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Images of 'X 3000' found, 29

 
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Asteraceae

NHM1456550

Asteraceae

NHM1456550

 
Planetary nebula NGC 6543 in the Dragon - Planetary nebula NGC 6543 in Draco - Composite view of the planetary nebula NGC 6543 in the Dragon obtained by the Hubble space telescope and X-ray (blue) by the Chandra satellite. NGC 6543 is located about 3000 years of light from Earth. This composite of data from Nasa's Chandra X - ray Observatory and Hubble Space Telescope is a new look for NGC 6543, better known as the Cat's Eye nebula. This famous object is a so - called planetary nebula that represents a phase of stellar evolution that the Sun should experience several billion years from now. When a star like the Sun begins to run out of fuel, it becomes what is known as a red giant. In this phase, a star sheds some of its outer layers, eventually leaving behind a hot core that collapses to form a dense white dwarf star. A fast wind emanating from the hot core rams into the ejected atmosphere, pushes it outward, and creates the graceful filamentary structures seen with optical telescopes

PIX4623257

Planetary nebula NGC 6543 in the Dragon - Planetary nebula NGC 6543 in Draco - Composite view of the planetary nebula NGC 6543 in the Dragon obtained by the Hubble space telescope and X-ray (blue) by the Chandra satellite. NGC 6543 is located about 3000 years of light from Earth. This composite of data from Nasa's Chandra X - ray Observatory and Hubble Space Telescope is a new look for NGC 6543, better known as the Cat's Eye nebula. This famous object is a so - called planetary nebula that represents a phase of stellar evolution that the Sun should experience several billion years from now. When a star like the Sun begins to run out of fuel, it becomes what is known as a red giant. In this phase, a star sheds some of its outer layers, eventually leaving behind a hot core that collapses to form a dense white dwarf star. A fast wind emanating from the hot core rams into the ejected atmosphere, pushes it outward, and creates the graceful filamentary structures seen with optical telescopes

PIX4623257

 
Cup with reliefs of rams, 3000 BC (carved limestone)

Sumerian

Luisa Ricciarini

LRI4685433

Cup with reliefs of rams, 3000 BC (carved limestone)

Sumerian

Luisa Ricciarini

LRI4685433

 
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Pendant, about 3000 BCE (white nephrite, rust, yellow, buff striations)

Prehistoric

IMA1561295

Pendant, about 3000 BCE (white nephrite, rust, yellow, buff striations)

Prehistoric

IMA1561295

 
Art; Animal Figure

WGL1122235

Art; Animal Figure

WGL1122235

 
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Chenopodium album

NHM1450093

Chenopodium album

NHM1450093

 
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Quercus robur

NHM1450092

Quercus robur

NHM1450092

 
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Storage Devices Microfiche, 1975

UIS5077957

Storage Devices Microfiche, 1975

UIS5077957

 
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  • Permission required for non-editorial use (inc book covers). Please contact us
Image Restrictions
  • Content within this photograph may require additional clearances (eg: trademark and personality rights) depending on Licensee's specific use of material, which may include book and magazine cover use.
Usage restrictions from our Content Partners
  • Minimum fee applies to this image;Only available to clients invoiced in Australia, Belgium, Brazil, Bulgaria, Canada, China, Cyprus, Czech Republic, Estonia, Finland, France, French Southern Territories, Greece, Hong Kong, Hungary, India, Ireland, Israel, Italy, Lebanon, Luxembourg, Mexico, the Netherlands, New Zealand, Portugal, Qatar, Republic of Korea, Romania, Russian Federation, Singapore, South Africa, Spain, Sweden, Switzerland, Taiwan, Turkey, United Arab Emirates, United Kingdom and United States
STONE TEMPLE PILOTS SINGER WEILAND, 2001-11-19 (photo)

Ethan Miller

REU8517450

STONE TEMPLE PILOTS SINGER WEILAND, 2001-11-19 (photo)

Ethan Miller

REU8517450

 
March: Chaotic terrain between Kasei Valles and Sacra Fossae - Mars: Chaotic terrain between Kasei Valles and Sacra Fossae - Region bordering Kasei Valles (top) and Sacra Fossae (bottom). Kasei Valles is one of the largest Martian canal systems. The large impact crater on the right is 35 km in diameter. The image covering an area of 225 km by 95 km was obtained by the Mars Express probe. Mars Express flew over the boundary between Kasei Valles and Sacra Fossae and imaged the region, acquiring spectacular views of the chaotic terrain in the area. The images are centred at 12* N/285* E and have a ground resolution of about 21 m/pixel. They cover 225 x 95 km or 21.375 sq km, an area roughly half the size of the Netherlands. The upper portion of the image swath shows the eastern margin of Kasei Valles and the western margin of the Lunae Planum plateau and the adjoining Sacra Fossae. Kasei Valles is one of the largest outflow channels on Mars, spanning 3000 km, from the Chryse Planitia basi

PIX4616154

March: Chaotic terrain between Kasei Valles and Sacra Fossae - Mars: Chaotic terrain between Kasei Valles and Sacra Fossae - Region bordering Kasei Valles (top) and Sacra Fossae (bottom). Kasei Valles is one of the largest Martian canal systems. The large impact crater on the right is 35 km in diameter. The image covering an area of 225 km by 95 km was obtained by the Mars Express probe. Mars Express flew over the boundary between Kasei Valles and Sacra Fossae and imaged the region, acquiring spectacular views of the chaotic terrain in the area. The images are centred at 12* N/285* E and have a ground resolution of about 21 m/pixel. They cover 225 x 95 km or 21.375 sq km, an area roughly half the size of the Netherlands. The upper portion of the image swath shows the eastern margin of Kasei Valles and the western margin of the Lunae Planum plateau and the adjoining Sacra Fossae. Kasei Valles is one of the largest outflow channels on Mars, spanning 3000 km, from the Chryse Planitia basi

PIX4616154

 
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  • Content within this photograph may require additional clearances (eg: trademark and personality rights) depending on Licensee's specific use of material, which may include book and magazine cover use.
Classic Motorbike Frera SK 350 (photo)

GRL5613945

Classic Motorbike Frera SK 350 (photo)

GRL5613945

 
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  • Content within this photograph may require additional clearances (eg: trademark and personality rights) depending on Licensee's specific use of material, which may include book and magazine cover use.
Classic Motorbike Frera SK 350 (photo)

GRL5614152

Classic Motorbike Frera SK 350 (photo)

GRL5614152

 
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  • Content within this photograph may require additional clearances (eg: trademark and personality rights) depending on Licensee's specific use of material, which may include book and magazine cover use.
Classic Motorbike Frera SK 350, Trademark (photo)

GRL5614150

Classic Motorbike Frera SK 350, Trademark (photo)

GRL5614150

 
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  • Content within this photograph may require additional clearances (eg: trademark and personality rights) depending on Licensee's specific use of material, which may include book and magazine cover use.
Classic Motorbike Frera SK 350 (photo)

GRL5613946

Classic Motorbike Frera SK 350 (photo)

GRL5613946

 
Image Restrictions
  • Content within this photograph may require additional clearances (eg: trademark and personality rights) depending on Licensee's specific use of material, which may include book and magazine cover use.
Classic Motorbike Frera SK 350 (photo)

GRL5614151

Classic Motorbike Frera SK 350 (photo)

GRL5614151

 
Planetary nebula NGC 6537 in Sagittarius - Hubble observations have revealed huge waves sculpted in the Red Spider nebula. This warm and windy planetary nebula harbours one of the hottest stars in the Universe and its powerful stellar winds generate waves 100 billion kilometers high - intimidating for even the bravest space surfers. The Red Spider Nebula, NGC 6537, is a striking 'butterfly' or bipolar (two - lobed) planetary nebula. Planetary nebulae are the glowing embers of ordinary stars, such as our Sun. At the end of their lives these stars expel most of their material into space, often forming a two - lobed structure as in the case of the Red Spider. These waves are driven by stellar winds radiating from the hot central star, much as a wind passing over a lake can generate waves on the water. The waves reach peaks 100 billion kilometers high and must have been produced by a powerful wind blowing with a speed of 2000 - 4500 kilometers per second (about 7 - 16 million km/hr). The w

PIX4623214

Planetary nebula NGC 6537 in Sagittarius - Hubble observations have revealed huge waves sculpted in the Red Spider nebula. This warm and windy planetary nebula harbours one of the hottest stars in the Universe and its powerful stellar winds generate waves 100 billion kilometers high - intimidating for even the bravest space surfers. The Red Spider Nebula, NGC 6537, is a striking 'butterfly' or bipolar (two - lobed) planetary nebula. Planetary nebulae are the glowing embers of ordinary stars, such as our Sun. At the end of their lives these stars expel most of their material into space, often forming a two - lobed structure as in the case of the Red Spider. These waves are driven by stellar winds radiating from the hot central star, much as a wind passing over a lake can generate waves on the water. The waves reach peaks 100 billion kilometers high and must have been produced by a powerful wind blowing with a speed of 2000 - 4500 kilometers per second (about 7 - 16 million km/hr). The w

PIX4623214

 
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Lake Placid, N.Y., USA, 198002: Olympic Lake Placid 1980 …, 1980 (photo)

NTB8710128

Lake Placid, N.Y., USA, 198002: Olympic Lake Placid 1980 …, 1980 (photo)

NTB8710128

 
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  • Content within this photograph may require additional clearances (eg: trademark and personality rights) depending on Licensee's specific use of material, which may include book and magazine cover use.
Usage restrictions from our Content Partners
  • Minimum fee applies to this image;Only available to clients invoiced in Australia, Belgium, Brazil, Bulgaria, Canada, China, Cyprus, Czech Republic, Estonia, Finland, France, French Southern Territories, Greece, Hong Kong, Hungary, India, Ireland, Israel, Italy, Lebanon, Luxembourg, Mexico, the Netherlands, New Zealand, Portugal, Qatar, Republic of Korea, Romania, Russian Federation, Singapore, South Africa, Spain, Sweden, Switzerland, Taiwan, Turkey, United Arab Emirates, United Kingdom and United States
INDONESIAN ILLEGAL VCD TRADERS WRAP THEIR MERCHANDISE IN JAKARTA, 2002-05-02 (photo)

BEAWIHARTA

REU7972374

INDONESIAN ILLEGAL VCD TRADERS WRAP THEIR MERCHANDISE IN JAKARTA, 2002-05-02 (photo)

BEAWIHARTA

REU7972374

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