File:NorthPoleRotatedContrastAnnotated_160223.jpg
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پەڕگەی سەرەکی (٣٬٤٧٧ × ٢٬١٤٣ پیکسڵ، قەبارەی پەڕگە: ٥٫٨٧ مێگابایت، جۆری ئێم ئای ئێم ئی: image/jpeg)
ئەم پەڕگە لە Wikimedia Commonsەوەیە و لەوانەیە لە پڕۆژەکانی دیکەش بەکار ھاتبێت. پێناسەکەی لەسەر پەڕەی وەسفی پەڕگەکە لە خوارەوە نیشان دراوە.
وەسفNorthPoleRotatedContrastAnnotated 160223.jpg |
English: This ethereal scene captured by NASA’s New Horizons spacecraft tells yet another story of Pluto’s diversity of geological and compositional features—this time in an enhanced color image of the north polar area.
Long canyons run vertically across the polar area—part of the informally named Lowell Regio, named for Percival Lowell, who founded Lowell Observatory and initiated the search that led to Pluto’s discovery. The widest of the canyons (marked in yellow) – is about 45 miles (75 kilometers) wide and runs close to the north pole. Roughly parallel subsidiary canyons to the east and west (in green) are approximately 6 miles (10 kilometers) wide. The degraded walls of these canyons appear to be much older than the more sharply defined canyon systems elsewhere on Pluto, perhaps because the polar canyons are older and made of weaker material. These canyons also appear to represent evidence for an ancient period of tectonics. A shallow, winding valley (in blue) runs the entire length of the canyon floor. To the east of these canyons, another valley (pink) winds toward the bottom-right corner of the image. The nearby terrain, at bottom right, appears to have been blanketed by material that obscures small-scale topographic features, creating a ‘softened’ appearance for the landscape. Large, irregularly-shaped pits (in red), reach 45 miles (70 kilometers) across and 2.5 miles (4 kilometers) deep, scarring the region. These pits may indicate locations where subsurface ice has melted or sublimated from below, causing the ground to collapse. The color and composition of this region – shown in enhanced color – also are unusual. High elevations show up in a distinctive yellow, not seen elsewhere on Pluto. The yellowish terrain fades to a uniform bluish gray at lower elevations and latitudes. New Horizons' infrared measurements show methane ice is abundant across Lowell Regio, and there is relatively little nitrogen ice. One possibility is that the yellow terrains may correspond to older methane deposits that have been more processed by solar radiation than the bluer terrain. This image was obtained by New Horizons’ Ralph/Multispectral Visible Imaging Camera (MVIC). The image resolution is approximately 2,230 feet (680 meters) per pixel. The lower edge of the image measures about 750 miles (1,200 kilometers) long. It was obtained at a range of approximately 21,100 miles (33,900 kilometers) from Pluto, about 45 minutes before New Horizons’ closest approach on July 14, 2015. |
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سەرچاوە |
http://pluto.jhuapl.edu/Multimedia/Science-Photos/pics/NorthPoleRotatedContrastAnnotated_160223.jpg See also http://photojournal.jpl.nasa.gov/catalog/PIA20473 |
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بەرھەمھێنەر | NASA/Johns Hopkins University Applied Physics Laboratory/Southwest Research Institute | ||||||
ڕێپێدان (بەکارھێنانەوەی ئەم پەڕگەیە) |
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بەندەکانی لەم پەڕگەیەدا دەردەکەون
depicts ئینگلیزی
٢٦ شوباتی 2016
مێژووی پەڕگە
کرتە بکە لەسەر یەکێک لە ڕێکەوت/کاتەکان بۆ بینینی پەڕگەکە بەو شێوەی لەو کاتەدا بووە.
ڕێکەوت/کات | ھێما | ئەندازە | بەکارھێنەر | تێبینی | |
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هەنووکە | ٠٣:٠٢، ٢٨ی شوباتی ٢٠١٦ | ٣٬٤٧٧ لە ٢٬١٤٣ (٥٫٨٧ مێگابایت) | PlanetUser | Transferred from http://pluto.jhuapl.edu/Multimedia/Science-Photos/pics/NorthPoleRotatedContrastAnnotated_160223.jpg |
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دراوی مێتا
ئەم پەڕگە زانیاری زێدەی ھەیە، کە لەوە دەچێت کامێرا یان ھێماگر (scanner) خستبێتیە سەری. ئەگەر پەڕگەکە لە حاڵەتی سەرەتاییەکەیەوە دەستکاری کرابێ، شایەد بڕێ لە بڕگەکان بە تەواوی زانیارەکانی وێنە گۆڕدراوەکە نیشان نەدەن.
ئاڕاستە | ئاسایی |
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شێوازی ئاسۆیی | ٧٢٫٠٠٩ dpi |
شێوازی ستوونی | ٧٢٫٠٠٩ dpi |
نەرمەواڵەی بەکارهاتوو | Adobe Photoshop CS6 (Macintosh) |
ڕێکەوتی و کاتی گۆڕانی پەڕگە | ٢١:١٤، ٢٣ی شوباتی ٢٠١٦ |
بۆشایی رهنگ | sRGB |
ڕێکەوت و کاتی بە دیجیتاڵی کردن | ١٠:٥٦، ٢٢ی ئەیلوولی ٢٠١٥ |
Date metadata was last modified | ١٣:١٤، ٢٣ی شوباتی ٢٠١٦ |
Unique ID of original document | xmp.did:43723C24DC346811822A86A8AA2FEDDE |