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Bilder zu 'Anni 30' gefunden, 103,082

Nepal: Carved temple roof strut at the Buddhist Rudra Varna Mahavihar (Uku Bahal) temple, Patan, Kathmandu

Nepal: Carved temple roof strut at the Buddhist Rudra Varna Mahavihar (Uku Bahal) temple, Patan, Kathmandu

Chaweewan Chuchuay

PFH2635065

Nepal: A depiction of Shiva on a carved temple roof strut at the Buddhist Rudra Varna Mahavihar (Uku Bahal) temple, Patan, Kathmandu

Nepal: A depiction of Shiva on a carved temple roof strut at the Buddhist Rudra Varna Mahavihar (Uku Bahal) temple, Patan, Kathmandu

Chaweewan Chuchuay

PFH2635069

Nepal: A depiction of Shiva on a carved temple roof strut at the Buddhist Rudra Varna Mahavihar (Uku Bahal) temple, Patan, Kathmandu

Nepal: A depiction of Shiva on a carved temple roof strut at the Buddhist Rudra Varna Mahavihar (Uku Bahal) temple, Patan, Kathmandu

Chaweewan Chuchuay

PFH2635066

Nepal: Carved temple roof strut at the Buddhist Rudra Varna Mahavihar (Uku Bahal) temple, Patan, Kathmandu

Nepal: Carved temple roof strut at the Buddhist Rudra Varna Mahavihar (Uku Bahal) temple, Patan, Kathmandu

Chaweewan Chuchuay

PFH2635070

Centre de la nebula Omega (M17) by HST - Center of the Omega Nebula, a hotbed of newly born stars wrapped in colorful blankets of glowing gas and cradled in an enormous cold, dark hydrogen cloud. This picture was taken by the Advanced Camera for Surveys (ACS) aboard Nasa's Hubble Space Telescope. The region of the nebula shown in this photograph is about 3,500 times wider than our solar system. The area represents about 60 percent of the total view captured by ACS. The nebula, also called M17 and the Swan Nebula, resides 5,500 light - years away in the constellation Sagittarius. Like its famous cousin in Orion, the Swan Nebula is illuminated by ultraviolet radiation from young, massive stars, located just beyond the upper right corner of the image. Each star is about six times hotter and 30 times more massive than the Sun. The powerful radiation from these stars evaporates and erodes the dense cloud of cold gas within which the stars formed. The blistered walls of the hollow cloud shin

Centre de la nebula Omega (M17) by HST - Center of the Omega Nebula, a hotbed of newly born stars wrapped in colorful blankets of glowing gas and cradled in an enormous cold, dark hydrogen cloud. This picture was taken by the Advanced Camera for Surveys (ACS) aboard Nasa's Hubble Space Telescope. The region of the nebula shown in this photograph is about 3,500 times wider than our solar system. The area represents about 60 percent of the total view captured by ACS. The nebula, also called M17 and the Swan Nebula, resides 5,500 light - years away in the constellation Sagittarius. Like its famous cousin in Orion, the Swan Nebula is illuminated by ultraviolet radiation from young, massive stars, located just beyond the upper right corner of the image. Each star is about six times hotter and 30 times more massive than the Sun. The powerful radiation from these stars evaporates and erodes the dense cloud of cold gas within which the stars formed. The blistered walls of the hollow cloud shin

PIX4620159

Center of the Omega Nebula (M17) in the sagittarius seen by HST - Center of the Omega Nebula, a hotbed of newly born stars wrapped in colorful blankets of glowing gas and cradled in an enormous cold, dark hydrogen cloud. This picture was taken by the Advanced Camera for Surveys (ACS) aboard Nasa's Hubble Space Telescope. The region of the nebula shown in this photograph is about 3,500 times wider than our solar system. The area represents about 60 percent of the total view captured by ACS. The nebula, also called M17 and the Swan Nebula, resides 5,500 light - years away in the constellation Sagittarius. Like its famous cousin in Orion, the Swan Nebula is illuminated by ultraviolet radiation from young, massive stars, located just beyond the upper right corner of the image. Each star is about six times hotter and 30 times more massive than the Sun. The powerful radiation from these stars evaporates and erodes the dense cloud of cold gas within which the stars formed. The blistered walls

Center of the Omega Nebula (M17) in the sagittarius seen by HST - Center of the Omega Nebula, a hotbed of newly born stars wrapped in colorful blankets of glowing gas and cradled in an enormous cold, dark hydrogen cloud. This picture was taken by the Advanced Camera for Surveys (ACS) aboard Nasa's Hubble Space Telescope. The region of the nebula shown in this photograph is about 3,500 times wider than our solar system. The area represents about 60 percent of the total view captured by ACS. The nebula, also called M17 and the Swan Nebula, resides 5,500 light - years away in the constellation Sagittarius. Like its famous cousin in Orion, the Swan Nebula is illuminated by ultraviolet radiation from young, massive stars, located just beyond the upper right corner of the image. Each star is about six times hotter and 30 times more massive than the Sun. The powerful radiation from these stars evaporates and erodes the dense cloud of cold gas within which the stars formed. The blistered walls

PIX4620193

Nepal: A depiction of Shiva on a carved temple roof strut at the Buddhist Rudra Varna Mahavihar (Uku Bahal) temple, Patan, Kathmandu

Nepal: A depiction of Shiva on a carved temple roof strut at the Buddhist Rudra Varna Mahavihar (Uku Bahal) temple, Patan, Kathmandu

Chaweewan Chuchuay

PFH2635067

Nepal: A depiction of Shiva on a carved temple roof strut at the Buddhist Rudra Varna Mahavihar (Uku Bahal) temple, Patan, Kathmandu

Nepal: A depiction of Shiva on a carved temple roof strut at the Buddhist Rudra Varna Mahavihar (Uku Bahal) temple, Patan, Kathmandu

Chaweewan Chuchuay

PFH2635068

Thomas Noel-Hill, 2nd Baron Berwick of Attingham, FSA (1770-1832)

Thomas Noel-Hill, 2nd Baron Berwick of Attingham, FSA (1770-1832)

Romney, George (1734-1802)

USB1160481

Hubble deep field sud - Hubble deep field south - In the southern constellation of Toucan, the Hubble space telescope posed 75h to obtain this image of the distant universe. Thousands of galaxies away from 1 to 12 billion light years are visible in this image. From Earth, the target field is the one “” that one would see through the eye of a needle held at arm's length.” If the distribution of galaxies over the entire Celestial vault were similar to this field, the number of galaxies observable up to magnitude 30 would be 50 billion. This picture is the culmination of a 10 - day - long observation called the Hubble Deep Field South which was carried out in October 1998. This new “” far - look”” complements the original Hubble “” deep field””” taken in late 1995, when Hubble was aimed at a small patch of space near the Big Dipper. The new region is in the constellation Tucana, near the south celestial pole. Hubble's sharp vision allows astronomers to sort galaxy shapes. The image is dom

Hubble deep field sud - Hubble deep field south - In the southern constellation of Toucan, the Hubble space telescope posed 75h to obtain this image of the distant universe. Thousands of galaxies away from 1 to 12 billion light years are visible in this image. From Earth, the target field is the one “” that one would see through the eye of a needle held at arm's length.” If the distribution of galaxies over the entire Celestial vault were similar to this field, the number of galaxies observable up to magnitude 30 would be 50 billion. This picture is the culmination of a 10 - day - long observation called the Hubble Deep Field South which was carried out in October 1998. This new “” far - look”” complements the original Hubble “” deep field””” taken in late 1995, when Hubble was aimed at a small patch of space near the Big Dipper. The new region is in the constellation Tucana, near the south celestial pole. Hubble's sharp vision allows astronomers to sort galaxy shapes. The image is dom

PIX4613806

New Horizons closest approach to Pluto - Artist's view of the New Horizons probe near Pluto and its largest satellite Charon. The New Horizons probe was launched on 19 January 2006 to Jupiter, then Pluto and Charon, which it will reach in 2015 and Kuiper's objects in 2020. Nasa's New Horizons unmanned spacecraft flies into the shadow of dwarf planet Pluto and its moon Charon. New Horizons has been en route to Pluto since its launch from Earth in 2006 and is scheduled to make its closest approach on 14 July 2015. New Horizons will be traveling at a velocity relative to Pluto of 30,800 mph, far too fast for it to enter orbit around and become a satellite of Pluto. Instead after passing Pluto, New Horizons will continue farther into the Kuiper belt searching for other objects with diameters of 30 to 60 miles. New Horizons is about the size and shape of a grand piano and weighed 1,054 pounds at launch. The high - gain dish antenna is about 7 feet in diameter and is employed for communicati

New Horizons closest approach to Pluto - Artist's view of the New Horizons probe near Pluto and its largest satellite Charon. The New Horizons probe was launched on 19 January 2006 to Jupiter, then Pluto and Charon, which it will reach in 2015 and Kuiper's objects in 2020. Nasa's New Horizons unmanned spacecraft flies into the shadow of dwarf planet Pluto and its moon Charon. New Horizons has been en route to Pluto since its launch from Earth in 2006 and is scheduled to make its closest approach on 14 July 2015. New Horizons will be traveling at a velocity relative to Pluto of 30,800 mph, far too fast for it to enter orbit around and become a satellite of Pluto. Instead after passing Pluto, New Horizons will continue farther into the Kuiper belt searching for other objects with diameters of 30 to 60 miles. New Horizons is about the size and shape of a grand piano and weighed 1,054 pounds at launch. The high - gain dish antenna is about 7 feet in diameter and is employed for communicati

Walter B Myers

PIX4607362

Victoria Cross, 2nd Lieutenant R P Hallowes, Duke of Cambridge's Own (Middlesex Regiment), 1915 (metal)

Victoria Cross, 2nd Lieutenant R P Hallowes, Duke of Cambridge's Own (Middlesex Regiment), 1915 (metal)

British School, (20th century)

NAM5921595

Victoria Cross, 2nd Lieutenant R P Hallowes, Duke of Cambridge's Own (Middlesex Regiment), 1915 (metal)

Victoria Cross, 2nd Lieutenant R P Hallowes, Duke of Cambridge's Own (Middlesex Regiment), 1915 (metal)

British School, (20th century)

NAM5921596

Gatun Lock, Panama Canal, Panama (photo)

Gatun Lock, Panama Canal, Panama (photo)

Sergi Reboredo

SRB1202607

Sir John Brownlow ('Young Sir John) 3rd Bt (1659-1697)

Sir John Brownlow ('Young Sir John) 3rd Bt (1659-1697)

Closterman, J. (1660-1711) & Riley, J. (1646-91)

USB1160729

Tyndall Glacier, Chile - Tyndall Glacier, Chile - The Tyndall Glacier in Torres del Paine National Park in Chile, observed from the International Space Station in November 2007. Tyndall Glacier is located in the Torres del Paine National Park in Chile. This glacier, which has a total area of 331 square kilometers and a length of 32 kilometers (based on 1996 measurements), begins in the Patagonian Andes Mountains to the west and terminates in Lago Geikie. The digital astronaut photograph taken in november 2007 records visible light in red, green, and blue wavelengths (true color). The Tyndall Glacier terminus has retreated significantly during the past 17 years. Significant ice loss was also observed earlier this year at Grey Glacier, about 30 kilometers to the north - northeast, suggesting both glaciers are responding similarly to regional changes in temperature and precipitation. A medial moraine is visible in the center of the glacier, extending along its length (top image, center le

Tyndall Glacier, Chile - Tyndall Glacier, Chile - The Tyndall Glacier in Torres del Paine National Park in Chile, observed from the International Space Station in November 2007. Tyndall Glacier is located in the Torres del Paine National Park in Chile. This glacier, which has a total area of 331 square kilometers and a length of 32 kilometers (based on 1996 measurements), begins in the Patagonian Andes Mountains to the west and terminates in Lago Geikie. The digital astronaut photograph taken in november 2007 records visible light in red, green, and blue wavelengths (true color). The Tyndall Glacier terminus has retreated significantly during the past 17 years. Significant ice loss was also observed earlier this year at Grey Glacier, about 30 kilometers to the north - northeast, suggesting both glaciers are responding similarly to regional changes in temperature and precipitation. A medial moraine is visible in the center of the glacier, extending along its length (top image, center le

PIX4675989

Planetary nebula myCN18 dans la Mouche/HST - This is an image of MyCN18, a young planetary nebula located about 8,000 light - years away, taken with the Wide Field and Planetary Camera 2 (WFPC2) aboard Nasa's Hubble Space Telescope (HST). This picture has been composed from three separate images taken in the light of ionized nitrogen (represented by red), hydrogen (green), and doubly - ionized oxygen (blue). The results are of great interest because they shed new light on the poorly understood ejection of stellar matter which accompanies the slow death of Sun - like stars. According to one theory for the formation of planetary nebulae, the hourglass shape is produced by the expansion of a fast stellar wind within a slowly expanding cloud which is more dense near its equator than near its poles. What appears as a bright elliptical ring in the center, and at first sight might be mistaken for an equatorially dense region, is seen on closer inspection to be a potato shaped structure with a

Planetary nebula myCN18 dans la Mouche/HST - This is an image of MyCN18, a young planetary nebula located about 8,000 light - years away, taken with the Wide Field and Planetary Camera 2 (WFPC2) aboard Nasa's Hubble Space Telescope (HST). This picture has been composed from three separate images taken in the light of ionized nitrogen (represented by red), hydrogen (green), and doubly - ionized oxygen (blue). The results are of great interest because they shed new light on the poorly understood ejection of stellar matter which accompanies the slow death of Sun - like stars. According to one theory for the formation of planetary nebulae, the hourglass shape is produced by the expansion of a fast stellar wind within a slowly expanding cloud which is more dense near its equator than near its poles. What appears as a bright elliptical ring in the center, and at first sight might be mistaken for an equatorially dense region, is seen on closer inspection to be a potato shaped structure with a

PIX4623735

Nebula NGC 6726 - 27 - 29 in the Southern Crown - The Corona Australis nebula (NGC 6726 - 27 - 29) Image of R Coronae Australis region in the southern Milky Way, obtained with the Wide Field Imager (WFI) (camera) at the 2.2 - m MPG/ESO Telescope on La Silla (Chile). The sky field shown measures approx. 33.7 x 31.9 arcmin2 (about the diameter of the full moon). The R Coronae Australis complex of young stars and interstellar gas clouds is one of the nearest star - forming regions, at a distance of approx. 500 light - years from the Sun. It is seen in the southern constellation of that name (The “Southern Crown”). R Coronae Australis, the bright star from which the entire complex is named, is located at the center of the field and illuminates the reddish nebula around it. The bright star in the lower part, illuminating a somewhat bluer nebula, is known as TY Coronae Australis. The brightness of these two stars and several others in the same field is variable. They belong to the so - calle

Nebula NGC 6726 - 27 - 29 in the Southern Crown - The Corona Australis nebula (NGC 6726 - 27 - 29) Image of R Coronae Australis region in the southern Milky Way, obtained with the Wide Field Imager (WFI) (camera) at the 2.2 - m MPG/ESO Telescope on La Silla (Chile). The sky field shown measures approx. 33.7 x 31.9 arcmin2 (about the diameter of the full moon). The R Coronae Australis complex of young stars and interstellar gas clouds is one of the nearest star - forming regions, at a distance of approx. 500 light - years from the Sun. It is seen in the southern constellation of that name (The “Southern Crown”). R Coronae Australis, the bright star from which the entire complex is named, is located at the center of the field and illuminates the reddish nebula around it. The bright star in the lower part, illuminating a somewhat bluer nebula, is known as TY Coronae Australis. The brightness of these two stars and several others in the same field is variable. They belong to the so - calle

PIX4620222

A Horse called 'Wenn', with his Groom and other Figures, at Newmarket

A Horse called 'Wenn', with his Groom and other Figures, at Newmarket

Brook, Joseph (fl.1690-1725)

USB1156641

Supposed Portrait of Mary of Guise, Queen of Scotland (15151560)

Supposed Portrait of Mary of Guise, Queen of Scotland (15151560)

English School, (17th century)

USB1160072

Sir John Brownlow ('Young Sir John) 3rd Bt (1659-1697)

Sir John Brownlow ('Young Sir John) 3rd Bt (1659-1697)

USB1160788

My Sicily, 1976 (16mm negative, 2K/sound scan)

My Sicily, 1976 (16mm negative, 2K/sound scan)

MOD7063125

President John F Kennedy on the Cuban Arms Build-Up 1962

President John F Kennedy on the Cuban Arms Build-Up 1962

BOF6284657

MOD7063111

Release Of Watergate Tapes - President Richard M. Nixon

Release Of Watergate Tapes - President Richard M. Nixon

BOF7336651

Prince Rupert (1619-82) nephew of King Charles I (1600-49) (oil on canvas)

Prince Rupert (1619-82) nephew of King Charles I (1600-49) (oil on canvas)

Honthorst, Gerrit van (1590-1656)

WLN69592

A bronze figure of H.R.H. The Prince of Wales, later Edward VIII, dressed for tennis, c.1920s-1930s (bronze, light brown patina)

A bronze figure of H.R.H. The Prince of Wales, later Edward VIII, dressed for tennis, c.1920s-1930s (bronze, light brown patina)

Jagger, Charles Sergeant (1885-1934)

CH991009

The "Prince Charles" in storm, 1938

The "Prince Charles" in storm, 1938

Scherl

SZT5173980

Erasmus reading to the young Emperor Charles V, Brussels, 1511 (litho)

Erasmus reading to the young Emperor Charles V, Brussels, 1511 (litho)

Hamman, Edouard Jean Conrad (1819-88) (after)

LLM7172862

H.R.H. Prince of Wales, 1921-2 ; 1935 (bronze with a light brown patina)

H.R.H. Prince of Wales, 1921-2 ; 1935 (bronze with a light brown patina)

Jagger, Charles Sergeant (1885-1934)

CH1197090

Carol II or Charles II (1893-1953), 1930s (oil on canvas)

Carol II or Charles II (1893-1953), 1930s (oil on canvas)

Lakhovsky, Arnold Borisovich (1880-1937)

FIA5401399

Prince Charles Edward (colour litho)

Prince Charles Edward (colour litho)

English School, (20th century)

LLM7190977

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