Archivo:Grey Glacier, Chile.jpg

Contenido de la página no disponible en otros idiomas.
De Wikipedia, la enciclopedia libre

Ver la imagen en su resolución original(1000 × 750 píxeles; tamaño de archivo: 398 kB; tipo MIME: image/jpeg)

Resumen

Descripción
English: This image is a photograph taken by an astronaut aboard the International Space Station, and it captures a striking blue colouration of the glacier. The colouring is due to the ice’s absorption of red wavelengths of light and scattering of blue wavelengths of light as it is transmitted through the ice. Certain portions of the glacier visible in the image are indeed grey. Linear grey-brown moraines are accumulations of soil and rock debris that form along the edges of a glacier as it flows downhill across the landscape (much like a bulldozer blade). Glaciers flowing down slope through adjacent feeder valleys ultimately meet, and debris entrained along their sides becomes concentrated in the central portion of the resulting single, large glacier—much as smaller streams of water join to form a single large river. Three of these medial moraines are visible in the ice mass at image centre left. Gray-brown patches of debris from adjacent mountainsides colour the surface of the easternmost lobe of the glacier (image top). Several crevasse fields are visible in the image. The crevasses, each a small canyon in the ice, form as a result of stress between slower- and faster-moving ice within the glacier. The crevasse patterns of Grey Glacier are complex, perhaps due to the three-lobed nature of its terminus, or end, into Grey Lake. The rugged surface of the glacier is also demonstrated by the jagged shadows it casts onto the surface of the lake. Grey Glacier, like others in southern Patagonia, loses ice from its terminus as it enters the water, a process known as calving. Calving produces large free-floating chunks of ice; some floating ice is visible near the central glacier lobe.


International Space Station InsigniaISS Crew Earth Observations: ISS015-E-10704International Space Station Insignia
Identification
Mission ISS015 (Expedition 15)
Roll E
Frame 10704
Country or Geographic Name Chile
Features GREY GLACIER, GREY LAKE
Center Point Latitude -50.9° N
Center Point Longitude -73.2° E
Camera
Camera Tilt 38°
Camera Focal Length 800 mm
Camera Kodak DCS760C Electronic Still Camera
Film 3060 x 2036 pixel CCD, RGBG array.
Quality
Percentage of Cloud Cover 0-10%
Nadir What is Nadir?
Date 2007-06-04
Time 17:57:44
Nadir Point Latitude -51.1° N
Nadir Point Longitude -70.9° E
Nadir to Photo Center Direction West
Sun Azimuth 342°
Spacecraft Altitude 181 nautical miles (335 km)
Sun Elevation Angle 15°
Orbit Number 880
Original image caption
The Southern Patagonian Icefield of Chile and Argentina hosts several spectacular glaciers—including Grey Glacier located in the Torres del Paine National Park in Chile. This glacier, which in 1996 had a measured total area of 270 square kilometers and a length of 28 kilometers (104 square miles in area, 17 miles long), begins in the Patagonian Andes Mountains to the west and terminates in three distinct lobes into Grey Lake. The image is a photograph taken by an astronaut aboard the International Space Station, and it captures a striking blue coloration of the glacier. The coloring is due to the ice’s absorption of red wavelengths of light and scattering of blue wavelengths of light as it is transmitted through the ice.

Certain portions of the glacier visible in the image are indeed gray. Linear gray-brown moraines are accumulations of soil and rock debris that form along the edges of a glacier as it flows downhill across the landscape (much like a bulldozer blade). Glaciers flowing downslope through adjacent feeder valleys ultimately meet, and debris entrained along their sides becomes concentrated in the central portion of the resulting single, large glacier—much as smaller streams of water join to form a single large river. Three of these medial moraines are visible in the ice mass at image center left.

Gray-brown patches of debris from adjacent mountainsides color the surface of the easternmost lobe of the glacier (image top). Several crevasse fields are visible in the image. The crevasses, each a small canyon in the ice, form as a result of stress between slower- and faster-moving ice within the glacier. The crevasse patterns of Grey Glacier are complex, perhaps due to the three-lobed nature of its terminus, or end, into Grey Lake. The rugged surface of the glacier is also demonstrated by the jagged shadows it casts onto the surface of the lake.

All three lobes of Grey Glacier have retreated over the past 22 years, with the greatest loss of ice occurring along the westernmost lobe terminus. Grey Glacier, like others in southern Patagonia, loses ice from its terminus as it enters the water, a process known as calving. Calving produces large free-floating chunks of ice; some floating ice is visible near the central glacier lobe in the upper image. The observed retreat means that ice loss has been greater than ice replenishment. It is most likely due to a combination of increased regional temperatures and changes in precipitation amounts.

Fecha
Fuente NASA Earth Observatory
Autor Image provided by the ISS Crew Earth Observations experiment and the Image Science & Analysis Laboratory, Johnson Space Center.

Image acquired with a Kodak 760C digital camera using an 800 mm lens.

Licencia

Public domain Este archivo es de dominio público porque fue creado por la NASA. Las políticas sobre copyright de la NASA estipulan que «el material de la NASA no está protegido con copyright a menos que se indique lo contrario». (Políticas sobre copyright de la NASA o Políticas sobre la utilización de imágenes del Jet Propulsion Laboratory).
Advertencias:
  • El uso del logotipo de la NASA (incluidos el logotipo actual y los anteriores) está restringido.
  • El sitio web de la NASA almacena una gran cantidad de imágenes del Programa Espacial de la URSS, de la Agencia Espacial Federal Rusa y otras agencias espaciales no estadounidenses. Estas imágenes no son de dominio público.
  • Material del Telescopio espacial Hubble puede tener copyright si no proviene explícitamente del Space Telescope Science Institute. [1]
  • Todo el material creado por la sonda espacial SOHO está protegido por copyright y requiere permiso para ser utilizado con fines comerciales o no educativos. [2]
  • Las imágenes que figuran en el sitio web Astronomy Picture of the Day (APOD) pueden tener copyright. [3]

Leyendas

Añade una explicación corta acerca de lo que representa este archivo

Elementos representados en este archivo

representa a

Historial del archivo

Haz clic sobre una fecha y hora para ver el archivo tal como apareció en ese momento.

Fecha y horaMiniaturaDimensionesUsuarioComentario
actual16:07 5 jul 2009Miniatura de la versión del 16:07 5 jul 20091000 × 750 (398 kB)Originalwana{{Information |Description={{en|1=This image is a photograph taken by an astronaut aboard the International Space Station, and it captures a striking blue colouration of the glacier. The colouring is due to the ice’s absorption of red wavelengths of lig

Las siguientes páginas usan este archivo:

Uso global del archivo

Las wikis siguientes utilizan este archivo:

Metadatos