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The Gateway to Astronaut Photography of Earth
(NASA Crew Earth Observations)
Astronaut Photography of Earth - Display Record
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IdentificationMission: ISS012 Roll: E Frame: 14618 Mission ID on the Film or image: ISS012
Country or Geographic Name: CHINA
Features: PUMA LAKE, ICE, TIBETAN PLATEAU
Center Point Latitude: 28.6 Center Point Longitude: 90.3 (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: 21
Camera Focal Length: 400mm
Camera: E4: Kodak DCS760C Electronic Still Camera
Film: 3060E : 3060 x 2036 pixel CCD, RGBG array.
Percentage of Cloud Cover: 10 (0-10)
NadirGMT Date: 20060106 (YYYYMMDD) GMT Time: 084014 (HHMMSS)
Nadir Point Latitude: 28.6, Longitude: 89.1 (Negative numbers indicate south for latitude and west for longitude)
Nadir to Photo Center Direction: East
Sun Azimuth: 220 (Clockwise angle in degrees from north to the sun measured at the nadir point)
Spacecraft Altitude: 186 nautical miles (344 km)
Sun Elevation Angle: 27 (Angle in degrees between the horizon and the sun, measured at the nadir point)
Orbit Number: 766
CaptionsLake Puma Yumco, Tibet, China
The alpine lakes of the Tibetan Plateau are some of the most remote in the world. This mosaic of astronaut photographs, taken along a single International Space Station orbit track, depicts Lake Puma Yumco during the winter season. The lake is located at an elevation of 5,030 meters above sea level (16,503 feet), and is considered ultraoligotrophic, meaning that nutrient concentrations in both the water column and lake sediments are extremely low. Water in such lakes tends to be blue to blue-green and to have high clarity due to low levels of photosynthesizing organisms such as phytoplankton. Color change in these lakes is usually due to shallowing of the wateróblue indicating deeper water. A depth transition is visible along the west-southwest shoreline of Lake Puma Yumco at the lower left of image.
The most striking feature of the image mosaic is the intricate ice block pattern on the lake surface. The maximum dimensions of the lake are 31 kilometers by 14 kilometers (1 kilometer is about 0.6 miles), indicating that the ice blocks range from less than ten to hundreds of meters in diameter. The ice pattern is caused by repeated cycles of freezing, fracturing, and refreezing of the ice due to variations in temperature and wind-induced ice motion. A prominent white linear feature extending north-south across the center of the lake is suggestive of an ice ridge formed by east-west winds subsequently highlighted by snow. Similar features are visible along the eastern and southern shorelines and in the southwestern portion of the lake. Records from the nearest weather station to Lake Puma Yumco (approximately 140 kilometers to the northeast at Llasa, Tibet) indicate that daily day-night temperatures varied on average from -7 to 14 degrees Celsius (about 19 to 57 degrees Fahrenheit) during the week preceding acquisition of the astronaut photographs.
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Recommended Citation: Earth Science and Remote Sensing Unit, NASA-Johnson Space Center. "The Gateway to Astronaut Photography of Earth." .