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Mars: Martian face in the region of Cydonia - Mars: cydonia face - Image obtained on 25 July 1976 by the probe Viking 1 at 1873 km from Mars. The picture shows eroded mesa - like landforms. The huge rock formation in the center, which resemble a human head, is formed by shadows giving the illusion of eyes, nose and mouth. The feature is 1.5 kilometers (one mile) across, with the sun angle at approximately 20 degrees. The speckled appearance of the image is due to bit errors, emphasized by enlargement of the photo. The picture was taken by Viking 1 orbiter on July 25 from a range of 1873 kilometers (1162 miles)

Mars: Martian face in the region of Cydonia - Mars: cydonia face - Image obtained on 25 July 1976 by the probe Viking 1 at 1873 km from Mars. The picture shows eroded mesa - like landforms. The huge rock formation in the center, which resemble a human head, is formed by shadows giving the illusion of eyes, nose and mouth. The feature is 1.5 kilometers (one mile) across, with the sun angle at approximately 20 degrees. The speckled appearance of the image is due to bit errors, emphasized by enlargement of the photo. The picture was taken by Viking 1 orbiter on July 25 from a range of 1873 kilometers (1162 miles)

PIX4615174

Philips' large revolving planisphere, 1850-1886

Philips' large revolving planisphere, 1850-1886

UIS5087862

Comparative Magnitudes of the Planets', c 1851

Comparative Magnitudes of the Planets', c 1851

UIS5096136

Saxony, GDR, historical, Vacation, Holidays, Leisure, Recreation, Local …, 1975 (photo)

Saxony, GDR, historical, Vacation, Holidays, Leisure, Recreation, Local …, 1975 (photo)

Sächsische Zeitung

IMO8755496

Sewing Machines Wheeler and Wilson D12 twin-needle lock-stitch sewing machine, 1890

Sewing Machines Wheeler and Wilson D12 twin-needle lock-stitch sewing machine, 1890

UIS5061231

Comparative Magnitudes of the Planets', c 1851

Comparative Magnitudes of the Planets', c 1851

UIS5090305

Arabic treatise on physiognomy

Arabic treatise on physiognomy

UIG2625452

Youth Hostel Paul Neck in …, 1975 (photo)

Youth Hostel Paul Neck in …, 1975 (photo)

Sächsische Zeitung

IMO8755464

The Passion façade, Sagrada Familia, Barcelona, Spain (photo)

The Passion façade, Sagrada Familia, Barcelona, Spain (photo)

Gaudi, Antoni (1852-1926)

Jean-Paul Paireault

JPP7298518

Penicillin culture flask, 1943 A photograph of a culture flask growing penicillin, taken by James Jarche for 'Illustrated' magazine in 1943

Penicillin culture flask, 1943 A photograph of a culture flask growing penicillin, taken by James Jarche for 'Illustrated' magazine in 1943

UIS5082908

First tubular tramway project in Paris (underground electric railway between Vincennes and Bois de Boulogne) - map of the route - cut under the rue de Rivoli showing the tunnel and the drains as well as the ventilation system, near the Saint-Jacques tower - drilling and tunnel construction - view of a station under section and elevation - engraving of A. Normand in one of the Illustrous Universe no 1948, 23 July 1892 - extrat from the text: “” The City Council has just adopted the project presented by Mr. Berlier... The Bastille station will be open air and will have a monumental appearance. All other stations will be underground... We see that this project reunited all the conditions for success. Who knows? Perhaps it will be the beginning of this famous Metropolitain that we have been talking about for so long and never seen - Paris metro - see also GUT8056, GUT8074 and GUT8075 -

First tubular tramway project in Paris (underground electric railway between Vincennes and Bois de Boulogne) - map of the route - cut under the rue de Rivoli showing the tunnel and the drains as well as the ventilation system, near the Saint-Jacques tower - drilling and tunnel construction - view of a station under section and elevation - engraving of A. Normand in one of the Illustrous Universe no 1948, 23 July 1892 - extrat from the text: “” The City Council has just adopted the project presented by Mr. Berlier... The Bastille station will be open air and will have a monumental appearance. All other stations will be underground... We see that this project reunited all the conditions for success. Who knows? Perhaps it will be the beginning of this famous Metropolitain that we have been talking about for so long and never seen - Paris metro - see also GUT8056, GUT8074 and GUT8075 -

Patrice Cartier

PCT4293742

The Sun, taken at 10

The Sun, taken at 10

UIS5099634

The Sun, taken at 2pm, 25 July 1862

The Sun, taken at 2pm, 25 July 1862

UIS5099621

The Sun, taken at 10

The Sun, taken at 10

UIS5099627

Penicillin culture flasks, 1943

Penicillin culture flasks, 1943

UIS5082905

ISS: modules Unity, Zarya and Zvezda 10/2000 - ISS: modules Unity, Zarya and Zvezda 10/2000 - The international space station shortly before docking with the shuttle Discovery. 12/10/2000. Not long before the link - up of the Space Shuttle Discovery and the International Space Station (ISS), a crew member onboard the shuttle used a handheld 70 mm camera to grab this image of the station. Backdropped against the blackness of space, all the current elements are visible, though this particular angle makes them difficult to delineate. Nearest the camera is the Progress supply ship, attached to the service module or Zvezda, which connects to the functional cargo block (FGB) or Zarya. At the top or far end in this vew is the U.S. - built Unity Node 1. Once the STS - 92 crew completed its work, the addition of the Z1 Truss and a third pressurized mating adapter changed the appearance considerably. Oct 12 2000

ISS: modules Unity, Zarya and Zvezda 10/2000 - ISS: modules Unity, Zarya and Zvezda 10/2000 - The international space station shortly before docking with the shuttle Discovery. 12/10/2000. Not long before the link - up of the Space Shuttle Discovery and the International Space Station (ISS), a crew member onboard the shuttle used a handheld 70 mm camera to grab this image of the station. Backdropped against the blackness of space, all the current elements are visible, though this particular angle makes them difficult to delineate. Nearest the camera is the Progress supply ship, attached to the service module or Zvezda, which connects to the functional cargo block (FGB) or Zarya. At the top or far end in this vew is the U.S. - built Unity Node 1. Once the STS - 92 crew completed its work, the addition of the Z1 Truss and a third pressurized mating adapter changed the appearance considerably. Oct 12 2000

PIX4599994

Eruption de la Soufriere - Ile de Montserrat - Volcanic eruption of Soufriere Hills - Montserrat - Eruption of the Soufriere volcano on the island of Montserrat in the Caribbean, seen from the International Space Station (ISS) on October 11, 2009. The Soufriere Hills, a volcano on the island of Montserrat, in the Lesser Antilles island chain in the Caribbean Sea, has been active since 1995. This oblique astronaut photograph from the International Space Station (ISS) captures a white-to-gray ash and steam plume extending westwards from the volcano on October 11, 2009. While much of the island is covered in green vegetation, gray deposits that include pyroclastic flows and volcanic mudflows (lahars) are visible extending from the volcano towards the coastline. The silver-gray appearance of the Caribbean Sea surface is due to sunglint, which is the mirror-like reflection of sunlight off the water surface back towards the handheld camera onboard the ISS. The sunglint highlights surface wav

Eruption de la Soufriere - Ile de Montserrat - Volcanic eruption of Soufriere Hills - Montserrat - Eruption of the Soufriere volcano on the island of Montserrat in the Caribbean, seen from the International Space Station (ISS) on October 11, 2009. The Soufriere Hills, a volcano on the island of Montserrat, in the Lesser Antilles island chain in the Caribbean Sea, has been active since 1995. This oblique astronaut photograph from the International Space Station (ISS) captures a white-to-gray ash and steam plume extending westwards from the volcano on October 11, 2009. While much of the island is covered in green vegetation, gray deposits that include pyroclastic flows and volcanic mudflows (lahars) are visible extending from the volcano towards the coastline. The silver-gray appearance of the Caribbean Sea surface is due to sunglint, which is the mirror-like reflection of sunlight off the water surface back towards the handheld camera onboard the ISS. The sunglint highlights surface wav

PIX4677507

ISS: modules Unity, Zarya and Zvezda 10/2000 - ISS: modules Unity, Zarya and Zvezda 10/2000 - The international space station shortly before docking with the shuttle Discovery. 12/10/2000. Not long before the link - up of the Space Shuttle Discovery and the International Space Station (ISS), a crew member onboard the shuttle used a handheld 70 mm camera to grab this image of the station. Backdropped against the blackness of space, all the current elements are visible, though this particular angle makes them difficult to delineate. Nearest the camera is the Progress supply ship, attached to the service module or Zvezda, which connects to the functional cargo block (FGB) or Zarya. At the top or far end in this vew is the U.S. - built Unity Node 1. Once the STS - 92 crew completed its work, the addition of the Z1 Truss and a third pressurized mating adapter changed the appearance considerably. Oct 12 2000

ISS: modules Unity, Zarya and Zvezda 10/2000 - ISS: modules Unity, Zarya and Zvezda 10/2000 - The international space station shortly before docking with the shuttle Discovery. 12/10/2000. Not long before the link - up of the Space Shuttle Discovery and the International Space Station (ISS), a crew member onboard the shuttle used a handheld 70 mm camera to grab this image of the station. Backdropped against the blackness of space, all the current elements are visible, though this particular angle makes them difficult to delineate. Nearest the camera is the Progress supply ship, attached to the service module or Zvezda, which connects to the functional cargo block (FGB) or Zarya. At the top or far end in this vew is the U.S. - built Unity Node 1. Once the STS - 92 crew completed its work, the addition of the Z1 Truss and a third pressurized mating adapter changed the appearance considerably. Oct 12 2000

PIX4599996

Parade of the Planets, 2017 (digital photo)

Parade of the Planets, 2017 (digital photo)

Lewis, Martin (21st century)

MMM7340924

Nebula near the star S Mon in Unicorn - Fox Fur nebula in Monoceros - Nebula around the bright star S Monocerotis in the constellation Unicorn. S My belongs to a young cluster of stars located about 2600 years from Earth. The region around the 4.7 magnitude star S Mon is a fascinating mixture of red fluorescent hydrogen and dark, obscuring dust lanes. Some dust patches are close enough to bright stars to reflect light from them; these appear blue for the same reason that the day - time sky is blue - because some of the interstellar particles preferentially scatter blue light. The dust is mixed with gas and this affects the appearance of the emission nebulae, giving some of the faintest a curious 'fox fur' texture in this enhanced photograph. S Mon is part of a young open cluster of stars named NGC 2264 located about 2600 light years away, just north of the Cone nebula

Nebula near the star S Mon in Unicorn - Fox Fur nebula in Monoceros - Nebula around the bright star S Monocerotis in the constellation Unicorn. S My belongs to a young cluster of stars located about 2600 years from Earth. The region around the 4.7 magnitude star S Mon is a fascinating mixture of red fluorescent hydrogen and dark, obscuring dust lanes. Some dust patches are close enough to bright stars to reflect light from them; these appear blue for the same reason that the day - time sky is blue - because some of the interstellar particles preferentially scatter blue light. The dust is mixed with gas and this affects the appearance of the emission nebulae, giving some of the faintest a curious 'fox fur' texture in this enhanced photograph. S Mon is part of a young open cluster of stars named NGC 2264 located about 2600 light years away, just north of the Cone nebula

PIX4618692

The launch of an English ship, probably the 'James Galley', c.1676 (graphite & wash, grey)

The launch of an English ship, probably the 'James Galley', c.1676 (graphite & wash, grey)

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

MMM7342596

The Passion façade, Sagrada Familia, Barcelona, Spain (photo)

The Passion façade, Sagrada Familia, Barcelona, Spain (photo)

Gaudi, Antoni (1852-1926)

Jean-Paul Paireault

JPP7298501

Ecce Homo, Sagrada Familia, Barcelona, Spain

Ecce Homo, Sagrada Familia, Barcelona, Spain

Gaudi, Antoni (1852-1926)

Jean-Paul Paireault

JPP7298534

The Passion façade, Sagrada Familia, Barcelona, Spain (photo)

The Passion façade, Sagrada Familia, Barcelona, Spain (photo)

Gaudi, Antoni (1852-1926)

Jean-Paul Paireault

JPP7298510

The Passion façade, Sagrada Familia, Barcelona, Spain (photo)

The Passion façade, Sagrada Familia, Barcelona, Spain (photo)

Gaudi, Antoni (1852-1926)

Jean-Paul Paireault

JPP7298512

The Passion façade, Sagrada Familia, Barcelona, Spain (photo)

The Passion façade, Sagrada Familia, Barcelona, Spain (photo)

Gaudi, Antoni (1852-1926)

Jean-Paul Paireault

JPP7298492

The Passion façade, Sagrada Familia, Barcelona, Spain (photo)

The Passion façade, Sagrada Familia, Barcelona, Spain (photo)

Gaudi, Antoni (1852-1926)

Jean-Paul Paireault

JPP7298495

The Passion façade, Sagrada Familia, Barcelona, Spain (photo)

The Passion façade, Sagrada Familia, Barcelona, Spain (photo)

Gaudi, Antoni (1852-1926)

Jean-Paul Paireault

JPP7298497

The Passion façade, Sagrada Familia, Barcelona, Spain (photo)

The Passion façade, Sagrada Familia, Barcelona, Spain (photo)

Gaudi, Antoni (1852-1926)

Jean-Paul Paireault

JPP7298498

The Passion façade, Sagrada Familia, Barcelona, Spain (photo)

The Passion façade, Sagrada Familia, Barcelona, Spain (photo)

Gaudi, Antoni (1852-1926)

Jean-Paul Paireault

JPP7298511

Black Holes in 3C75 - Black Holes in 3C75 - Composite X-ray image (blue) and radio (pink) of the active galaxy 3C 75. At the center of this very hot gas mass, two supermassive black holes separated by 25,000 years - light form a binary system of black holes (the two bright points). This composite X - ray/radio image of Abell 400 shows radio jets (pink), immersed in a vast cloud of multimillion degree X - ray emitting gas (blue) that pervades the cluster. The jets emanate from the vicinity of two supermassive black holes (bright spots in the image) in the galaxy. Chandra and radio data confirm that the unusual structure is due to the merger of two large galaxies, whose supermassive black holes are bound together by their mutual gravity. The swept - back appearance of the radio jets is produced by the rapid motion of the galaxy through the hot gas of the cluster, in much the same way that a motorcyclist's scarf is swept back while speeding down the road

Black Holes in 3C75 - Black Holes in 3C75 - Composite X-ray image (blue) and radio (pink) of the active galaxy 3C 75. At the center of this very hot gas mass, two supermassive black holes separated by 25,000 years - light form a binary system of black holes (the two bright points). This composite X - ray/radio image of Abell 400 shows radio jets (pink), immersed in a vast cloud of multimillion degree X - ray emitting gas (blue) that pervades the cluster. The jets emanate from the vicinity of two supermassive black holes (bright spots in the image) in the galaxy. Chandra and radio data confirm that the unusual structure is due to the merger of two large galaxies, whose supermassive black holes are bound together by their mutual gravity. The swept - back appearance of the radio jets is produced by the rapid motion of the galaxy through the hot gas of the cluster, in much the same way that a motorcyclist's scarf is swept back while speeding down the road

PIX4613531

The Passion façade, Sagrada Familia, Barcelona, Spain (photo)

The Passion façade, Sagrada Familia, Barcelona, Spain (photo)

Gaudi, Antoni (1852-1926)

Jean-Paul Paireault

JPP7298493

The Passion façade, Sagrada Familia, Barcelona, Spain (photo)

The Passion façade, Sagrada Familia, Barcelona, Spain (photo)

Gaudi, Antoni (1852-1926)

Jean-Paul Paireault

JPP7298494

The Passion façade, Sagrada Familia, Barcelona, Spain (photo)

The Passion façade, Sagrada Familia, Barcelona, Spain (photo)

Gaudi, Antoni (1852-1926)

Jean-Paul Paireault

JPP7298496

The Passion façade, Sagrada Familia, Barcelona, Spain (photo)

The Passion façade, Sagrada Familia, Barcelona, Spain (photo)

Gaudi, Antoni (1852-1926)

Jean-Paul Paireault

JPP7298499

South of France at Night - South of France at Night - South of France at Night view from the International Space Station (ISS) on April 28, 2010. On the left, the city of Turin in Italy, in the lower centre, the city of Lyon, near the coast on the right, Marseille. The light of the Moon is reflected in the Mediterranean Sea near Corsica. The brightly lit metropolitan areas of Torino (Italy), Lyon, and Marseille (both in France) stand out amidst numerous smaller urban areas in this dramatic astronaut photograph. The image captures the nighttime appearance of the France - Italy border. The southwestern end of the Alps Mountains separates the two countries. The island of Corsica is visible in the Ligurian Sea to the south (image top). The full moon reflects brightly on the water surface and also illuminates the tops of low patchy clouds over the border (image center). This image was taken by an International Space Station (ISS) astronaut at approximately 11:55 p.m. local time, on April 28

South of France at Night - South of France at Night - South of France at Night view from the International Space Station (ISS) on April 28, 2010. On the left, the city of Turin in Italy, in the lower centre, the city of Lyon, near the coast on the right, Marseille. The light of the Moon is reflected in the Mediterranean Sea near Corsica. The brightly lit metropolitan areas of Torino (Italy), Lyon, and Marseille (both in France) stand out amidst numerous smaller urban areas in this dramatic astronaut photograph. The image captures the nighttime appearance of the France - Italy border. The southwestern end of the Alps Mountains separates the two countries. The island of Corsica is visible in the Ligurian Sea to the south (image top). The full moon reflects brightly on the water surface and also illuminates the tops of low patchy clouds over the border (image center). This image was taken by an International Space Station (ISS) astronaut at approximately 11:55 p.m. local time, on April 28

PIX4665176

S star Monocerotis and nebula - Fox Fur nebula in Monoceros - The region to the right of the bright star S Monocerotis is called Fox Fur nebula. This region where gas mixes with interstellar dust is located above the Cone nebula, about 2600 light years from Earth. Image obtained with a 61 cm telescope, composite of several images. The region around the 4.7 magnitude star S Mon is a fascinating mixture of red fluorescent hydrogen and dark, obscuring dust lanes. Some dust patches are close enough to bright stars to reflect light from them; these appear blue for the same reason that the day - time sky is blue - because some of the interstellar particles preferentially scatter blue light. The dust is mixed with gas and this affects the appearance of the emission nebulae, giving some of the faintest a curious 'fox fur' texture in this photograph. S Mon is part of a young open cluster of stars named NGC 2264 located about 2600 light years away, just north of the Cone nebula. Image taken with

S star Monocerotis and nebula - Fox Fur nebula in Monoceros - The region to the right of the bright star S Monocerotis is called Fox Fur nebula. This region where gas mixes with interstellar dust is located above the Cone nebula, about 2600 light years from Earth. Image obtained with a 61 cm telescope, composite of several images. The region around the 4.7 magnitude star S Mon is a fascinating mixture of red fluorescent hydrogen and dark, obscuring dust lanes. Some dust patches are close enough to bright stars to reflect light from them; these appear blue for the same reason that the day - time sky is blue - because some of the interstellar particles preferentially scatter blue light. The dust is mixed with gas and this affects the appearance of the emission nebulae, giving some of the faintest a curious 'fox fur' texture in this photograph. S Mon is part of a young open cluster of stars named NGC 2264 located about 2600 light years away, just north of the Cone nebula. Image taken with

Adam Block

PIX4618724

Meditation, 1870 (oil on canvas)

Meditation, 1870 (oil on canvas)

Perrault, Leon Bazile (1832-1908)

MAN5043066

Hide and Seek, 1789 (oil on panel) (pair to 347761)

Hide and Seek, 1789 (oil on panel) (pair to 347761)

Garnier, Michel (1753-1829)

CH3477860

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 at the VLT in December 2001. NGC 3627, also known as Messier 66, is a beautiful spiral with a well - developed central bulge. It also displays large - scale dust lanes. Many regions of warm hydrogen gas are seen throughout the disc of this galaxy. The latter regions are being ionised by radiation from clusters of newborn stars. Very active star - formation is most likely also occurring in the nuclear regions of NGC 3627.The galaxy forms, together with its neighbours M 65 and NGC 3628, the so - called “Leo Triplet””; they are located at a distance of about 35 million light - years. M 66 is the largest of the three. Its spiral arms appear distorted and displaced above the main plane of the galaxy. The as

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 at the VLT in December 2001. NGC 3627, also known as Messier 66, is a beautiful spiral with a well - developed central bulge. It also displays large - scale dust lanes. Many regions of warm hydrogen gas are seen throughout the disc of this galaxy. The latter regions are being ionised by radiation from clusters of newborn stars. Very active star - formation is most likely also occurring in the nuclear regions of NGC 3627.The galaxy forms, together with its neighbours M 65 and NGC 3628, the so - called “Leo Triplet””; they are located at a distance of about 35 million light - years. M 66 is the largest of the three. Its spiral arms appear distorted and displaced above the main plane of the galaxy. The as

PIX4610814

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

Queen Henrietta Maria, c.1632 (w/c on vellum)

Queen Henrietta Maria, c.1632 (w/c on vellum)

Hoskins, John (1595-1664)

ROC3707661

Nebula IC 1396 in Cephee infrared view - 18/12/2003 The large composite image on the left is a product of combining data from the observator's multiband imaging photometer and the infrared array camera. The thermal emission at 24 microns measured by the photometer (red) is combined with near - infrared emission from the camera at 3.6/4.5 microns (blue) and from 5.8/8.0 microns (green). The colors of the diffuse emission and filaments vary, and are a combination of molecular hydrogen (which tends to be green) and polycyclic aromatic hydrocarbon (brown) emissions. Nasa's Spitzer Space Telescope image of a glowing stellar nursery provides a spectacular contrast to the opaque cloud seen in visible light. The Elephant's Trunk Nebula is an elongated dark globule within the emission nebula IC 1396 in the constellation of Cepheus. Located at a distance of 2,450 light - years, the globule is a condensation of dense gas that is barely surviving the strong ionizing radiation from a nearby massive

Nebula IC 1396 in Cephee infrared view - 18/12/2003 The large composite image on the left is a product of combining data from the observator's multiband imaging photometer and the infrared array camera. The thermal emission at 24 microns measured by the photometer (red) is combined with near - infrared emission from the camera at 3.6/4.5 microns (blue) and from 5.8/8.0 microns (green). The colors of the diffuse emission and filaments vary, and are a combination of molecular hydrogen (which tends to be green) and polycyclic aromatic hydrocarbon (brown) emissions. Nasa's Spitzer Space Telescope image of a glowing stellar nursery provides a spectacular contrast to the opaque cloud seen in visible light. The Elephant's Trunk Nebula is an elongated dark globule within the emission nebula IC 1396 in the constellation of Cepheus. Located at a distance of 2,450 light - years, the globule is a condensation of dense gas that is barely surviving the strong ionizing radiation from a nearby massive

PIX4622272

Remnants of Supernova of Vails - detail - Pencil Nebula (NGC 2376) - Remnants from a star that exploded thousands of years ago created a celestial abstract portrait, as captured in this image of the Pencil Nebula. Officially known as NGC 2736, the Pencil Nebula is part of the huge Vela supernova remnant, located in the southern constellation Vela. Discovered by Sir John Herschel in the 1840s, the nebula's linear appearance triggered its popular name. The nebula's shape suggests that it is part of the supernova shock wave that recently encountered a region of dense gas. It is this interaction that causes the nebula to glow, appearing like a rippled sheet. In this snapshot, astronomers are looking along the edge of the undulating sheet of gas. This view shows large, wispy filamentary structures, smaller bright knots of gas, and patches of diffuse gas. The Hubble Heritage Team used the Advanced Camera for Surveys in October 2002 to observe the nebula. The region of the Pencil Nebula captu

Remnants of Supernova of Vails - detail - Pencil Nebula (NGC 2376) - Remnants from a star that exploded thousands of years ago created a celestial abstract portrait, as captured in this image of the Pencil Nebula. Officially known as NGC 2736, the Pencil Nebula is part of the huge Vela supernova remnant, located in the southern constellation Vela. Discovered by Sir John Herschel in the 1840s, the nebula's linear appearance triggered its popular name. The nebula's shape suggests that it is part of the supernova shock wave that recently encountered a region of dense gas. It is this interaction that causes the nebula to glow, appearing like a rippled sheet. In this snapshot, astronomers are looking along the edge of the undulating sheet of gas. This view shows large, wispy filamentary structures, smaller bright knots of gas, and patches of diffuse gas. The Hubble Heritage Team used the Advanced Camera for Surveys in October 2002 to observe the nebula. The region of the Pencil Nebula captu

PIX4582819

Galaxy has 13 billion years - light in cluster CL1358+62 - Galaxy 13 billion light - years away - Image obtained by the Hubble space telescope of the galaxy cluster CL1358+62. This cluster reveals to us, by a gravitational mirage effect, the deformed image of a galaxy, located behind the cluster at a distance of 13 billion years - light (the red crescent at the bottom right of the image). At the top right, a close-up of this arc reveals brighter points, indicating a strong star-forming activity within this galaxy. At the bottom right, a modeling of this arc. A NASA Hubble Space Telescope image of the galaxy cluster CL1358+62 has uncovered a gravitationally - lensed image of a more distant galaxy located far beyond the cluster. The gravitationally - lensed image appears as a red crescent to the lower right of center. The galaxy's image is brightened, magnified, and smeared into an arc - shape by the gravitational influence of the intervening galaxy cluster, which acts like a gigantic le

Galaxy has 13 billion years - light in cluster CL1358+62 - Galaxy 13 billion light - years away - Image obtained by the Hubble space telescope of the galaxy cluster CL1358+62. This cluster reveals to us, by a gravitational mirage effect, the deformed image of a galaxy, located behind the cluster at a distance of 13 billion years - light (the red crescent at the bottom right of the image). At the top right, a close-up of this arc reveals brighter points, indicating a strong star-forming activity within this galaxy. At the bottom right, a modeling of this arc. A NASA Hubble Space Telescope image of the galaxy cluster CL1358+62 has uncovered a gravitationally - lensed image of a more distant galaxy located far beyond the cluster. The gravitationally - lensed image appears as a red crescent to the lower right of center. The galaxy's image is brightened, magnified, and smeared into an arc - shape by the gravitational influence of the intervening galaxy cluster, which acts like a gigantic le

PIX4565674

Barree spiral galaxy UGC 12158 - Galaxy UGC 12158 - The galaxy UGC 12158, is about 400 million light years away from Earth in the constellation Pegase. In this image obtained by the Hubble space telescope, a blue star is visible near the center of the galaxy (lower left), it is a supernova, SN 2004ef. The galaxy captured in this image, called UGC 12158, certainly isn't camera - shy: this spiral stunner is posing face - on to the NASA/ESA Hubble Space Telescope's Advanced Camera for Surveys, revealing its structure in fine detail. UGC 12158 is an excellent example of a barred spiral galaxy in the Hubble sequence - - a scheme used to categorise galaxies based on their shapes. Barred spirals, as the name suggest, feature spectacular swirling arms of stars that emanate from a bar - shaped centre. Such bar structures are common, being found in about two thirds of spiral galaxies, and are thought to act as funnels, guiding gas to their galactic centres where it accumulates to form newborn st

Barree spiral galaxy UGC 12158 - Galaxy UGC 12158 - The galaxy UGC 12158, is about 400 million light years away from Earth in the constellation Pegase. In this image obtained by the Hubble space telescope, a blue star is visible near the center of the galaxy (lower left), it is a supernova, SN 2004ef. The galaxy captured in this image, called UGC 12158, certainly isn't camera - shy: this spiral stunner is posing face - on to the NASA/ESA Hubble Space Telescope's Advanced Camera for Surveys, revealing its structure in fine detail. UGC 12158 is an excellent example of a barred spiral galaxy in the Hubble sequence - - a scheme used to categorise galaxies based on their shapes. Barred spirals, as the name suggest, feature spectacular swirling arms of stars that emanate from a bar - shaped centre. Such bar structures are common, being found in about two thirds of spiral galaxies, and are thought to act as funnels, guiding gas to their galactic centres where it accumulates to form newborn st

PIX4613612

Kepler - 186f, the first Earth - size Planet in the Habitable Zone - Kepler - 186f is the first Earth-sized planet in the habitable zone of its star to be discovered. It orbits Kepler - 186, a red dwarf located in the constellation of Swan, between 490 and 500 years of light from the Earth. The artist's concept depicts Kepler - 186f, the first validated Earth - size planet to orbit a distant star in the habitable zone - - a range of distance from a star where liquid water might pool on the planet's surface. The discovery of Kepler - 186f confirms that Earth - size planets exist in the habitable zones of other stars and signals a significant step closer to finding a world similar to Earth. The size of Kepler - 186f is known to be less than ten percent larger than Earth, but its mass, composition and density are not known. Previous research suggests that a planet the size of Kepler - 186f is likely to be rocky. Prior to this discovery, the “” record holder”” for the most “” Earth - like”

Kepler - 186f, the first Earth - size Planet in the Habitable Zone - Kepler - 186f is the first Earth-sized planet in the habitable zone of its star to be discovered. It orbits Kepler - 186, a red dwarf located in the constellation of Swan, between 490 and 500 years of light from the Earth. The artist's concept depicts Kepler - 186f, the first validated Earth - size planet to orbit a distant star in the habitable zone - - a range of distance from a star where liquid water might pool on the planet's surface. The discovery of Kepler - 186f confirms that Earth - size planets exist in the habitable zones of other stars and signals a significant step closer to finding a world similar to Earth. The size of Kepler - 186f is known to be less than ten percent larger than Earth, but its mass, composition and density are not known. Previous research suggests that a planet the size of Kepler - 186f is likely to be rocky. Prior to this discovery, the “” record holder”” for the most “” Earth - like”

PIX4574126

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