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Astronaut Photography of Earth - Display Record
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IdentificationMission: ISS024 Roll: E Frame: 8396 Mission ID on the Film or image: ISS024
Country or Geographic Name: PERU
Features: SABANCAYA VOLCANO, LAVA FLOWS, AMPATO VOLCANO, HUALCA HUALCA VOLCANO
Center Point: Latitude: -15.8 Longitude: -71.8 (Negative numbers indicate south for latitude and west for longitude)
Stereo: (Yes indicates there is an adjacent picture of the same area)
ONC Map ID: JNC Map ID:
CameraCamera Tilt: 17
Camera Focal Length: 400mm
Camera: N2: Nikon D2Xs
Film: 4288E : 4288 x 2848 pixel CMOS sensor, RGBG imager color filter.
Percentage of Cloud Cover: 10 (0-10)
GMT Date: 20100715 (YYYYMMDD) GMT Time: 140740 (HHMMSS)
Nadir Point Latitude: -15.7, Longitude: -72.8 (Negative numbers indicate south for latitude and west for longitude)
Nadir to Photo Center Direction: East
Sun Azimuth: 49 (Clockwise angle in degrees from north to the sun measured at the nadir point)
Spacecraft Altitude: 192 nautical miles (356 km)
Sun Elevation Angle: 34 (Angle in degrees between the horizon and the sun, measured at the nadir point)
Orbit Number: 2793
CaptionsSabancaya Volcano, Perú
The 5,967-meter- (19,577-foot-) high Sabancaya stratovolcano (Nevado Sabancaya in the local language) is located in southern Perú, approximately 70 kilometers (40 miles) northwest of the city of Arequipa. The name Sabancaya means “tongue of fire” in the Quechua Indian language.
Sabancaya is part of a volcanic complex that includes two other nearby (and older) volcanoes, neither of which has been active historically. In this detailed astronaut photograph, Nevado Ampato is visible to the south (image left), and the lower flanks of Nevado Hualca Hualca are visible to the north (image top right). The snowy peaks of the three volcanoes provide a stark contrast to the surrounding desert of the Puna Plateau.
Sabancaya’s first historical record of an eruption dates to 1750. The most recent eruptive activity at the volcano occurred in July 2003, and it deposited ash on the volcano’s summit and northeastern flank. Volcanism at Sabancaya is fueled by magma generated at the subduction zone between the Nazca and South American tectonic plates.
Magma can erupt to the surface and form lava flows through the volcano’s summit (frequently forming a crater), but it can also erupt from lava domes and flank vents along the volcano’s sides. Lava has issued from all of these points at Sabancaya, forming numerous gray to dark brown scalloped lobes that extend in all directions except southwards (image center).
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Recommended Citation: Earth Science and Remote Sensing Unit, NASA-Johnson Space Center. "The Gateway to Astronaut Photography of Earth." .