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'Kaelte' Bilder und Clips Suchergebnisse page 2071 of 24

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Bilder zu 'Kaelte' gefunden, 2,096

 
Cod hanging to dry on wooden racks in front of the mountain Olstinden, 2022 (photography)

Sergi Reboredo

SRB7333284

Cod hanging to dry on wooden racks in front of the mountain Olstinden, 2022 (photography)

Sergi Reboredo

SRB7333284

 
Village of Sakrisoy on Moskenesoya Island in Lofoten Islands, 2022 (photography)

Sergi Reboredo

SRB7333285

Village of Sakrisoy on Moskenesoya Island in Lofoten Islands, 2022 (photography)

Sergi Reboredo

SRB7333285

 
Nebula NGC 1333 in Persee infrared view - NGC 1333 star - forming region seen in infrared. - NGC 1333 is a nebula located between 700 and 1000 years - light of the Earth. It's a reflexion nebula and a star-forming region. Viewed here in infrared by the Spitzer space telescope, young stars become visible. Jets of matter, in yellow - green, emerge from extremely young embryonic stars. Located between 700 and 1000 light - years from Earth in the constellation Perseus, the reflection nebula called NGC 1333 is seen here in infrared pictured by the Spitzer Space Telescope. The young stars in NGC 1333 do not form a single cluster, but are split between two sub-groups. One group is to the north near the nebula, dominated by the infrared light from warm dust shown as red in the image. The other group is south, where the features shown in yellow and green abound in the densest part of the natal gas cloud. The knotty yellow - green features are glowing shock fronts where jets of material, spewed

PIX4617526

Nebula NGC 1333 in Persee infrared view - NGC 1333 star - forming region seen in infrared. - NGC 1333 is a nebula located between 700 and 1000 years - light of the Earth. It's a reflexion nebula and a star-forming region. Viewed here in infrared by the Spitzer space telescope, young stars become visible. Jets of matter, in yellow - green, emerge from extremely young embryonic stars. Located between 700 and 1000 light - years from Earth in the constellation Perseus, the reflection nebula called NGC 1333 is seen here in infrared pictured by the Spitzer Space Telescope. The young stars in NGC 1333 do not form a single cluster, but are split between two sub-groups. One group is to the north near the nebula, dominated by the infrared light from warm dust shown as red in the image. The other group is south, where the features shown in yellow and green abound in the densest part of the natal gas cloud. The knotty yellow - green features are glowing shock fronts where jets of material, spewed

PIX4617526

 
Aiguille du Midi and Grands Mulets from the Peit Plateau

UTD2840425

Aiguille du Midi and Grands Mulets from the Peit Plateau

UTD2840425

 
While her family have their meal inside a tent, a woman sits outside by a makeshift stove and prepares food using sticks and twigs collected from the barren land around the Maslakh Refugee Camp for Internally Displaced People (IDP), near the city of Herat Until draught condition improves in Bagdhis province where they have migrated from, her family will have to spend nights under these tents where temperatures often reaches several degrees below freezing. As a result of such little protection, often children and older people die from the cold. Lack of access to a food and water only aggravates these miseries Afghanistan. With ongoing conflicts and emergencies like draughts in Afghanistan and some 7.5 million people requiring international support -- two-thirds of whom are children and women -- humanitarian agencies are focussing on saving lives during the winter period. (photo)

UIG795804

While her family have their meal inside a tent, a woman sits outside by a makeshift stove and prepares food using sticks and twigs collected from the barren land around the Maslakh Refugee Camp for Internally Displaced People (IDP), near the city of Herat Until draught condition improves in Bagdhis province where they have migrated from, her family will have to spend nights under these tents where temperatures often reaches several degrees below freezing. As a result of such little protection, often children and older people die from the cold. Lack of access to a food and water only aggravates these miseries Afghanistan. With ongoing conflicts and emergencies like draughts in Afghanistan and some 7.5 million people requiring international support -- two-thirds of whom are children and women -- humanitarian agencies are focussing on saving lives during the winter period. (photo)

UIG795804

 
Woolly rhinoceros - Woolly rhinoceros - Woolly rhinoceros (Coelodonta antiquitatis), also known as cloisonnee nostrils, was a species of large rhinoceros (1.6 to 2 metres high at withers and up to 3.5 metres long, weighing 2 to 3 tonnes) characterized by A thick woolly fleece. He lived in the cold steppes which covered in Pleistocene much of Eurasia. At its peak, less than 30,000 years ago, it was found from central Spain and southern England to Mongolia and southern Siberia. A woolly rhinoceros (Coelodonta antiquitatis) wanders the snow-covered terrain of Northern Europe 200 thousand years ago. In the foreground is a common rabbit of the family Leporidae. About the size, and maybe a little larger, than today's white rhinoceros, the woolly rhinoceros is believed to be related to the modern Sumatran rhinoceros. Covered with thick fur (AKA pelage), this stocky herbivore was well-suited to the cold climates associated with the Pleistocene glaciations. Woolly rhinoceros remains have been f

Walter B Myers

PIX4664585

Woolly rhinoceros - Woolly rhinoceros - Woolly rhinoceros (Coelodonta antiquitatis), also known as cloisonnee nostrils, was a species of large rhinoceros (1.6 to 2 metres high at withers and up to 3.5 metres long, weighing 2 to 3 tonnes) characterized by A thick woolly fleece. He lived in the cold steppes which covered in Pleistocene much of Eurasia. At its peak, less than 30,000 years ago, it was found from central Spain and southern England to Mongolia and southern Siberia. A woolly rhinoceros (Coelodonta antiquitatis) wanders the snow-covered terrain of Northern Europe 200 thousand years ago. In the foreground is a common rabbit of the family Leporidae. About the size, and maybe a little larger, than today's white rhinoceros, the woolly rhinoceros is believed to be related to the modern Sumatran rhinoceros. Covered with thick fur (AKA pelage), this stocky herbivore was well-suited to the cold climates associated with the Pleistocene glaciations. Woolly rhinoceros remains have been f

Walter B Myers

PIX4664585

 
Detail nebuleuse de la Tete de Cheval by HST - The Horsehead, also known as Barnard 33, is a cold, dark cloud of gas and dust, silhouetted against the bright nebula, IC 434. The bright area at the top left edge is a young star still embedded in its nursery of gas and dust. Radiation from this hot star is eroding its gaseous birthplace. A massive star located outside Hubble's view is, in a similar fashion, sculpting the top of the Horsehead itself. The Horsehead, located in the constellation Orion, is a cousin of the famous pillars of dust and gas known as the Eagle nebula. Both tower - like nebulae are cocoons of young stars. The Horsehead nebula lies just south of the bright star Zeta Orionis, which is easily visible to the unaided eye as the left - hand star in the line of three that form Orion's Belt. Amateur astronomers often use the Horsehead as a test of their observing skills - it is known as one of the more difficult objects to observe visually with an amateur - sized telescope

PIX4621980

Detail nebuleuse de la Tete de Cheval by HST - The Horsehead, also known as Barnard 33, is a cold, dark cloud of gas and dust, silhouetted against the bright nebula, IC 434. The bright area at the top left edge is a young star still embedded in its nursery of gas and dust. Radiation from this hot star is eroding its gaseous birthplace. A massive star located outside Hubble's view is, in a similar fashion, sculpting the top of the Horsehead itself. The Horsehead, located in the constellation Orion, is a cousin of the famous pillars of dust and gas known as the Eagle nebula. Both tower - like nebulae are cocoons of young stars. The Horsehead nebula lies just south of the bright star Zeta Orionis, which is easily visible to the unaided eye as the left - hand star in the line of three that form Orion's Belt. Amateur astronomers often use the Horsehead as a test of their observing skills - it is known as one of the more difficult objects to observe visually with an amateur - sized telescope

PIX4621980

 
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Switzerland Eiger Salvage, 1961 (b/w photo)

Stringer (STR)

KES6244771

Switzerland Eiger Salvage, 1961 (b/w photo)

Stringer (STR)

KES6244771

 
Mont Mandit

UTD2840427

Mont Mandit

UTD2840427

 
View from Montblanc to the Chamonix Valley and to the North

UTD2840432

View from Montblanc to the Chamonix Valley and to the North

UTD2840432

 
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Switzerland Eiger Salvage, 1957 (b/w photo)

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KES6245079

Switzerland Eiger Salvage, 1957 (b/w photo)

Stringer (STR)

KES6245079

 
Zusätzliche Genehmigungen
  • Permission required for non-editorial use (inc book and magazine covers). Please contact us
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Switzerland Eiger Salvage, 1959 (b/w photo)

Stringer (STR)

KES6244769

Switzerland Eiger Salvage, 1959 (b/w photo)

Stringer (STR)

KES6244769

 
Comete of Halley - Halley's comet - View on April 10, 1986

PIX4569954

Comete of Halley - Halley's comet - View on April 10, 1986

PIX4569954

 
Star Formation in the Southern Cross - Star Formation in the Southern Cross - Part of the lactee route in the constellation of the Southern Cross seen in infrared by the Herschel space telescope. The hottest dust appears in blue, the coldest ones appear in red, the new stars will be born. Composite images obtained by SPIRE and PACS instruments on September 3, 2009. Some of the coldest and darkest dust in space shines brightly in this infrared image from the Herschel Observatory, a European Space Agency mission with important participation from NASA. The image is a composite of light captured simultaneously by two of Herschel's three instruments - - the photodetector array camera and spectrometer, and its spectral and photometric imaging receiver. The image reveals a cold and turbulent region where material is just beginning to condense into new stars. It is located in the plane of our Milky Way galaxy, 60 degrees from the center. Blue shows warmer material, red the coolest. The red fil

PIX4621141

Star Formation in the Southern Cross - Star Formation in the Southern Cross - Part of the lactee route in the constellation of the Southern Cross seen in infrared by the Herschel space telescope. The hottest dust appears in blue, the coldest ones appear in red, the new stars will be born. Composite images obtained by SPIRE and PACS instruments on September 3, 2009. Some of the coldest and darkest dust in space shines brightly in this infrared image from the Herschel Observatory, a European Space Agency mission with important participation from NASA. The image is a composite of light captured simultaneously by two of Herschel's three instruments - - the photodetector array camera and spectrometer, and its spectral and photometric imaging receiver. The image reveals a cold and turbulent region where material is just beginning to condense into new stars. It is located in the plane of our Milky Way galaxy, 60 degrees from the center. Blue shows warmer material, red the coolest. The red fil

PIX4621141

 
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

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

 
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Desert Victory pt 1 - British fighting in North Africa, victory with Churchill, women in factories, WWII 1943 (HD)

BOF2654937

Desert Victory pt 1 - British fighting in North Africa, victory with Churchill, women in factories, WWII 1943 (HD)

BOF2654937

 
Spiral galaxy M33 infrared view - Spiral galaxy M33 seen in infrared - M33, (NGC 598), the galaxy of the Triangle, is located about 2.9 million years ago - light from Earth. It belongs to the local group, just like our galaxy or Andromede galaxy. This infrared image from the Spitzer space telescope shows stars in blue, gas in green, star formations in red - orange. Red dots are distant galaxies. In infrared, the galaxy appears larger than visible light, revealing cold gas and dust that spread around the galaxy. Also known as M33 or NGC 598, the Triangulum Galaxy is part of the Local Group of galaxies, which includes the Andromeda Galaxy (M31) and our galaxy, the Milky Way. M33 is over thirty thousand light - years across, and more than two million light - years away. Viewed here with Spitzer's infrared eyes, this elegant spiral galaxy sparkles with color and detail. Stars appear as glistening blue gems (several of which are actually foreground stars in our own galaxy), while dust rich

PIX4609334

Spiral galaxy M33 infrared view - Spiral galaxy M33 seen in infrared - M33, (NGC 598), the galaxy of the Triangle, is located about 2.9 million years ago - light from Earth. It belongs to the local group, just like our galaxy or Andromede galaxy. This infrared image from the Spitzer space telescope shows stars in blue, gas in green, star formations in red - orange. Red dots are distant galaxies. In infrared, the galaxy appears larger than visible light, revealing cold gas and dust that spread around the galaxy. Also known as M33 or NGC 598, the Triangulum Galaxy is part of the Local Group of galaxies, which includes the Andromeda Galaxy (M31) and our galaxy, the Milky Way. M33 is over thirty thousand light - years across, and more than two million light - years away. Viewed here with Spitzer's infrared eyes, this elegant spiral galaxy sparkles with color and detail. Stars appear as glistening blue gems (several of which are actually foreground stars in our own galaxy), while dust rich

PIX4609334

 
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Passing Fitz Clarence Rock, August 26, 1871, engraving from Narrative of north polar expedition, US ship Polaris, Captain Charles Francis Hall (1821-1871) commanding. Greenland, 19th century

DGA773826

Passing Fitz Clarence Rock, August 26, 1871, engraving from Narrative of north polar expedition, US ship Polaris, Captain Charles Francis Hall (1821-1871) commanding. Greenland, 19th century

DGA773826

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