ISS013-E-66488
NASA Photo ID | ISS013-E-66488 |
Focal Length | 800mm |
Date taken | 2006.08.14 |
Time taken | 12:43:59 GMT |
Resolutions offered for this image:
1000 x 661 pixels 357 x 540 pixels 540 x 720 pixels 3032 x 2064 pixels 639 x 435 pixels
1000 x 661 pixels 357 x 540 pixels 540 x 720 pixels 3032 x 2064 pixels 639 x 435 pixels
Cloud masks available for this image:
Country or Geographic Name: | PERU |
Features: | UBINAS VOLCANO, ASH CLOUD |
Features Found Using Machine Learning: | |
Cloud Cover Percentage: | 10 (1-10)% |
Sun Elevation Angle: | 21° |
Sun Azimuth: | 66° |
Camera: | Kodak DCS760c Electronic Still Camera |
Focal Length: | 800mm |
Camera Tilt: | 38 degrees |
Format: | 3060E: 3060 x 2036 pixel CCD, RGBG array |
Film Exposure: | |
Additional Information | |
Width | Height | Annotated | Cropped | Purpose | Links |
---|---|---|---|---|---|
1000 pixels | 661 pixels | No | Yes | Earth From Space collection | Download Image |
357 pixels | 540 pixels | Yes | Yes | Earth From Space collection | Download Image |
540 pixels | 720 pixels | Yes | Yes | NASA's Earth Observatory web site | Download Image |
3032 pixels | 2064 pixels | No | No | Download Image | |
639 pixels | 435 pixels | No | No | Download Image |
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Image Caption: Ash Cloud from Mount Ubinas, Peru
Subduction of the Nazca tectonic plate along the western coast of South America forms the high Peruvian Andes. The subduction (movement of one plate beneath another) also produces magma, feeding a chain of historically active volcanoes along the western front of the mountains. The most active of these volcanoes in Peru is Ubinas. A typical, steep-sided stratovolcano comprised primarily of layers of silica-rich lava flows, it has a summit elevation of 5,672 meters (18,609 feet). At 1.4 kilometers (0.87 miles) across, the volcano's caldera gives it a truncated profile. Hardened lava flows from past eruptions linger on the volcano's flanks.
This oblique image (looking at an angle) from the International Space Station (ISS) captures an ash cloud first observed on satellite imagery at 11:00 GMT on August 14, 2006. An ISS astronaut took this picture one hour and 45 minutes later. The ash cloud caused the Buenos Aires Volcanic Ash Advisory Center to issue an aviation hazard warning. Minor to moderately explosive eruptions of ash and pumice characterize modern activity at Ubinas. Pumice and ash blanket the volcanic cone and surrounding area, giving this image an overall gray appearance. Shadowing of the western flank of Ubinas throws several lava flows into sharp relief, and highlights the steep slopes at the flow fronts--common characteristics of thick, slow-moving lavas. The most recent major eruption of Ubinas occurred in 1969, although its historical record of activity extends back to the 16th century.
Subduction of the Nazca tectonic plate along the western coast of South America forms the high Peruvian Andes. The subduction (movement of one plate beneath another) also produces magma, feeding a chain of historically active volcanoes along the western front of the mountains. The most active of these volcanoes in Peru is Ubinas. A typical, steep-sided stratovolcano comprised primarily of layers of silica-rich lava flows, it has a summit elevation of 5,672 meters (18,609 feet). At 1.4 kilometers (0.87 miles) across, the volcano's caldera gives it a truncated profile. Hardened lava flows from past eruptions linger on the volcano's flanks.
This oblique image (looking at an angle) from the International Space Station (ISS) captures an ash cloud first observed on satellite imagery at 11:00 GMT on August 14, 2006. An ISS astronaut took this picture one hour and 45 minutes later. The ash cloud caused the Buenos Aires Volcanic Ash Advisory Center to issue an aviation hazard warning. Minor to moderately explosive eruptions of ash and pumice characterize modern activity at Ubinas. Pumice and ash blanket the volcanic cone and surrounding area, giving this image an overall gray appearance. Shadowing of the western flank of Ubinas throws several lava flows into sharp relief, and highlights the steep slopes at the flow fronts--common characteristics of thick, slow-moving lavas. The most recent major eruption of Ubinas occurred in 1969, although its historical record of activity extends back to the 16th century.