. To the south, Arp 322 (or Hickson 56), is a group of 5 galaxies far farther away, located about 300 million light years away from Earth. NGC 3718 and its companion NGC 3729 (left) are physically related members of the Ursa Major galaxy cluster. The two galaxies appear to orbit each other at a projected separation of 147,000 light years. NGC 3718 (Arp 214) seems to have a rudimentary bar and spiral structure although it is recognized as a peculiar galaxy and as such is listed within ARP's Atlas of Peculiar Galaxies. NGC 3718 contains an active galactic nucleus (AGN) and is known as a Seyfert type 1.9 galaxy. Its strange shape is

R. Gendler

PIX4610948

Centaurus A elliptical galaxy (NGC 5128) in Centaurus - Galaxy Centaurus A (NGC 5128) - The galaxy NGC 5128 is located about 13 million light years away from Earth in the southern constellation of Centaurus. A broad dark band crosses it in the middle, a probable vestige of a collision with a spiral galaxy. This Giant Galaxy is a powerful radio source known as Centaurus A. It is an active galaxy whose energy comes from a supermassive black hole. The green dot visible in the dust strip is a supernova, the supernova 1986g. It appears green because the red filter image that made this trichromy image was only taken a year after the event and the supernova had weakened. Image obtained from the 3.9m telescope of Siding Spring, Australia. Centaurus A is a most unusual galaxy. The circular, uniformly bright portion is composed of several thousand million stars, most of them old and yellowish. The galaxy is girded by a dense dust lane which obscures and reddens the light of stars behind it. Some

Centaurus A elliptical galaxy (NGC 5128) in Centaurus - Galaxy Centaurus A (NGC 5128) - The galaxy NGC 5128 is located about 13 million light years away from Earth in the southern constellation of Centaurus. A broad dark band crosses it in the middle, a probable vestige of a collision with a spiral galaxy. This Giant Galaxy is a powerful radio source known as Centaurus A. It is an active galaxy whose energy comes from a supermassive black hole. The green dot visible in the dust strip is a supernova, the supernova 1986g. It appears green because the red filter image that made this trichromy image was only taken a year after the event and the supernova had weakened. Image obtained from the 3.9m telescope of Siding Spring, Australia. Centaurus A is a most unusual galaxy. The circular, uniformly bright portion is composed of several thousand million stars, most of them old and yellowish. The galaxy is girded by a dense dust lane which obscures and reddens the light of stars behind it. Some

PIX4612278

Elliptical galaxy Centaurus A (NGC 5128) in the Centaurus - Galaxy Centaurus A (NGC 5128). Wide field - The NGC 5128 galaxy is about 13 million light years away from Earth. Image obtained from the 1.2m telescope of Siding Spring, Australia. Centaurus A is a most unusual galaxy, set in a rich part of the southern sky. not only are there plenty of stars here to catch the eye, but the region is rich in galaxies as well. One of the nearer galaxies, at 13 million light years away, Centaurus A is the most powerful nearby radio source and is also a copious source of X - and gamma rays as well as visible and infrared radiation

Elliptical galaxy Centaurus A (NGC 5128) in the Centaurus - Galaxy Centaurus A (NGC 5128). Wide field - The NGC 5128 galaxy is about 13 million light years away from Earth. Image obtained from the 1.2m telescope of Siding Spring, Australia. Centaurus A is a most unusual galaxy, set in a rich part of the southern sky. not only are there plenty of stars here to catch the eye, but the region is rich in galaxies as well. One of the nearer galaxies, at 13 million light years away, Centaurus A is the most powerful nearby radio source and is also a copious source of X - and gamma rays as well as visible and infrared radiation

PIX4612296

Crater of Bromo volcano, Java island, Indonesia (photo)

Crater of Bromo volcano, Java island, Indonesia (photo)

L. Gerosa

DGA1135103

Ash fall from Karymsky Volcano, Russia, Natural Colour Satellite Image (photo)

Ash fall from Karymsky Volcano, Russia, Natural Colour Satellite Image (photo)

UIG3274382

Spiral galaxy M81 in the Great Bear - Spiral galaxy M81 in Ursa Major - The spiral galaxy M81 is located 12 million years ago - light from Earth. Its arms are home to star-forming regions while its core is surrounded by much older yellow stars. An irregular dwarf galaxy, PGC 28757 (Holmberg IX), is visible at the top of the picture. M81 is the brightest member of the nearby galactic group called the M81 group. This group contains at least 25 other members including the peculiar starburst galaxy M82, the peculiar galaxy NGC 3077 and many dwarfs galaxies. The core galaxies of the group (M81, M82, NGC 3077, NGC 2976) are strongly interacting and are all imbedded within a large and extended molecular gas cloud. The Dwarf irregular Holmberg IX (seen above M81 in the image) most likely condensed from tidal debri existing between M81 and M82. M81 has the distinction of being the nearest spiral galaxy to have an active galactic nucleus (AGN). AGN galaxies are luminous galaxies that demonstrate

Spiral galaxy M81 in the Great Bear - Spiral galaxy M81 in Ursa Major - The spiral galaxy M81 is located 12 million years ago - light from Earth. Its arms are home to star-forming regions while its core is surrounded by much older yellow stars. An irregular dwarf galaxy, PGC 28757 (Holmberg IX), is visible at the top of the picture. M81 is the brightest member of the nearby galactic group called the M81 group. This group contains at least 25 other members including the peculiar starburst galaxy M82, the peculiar galaxy NGC 3077 and many dwarfs galaxies. The core galaxies of the group (M81, M82, NGC 3077, NGC 2976) are strongly interacting and are all imbedded within a large and extended molecular gas cloud. The Dwarf irregular Holmberg IX (seen above M81 in the image) most likely condensed from tidal debri existing between M81 and M82. M81 has the distinction of being the nearest spiral galaxy to have an active galactic nucleus (AGN). AGN galaxies are luminous galaxies that demonstrate

R. Gendler

PIX4610379

The Adventures of Special Correspondents on Active Service (engraving)

The Adventures of Special Correspondents on Active Service (engraving)

Villiers, Frederic (1851-1922) (after)

LIP1044796

Eruption at Chikurachki Volcano, Russia, Natural Colour Satellite Image (photo)

Eruption at Chikurachki Volcano, Russia, Natural Colour Satellite Image (photo)

UIG3274834

Mount Agung, active volcano, Bali, Indonesia (photo)

Mount Agung, active volcano, Bali, Indonesia (photo)

DGA1134528

Elliptical Galaxy Centaurus A (NGC 5128) - The galaxy Centaurus A - The galaxy NGC 5128 is located about 13 million light years away from Earth in the southern constellation of Centaurus. This giant galaxy is a powerful radio source known as Centaurus A. The central dark band would be the rest of dust in a spiral galaxy smaller than the giant galaxy would have cannibalized. Centaurus A is an active galaxy whose energy comes from a supermassive black hole. Image made with an amateur instrument, a 130 mm bezel. Designated as radio source Centaurus A, NGC 5128 is one of the most peculiar galaxies in the sky. It is bisected by a dark lane that is considered the dust remnant of a smaller spiral galaxy that was cannibalized by the larger elliptical galaxy. The collision resulted in a burst of star formation. A gigantic black hole equivalent to one billion solar masses resides inside NGC 5128

Elliptical Galaxy Centaurus A (NGC 5128) - The galaxy Centaurus A - The galaxy NGC 5128 is located about 13 million light years away from Earth in the southern constellation of Centaurus. This giant galaxy is a powerful radio source known as Centaurus A. The central dark band would be the rest of dust in a spiral galaxy smaller than the giant galaxy would have cannibalized. Centaurus A is an active galaxy whose energy comes from a supermassive black hole. Image made with an amateur instrument, a 130 mm bezel. Designated as radio source Centaurus A, NGC 5128 is one of the most peculiar galaxies in the sky. It is bisected by a dark lane that is considered the dust remnant of a smaller spiral galaxy that was cannibalized by the larger elliptical galaxy. The collision resulted in a burst of star formation. A gigantic black hole equivalent to one billion solar masses resides inside NGC 5128

Jerry Lodriguss

PIX4612235

Barree spiral galaxy NGC 1365 in the Furnace - Barred spiral galaxy NGC 1365 in Fornax - NGC 1365 is a barree spiral galaxy that extends over 200,000 years - light. Located 60 million years ago - light, it belongs to the cluster of galaxies of the Furnace. Image obtained in 1999 by the European telescope Antu of the VLT in Chile. NGC 1365 is one of the most prominent “” barred”” galaxies in the sky. It is a supergiant galaxy with a diameter of about 200,000 light - years, seen in the direction of the southern constellation Fornax. It is a major member of the Fornax Cluster of Galaxies. The distance is about 60 million light - years. A massive straight bar runs through this galaxy and contains the nucleus at the centre. It consists mostly of older stars that give a reddish colour to the bar.The gravitational perturbation from the bar causes interstellar gas and dust clouds to form a pair of spiral arms that extend from the ends of the bar. Young luminous hot stars, born out of the inter

Barree spiral galaxy NGC 1365 in the Furnace - Barred spiral galaxy NGC 1365 in Fornax - NGC 1365 is a barree spiral galaxy that extends over 200,000 years - light. Located 60 million years ago - light, it belongs to the cluster of galaxies of the Furnace. Image obtained in 1999 by the European telescope Antu of the VLT in Chile. NGC 1365 is one of the most prominent “” barred”” galaxies in the sky. It is a supergiant galaxy with a diameter of about 200,000 light - years, seen in the direction of the southern constellation Fornax. It is a major member of the Fornax Cluster of Galaxies. The distance is about 60 million light - years. A massive straight bar runs through this galaxy and contains the nucleus at the centre. It consists mostly of older stars that give a reddish colour to the bar.The gravitational perturbation from the bar causes interstellar gas and dust clouds to form a pair of spiral arms that extend from the ends of the bar. Young luminous hot stars, born out of the inter

PIX4609836

Spiral galaxy M77 in the Whale - Active galaxy M77 (NGC 1068) in Cetus - M77 (NGC 1068) This active galaxy is a typical example of a galaxy in Seyfert II. It has an active core and houses a massive black hole. She is the object of intense star formation in her spiral arms. NGC 1068 is around 50 million years of light from Earth. M77 is an archetypical example of a Seyfert type II galaxy and the brightest galaxy of its class. M77 is a large galaxy and together with its faint outer spiral arms may extend up to 170,000 light years across. It is located about 50 million light years away in Cetus constellation. In contrast to a normal galactic nucleus the energy released from the Seyfert nucleus arises from a nonstellar source. The central engine of the Seyfert nucleus (and all AGN) is believed to be an accretion disk that continuously drops matter into a supermassive black hole

Spiral galaxy M77 in the Whale - Active galaxy M77 (NGC 1068) in Cetus - M77 (NGC 1068) This active galaxy is a typical example of a galaxy in Seyfert II. It has an active core and houses a massive black hole. She is the object of intense star formation in her spiral arms. NGC 1068 is around 50 million years of light from Earth. M77 is an archetypical example of a Seyfert type II galaxy and the brightest galaxy of its class. M77 is a large galaxy and together with its faint outer spiral arms may extend up to 170,000 light years across. It is located about 50 million light years away in Cetus constellation. In contrast to a normal galactic nucleus the energy released from the Seyfert nucleus arises from a nonstellar source. The central engine of the Seyfert nucleus (and all AGN) is believed to be an accretion disk that continuously drops matter into a supermassive black hole

Jim Misti

PIX4609594

Active galaxy NGC 1068 in the Whale - Active galaxy M77 (NGC 1068) in Cetus - This active galaxy is the typical example of a galaxy of Seyfert II. M77 (NGC 1068) has an active core and houses a massive black hole. She is the object of intense star formation in her spiral arms. NGC 1068 is around 50 million years of light from Earth. Image obtained with a telescope 61 cm in diameter. Located about 60 million light years from Earth, towards the direction of the constellation named Cetus, is an enormous galaxy, much larger than our own, that is surrounded by a even larger cloud of obscuring dust. M77 (NGC 1068) has a powerful jet pouring copious amounts of material into inter - galactic space at enormous speed. This galaxy is a seyfert II type with an active nucleus. It is now believed that the source of this conmotion is a super - massive black hole, ten million times more massive than our Sun, in the process of absorbing material that has ventured too close. Image taken with a 24 - inch

Active galaxy NGC 1068 in the Whale - Active galaxy M77 (NGC 1068) in Cetus - This active galaxy is the typical example of a galaxy of Seyfert II. M77 (NGC 1068) has an active core and houses a massive black hole. She is the object of intense star formation in her spiral arms. NGC 1068 is around 50 million years of light from Earth. Image obtained with a telescope 61 cm in diameter. Located about 60 million light years from Earth, towards the direction of the constellation named Cetus, is an enormous galaxy, much larger than our own, that is surrounded by a even larger cloud of obscuring dust. M77 (NGC 1068) has a powerful jet pouring copious amounts of material into inter - galactic space at enormous speed. This galaxy is a seyfert II type with an active nucleus. It is now believed that the source of this conmotion is a super - massive black hole, ten million times more massive than our Sun, in the process of absorbing material that has ventured too close. Image taken with a 24 - inch

Adam Block

PIX4609602

Spiral galaxy NGC 1566 in the bream - The Seyfert Galaxy NGC 1566: NGC 1566 is a spiral galaxy located about 40 million light years ago. Its core is very bright. It is an active galaxy called Seyfert, which probably houses a black hole in its heart. Image obtained with the Hubble telescope - NGC 1566 is a galaxy located approximately 40 million light-years away in the constellation of Dorado (The Dolphinfish). NGC 1566 is an intermediate spiral galaxy, meaning that while it does not have a well defined bar-shaped region of stars at its centre - like barred spirals - it is not quite an unbarred spiral either (heic9902o). The small but extremely bright nucleus of NGC 1566 is clearly visible in this image, a telltale sign of its membership of the Seyfert class of galaxies. The centres of such galaxies are very active and luminous, emitting strong bursts of radiation and potentially harbouring supermassive black holes that are many millions of times the mass of the Sun. NGC 1566 is not jus

Spiral galaxy NGC 1566 in the bream - The Seyfert Galaxy NGC 1566: NGC 1566 is a spiral galaxy located about 40 million light years ago. Its core is very bright. It is an active galaxy called Seyfert, which probably houses a black hole in its heart. Image obtained with the Hubble telescope - NGC 1566 is a galaxy located approximately 40 million light-years away in the constellation of Dorado (The Dolphinfish). NGC 1566 is an intermediate spiral galaxy, meaning that while it does not have a well defined bar-shaped region of stars at its centre - like barred spirals - it is not quite an unbarred spiral either (heic9902o). The small but extremely bright nucleus of NGC 1566 is clearly visible in this image, a telltale sign of its membership of the Seyfert class of galaxies. The centres of such galaxies are very active and luminous, emitting strong bursts of radiation and potentially harbouring supermassive black holes that are many millions of times the mass of the Sun. NGC 1566 is not jus

PIX4609939

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