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The European launch vehicle Vega - Illustration - European Vega Launcher - Illustration - Vega is a European Space Agency (ESA) launcher capable of placing a payload of up to 2 tonnes in low orbit. It is expected that it will join from 2010 the range of launchers of the space agency, which includes launchers Soyuz and Ariane. View of Vega artist on his shooting pitch at the Guyanese Space Center (CSG) in Kourou. Artist view of the new launch pad of ESA's Vega small satellite launcher at the Guyana Space Centre (CSG), Europe's Space Port, in Kourou, French Guiana. The Vega launcher will be operated from the former Ariane Launch Complex n* 1 (ELA-1), which was deactivated in 1989. Under development since 1998, the Vega launcher is an all - solid three - stage vehicle with a liquid - fuelled injection module, based on proven technologies from Ariane 5 booster stages and Fiatavio's Zefiro solid rocket motor. Vega will be marketed and operated by Arianespace, in parallel to Ariane 5. Vega i

The European launch vehicle Vega - Illustration - European Vega Launcher - Illustration - Vega is a European Space Agency (ESA) launcher capable of placing a payload of up to 2 tonnes in low orbit. It is expected that it will join from 2010 the range of launchers of the space agency, which includes launchers Soyuz and Ariane. View of Vega artist on his shooting pitch at the Guyanese Space Center (CSG) in Kourou. Artist view of the new launch pad of ESA's Vega small satellite launcher at the Guyana Space Centre (CSG), Europe's Space Port, in Kourou, French Guiana. The Vega launcher will be operated from the former Ariane Launch Complex n* 1 (ELA-1), which was deactivated in 1989. Under development since 1998, the Vega launcher is an all - solid three - stage vehicle with a liquid - fuelled injection module, based on proven technologies from Ariane 5 booster stages and Fiatavio's Zefiro solid rocket motor. Vega will be marketed and operated by Arianespace, in parallel to Ariane 5. Vega i

PIX4604573

Sir Armine Wodehouse, MP, at a Review of his Regiment near Norwich, 1759 circa (oil on canvas)

Sir Armine Wodehouse, MP, at a Review of his Regiment near Norwich, 1759 circa (oil on canvas)

Morier, David (1705-70) (attr. to)

NAM5925038

The Restoration of Isaac to His Father Abraham 2013 (oil on canvas)

premium — The Restoration of Isaac to His Father Abraham 2013 (oil on canvas)

The Restoration of Isaac to His Father Abraham 2013 (oil on canvas)

Adcock, Rosemarie

RAD8926472

Saturn rings seen in ultraviolet by Cassini - Saturn's rings in utraviolet - Saturn rings seen in ultraviolet by the Cassini probe. The colours indicate a different distribution of the material within the rings. This false - color image of Saturn's main rings was made by combining data from multiple star occultations using the Cassini ultraviolet imaging spectrograph. During occultations, scientists observe the brightness of a star as the rings pass in front of the star. This provides a measurement of the amount of ring material between the spacecraft and the star. Cassini has given scientists the most detailed view yet of Saturn's densely packed B ring. Cassini found that this part of the rings is densely packed with clumps, called self - gravity wakes, separated by almost empty gaps. These clumps in Saturn's B ring are neatly organized and constantly colliding, which surprised scientists. The clumps in Saturn's B ring, 30 to 50 meters (100 to 160 feet) across, are too small to be see

Saturn rings seen in ultraviolet by Cassini - Saturn's rings in utraviolet - Saturn rings seen in ultraviolet by the Cassini probe. The colours indicate a different distribution of the material within the rings. This false - color image of Saturn's main rings was made by combining data from multiple star occultations using the Cassini ultraviolet imaging spectrograph. During occultations, scientists observe the brightness of a star as the rings pass in front of the star. This provides a measurement of the amount of ring material between the spacecraft and the star. Cassini has given scientists the most detailed view yet of Saturn's densely packed B ring. Cassini found that this part of the rings is densely packed with clumps, called self - gravity wakes, separated by almost empty gaps. These clumps in Saturn's B ring are neatly organized and constantly colliding, which surprised scientists. The clumps in Saturn's B ring, 30 to 50 meters (100 to 160 feet) across, are too small to be see

PIX4625061

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. This image obtained by the Kueyen telescope of the VLT in Chile on 1 February 2000 shows the star flames that occur in the dark band of the galaxy. Centaurus A is one of the foremost examples of a radio - loud active galactic nucleus (AGN). On images obtained at optical wavelengths, thick dust layers almost completely obscure the galaxy's centre. Until 1949, NGC 5128 was thought to be a strange object in the Milky Way, but it was then identified as a powerful radio galaxy and designated Centaurus A. The distance is about 10 - 13 million light - years (3 - 4 Mpc) and the apparent visual magnitude is about 8, or 5 times too faint to be seen with the unaided eye. There is strong evidence th

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. This image obtained by the Kueyen telescope of the VLT in Chile on 1 February 2000 shows the star flames that occur in the dark band of the galaxy. Centaurus A is one of the foremost examples of a radio - loud active galactic nucleus (AGN). On images obtained at optical wavelengths, thick dust layers almost completely obscure the galaxy's centre. Until 1949, NGC 5128 was thought to be a strange object in the Milky Way, but it was then identified as a powerful radio galaxy and designated Centaurus A. The distance is about 10 - 13 million light - years (3 - 4 Mpc) and the apparent visual magnitude is about 8, or 5 times too faint to be seen with the unaided eye. There is strong evidence th

PIX4612179

Members of 1st Airborne Division take cover in a shell hole, Arnhem, 17 September 1944 (b/w photo)

Members of 1st Airborne Division take cover in a shell hole, Arnhem, 17 September 1944 (b/w photo)

Smith, D.M. Sgt. (fl.1939-45)

NAM5922355

The Deserter Apprehended, 1815 circa (oil on canvas)

The Deserter Apprehended, 1815 circa (oil on canvas)

Smirke, Robert (1752-1845)

NAM5919846

Current in the Detroit of Messina (Sicily) seen by satellite - Waves in the Messina strait seen by satellite - The Detroit of Messina is a detroit in the Mediterranean Sea that separates the Italian peninsula from the island of Sicily. It connects the Ionian Sea to the Tyrrhenian Sea. Its smallest width is 3.3 km and its depth is less than 100 metres. The currents are therefore violent in places. In this satellite photo obtained by the Terra satellite on 11 August 2003, strong waves are visible. At the bottom left, the purple spot is Mount Etna. The Messina Strait is connecting the Tyrrhenian Sea with the Ionian Sea in Mediterranean sea. With 3 kilometers (2 miles) wide at its narrowest point it doesn't grow very deep, only about 90 meters (300 feet). The Messina Strait's strong currents can rip seaweed from the ocean floor. The main current runs from south to north, but a smaller current runs in the opposite direction. The currents alternate about every six hours, and the strait's com

Current in the Detroit of Messina (Sicily) seen by satellite - Waves in the Messina strait seen by satellite - The Detroit of Messina is a detroit in the Mediterranean Sea that separates the Italian peninsula from the island of Sicily. It connects the Ionian Sea to the Tyrrhenian Sea. Its smallest width is 3.3 km and its depth is less than 100 metres. The currents are therefore violent in places. In this satellite photo obtained by the Terra satellite on 11 August 2003, strong waves are visible. At the bottom left, the purple spot is Mount Etna. The Messina Strait is connecting the Tyrrhenian Sea with the Ionian Sea in Mediterranean sea. With 3 kilometers (2 miles) wide at its narrowest point it doesn't grow very deep, only about 90 meters (300 feet). The Messina Strait's strong currents can rip seaweed from the ocean floor. The main current runs from south to north, but a smaller current runs in the opposite direction. The currents alternate about every six hours, and the strait's com

PIX4667341

San Francisco Bay area view from space - San Francisco Bay area seen from space - San Francisco Bay area seen from space on April 17, 1998 from space shuttle Columbia. San Francisco Bay Area, California April 17, 1998. Considered one of the best natural harbors in the world, San Francisco Bay, with its various sediment patterns, can be seen in this unique near - vertical view. Surrounded by the San Francisco Metropolitan area to the west and southwest, the Berkeley and Oakland Metropolitan area to the east, and the San Jose Metropolitan (not visible on the image) to the southeast, San Francisco Bay is 50 miles (80 km) long and from 3 to 13 miles (5 to 21 km) wide. Waters of the Pacific Ocean (bottom of image) enter the bay through Golden Gate, a strait between two peninsulas. The world famous Golden Gate Bridge is discernible on the image connecting the two peninsulas. The bay is as deep as 100 feet (30 meters) in spots, with a channel 50 feet (15 meters) deep maintained through the sa

San Francisco Bay area view from space - San Francisco Bay area seen from space - San Francisco Bay area seen from space on April 17, 1998 from space shuttle Columbia. San Francisco Bay Area, California April 17, 1998. Considered one of the best natural harbors in the world, San Francisco Bay, with its various sediment patterns, can be seen in this unique near - vertical view. Surrounded by the San Francisco Metropolitan area to the west and southwest, the Berkeley and Oakland Metropolitan area to the east, and the San Jose Metropolitan (not visible on the image) to the southeast, San Francisco Bay is 50 miles (80 km) long and from 3 to 13 miles (5 to 21 km) wide. Waters of the Pacific Ocean (bottom of image) enter the bay through Golden Gate, a strait between two peninsulas. The world famous Golden Gate Bridge is discernible on the image connecting the two peninsulas. The bay is as deep as 100 feet (30 meters) in spots, with a channel 50 feet (15 meters) deep maintained through the sa

PIX4672866

Dresden, historical, GDR, Shopping, Trade, Supply New department store …, 1984 (photo)

Dresden, historical, GDR, Shopping, Trade, Supply New department store …, 1984 (photo)

Sächsische Zeitung

IMO8756127

The wreck of the 'Halsewell', Indiaman, c.1786 (oil on canvas)

The wreck of the 'Halsewell', Indiaman, c.1786 (oil on canvas)

Stothard, Thomas (1755-1834)

MMM7340072

M46 star cluster and planetary nebula NGC 2438 in the stern - Open Cluster M46 and Planetary Nebula NGC 2438 - M46 (NGC 2437) is a cluster of stars aged 5400 years - light. It contains about 500 stars, 150 of which are brilliant. It is about 300 million years old. The planetary nebula NGC 2438 does not appear to belong to this cluster, and must be closer although its distance is unknown. M46 is a rich open cluster that contains a real jewel, planetary nebula NGC 2438. At 6th magnitude, M46 contains about 100 bright stars, the brightest of which is magnitude 8.7. It is about one - half degree in apparent diameter, the same size as the full moon. It is estimated to be about 300 million years old. Planetary nebula NGC 2438 is about one arc minute in diameter and shines at 10th magnitude. A planetary nebula is a shell of gas puffed off by a star late in its life cycle. Three bright stars are visible inside of the nebula, although none of them are the true central star which shed the gas. T

M46 star cluster and planetary nebula NGC 2438 in the stern - Open Cluster M46 and Planetary Nebula NGC 2438 - M46 (NGC 2437) is a cluster of stars aged 5400 years - light. It contains about 500 stars, 150 of which are brilliant. It is about 300 million years old. The planetary nebula NGC 2438 does not appear to belong to this cluster, and must be closer although its distance is unknown. M46 is a rich open cluster that contains a real jewel, planetary nebula NGC 2438. At 6th magnitude, M46 contains about 100 bright stars, the brightest of which is magnitude 8.7. It is about one - half degree in apparent diameter, the same size as the full moon. It is estimated to be about 300 million years old. Planetary nebula NGC 2438 is about one arc minute in diameter and shines at 10th magnitude. A planetary nebula is a shell of gas puffed off by a star late in its life cycle. Three bright stars are visible inside of the nebula, although none of them are the true central star which shed the gas. T

Jerry Lodriguss

PIX4568057

Bell at Pool of luxury hotel Pimalai Resort, Kantiang Beach, Ko Lanta or Koh Lanta island, Krabi, Thailand, Asia (photo)

Bell at Pool of luxury hotel Pimalai Resort, Kantiang Beach, Ko Lanta or Koh Lanta island, Krabi, Thailand, Asia (photo)

Sergi Reboredo

SRB3585124

Pool, luxury hotel Pimalai Resort, Kantiang Beach, Ko Lanta or Koh Lanta island, Krabi, Thailand, Asia (photo)

Pool, luxury hotel Pimalai Resort, Kantiang Beach, Ko Lanta or Koh Lanta island, Krabi, Thailand, Asia (photo)

Sergi Reboredo

SRB3585126

Wellness and spa of hotel Pimalai Resort, Kantiang Beach, Ko Lanta or Koh Lanta island, Krabi, Thailand, Asia (photo)

Wellness and spa of hotel Pimalai Resort, Kantiang Beach, Ko Lanta or Koh Lanta island, Krabi, Thailand, Asia (photo)

Sergi Reboredo

SRB3585120

Admiral Sir William Cornwallis (1744-1819), late 18th century to early 19th century (oil on canvas)

Admiral Sir William Cornwallis (1744-1819), late 18th century to early 19th century (oil on canvas)

Gardner, Daniel (1750-1805) (after)

MMM7337873

Foot massage in a spa of hotel Pimalai Resort, Kantiang Beach, Ko Lanta or Koh Lanta island, Krabi, Thailand, Asia (photo)

Foot massage in a spa of hotel Pimalai Resort, Kantiang Beach, Ko Lanta or Koh Lanta island, Krabi, Thailand, Asia (photo)

Sergi Reboredo

SRB3585119

Bell at Pool of luxury hotel Pimalai Resort, Kantiang Beach, Ko Lanta or Koh Lanta island, Krabi, Thailand, Asia (photo)

Bell at Pool of luxury hotel Pimalai Resort, Kantiang Beach, Ko Lanta or Koh Lanta island, Krabi, Thailand, Asia (photo)

Sergi Reboredo

SRB3585123

Pool, luxury hotel Pimalai Resort, Kantiang Beach, Ko Lanta or Koh Lanta island, Krabi, Thailand, Asia (photo)

Pool, luxury hotel Pimalai Resort, Kantiang Beach, Ko Lanta or Koh Lanta island, Krabi, Thailand, Asia (photo)

Sergi Reboredo

SRB3585125

Spiral galaxy NGC 3370 in the Lion - Spiral galaxy NGC 3370 in Leo - The spiral galaxy NGC 3370 is located about 100 million years away - light from Earth. In November 1994, light emitting from a supernova type Ia, SN 1994ae, part of this galaxy, reached Earth. In this image taken by the Hubble space telescope in May 2003, this supernova is no longer detectable. On the other hand, the telescope was able to observe in this galaxy cepheides, variable stars used to accurately measure distances in the universe and calculate the rate of expansion of the universe. Many galaxies are visible in the background. The majestic dusty spiral, NGC 3370, looms in the foreground in this NASA Hubble Space Telescope image. Recent observations taken with the Advanced Camera for Surveys show intricate spiral arm structure spotted with hot areas of new star formation. In November 1994, the light of a supernova in nearby NGC 3370 reached Earth. This stellar outburst briefly outshone all of the tens of billio

Spiral galaxy NGC 3370 in the Lion - Spiral galaxy NGC 3370 in Leo - The spiral galaxy NGC 3370 is located about 100 million years away - light from Earth. In November 1994, light emitting from a supernova type Ia, SN 1994ae, part of this galaxy, reached Earth. In this image taken by the Hubble space telescope in May 2003, this supernova is no longer detectable. On the other hand, the telescope was able to observe in this galaxy cepheides, variable stars used to accurately measure distances in the universe and calculate the rate of expansion of the universe. Many galaxies are visible in the background. The majestic dusty spiral, NGC 3370, looms in the foreground in this NASA Hubble Space Telescope image. Recent observations taken with the Advanced Camera for Surveys show intricate spiral arm structure spotted with hot areas of new star formation. In November 1994, the light of a supernova in nearby NGC 3370 reached Earth. This stellar outburst briefly outshone all of the tens of billio

PIX4610684

Spiral galaxy NGC 3370 in the Lion - Spiral galaxy NGC 3370 in Leo - The spiral galaxy NGC 3370 is located about 100 million years away - light from Earth. In November 1994, light emitting from a supernova type Ia, SN 1994ae, part of this galaxy, reached Earth. In this image taken by the Hubble space telescope in May 2003, this supernova is no longer detectable. On the other hand, the telescope was able to observe in this galaxy cepheides, variable stars used to accurately measure distances in the universe and calculate the rate of expansion of the universe. Many galaxies are visible in the background. The majestic dusty spiral, NGC 3370, looms in the foreground in this NASA Hubble Space Telescope image. Recent observations taken with the Advanced Camera for Surveys show intricate spiral arm structure spotted with hot areas of new star formation. In November 1994, the light of a supernova in nearby NGC 3370 reached Earth. This stellar outburst briefly outshone all of the tens of billio

Spiral galaxy NGC 3370 in the Lion - Spiral galaxy NGC 3370 in Leo - The spiral galaxy NGC 3370 is located about 100 million years away - light from Earth. In November 1994, light emitting from a supernova type Ia, SN 1994ae, part of this galaxy, reached Earth. In this image taken by the Hubble space telescope in May 2003, this supernova is no longer detectable. On the other hand, the telescope was able to observe in this galaxy cepheides, variable stars used to accurately measure distances in the universe and calculate the rate of expansion of the universe. Many galaxies are visible in the background. The majestic dusty spiral, NGC 3370, looms in the foreground in this NASA Hubble Space Telescope image. Recent observations taken with the Advanced Camera for Surveys show intricate spiral arm structure spotted with hot areas of new star formation. In November 1994, the light of a supernova in nearby NGC 3370 reached Earth. This stellar outburst briefly outshone all of the tens of billio

PIX4610713

Interacting galaxies NGC 4038 - 4039 in the Raven - The Antennae galaxy in Corvus - The galaxy NGC 4038 - 39 (antenna galaxy) is located about 45 million years ago - light. These two galaxies are interacting. The collision started at least 100 million years ago causes intense star formation. These images made by the Hubble space telescope on 20 January 1996 show in detail the nuclei of these two twin galaxies (right) as well as clusters of blue stars, consisting of young and massive stars (left). The scale bar at the top of each image represents 1500 years - light. These four close - up views are taken from a head - on collision between two spiral galaxies, called the Antennae galaxies, seen at image center. The scale bar at the top of each image is 1,500 light - years across. Left: the collision triggers the birth of new stars in brilliant blue star clusters, the brightest of which contains roughly a million stars. The star clusters are blue because they are very young, the youngest b

Interacting galaxies NGC 4038 - 4039 in the Raven - The Antennae galaxy in Corvus - The galaxy NGC 4038 - 39 (antenna galaxy) is located about 45 million years ago - light. These two galaxies are interacting. The collision started at least 100 million years ago causes intense star formation. These images made by the Hubble space telescope on 20 January 1996 show in detail the nuclei of these two twin galaxies (right) as well as clusters of blue stars, consisting of young and massive stars (left). The scale bar at the top of each image represents 1500 years - light. These four close - up views are taken from a head - on collision between two spiral galaxies, called the Antennae galaxies, seen at image center. The scale bar at the top of each image is 1,500 light - years across. Left: the collision triggers the birth of new stars in brilliant blue star clusters, the brightest of which contains roughly a million stars. The star clusters are blue because they are very young, the youngest b

PIX4611053

Heat wave over Spain - 01 - 07 - 2004 - Heat wave over Spain July 1st 2004 - From 29 June to 4 July 2004, a heat wave passed through Spain with ground temperatures reaching 57 degrees Celsius and an air temperature exceeding 40 degrees. Image obtained on 1 July 2004 by the Aqua satellite and the MODIS instrument showing surface temperatures; in red the highest temperatures, in pink the coldest. From June 29 to July 4, 2004, an intense heat wave swept across southern Spain, bringing air temperatures that soared above 40 degrees Celsius, and land surface temperatures near 57 degrees. On July 1, 2004, Spain (roughly the right - most three - quarters of the peninsula) and Portugal (left - hand quarter) were in the midst of a blistering heat wave that cost several people their lives. When the Moderate Resolution Imaging Spectroradiometer (MODIS) on the Aqua satellite captured this image (13:35 UTC, or 2:35 p.m. local time in Lisbon, Portugal) cool, sheltering clouds hugged only the northern

Heat wave over Spain - 01 - 07 - 2004 - Heat wave over Spain July 1st 2004 - From 29 June to 4 July 2004, a heat wave passed through Spain with ground temperatures reaching 57 degrees Celsius and an air temperature exceeding 40 degrees. Image obtained on 1 July 2004 by the Aqua satellite and the MODIS instrument showing surface temperatures; in red the highest temperatures, in pink the coldest. From June 29 to July 4, 2004, an intense heat wave swept across southern Spain, bringing air temperatures that soared above 40 degrees Celsius, and land surface temperatures near 57 degrees. On July 1, 2004, Spain (roughly the right - most three - quarters of the peninsula) and Portugal (left - hand quarter) were in the midst of a blistering heat wave that cost several people their lives. When the Moderate Resolution Imaging Spectroradiometer (MODIS) on the Aqua satellite captured this image (13:35 UTC, or 2:35 p.m. local time in Lisbon, Portugal) cool, sheltering clouds hugged only the northern

PIX4664825

Remains of the supernova Tycho in X by Chandra - In 1572, the Danish astronomer Tycho Brahe observed and studied the explosion of a star that became known as Tycho's supernova.

Remains of the supernova Tycho in X by Chandra - In 1572, the Danish astronomer Tycho Brahe observed and studied the explosion of a star that became known as Tycho's supernova.

PIX4582485

Central region of the Tarantula Nebula - The Tarantula Nebula - The Tarantula Nebula (or 30 Dorada) is the largest star-forming region of the Magellan Cloud. It is located 170,000 light years ago in the constellation Dorado (southern hemisphere). At the center of this nebula, the open cluster of R136 stars, clusters of young, hot and massive stars, aged just 5 million years. Mosaic of 5 images obtained by the Hubble space telescope. Vast Star - Forming Region 30 Doradus Nasa's Hubble Space Telescope has snapped a panoramic portrait of a vast, sculpted landscape of gas and dust where thousands of stars are being born. This fertile star - forming region, called the 30 Doradus Nebula, has a sparkling stellar centerpiece: the most spectacular cluster of massive stars in our cosmic neighborhood of about 25 galaxies. The mosaic picture shows that ultraviolet radiation and high - speed material unleashed by the stars in the cluster, called R136, are weaving a tapestry of creation and destruct

Central region of the Tarantula Nebula - The Tarantula Nebula - The Tarantula Nebula (or 30 Dorada) is the largest star-forming region of the Magellan Cloud. It is located 170,000 light years ago in the constellation Dorado (southern hemisphere). At the center of this nebula, the open cluster of R136 stars, clusters of young, hot and massive stars, aged just 5 million years. Mosaic of 5 images obtained by the Hubble space telescope. Vast Star - Forming Region 30 Doradus Nasa's Hubble Space Telescope has snapped a panoramic portrait of a vast, sculpted landscape of gas and dust where thousands of stars are being born. This fertile star - forming region, called the 30 Doradus Nebula, has a sparkling stellar centerpiece: the most spectacular cluster of massive stars in our cosmic neighborhood of about 25 galaxies. The mosaic picture shows that ultraviolet radiation and high - speed material unleashed by the stars in the cluster, called R136, are weaving a tapestry of creation and destruct

PIX4618215

Spiral Galaxy M66 in the Lion - Spiral galaxy M66 in Leo - M66 (NGC 3627) is a spiral galaxy located at a distance of about 35 million years - light. M66, with its neighbors M65 and NGC 3628, forms a remarkable triplet of galaxies, called the Lion Triplet or the M66 Group. Image obtained by the Hubble Space Telescope. The unusual spiral galaxy, Messier 66, is located at a distance of about 35 million light - years in the constellation of Leo. Together with Messier 65 and NGC 3628, Messier 66 is one third of the Leo Triplet, a trio of interacting spiral galaxies, part of the larger Messier 66 group. Messier 66 wins out in size over its fellow triplets - - it is about 100 000 light - years across. Messier 66 is the proud owner of exclusive asymmetric spiral arms which seem to climb above the galaxy's main disc and an apparently displaced nucleus. This asymmetry is unusual; most often, dense waves of gas, dust and newly born stars wind about the galaxy's centre in a symmetric way. Astrono

Spiral Galaxy M66 in the Lion - Spiral galaxy M66 in Leo - M66 (NGC 3627) is a spiral galaxy located at a distance of about 35 million years - light. M66, with its neighbors M65 and NGC 3628, forms a remarkable triplet of galaxies, called the Lion Triplet or the M66 Group. Image obtained by the Hubble Space Telescope. The unusual spiral galaxy, Messier 66, is located at a distance of about 35 million light - years in the constellation of Leo. Together with Messier 65 and NGC 3628, Messier 66 is one third of the Leo Triplet, a trio of interacting spiral galaxies, part of the larger Messier 66 group. Messier 66 wins out in size over its fellow triplets - - it is about 100 000 light - years across. Messier 66 is the proud owner of exclusive asymmetric spiral arms which seem to climb above the galaxy's main disc and an apparently displaced nucleus. This asymmetry is unusual; most often, dense waves of gas, dust and newly born stars wind about the galaxy's centre in a symmetric way. Astrono

PIX4610836

Passenger liner SS 'Normandie' (1932), c.1932 (wood, brass;silver, steel, paint;varnish)

Passenger liner SS 'Normandie' (1932), c.1932 (wood, brass;silver, steel, paint;varnish)

Montera, J. (fl.c.1932)

MMM7339843

Mars surface seen by the rover Curiosity 04/2015 - Martian surface seen from the rover Curiosity 04/2015 - Panorama of the surface of Mars on Mount Sharp. Mosaic of images obtained by the rover Curiosity and his camera Mastcam on 10 and 11 April 2015. A southward - looking panorama combining images from both cameras of the Mast Camera (Mastcam) instrument on Nasa's Curiosity Mars Rover shows diverse geological textures on Mount Sharp. Three years after landing on Mars, the mission is investigating this layered mountain for evidence about changes in Martian environmental conditions, from an ancient time when conditions were favorable for microbial life to the much - drier present. Gravel and sand ripples fill the foreground, typical of terrains that Curiosity traversed to reach Mount Sharp from its landing site. Outcrops in the midfield are of two types: dust - covered, smooth bedrock that forms the base of the mountain, and sandstone ridges that shed boulders as they erode. Rounded but

Mars surface seen by the rover Curiosity 04/2015 - Martian surface seen from the rover Curiosity 04/2015 - Panorama of the surface of Mars on Mount Sharp. Mosaic of images obtained by the rover Curiosity and his camera Mastcam on 10 and 11 April 2015. A southward - looking panorama combining images from both cameras of the Mast Camera (Mastcam) instrument on Nasa's Curiosity Mars Rover shows diverse geological textures on Mount Sharp. Three years after landing on Mars, the mission is investigating this layered mountain for evidence about changes in Martian environmental conditions, from an ancient time when conditions were favorable for microbial life to the much - drier present. Gravel and sand ripples fill the foreground, typical of terrains that Curiosity traversed to reach Mount Sharp from its landing site. Outcrops in the midfield are of two types: dust - covered, smooth bedrock that forms the base of the mountain, and sandstone ridges that shed boulders as they erode. Rounded but

PIX4616735

Admiral Augustus Keppel (1725-1786), 1765 (oil on canvas)

Admiral Augustus Keppel (1725-1786), 1765 (oil on canvas)

Reynolds, Joshua (1723-92)

MMM7337952

Galaxy cluster Abell 2667 - Galaxy cluster Abell 2667 - In this image of the galaxy cluster Abell 2667, a spiral galaxy, at the top left of the image, seems to leave a trail of gas and stars in its wake. Attracted by the high gravity of Abell 2667, this “galaxy - comete” plunges into the cluster at a speed of 3.5 million km/h, losing its gas and young stars. This phenomene may explain the presence of isolated stars in the centre of galaxy clusters. On the right, a further galaxy appears as a gravitational arc. Image obtained by the Hubble Space Telescope in October 2001. The NASA/ESA Hubble Space Telescope, in collaboration with several other ground - and space - based telescopes, has captured a galaxy being ripped apart by a galaxy cluster's gravitational field and harsh environment. The finding sheds light on the mysterious process by which gas - rich spiral - shaped galaxies might evolve into gas - poor irregular - or elliptical - shaped galaxies over billions of years. The new obse

Galaxy cluster Abell 2667 - Galaxy cluster Abell 2667 - In this image of the galaxy cluster Abell 2667, a spiral galaxy, at the top left of the image, seems to leave a trail of gas and stars in its wake. Attracted by the high gravity of Abell 2667, this “galaxy - comete” plunges into the cluster at a speed of 3.5 million km/h, losing its gas and young stars. This phenomene may explain the presence of isolated stars in the centre of galaxy clusters. On the right, a further galaxy appears as a gravitational arc. Image obtained by the Hubble Space Telescope in October 2001. The NASA/ESA Hubble Space Telescope, in collaboration with several other ground - and space - based telescopes, has captured a galaxy being ripped apart by a galaxy cluster's gravitational field and harsh environment. The finding sheds light on the mysterious process by which gas - rich spiral - shaped galaxies might evolve into gas - poor irregular - or elliptical - shaped galaxies over billions of years. The new obse

PIX4565700

Caister Castle, Norfolk

Caister Castle, Norfolk

Beaumont, George Howland (1753-1827)

USB1159949

Passenger liner SS 'Normandie' (1932), c.1932 (wood, organic, metal: brass, metal: silver, metal: steel, inorganic, paint, coating: varnish)

Passenger liner SS 'Normandie' (1932), c.1932 (wood, organic, metal: brass, metal: silver, metal: steel, inorganic, paint, coating: varnish)

Montera, J. (fl.c.1932)

MMM7339845

The 'St Andrew' at Sea in a Moderate Breeze, c.1673 (oil on canvas)

The 'St Andrew' at Sea in a Moderate Breeze, c.1673 (oil on canvas)

Velde, Willem van de, the Younger (1633-1707)

MMM7342592

Interacting galaxies UGC 8058 - Interacting galaxies UGC 8058 - The galaxy UGC 8058 (Markarian 231) is located about 600 million light years away from Earth in the constellation Big Bear. This interacting galaxy houses a quasar in its center. It is one of the brightest ultra-bright infrared galaxy known to date. It has a central black hole and intense star formations are observed. Image obtained by the Hubble Space Telescope on May 10, 2002. The extraordinary galaxy UGC 8058, also known as Markarian 231, was discovered in 1969 as part of a survey searching for galaxies with strong ultraviolet radiation. It has long tidal tails and a disturbed shape. Results from the first spectrum showed clear signs of the presence of a powerful quasar in the center that made Markarian 231 unique in the Markarian sample. Markarian 231 has maintained its reputation as an exceptional object since those early observations and continues to be a favorite target in all wavelength regimes. Its infrared lumino

Interacting galaxies UGC 8058 - Interacting galaxies UGC 8058 - The galaxy UGC 8058 (Markarian 231) is located about 600 million light years away from Earth in the constellation Big Bear. This interacting galaxy houses a quasar in its center. It is one of the brightest ultra-bright infrared galaxy known to date. It has a central black hole and intense star formations are observed. Image obtained by the Hubble Space Telescope on May 10, 2002. The extraordinary galaxy UGC 8058, also known as Markarian 231, was discovered in 1969 as part of a survey searching for galaxies with strong ultraviolet radiation. It has long tidal tails and a disturbed shape. Results from the first spectrum showed clear signs of the presence of a powerful quasar in the center that made Markarian 231 unique in the Markarian sample. Markarian 231 has maintained its reputation as an exceptional object since those early observations and continues to be a favorite target in all wavelength regimes. Its infrared lumino

PIX4613687

Barree spiral galaxy NGC 1097 in the Furnace - Barred spiral galaxy NGC 1097 in Fornax - Located at a distance of about 45 million years - light, NGC 1097 is the object of intense star formation and is an active core galaxy with a supermassive black hole in its heart. Image obtained by the Hubble Space Telescope (HST). The NASA/ESA Hubble Space Telescope provides us with a spectacular image of the bright star - forming ring that surrounds the heart of the barred spiral galaxy NGC 1097. In this image, the larger - scale structure of the galaxy is barely visible: its comparatively dim spiral arms, which surround its heart in a loose embrace, reach out beyond the edges of this frame. This face - on galaxy, lying 45 million light - years away from Earth in the southern constellation of Fornax (The Furnace), is particularly attractive for astronomers. NGC 1097 is a Seyfert galaxy. Lurking at the very centre of the galaxy, a supermassive black hole 100 million times the mass of our Sun is gr

Barree spiral galaxy NGC 1097 in the Furnace - Barred spiral galaxy NGC 1097 in Fornax - Located at a distance of about 45 million years - light, NGC 1097 is the object of intense star formation and is an active core galaxy with a supermassive black hole in its heart. Image obtained by the Hubble Space Telescope (HST). The NASA/ESA Hubble Space Telescope provides us with a spectacular image of the bright star - forming ring that surrounds the heart of the barred spiral galaxy NGC 1097. In this image, the larger - scale structure of the galaxy is barely visible: its comparatively dim spiral arms, which surround its heart in a loose embrace, reach out beyond the edges of this frame. This face - on galaxy, lying 45 million light - years away from Earth in the southern constellation of Fornax (The Furnace), is particularly attractive for astronomers. NGC 1097 is a Seyfert galaxy. Lurking at the very centre of the galaxy, a supermassive black hole 100 million times the mass of our Sun is gr

PIX4609655

Auckland Region (New Zealand) satellite view - Auckland, New Zealand - Auckland Region, the largest urban area in New Zealand, in the North Island, viewed by Landsat satellite - 7 August 27, 2002. Auckland, New Zealand's largest city, is located on the country's North Island. Nearly a third of New Zealand's population lives in Auckland - - more than three million people. This natural - color (photo - like) image of Auckland was acquired on August 27, 2002, by Nasa's Landsat 7 satellite. The most densely developed areas appear white and gray, while suburban areas appear grayish green - - a mixture of houses, streets, and lawns. The city spreads out across various peninsulas surrounding Tamaki Strait and other bays and inlets. The city has been built up around the Auckland Volcanic Field; within a 20 - kilometer (12.4 - mile) radius of the heart of the city, there are 49 volcanoes, most of them small cones less than 150 meters (492 feet) high. Many of them have been protected as parks or

Auckland Region (New Zealand) satellite view - Auckland, New Zealand - Auckland Region, the largest urban area in New Zealand, in the North Island, viewed by Landsat satellite - 7 August 27, 2002. Auckland, New Zealand's largest city, is located on the country's North Island. Nearly a third of New Zealand's population lives in Auckland - - more than three million people. This natural - color (photo - like) image of Auckland was acquired on August 27, 2002, by Nasa's Landsat 7 satellite. The most densely developed areas appear white and gray, while suburban areas appear grayish green - - a mixture of houses, streets, and lawns. The city spreads out across various peninsulas surrounding Tamaki Strait and other bays and inlets. The city has been built up around the Auckland Volcanic Field; within a 20 - kilometer (12.4 - mile) radius of the heart of the city, there are 49 volcanoes, most of them small cones less than 150 meters (492 feet) high. Many of them have been protected as parks or

PIX4675653

Andromede Galaxy (M31) infrared view - The Andromeda galaxy seen in infrared - This image shows the difference in infrared radiation between the light emitted by the aged stars (blue) and that emitted by the dust (star-forming zone, yellow and red). This image obtained by the WISE satellite also distinguishes the two Andromede satellite galaxies, M32 (above the nucleus of the Andromede galaxy) and NGC 205 (M110) below. Infrared composite at the following wavelengths: 3.4 and 4.6 microns (blue), 12 microns (green), and 22 microns dust sensitive, red. M31, is captured in full in this new image from Nasa's Wide - field Infrared Survey Explorer, or WISE. The mosaic covers an area equivalent to more than 100 full moons, or five degrees across the sky. WISE used all four of its infrared detectors to capture this picture (3.4 - and 4.6 - micron light is colored blue; 12 - micron light is green; and 22 - micron light is red). Blue highlights mature stars, while yellow and red show dust heated

Andromede Galaxy (M31) infrared view - The Andromeda galaxy seen in infrared - This image shows the difference in infrared radiation between the light emitted by the aged stars (blue) and that emitted by the dust (star-forming zone, yellow and red). This image obtained by the WISE satellite also distinguishes the two Andromede satellite galaxies, M32 (above the nucleus of the Andromede galaxy) and NGC 205 (M110) below. Infrared composite at the following wavelengths: 3.4 and 4.6 microns (blue), 12 microns (green), and 22 microns dust sensitive, red. M31, is captured in full in this new image from Nasa's Wide - field Infrared Survey Explorer, or WISE. The mosaic covers an area equivalent to more than 100 full moons, or five degrees across the sky. WISE used all four of its infrared detectors to capture this picture (3.4 - and 4.6 - micron light is colored blue; 12 - micron light is green; and 22 - micron light is red). Blue highlights mature stars, while yellow and red show dust heated

PIX4608987

Nebula NGC 604 in the galaxy M33 - NGC 604 star forming nebula - NGC 604, is a very large star-forming region located in the galaxy M33 of the Triangle. This image is a composite of X-ray images (blue) obtained by the Chandra Space Telescope and visible (green and red) by the Hubble Space Telescope. The study of very hot gas observed in X-ray allows us to better understand the star formation activity within this nebula. NGC 604, is one of the largest known seething cauldrons of star birth in a nearby galaxy. NGC 604 is similar to familiar star - birth regions in our Milky Way galaxy, such as the Orion Nebula, but it is vastly larger in extent and contains many more recently formed stars. This monstrous star - birth region contains more than 200 brilliant blue stars within a cloud of glowing gases some 1,300 light - years across, nearly 100 times the size of the Orion Nebula. The bright stars in NGC 604 are extremely young having formed a mere 3 million years ago. The most massive stars

Nebula NGC 604 in the galaxy M33 - NGC 604 star forming nebula - NGC 604, is a very large star-forming region located in the galaxy M33 of the Triangle. This image is a composite of X-ray images (blue) obtained by the Chandra Space Telescope and visible (green and red) by the Hubble Space Telescope. The study of very hot gas observed in X-ray allows us to better understand the star formation activity within this nebula. NGC 604, is one of the largest known seething cauldrons of star birth in a nearby galaxy. NGC 604 is similar to familiar star - birth regions in our Milky Way galaxy, such as the Orion Nebula, but it is vastly larger in extent and contains many more recently formed stars. This monstrous star - birth region contains more than 200 brilliant blue stars within a cloud of glowing gases some 1,300 light - years across, nearly 100 times the size of the Orion Nebula. The bright stars in NGC 604 are extremely young having formed a mere 3 million years ago. The most massive stars

PIX4617509

Galaxies Group: Stephan's Quintet in Pegase - Stephan's Quintet group of galaxies - Image obtained with the Hubble space telescope. This group of 5 galaxies is located about 270 million light years away from Earth. In this image three star-forming regions are visible: in the long arm of NGC 7319 (near the center); the gas debris of two galaxies, NGC 7318B and NGC 7318A (upper right); and in the upper left. Blue indicates that these stars are young. The NASA Hubble Space Telescope photo shows three regions of star birth: the long, sweeping tail and spiral arms of NGC 7319 [near center]; the gaseous debris of two galaxies, NGC 7318B and NGC 7318A [top right]; and the area north of those galaxies, dubbed the northern starburst region [top left]. The clusters' bluish color indicates that they're relatively young. Their ages span from about 2 million to more than 1 billion years old. The brilliant star clusters in NGC 7318B's spiral arm (about 30,000 light - years long) and the northern sta

Galaxies Group: Stephan's Quintet in Pegase - Stephan's Quintet group of galaxies - Image obtained with the Hubble space telescope. This group of 5 galaxies is located about 270 million light years away from Earth. In this image three star-forming regions are visible: in the long arm of NGC 7319 (near the center); the gas debris of two galaxies, NGC 7318B and NGC 7318A (upper right); and in the upper left. Blue indicates that these stars are young. The NASA Hubble Space Telescope photo shows three regions of star birth: the long, sweeping tail and spiral arms of NGC 7319 [near center]; the gaseous debris of two galaxies, NGC 7318B and NGC 7318A [top right]; and the area north of those galaxies, dubbed the northern starburst region [top left]. The clusters' bluish color indicates that they're relatively young. Their ages span from about 2 million to more than 1 billion years old. The brilliant star clusters in NGC 7318B's spiral arm (about 30,000 light - years long) and the northern sta

PIX4565466

Planetary nebula CRL 2688 dans le Swan/HST - This image of the Egg Nebula, also known as CRL2688 and located roughly 3,000 light - years from us, was taken in red light with the Wide Field and Planetary Camera 2 (WFPC2) aboard Nasa's Hubble Space Telescope.The image shows a pair of mysterious “” searchlight” beams emerging from a hidden star, criss - Yeah. crossed by numerous bright arcs. This image sheds new light on the poorly understood ejection of stellar matter which accompanies the slow death of Sun - like stars. The image is shown in false color. The central star in CRL2688 was a red giant a few hundred years ago. The nebula is really a large cloud of dust and gas ejected by the star, expanding at a speed of 20 km/s (115,000 mph). A dense cocoon of dust (the dark band in the image center) enshrouds the star and hides it from our view. Starlight escapes more easily in directions where the cocoon is thinner, and is reflected towards us by dust particles in the cloud, giving it its

Planetary nebula CRL 2688 dans le Swan/HST - This image of the Egg Nebula, also known as CRL2688 and located roughly 3,000 light - years from us, was taken in red light with the Wide Field and Planetary Camera 2 (WFPC2) aboard Nasa's Hubble Space Telescope.The image shows a pair of mysterious “” searchlight” beams emerging from a hidden star, criss - Yeah. crossed by numerous bright arcs. This image sheds new light on the poorly understood ejection of stellar matter which accompanies the slow death of Sun - like stars. The image is shown in false color. The central star in CRL2688 was a red giant a few hundred years ago. The nebula is really a large cloud of dust and gas ejected by the star, expanding at a speed of 20 km/s (115,000 mph). A dense cocoon of dust (the dark band in the image center) enshrouds the star and hides it from our view. Starlight escapes more easily in directions where the cocoon is thinner, and is reflected towards us by dust particles in the cloud, giving it its

PIX4623752

Star Vega in the Lyre - Star Vega in infrared - 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 after Sirius in the northern hemisphere. It's seen here in infrared by the Spitzer space telescope. Observed in this wavelength, the dust cloud surrounding the star appears. Nasa's Spitzer Space Telescope captured these images of the star Vega, located 25 light years away in the constellation Lyra. Spitzer was able to detect the heat radiation from the cloud of dust around the star and found that the debris disk is much larger than previously thought. This side - by - side comparison, taken by Spitzer's multiband imaging photometer, shows the warm infrared glows from dust particles orbiting the star at wavelengths of 24 microns (on the left in blue) and 70 microns (on the right in red). Both images show a very large, circular and smooth debris disk. The disk radius extends to at least 815 astronomical

Star Vega in the Lyre - Star Vega in infrared - 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 after Sirius in the northern hemisphere. It's seen here in infrared by the Spitzer space telescope. Observed in this wavelength, the dust cloud surrounding the star appears. Nasa's Spitzer Space Telescope captured these images of the star Vega, located 25 light years away in the constellation Lyra. Spitzer was able to detect the heat radiation from the cloud of dust around the star and found that the debris disk is much larger than previously thought. This side - by - side comparison, taken by Spitzer's multiband imaging photometer, shows the warm infrared glows from dust particles orbiting the star at wavelengths of 24 microns (on the left in blue) and 70 microns (on the right in red). Both images show a very large, circular and smooth debris disk. The disk radius extends to at least 815 astronomical

PIX4571758

Planet around the star Fomalhaut - Planet orbiting star Fomalhaut - First visible light photo of an extrasolar planet obtained by the space telescope Hubble. The planet called Fomalhaut b, is a planet with a mass close to Jupiter, orbiting the star Fomalhaut, 25 years - light from Earth in the constellation of Southern Fish. The star Fomalhaut (indicated by a white dot) is hidden here to show the dust disc surrounding it and the position of the planet. Located at a distance of about four times that separating Neptune from the Sun, Fomalhaut b makes a complete orbit around its star in 872 years. November 2008 - This image, taken with the Advanced Camera for Surveys aboard the NASA/ESA Hubble Space Telescope, shows the newly discovered planet, Fomalhaut b, orbiting its parent star, Fomalhaut. The small white box at lower right pinpoints the planet's location. Fomalhaut b has carved a path along the inner edge of a vast, dusty debris ring encircling Fomalhaut that is 34.5 billion kilomete

Planet around the star Fomalhaut - Planet orbiting star Fomalhaut - First visible light photo of an extrasolar planet obtained by the space telescope Hubble. The planet called Fomalhaut b, is a planet with a mass close to Jupiter, orbiting the star Fomalhaut, 25 years - light from Earth in the constellation of Southern Fish. The star Fomalhaut (indicated by a white dot) is hidden here to show the dust disc surrounding it and the position of the planet. Located at a distance of about four times that separating Neptune from the Sun, Fomalhaut b makes a complete orbit around its star in 872 years. November 2008 - This image, taken with the Advanced Camera for Surveys aboard the NASA/ESA Hubble Space Telescope, shows the newly discovered planet, Fomalhaut b, orbiting its parent star, Fomalhaut. The small white box at lower right pinpoints the planet's location. Fomalhaut b has carved a path along the inner edge of a vast, dusty debris ring encircling Fomalhaut that is 34.5 billion kilomete

PIX4573100

Planet around the star Fomalhaut - Planet orbiting star Fomalhaut - First visible light photo of an extrasolar planet obtained by the space telescope Hubble. The planet called Fomalhaut b, is a planet with a mass close to Jupiter, orbiting the star Fomalhaut, 25 years - light from Earth in the constellation of Southern Fish. The star Fomalhaut (indicated by a white dot) is hidden here to show the dust disc surrounding it and the position of the planet. Located at a distance of about four times that separating Neptune from the Sun, Fomalhaut b makes a complete orbit around its star in 872 years. November 2008 - This image, taken with the Advanced Camera for Surveys aboard the NASA/ESA Hubble Space Telescope, shows the newly discovered planet, Fomalhaut b, orbiting its parent star, Fomalhaut. The small white box at lower right pinpoints the planet's location. Fomalhaut b has carved a path along the inner edge of a vast, dusty debris ring encircling Fomalhaut that is 34.5 billion kilomete

Planet around the star Fomalhaut - Planet orbiting star Fomalhaut - First visible light photo of an extrasolar planet obtained by the space telescope Hubble. The planet called Fomalhaut b, is a planet with a mass close to Jupiter, orbiting the star Fomalhaut, 25 years - light from Earth in the constellation of Southern Fish. The star Fomalhaut (indicated by a white dot) is hidden here to show the dust disc surrounding it and the position of the planet. Located at a distance of about four times that separating Neptune from the Sun, Fomalhaut b makes a complete orbit around its star in 872 years. November 2008 - This image, taken with the Advanced Camera for Surveys aboard the NASA/ESA Hubble Space Telescope, shows the newly discovered planet, Fomalhaut b, orbiting its parent star, Fomalhaut. The small white box at lower right pinpoints the planet's location. Fomalhaut b has carved a path along the inner edge of a vast, dusty debris ring encircling Fomalhaut that is 34.5 billion kilomete

PIX4573107

Nebulae NGC 6334 and NGC 6357 in Scorpio - Nebulae NGC 6334 and NGC 6357 in Scorpius: These nebulae are located about 5500 light years from Earth - Located in the constellation of Scorpius, the Cat's Paw Nebula resemble a faint, luminous paw-print on the sky. Deep images reveal that the nebula is about a degree across in the sky. At a distance of about 5500 light-years away it is a truly vast structure spanning almost 100 light-years across. The sculpted gases of NGC 6334 are illuminated by the light of numerous powerful stars, some exceeding 10 solar masses. The two brilliant blue stars in the upper left are Lambda and Kappa Scorpii. Many of these luminous hot stars are surprisingly not visible because they lie within the dusty plane of our galaxy. At infrared wavelengths the numerous hot stars are revealed and the nature of this object as a region of massive star formation becomes clear. In the past decade water masers, molecular outflows, and x-ray sources have provided direct evide

Nebulae NGC 6334 and NGC 6357 in Scorpio - Nebulae NGC 6334 and NGC 6357 in Scorpius: These nebulae are located about 5500 light years from Earth - Located in the constellation of Scorpius, the Cat's Paw Nebula resemble a faint, luminous paw-print on the sky. Deep images reveal that the nebula is about a degree across in the sky. At a distance of about 5500 light-years away it is a truly vast structure spanning almost 100 light-years across. The sculpted gases of NGC 6334 are illuminated by the light of numerous powerful stars, some exceeding 10 solar masses. The two brilliant blue stars in the upper left are Lambda and Kappa Scorpii. Many of these luminous hot stars are surprisingly not visible because they lie within the dusty plane of our galaxy. At infrared wavelengths the numerous hot stars are revealed and the nature of this object as a region of massive star formation becomes clear. In the past decade water masers, molecular outflows, and x-ray sources have provided direct evide

R. Gendler

PIX4619391

The Birth of The Telephone Industry, 1928

The Birth of The Telephone Industry, 1928

BOF3823080

Attending to wounded on the Menin Road, Ypres, during the stiff fighting around Zonnebeke'. (b/w photo)

Attending to wounded on the Menin Road, Ypres, during the stiff fighting around Zonnebeke'. (b/w photo)

Unknown photographer, (20th century)

NAM5924344

Sinn Fein Prisoners, 1916

Sinn Fein Prisoners, 1916

IWF7405567

History of the 34th Infantry Division 1940s

History of the 34th Infantry Division 1940s

BOF6285928

Collection of singing-bird boxes (enamel & silver-gilt)

Collection of singing-bird boxes (enamel & silver-gilt)

Swiss School, (19th Century)

CH3025203

In The Studio, 1966 (oil on canvas)

In The Studio, 1966 (oil on canvas)

Majors, William (1930-82)

IMA1556862

Untitled (The Birth) 1938 (tempera on paper)

Untitled (The Birth) 1938 (tempera on paper)

Lawrence, Jacob (1917-2000)

IMA207286

Nappy Head Blues, 1997 (wood, paint & found objects)

Nappy Head Blues, 1997 (wood, paint & found objects)

Saar, Alison (b.1956)

IMA374378

Early flights of the North American X-15 rocket powered aircraft, 1959

Early flights of the North American X-15 rocket powered aircraft, 1959

BOF6284113

The Artist'S Party (oil on canvas)

The Artist'S Party (oil on canvas)

Delaney, Joseph (1904-1991)

IMA1557317

From the north and south to Vietnam, 1967

From the north and south to Vietnam, 1967

MOD6437277

The reign of Charles V of France, 1364-1380 (colour litho)

The reign of Charles V of France, 1364-1380 (colour litho)

Darrigan, Charles (fl.1935)

LLM5207725

18 Miniatures depicting various French historical figures (b/w photo)

18 Miniatures depicting various French historical figures (b/w photo)

CND165111

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