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Astronaut Photography of Earth - Display RecordSTS101-718-27Low-resolution Browse Image(Most browse images are not color adjusted.)ImagesConditions for Use of Images >>Image Transformation Tutorial >> Saving, Color Adjusting, and Printing Images >> Images to View on Your Computer Now
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Download a Keyhole Markup Language (KML) file for use in Google Earth. Electronic Image DataCamera files only apply to electronic still cameras.No sound file available. IdentificationMission: STS101 Roll: 718 Frame: 27 Mission ID on the Film or image: STS101Country or Geographic Name: IRAN Features: PAN-STR. OF HORMUZ, DUST Center Point Latitude: 27.5 Center Point Longitude: 54.0 (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: High ObliqueCamera Focal Length: 40mm Camera: HB: Hasselblad Film: 5069 : Kodak Elite 100S, E6 Reversal, Replaces Lumiere, Warmer in tone vs. Lumiere. QualityFilm Exposure:Percentage of Cloud Cover: 10 (0-10) NadirDate: 20000527 (YYYYMMDD)GMT Time: 070541 (HHMMSS)Nadir Point Latitude: 29.8, Longitude: 46.6 (Negative numbers indicate south for latitude and west for longitude) Nadir to Photo Center Direction: East Sun Azimuth: 103 (Clockwise angle in degrees from north to the sun measured at the nadir point) Spacecraft Altitude: 203 nautical miles (376 km) Sun Elevation Angle: 65 (Angle in degrees between the horizon and the sun, measured at the nadir point) Orbit Number: 124 CaptionsN. and S. Zagros Ranges & Persian GulfThe lobate Qatar peninsula and Bahrain, on the southwestern shore of the Persian Gulf, lie beyond the orbiter stabilizer in this southeastward view. Along the northern Gulf coast are the folded mountain ranges of Iran, where the contrasting structural styles in the Northern and Southern Zagros ranges are clearly visible. Folds of the Northern Zagros, at left just above the orbiter, are long and tight, whereas those of the Southern Zagros are broader and less continuous. The differing styles reflect the responses of different rock types to the collision of the Arabian and Eurasian tectonic plates. Arabia is moving northward and is descending beneath the Eurasian plate margin, resulting in the crumpling of strata along the margin. The dark rocks in the crescent along the Oman Peninsula (distant center) are remnants of oceanic crust that were uplifted about 70 million years ago, early in the collision of the two plates. Download Packaged File. This option downloads the following items, packaged into a single file, if they are available:
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