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Wedding dress of a woman of Nuremberg, 1577. Her headdress resemble a tower, and is made of beaten gold decorated with pearls and jewels. Handcolored copperplate engraving from Robert von Spalart's “” Historical Picture of the Costumes of the Principal People of Antiquity and of the Middle Ages,”” Vienna, 1811. Illustration based on Thomas Jefferys Collection of Dresses of Different Nations, Antient and Modern. After the Designs of Holbein, Van Dyke, Hollar, and others, London, 1757.

FLO4705748

Wedding dress of a woman of Nuremberg, 1577. Her headdress resemble a tower, and is made of beaten gold decorated with pearls and jewels. Handcolored copperplate engraving from Robert von Spalart's “” Historical Picture of the Costumes of the Principal People of Antiquity and of the Middle Ages,”” Vienna, 1811. Illustration based on Thomas Jefferys Collection of Dresses of Different Nations, Antient and Modern. After the Designs of Holbein, Van Dyke, Hollar, and others, London, 1757.

FLO4705748

 
Richat Structure - Mauritania - Richat structure seen from space - Richat structure, geological formation of volcanic origin, in Mauritania, observed by Space Shuttle Columbia in October 1995. The so-called Richat Structure is a geological formation in the Maur Adrar Desert in the African country of Mauritania. Although it resemble an impact crater, the Richat Structure formed when a volcanic dome hardened and gradually eroded, exposing the onion - like layers of rock. Image taken from the space shuttle Columbia in October 1995

PIX4659083

Richat Structure - Mauritania - Richat structure seen from space - Richat structure, geological formation of volcanic origin, in Mauritania, observed by Space Shuttle Columbia in October 1995. The so-called Richat Structure is a geological formation in the Maur Adrar Desert in the African country of Mauritania. Although it resemble an impact crater, the Richat Structure formed when a volcanic dome hardened and gradually eroded, exposing the onion - like layers of rock. Image taken from the space shuttle Columbia in October 1995

PIX4659083

 
Richat Structure - Mauritania - Richat structure seen from space - Richat structure, geological formation of volcanic origin, in Mauritania, observed from the International Space Station (ISS) in December 2006. The so-called Richat Structure is a geological formation in the Maur Adrar Desert in the African country of Mauritania. Although it resemble an impact crater, the Richat Structure formed when a volcanic dome hardened and gradually eroded, exposing the onion - like layers of rock. Image taken from the International space station (ISS) in December 2006

PIX4659096

Richat Structure - Mauritania - Richat structure seen from space - Richat structure, geological formation of volcanic origin, in Mauritania, observed from the International Space Station (ISS) in December 2006. The so-called Richat Structure is a geological formation in the Maur Adrar Desert in the African country of Mauritania. Although it resemble an impact crater, the Richat Structure formed when a volcanic dome hardened and gradually eroded, exposing the onion - like layers of rock. Image taken from the International space station (ISS) in December 2006

PIX4659096

 
Richat Structure - Mauritania - Richat structure seen from space - Richat structure, geological formation of volcanic origin, in Mauritania, observed from the International Space Station (ISS) in February 2009. The so-called Richat Structure is a geological formation in the Maur Adrar Desert in the African country of Mauritania. Although it resemble an impact crater, the Richat Structure formed when a volcanic dome hardened and gradually eroded, exposing the onion - like layers of rock. Image taken from the International space station (ISS) in February 2009

PIX4659106

Richat Structure - Mauritania - Richat structure seen from space - Richat structure, geological formation of volcanic origin, in Mauritania, observed from the International Space Station (ISS) in February 2009. The so-called Richat Structure is a geological formation in the Maur Adrar Desert in the African country of Mauritania. Although it resemble an impact crater, the Richat Structure formed when a volcanic dome hardened and gradually eroded, exposing the onion - like layers of rock. Image taken from the International space station (ISS) in February 2009

PIX4659106

 
Space shuttle Endeavour over Mauritania - Space shuttle above Richat structure, Mauritania - Space shuttle Endeavour seen above the Richat structure, a geological formation of volcanic origin, in Mauritania. Image obtained from the International Space Station (ISS) in 2002. The space shuttle Endeavour above the Richat Structure, a geological formation in the Maur Adrar Desert in the African country of Mauritania. Although it resemble an impact crater, the Richat Structure formed when a volcanic dome hardened and gradually eroded, exposing the onion - like layers of rock. Image taken from the international space station (ISS) in 2002

PIX4659122

Space shuttle Endeavour over Mauritania - Space shuttle above Richat structure, Mauritania - Space shuttle Endeavour seen above the Richat structure, a geological formation of volcanic origin, in Mauritania. Image obtained from the International Space Station (ISS) in 2002. The space shuttle Endeavour above the Richat Structure, a geological formation in the Maur Adrar Desert in the African country of Mauritania. Although it resemble an impact crater, the Richat Structure formed when a volcanic dome hardened and gradually eroded, exposing the onion - like layers of rock. Image taken from the international space station (ISS) in 2002

PIX4659122

 
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

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

 
Exploration of Titan - Illustration - Looking for life on Titan - An automatic probe explores a hydrocarbon marsh in search of traces of life. A robotic probe explores a frigid ethane lake on Titan. Like the European Space Agency's Huygens probe, this probe carries its own light source as the surface of Titan is only 0.1 percent as bright as the Earth's. Titan is host to a plethora of organic (carbon - based) compounds, hence this is one of the few places in the Solar System where life outside of the Earth may have evolved. In many ways, Titan resemble a frozen primordial Earth, though the greatest obstacle to Titan harboring life - - as we know it - - is the extreme cold. Even though all the chemical ingredients are present, Titan simply may not be warm enough to initiate the chemical reactions required for life. Perhaps sometime in the next decades such a mission to Titan will be a reality

Walter B Myers

PIX4626138

Exploration of Titan - Illustration - Looking for life on Titan - An automatic probe explores a hydrocarbon marsh in search of traces of life. A robotic probe explores a frigid ethane lake on Titan. Like the European Space Agency's Huygens probe, this probe carries its own light source as the surface of Titan is only 0.1 percent as bright as the Earth's. Titan is host to a plethora of organic (carbon - based) compounds, hence this is one of the few places in the Solar System where life outside of the Earth may have evolved. In many ways, Titan resemble a frozen primordial Earth, though the greatest obstacle to Titan harboring life - - as we know it - - is the extreme cold. Even though all the chemical ingredients are present, Titan simply may not be warm enough to initiate the chemical reactions required for life. Perhaps sometime in the next decades such a mission to Titan will be a reality

Walter B Myers

PIX4626138

 
Dust in Iris Nebula - Dust in Iris Nebula - The Iris Nebula (NGC 7023) is a reflexion nebula illuminated by the star HD 200775. This image obtained by the Hubble Space Telescope shows a detail of the nebula or HD star 200775 (at the top of the image, out of the field) illuminates tiny particles of dust. This close - up of an area in the northwest region of the large Iris Nebula (NGC 7023) seems to be clogged with cosmic dust. With bright light from the nearby star HD 200775 illuminating it from above, the dust resemble thick mounds of billowing cotton. It is actually made up of tiny particles of solid matter, with sizes from ten to a hundred times smaller than those of the dust grains we find at home. Both background and foreground stars are dotted throughout the image. North is down, East is right. The field of view is 3.3 arcminutes. The image is a composite of four images obtained by the Hubble space Telescope through blue, green, near - infrared and H - alpha filters

PIX4620558

Dust in Iris Nebula - Dust in Iris Nebula - The Iris Nebula (NGC 7023) is a reflexion nebula illuminated by the star HD 200775. This image obtained by the Hubble Space Telescope shows a detail of the nebula or HD star 200775 (at the top of the image, out of the field) illuminates tiny particles of dust. This close - up of an area in the northwest region of the large Iris Nebula (NGC 7023) seems to be clogged with cosmic dust. With bright light from the nearby star HD 200775 illuminating it from above, the dust resemble thick mounds of billowing cotton. It is actually made up of tiny particles of solid matter, with sizes from ten to a hundred times smaller than those of the dust grains we find at home. Both background and foreground stars are dotted throughout the image. North is down, East is right. The field of view is 3.3 arcminutes. The image is a composite of four images obtained by the Hubble space Telescope through blue, green, near - infrared and H - alpha filters

PIX4620558

 
Planetary Nebula Helix (NGC 7293) in Aquarius by HST - This composite image is a view of the colorful Helix Nebula taken with the Advanced Camera for Surveys aboard Nasa's Hubble Space Telescope and the Mosaic II Camera on the 4 - meter telescope at Cerro Tololo Inter - American Observatory in Chile. The object is so large that both telescopes were needed to capture a complete view. The Helix is a planetary nebula, the glowing gaseous envelope expelled by a dying, sun - like star. The Helix resemble a simple doughnut as seen from Earth. But looks can be deceiving. New evidence suggests that the Helix consists of two gaseous disks almost perpendicular to each other. One possible scenario for the Helix's complex structure is that the dying star has a companion star. One disk may be perpendicular to the dying star's spin axis, while the other may lie in the orbital plane of the two stars. The Helix, located 690 light - years away, is one of the closest planetary nebulas to Earth. The Hubb

PIX4623671

Planetary Nebula Helix (NGC 7293) in Aquarius by HST - This composite image is a view of the colorful Helix Nebula taken with the Advanced Camera for Surveys aboard Nasa's Hubble Space Telescope and the Mosaic II Camera on the 4 - meter telescope at Cerro Tololo Inter - American Observatory in Chile. The object is so large that both telescopes were needed to capture a complete view. The Helix is a planetary nebula, the glowing gaseous envelope expelled by a dying, sun - like star. The Helix resemble a simple doughnut as seen from Earth. But looks can be deceiving. New evidence suggests that the Helix consists of two gaseous disks almost perpendicular to each other. One possible scenario for the Helix's complex structure is that the dying star has a companion star. One disk may be perpendicular to the dying star's spin axis, while the other may lie in the orbital plane of the two stars. The Helix, located 690 light - years away, is one of the closest planetary nebulas to Earth. The Hubb

PIX4623671

 
Le Piton de la Fournaise, Ile de la Reunion - Piton de la Fournaise, Reunion island - Le Piton de la Fournaise seen by satellite EO - 1 on 16 January 2009. This shield volcano is one of the most active volcanoes in the world. Considered one of the world's most active volcanoes, Piton de la Fournaise occupies the east - southeastern end of Reunion Island in the western Indian Ocean. It is a shield volcano with a low, broad shape that resemble an ancient warrior shield. The volcano sports an 8 - kilometer - (5 - mile -) wide crater that slopes eastward to the coast. Within that crater sits a lava shield, Dolomieu, and most of Piton de la Fournaise's historic eruptions have occurred from the summit or flanks of Dolomieu. The Advanced Land Imager (ALI) on Nasa's Earth Observing - 1 satellite captured this image of Piton de la Fournaise on January 16, 2009. Dolomieu is the circular feature at the center of the large crater. Lava flows from earlier eruptions have left their marks around Dolo

PIX4659236

Le Piton de la Fournaise, Ile de la Reunion - Piton de la Fournaise, Reunion island - Le Piton de la Fournaise seen by satellite EO - 1 on 16 January 2009. This shield volcano is one of the most active volcanoes in the world. Considered one of the world's most active volcanoes, Piton de la Fournaise occupies the east - southeastern end of Reunion Island in the western Indian Ocean. It is a shield volcano with a low, broad shape that resemble an ancient warrior shield. The volcano sports an 8 - kilometer - (5 - mile -) wide crater that slopes eastward to the coast. Within that crater sits a lava shield, Dolomieu, and most of Piton de la Fournaise's historic eruptions have occurred from the summit or flanks of Dolomieu. The Advanced Land Imager (ALI) on Nasa's Earth Observing - 1 satellite captured this image of Piton de la Fournaise on January 16, 2009. Dolomieu is the circular feature at the center of the large crater. Lava flows from earlier eruptions have left their marks around Dolo

PIX4659236

 
Interacting galaxies NGC 4038 - 4039 in the Raven - The Antennae galaxy in Corvus - On the left, seen from the ground of the galaxy NGC 4038 - 39 (antenna galaxy), 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. On the right, the image made by the space telescope Hubble on 20 January 1996 shows in detail the nuclei of these two twin galaxies surrounded by young clusters of blue stars, more than 1000, made up of young and massive stars. At left, a ground - based telescopic view of the Antennae galaxies (known formally as NGC 4038/4039) - so named because a pair of long tails of luminous matter, formed by the gravitational tidal forces of their encounter, resemble an insect's antennae. The galaxies are located 45 million light - years away in the southern constellation Corvus. At right, the respective cores of the twin galaxies are the orange blobs, left and right of image

PIX4611051

Interacting galaxies NGC 4038 - 4039 in the Raven - The Antennae galaxy in Corvus - On the left, seen from the ground of the galaxy NGC 4038 - 39 (antenna galaxy), 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. On the right, the image made by the space telescope Hubble on 20 January 1996 shows in detail the nuclei of these two twin galaxies surrounded by young clusters of blue stars, more than 1000, made up of young and massive stars. At left, a ground - based telescopic view of the Antennae galaxies (known formally as NGC 4038/4039) - so named because a pair of long tails of luminous matter, formed by the gravitational tidal forces of their encounter, resemble an insect's antennae. The galaxies are located 45 million light - years away in the southern constellation Corvus. At right, the respective cores of the twin galaxies are the orange blobs, left and right of image

PIX4611051

 
Astronauts on Titan - Illustration - First steps on Titan - Astronauts explore Titan's surface. Perhaps some day in the far future humans will set foot on Saturn's mysterious moon Titan, one of the most interesting worlds in the Solar System. Larger than the planet Mercury, Earth's moon, and the dwarf planet Pluto, and second only in size to Jupiter's satellite Ganymede, Titan is the only known extraterrestrial world with a dense atmosphere that realistically could be visited by humans. A visit to Titan would require a space journey of a year or more and traverse over 700 million miles. Beneath Titan's 350 miles of atmosphere, intrepid explorers would likely find a dark, forbidding landscape of rock, ice, and possibly tarry layers of hydrocarbons and lakes of liquid ethane and/or methane (AKA natural gas). The Surface temperature would be around minus 300* F, cold enough to freeze exposed human tissue within seconds. There would be no oxygen to breathe, and any water to be found would

Walter B Myers

PIX4626158

Astronauts on Titan - Illustration - First steps on Titan - Astronauts explore Titan's surface. Perhaps some day in the far future humans will set foot on Saturn's mysterious moon Titan, one of the most interesting worlds in the Solar System. Larger than the planet Mercury, Earth's moon, and the dwarf planet Pluto, and second only in size to Jupiter's satellite Ganymede, Titan is the only known extraterrestrial world with a dense atmosphere that realistically could be visited by humans. A visit to Titan would require a space journey of a year or more and traverse over 700 million miles. Beneath Titan's 350 miles of atmosphere, intrepid explorers would likely find a dark, forbidding landscape of rock, ice, and possibly tarry layers of hydrocarbons and lakes of liquid ethane and/or methane (AKA natural gas). The Surface temperature would be around minus 300* F, cold enough to freeze exposed human tissue within seconds. There would be no oxygen to breathe, and any water to be found would

Walter B Myers

PIX4626158

 
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

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

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