@prefix dbo: .
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@prefix rdfs: .
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dbr:Outline_of_the_Solar_System dbo:wikiPageWikiLink dbr:Atmosphere_of_Mars .
@prefix foaf: .
@prefix wikipedia-en: .
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dbr:Mars_atmosphere dbo:wikiPageWikiLink dbr:Atmosphere_of_Mars ;
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dbr:Timeline_of_Mars_Science_Laboratory rdfs:seeAlso dbr:Atmosphere_of_Mars ;
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dbo:wikiPageWikiLink dbr:Atmosphere_of_Mars .
dbr:Planetary_science dbo:wikiPageWikiLink dbr:Atmosphere_of_Mars .
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dbr:Sample_Analysis_at_Mars dbo:wikiPageWikiLink dbr:Atmosphere_of_Mars .
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@prefix rdf: .
@prefix yago: .
dbr:Atmosphere_of_Mars rdf:type yago:Abstraction100002137 ,
yago:Condition113920835 ,
yago:WikicatPlanetaryAtmospheres ,
yago:Atmosphere114524849 ,
dbo:AnatomicalStructure .
@prefix owl: .
dbr:Atmosphere_of_Mars rdf:type owl:Thing ,
yago:Attribute100024264 ,
yago:State100024720 ;
rdfs:label "Atmosphere of Mars"@en ,
"\u706B\u661F\u306E\u5927\u6C17"@ja ,
"Atmosfera di Marte"@it ,
"Atmosf\u00E9ra Marsu"@cs ,
"\u0410\u0442\u043C\u043E\u0441\u0444\u0435\u0440\u0430 \u041C\u0430\u0440\u0441\u0430"@ru ,
"Atm\u00F3sfera de Marte"@es ,
"Mars atmosf\u00E4r"@sv ,
"Atmosph\u00E8re de Mars"@fr ,
"\u0410\u0442\u043C\u043E\u0441\u0444\u0435\u0440\u0430 \u041C\u0430\u0440\u0441\u0430"@uk ,
"Atmosfera Marsa"@pl ,
"Atmosph\u00E4re des Mars"@de ,
"Atmosfer Mars"@in ,
"\uD654\uC131\uC758 \uB300\uAE30"@ko ,
"\u0627\u0644\u063A\u0644\u0627\u0641 \u0627\u0644\u062C\u0648\u064A \u0641\u064A \u0627\u0644\u0645\u0631\u064A\u062E"@ar ,
"Atmosfera de Marte"@pt ,
"Atmaisf\u00E9ar agus aer\u00E1id Mharsa"@ga ,
"Atmosfera de Mart"@ca ,
"\u0391\u03C4\u03BC\u03CC\u03C3\u03C6\u03B1\u03B9\u03C1\u03B1 \u03C4\u03BF\u03C5 \u0386\u03C1\u03B7"@el ,
"\u706B\u661F\u5927\u6C23\u5C64"@zh ;
rdfs:comment "Atmosfera Marsa \u2013 pow\u0142oka gazowa otaczaj\u0105ca Marsa. Jest bardzo cienka i rozrzedzona w por\u00F3wnaniu z ziemsk\u0105, ci\u015Bnienie atmosferyczne wynosi od 30 Pa na wierzcho\u0142ku Olympus Mons do ponad 1155 Pa przy dnie Hellas Planitia. Sk\u0142ad atmosfery to g\u0142\u00F3wnie dwutlenek w\u0119gla (95,32%), azot (2,7%) i argon (1,6%). Pozosta\u0142e 0,38% stanowi\u0105 pierwiastki \u015Bladowe, w\u015Br\u00F3d kt\u00F3rych znajduje si\u0119 tak\u017Ce tlen. Uwa\u017Ca si\u0119, \u017Ce miliardy lat temu atmosfera Marsa by\u0142a g\u0119stsza i zawiera\u0142a wi\u0119cej tlenu ni\u017C ziemska."@pl ,
"Mars, planet ke-4 dari Matahari, memiliki atmosfer yang berbeda dengan atmosfer Bumi . Terdapat banyak ketertarikan dalam meneliti komposisinya sejak ditemukannya kandungan kecil metana, yang dapat menandai kehidupan di Mars."@in ,
"\u706B\u661F\u7684\u5927\u6C23\u5C64\uFF0C\u81EA\u5F9E\u706B\u661F\u767C\u73FE\u5C11\u91CF\u7532\u70F7\u4EE5\u4F86\uFF0C\u95DC\u65BC\u5176\u5982\u4F55\u7D44\u6210\u7684\u7814\u7A76\u8D8A\u4F86\u8D8A\u53D7\u5230\u95DC\u6CE8\uFF0C\u56E0\u70BA\u9019\u53EF\u80FD\u662F\u706B\u661F\u751F\u547D\u5B58\u5728\u7684\u8DE1\u8C61\uFF1B\u4E0D\u904E\u9019\u4E5F\u53EF\u80FD\u662F\u7531\u4F5C\u7528\u3001\u706B\u5C71\u4F5C\u7528\u6216\u7B49\u7121\u6A5F\u65B9\u5F0F\u6240\u9020\u6210\u7684\u3002 \u706B\u661F\u7684\u5927\u6C23\u5C64\u76F8\u5C0D\u8F03\u8584\uFF0C\u5730\u8868\u6C23\u58D3\u4F4E\u81F3\u5967\u6797\u5E15\u65AF\u5C71\u9802\u768430\u5E15\u3001\u9AD8\u81F3\u5E0C\u81D8\u5E73\u539F\u4F4E\u9EDE\u76841155\u5E15\u3002\u706B\u661F\u8868\u9762\u7684\u5E73\u5747\u6C23\u58D3\u70BA6\u767E\u5E15\uFF0C\u76F8\u6BD4\u4E4B\u4E0B\u5730\u7403\u6C23\u58D3\u70BA1013\u767E\u5E15\uFF0C\u4E5F\u5C31\u662F\u8AAA\u706B\u661F\u5927\u6C23\u58D3\u529B\u4E0D\u5230\u5730\u7403\u7684\u767E\u5206\u4E4B\u4E00\u3002\u706B\u661F\u5927\u6C23\u7E3D\u8CEA\u91CF\u70BA25\u5146\u5678\uFF0C\u800C\u5730\u7403\u70BA5148\u5146\u5678\uFF0C\u91D1\u661F\u5247\u70BA48\u4EAC\u5678\u3002\u7136\u800C\u5B83\u7684\u5927\u6C23\u6A19\u9AD8\u70BA11\u516C\u91CC\uFF0C\u6BD4\u5730\u7403\u76847\u516C\u91CC\u7A0D\u5927\u3002\u706B\u661F\u5927\u6C23\u542B\u670995%\u7684\u4E8C\u6C27\u5316\u78B3\u30013%\u7684\u6C2E\u6C23\u30011.6%\u7684\u6C2C\u6C23\u3001\u4E9B\u5FAE\u7684\u6C27\u6C23\u3001\u6C34\u6C23\u548C\u7532\u70F7\uFF0C\u5E73\u5747\u5206\u5B50\u91CF\u70BA43.34\u3002\u5927\u6C23\u4E2D\u9084\u5145\u6EFF\u5F88\u591A\u5875\u57C3\uFF0C\u4F7F\u5F97\u5F9E\u706B\u661F\u5730\u8868\u4F86\u770B\u662F\u9EC3\u8910\u8272\u7684\u3002\u706B\u661F\u63A2\u6E2C\u6F2B\u904A\u8005\u7684\u8CC7\u6599\u6307\u51FA\uFF0C\u9019\u4E9B\u61F8\u6D6E\u5FAE\u5875\u7D041.5\u5FAE\u7C73\u5BEC\u3002"@zh ,
"Die Atmosph\u00E4re des Mars besitzt eine Gesamtmasse von etwa 2,5 \u00D7 1016kg.Sie ist sehr d\u00FCnn, ihre Dichte betr\u00E4gt ca. 1,2 % der Dichte der Erdatmosph\u00E4re. Der mittlere atmosph\u00E4rische Druck auf Nullniveau betr\u00E4gt ca. 6 hPa (0,006 Bar), 6,36 hPa (0,00636 Bar) am mittleren Radius mit jahreszeitlichen Schwankungen von 4,0 hPa (0,0040 Bar) bis 8,7 hPa (0,0087 Bar). Das sind nur 0,6 % des mittleren Luftdrucks auf der Erde mit 1013 hPa (1,013 Bar) und entspricht etwa dem Druck, der in der Stratosph\u00E4re der Erde in 32 km H\u00F6he herrscht.Die Schallgeschwindigkeit in einer H\u00F6he von 15 km betr\u00E4gt 230 m/s.Auf der Oberfl\u00E4che des Mars liegt die Schallgeschwindigkeit f\u00FCr niedrige Frequenzen bei 240 m/s, f\u00FCr hohe Frequenzen bei etwa 250 m/s."@de ,
"\u706B\u661F\u306E\u5927\u6C17\u306F\u3001\u91D1\u661F\u306E\u5927\u6C17\u3088\u308A\u3082\u9059\u304B\u306B\u5E0C\u8584\u3067\u3042\u308B\u304C\u3001\u540C\u69D8\u306B\u4E3B\u306B\u4E8C\u9178\u5316\u70AD\u7D20\u3067\u69CB\u6210\u3055\u308C\u3066\u3044\u308B\u3002\u751F\u547D\u306E\u5B58\u5728\u3092\u793A\u5506\u3059\u308B\u75D5\u8DE1\u91CF\u306E\u30E1\u30BF\u30F3\u304C\u691C\u51FA\u3055\u308C\u3066\u304B\u3089\u305D\u306E\u7D44\u6210\u306B\u518D\u3073\u95A2\u5FC3\u304C\u96C6\u307E\u3063\u3066\u3044\u305F\u304C\u3001\u30E1\u30BF\u30F3\u306F\u706B\u5C71\u3084\u71B1\u6C34\u5674\u51FA\u5B54\u3067\u3082\u751F\u6210\u3057\u3046\u308B\u3002 \u706B\u661F\u8868\u9762\u306E\u5927\u6C17\u5727\u306F\u3001\u5E73\u5747750\u30D1\u30B9\u30AB\u30EB\u3067\u3042\u308A\u3001\u5730\u7403\u306E\u6D77\u9762\u4E0A\u306E\u5E73\u5747\u3067\u3042\u308B101.3\u30AD\u30ED\u30D1\u30B9\u30AB\u30EB\u306E\u304A\u3088\u305D0.75%\u3001\u91D1\u661F\u306E\u5E73\u57479.3\u30E1\u30AC\u30D1\u30B9\u30AB\u30EB\u306E\u308F\u305A\u304B0.0065%\u3067\u3042\u308B\u3002\u30AA\u30EA\u30F3\u30DD\u30B9\u5C71\u306E\u9802\u4E0A\u306E30\u30D1\u30B9\u30AB\u30EB\u304B\u3089\u30D8\u30E9\u30B9\u5E73\u539F\u306E\u6700\u6DF1\u90E8\u3067\u306E1,155\u30D1\u30B9\u30AB\u30EB\u307E\u3067\u5E45\u304C\u3042\u308B\u3002\u5730\u7403\u306E\u5927\u6C17\u306E\u8CEA\u91CF\u306F5148\u30C6\u30E9\u30C8\u30F3\u3067\u3042\u308B\u306E\u306B\u6BD4\u3079\u3066\u3001\u706B\u661F\u306E\u5927\u6C17\u306E\u8CEA\u91CF\u306F25\u30C6\u30E9\u30C8\u30F3\u3067\u3042\u308B\u3002\u30B9\u30B1\u30FC\u30EB\u30CF\u30A4\u30C8\u306F\u3001\u5730\u7403\u306E\u7D046km\u306B\u5BFE\u3057\u3066\u3001\u706B\u661F\u306F\u7D0411km\u3067\u3042\u308B\u3002\u706B\u661F\u306E\u5927\u6C17\u306E\u7D44\u6210\u306F\u300195%\u304C\u4E8C\u9178\u5316\u70AD\u7D20\u30013%\u304C\u7A92\u7D20\u30011.6%\u304C\u30A2\u30EB\u30B4\u30F3\u3067\u3042\u308A\u3001\u9178\u7D20\u3001\u4E00\u9178\u5316\u70AD\u7D20\u3001\u6C34\u3001\u30E1\u30BF\u30F3\u3001\u305D\u306E\u4ED6\u306E\u6C17\u4F53\u306F\u75D5\u8DE1\u91CF\u3067\u3042\u308B\u3002\u5E73\u5747\u306E\u30E2\u30EB\u8CEA\u91CF\u306F43.34g/mol\u3068\u306A\u308B\u3002\u5927\u6C17\u306B\u306F\u975E\u5E38\u306B\u5875\u304C\u591A\u304F\u3001\u706B\u661F\u306E\u8868\u9762\u304B\u3089\u7A7A\u3092\u898B\u308B\u3068\u3001\u660E\u308B\u3044\u8336\u8272\u304B\u3089\u6A59\u8272\u306B\u898B\u3048\u308B\u3002\u30DE\u30FC\u30BA\u30FB\u30A8\u30AF\u30B9\u30D7\u30ED\u30EC\u30FC\u30B7\u30E7\u30F3\u30FB\u30ED\u30FC\u30D0\u30FC\u304B\u3089\u306E\u30C7\u30FC\u30BF\u306F\u3001\u5927\u6C17\u4E2D\u306B\u6D6E\u904A\u3059\u308B\u5875\u306E\u7C92\u5B50\u306F\u76F4\u5F84\u7D041.5\u03BCm\u3067\u3042\u308B\u3053\u3068\u3092\u793A\u5506\u3057\u305F\u3002"@ja ,
"La atm\u00F3sfera de Marte est\u00E1 compuesta principalmente por di\u00F3xido de carbono (95%), nitr\u00F3geno (3%) y arg\u00F3n (1,6%), y contiene trazas de ox\u00EDgeno, agua y metano, siendo muy diferente a la atm\u00F3sfera de la Tierra. Recientemente ha habido mayor inter\u00E9s en el estudio de su composici\u00F3n por la detecci\u00F3n de peque\u00F1as cantidades de metano, que podr\u00EDan indicar la existencia de alguna forma de vida. Existe una continua p\u00E9rdida de atm\u00F3sfera que escapa al espacio exterior. Se calcula que cada segundo se pierden entre 1 y 2kg de atm\u00F3sfera.\u200B\u200B"@es ,
"\u0627\u0644\u063A\u0644\u0627\u0641 \u0627\u0644\u062C\u0648\u064A \u0644\u0644\u0645\u0631\u064A\u062E \u0647\u0648 \u0637\u0628\u0642\u0629 \u0627\u0644\u063A\u0627\u0632\u0627\u062A \u0627\u0644\u062A\u064A \u062A\u062D\u064A\u0637 \u0628\u0627\u0644\u0645\u0631\u064A\u062E. \u0648\u062A\u062D\u062A\u0648\u064A \u0628\u0634\u0643\u0644 \u0623\u0633\u0627\u0633\u064A \u0639\u0644\u0649 \u063A\u0627\u0632 \u062B\u0627\u0646\u064A \u0623\u0643\u0633\u064A\u062F \u0627\u0644\u0643\u0631\u0628\u0648\u0646 (95.32\u066A)\u060C \u0648\u063A\u0627\u0632 \u0627\u0644\u0646\u064A\u062A\u0631\u0648\u062C\u064A\u0646 \u0627\u0644\u062C\u0632\u064A\u0626\u064A (2.6\u066A) \u0648\u063A\u0627\u0632 \u0627\u0644\u0623\u0631\u062C\u0648\u0646 (1.9\u066A). \u0648\u0643\u0630\u0644\u0643 \u064A\u062A\u0636\u0645\u0646 \u0623\u064A\u0636\u0627\u064B \u0645\u0633\u062A\u0648\u064A\u0627\u062A \u0636\u0626\u064A\u0644\u0629 \u0645\u0646 \u0628\u062E\u0627\u0631 \u0627\u0644\u0645\u0627\u0621 \u0648\u0627\u0644\u0623\u0643\u0633\u062C\u064A\u0646 \u0648\u0623\u0648\u0644 \u0623\u0643\u0633\u064A\u062F \u0627\u0644\u0643\u0631\u0628\u0648\u0646 \u0648\u0627\u0644\u0647\u064A\u062F\u0631\u0648\u062C\u064A\u0646 \u0648\u063A\u0627\u0632\u0627\u062A \u0646\u0628\u064A\u0644\u0629 \u0623\u062E\u0631\u0649. \u0627\u0644\u063A\u0644\u0627\u0641 \u0627\u0644\u062C\u0648\u064A \u0644\u0644\u0645\u0631\u064A\u062E \u0623\u0631\u0642\u0651 \u0628\u0643\u062B\u064A\u0631 \u0645\u0646 \u0627\u0644\u063A\u0644\u0627\u0641 \u0627\u0644\u062C\u0648\u064A \u0644\u0644\u0623\u0631\u0636. \u064A\u0628\u0644\u063A \u0636\u063A\u0637 \u0627\u0644\u0633\u0637\u062D \u0641\u0642\u0637 \u062D\u0648\u0627\u0644\u064A 610 \u0628\u0627\u0643\u0633\u0644 (0.088 \u0631\u0637\u0644/\u0628\u0648\u0635\u0629 \u0645\u0631\u0628\u0639\u0629) \u0648\u0647\u0648 \u0623\u0642\u0644 \u0645\u0646 1% \u0645\u0646 \u0642\u064A\u0645\u0629 \u0627\u0644\u0623\u0631\u0636. \u064A\u0645\u0646\u0639 \u0627\u0644\u063A\u0644\u0627\u0641 \u0627\u0644\u062C\u0648\u064A \u0627\u0644\u062D\u0627\u0644\u064A \u0644\u0644\u0645\u0631\u064A\u062E \u0645\u0646 \u0648\u062C\u0648\u062F \u0627\u0644\u0645\u0627\u0621 \u0627\u0644\u0633\u0627\u0626\u0644 \u0639\u0644\u0649 \u0633\u0637\u0639 \u0627\u0644\u0645\u0631\u064A\u062E\u060C \u0644\u0643\u0646 \u062A\u0634\u064A\u0631 \u062F\u0631\u0627\u0633\u0627\u062A \u0643\u062B\u064A\u0631\u0629 \u0625\u0644\u0649 \u0623\u0646 \u0627\u0644\u063A\u0644\u0627\u0641 \u0627\u0644\u062C\u0648\u064A \u0644\u0644\u0645\u0631\u064A\u062E \u0643\u0627\u0646 \u0623\u0643\u062B\u0631 \u0633\u0645\u0643\u0627\u064B \u0641\u064A \u0645\u0627 \u0645\u0636\u0649. \u0623\u0639\u0644\u0649 \u0643\u062B\u0627\u0641\u0629 \u0644\u0644\u063A\u0644\u0627\u0641 \u0627\u0644\u062C\u0648\u064A \u0641\u064A \u0627\u0644\u0645\u0631\u064A\u062E \u0645\u062A\u0633\u0627\u0648\u064A\u0629 \u0645\u0639 \u0627\u0644\u0643\u062B\u0627\u0641\u0629 \u0627\u0644\u0645\u0648\u062C\u0648\u062F\u0629 \u0641\u0648\u0642 35 \u0643\u064A\u0644\u0648\u0645\u062A\u0631 \u0645\u0646 \u0633\u0637\u062D \u0627\u0644\u0623\u0631\u0636. \u0641\u0642\u062F \u0627\u0644\u063A\u0644\u0627\u0641 \u0627\u0644\u062C\u0648\u064A \u0644\u0644\u0645\u0631\u064A\u062E. \u0641\u0642\u062F \u0627\u0644\u063A\u0644\u0627\u0641 \u0627\u0644\u062C\u0648\u064A \u0644\u0644\u0645\u0631\u064A\u062E \u0643\u062A\u0644\u062A\u0647 \u0641\u064A \u0627\u0644\u0641\u0636\u0627\u0621 \u0639\u0628\u0631 \u0627\u0644\u062A\u0627\u0631\u064A\u062E\u060C \u0648\u0644\u0627 \u064A\u0632\u0627\u0644 \u062A\u0633\u0631\u0628 \u0627\u0644\u063A\u0627\u0632\u0627\u062A \u0645\u0633\u062A\u0645\u0631\u064B\u0627 \u062D\u062A\u0649 \u0627\u0644\u064A\u0648\u0645.\u0627\u0644\u063A\u0644\u0627\u0641 \u0627\u0644\u062C\u0648\u064A \u0644\u0644\u0645\u0631\u064A\u062E \u0623\u0643\u062B\u0631 \u0628\u0631\u0648\u062F\u0629 \u0645\u0646 \u0627\u0644\u063A\u0644"@ar ,
"Mars atmosf\u00E4r \u00E4r f\u00F6rh\u00E5llandevis tunn och best\u00E5r huvudsakligen av koldioxid (95,32 procent), med mindre delar kv\u00E4ve och argon. Det \u00E4r intressant att studera dess sammans\u00E4ttning, eftersom uppt\u00E4ckt av sp\u00E5r av vissa \u00E4mnen, exempelvis metan, skulle kunna indikera att det funnits liv p\u00E5 Mars. Atmosf\u00E4rstrycket \u00E4r cirka 6,35 hektopascal, motsvarande mindre \u00E4n 1 procent av jordens lufttryck. Trycket \u00E4r dock mycket varierande, beroende p\u00E5 stora h\u00F6jdskillnader samt p\u00E5 grund av att m\u00E4ngder av koldioxid p\u00E5 vintern kondenseras och d\u00E5 bildar omfattande polarkalotter."@sv ,
"L'atmosfera de Mart \u00E9s relativament prima i est\u00E0 composta principalment de di\u00F2xid de carboni (95,32%). Hi ha hagut un inter\u00E8s en l'estudi de la seva composici\u00F3 des de la detecci\u00F3 de traces de met\u00E0, que pot indicar la pres\u00E8ncia de vida a Mart, per\u00F2 tamb\u00E9 pot ser produ\u00EFt per un proc\u00E9s geoqu\u00EDmic, l'activitat volc\u00E0nica o hidrotermal."@ca ,
"T\u00E1 go leor eolais againn ar atmaisf\u00E9ar agus aer\u00E1id Mharsa. T\u00E1 10% de thoirt an Domhain i Mars, agus 25% d\u00E1 achar dromchla. T\u00E1 atmaisf\u00E9ar ag Mars, ach t\u00E1 s\u00E9 f\u00EDorthana\u00ED. T\u00E1 me\u00E1nbhr\u00FA an atmaisf\u00E9ir ar dhromchla Mharsa timpeall ar 750 Pa, n\u00F3 thart ar 0.75% de ghn\u00E1thbhr\u00FA an atmaisf\u00E9ir ar dhroim an Domhain seo againn. \u00D3n taobh eile, t\u00E1 an t-atmaisf\u00E9ar seo ag tan\u00FA n\u00EDos maille n\u00E1 \u00E1r n-atmaisf\u00E9ar f\u00E9in ag dul suas \u00F3 dhromchla an phl\u00E1in\u00E9id. D\u00E9-ocsa\u00EDd charb\u00F3in go pr\u00EDomha at\u00E1 ann, N\u00EDtrigin at\u00E1 i 3% de, agus arg\u00F3n at\u00E1 i 1.6%. Fosta, t\u00E1 meat\u00E1n agus ocsaigin i l\u00E1thair, chomh maith le triathgh\u00E1is eile seachas an t-arg\u00F3n - is \u00E9 sin, neon, criopt\u00F3n agus xean\u00F3n, n\u00F3 n\u00EDl imtharraingt Mharsa in ann g\u00E1s chomh h\u00E9adrom le h\u00E9iliam a choinne\u00E1il \u00F3 \u00E9al\u00FA go dt\u00ED an sp\u00E1s. Ar an gc\u00FAis ch\u00E9anna, n\u00EDl hidrigin shaor le f\u00E1il in "@ga ,
"\u0410\u0442\u043C\u043E\u0441\u0444\u0435\u0440\u0430 \u041C\u0430\u0440\u0441\u0430 \u2014 \u0433\u0430\u0437\u043E\u0432\u0430\u044F \u043E\u0431\u043E\u043B\u043E\u0447\u043A\u0430, \u043E\u043A\u0440\u0443\u0436\u0430\u044E\u0449\u0430\u044F \u043F\u043B\u0430\u043D\u0435\u0442\u0443 \u041C\u0430\u0440\u0441. \u0421\u0443\u0449\u0435\u0441\u0442\u0432\u0435\u043D\u043D\u043E \u043E\u0442\u043B\u0438\u0447\u0430\u0435\u0442\u0441\u044F \u043E\u0442 \u0437\u0435\u043C\u043D\u043E\u0439 \u0430\u0442\u043C\u043E\u0441\u0444\u0435\u0440\u044B \u043A\u0430\u043A \u043F\u043E \u0445\u0438\u043C\u0438\u0447\u0435\u0441\u043A\u043E\u043C\u0443 \u0441\u043E\u0441\u0442\u0430\u0432\u0443, \u0442\u0430\u043A \u0438 \u043F\u043E \u0444\u0438\u0437\u0438\u0447\u0435\u0441\u043A\u0438\u043C \u043F\u0430\u0440\u0430\u043C\u0435\u0442\u0440\u0430\u043C. \u0414\u0430\u0432\u043B\u0435\u043D\u0438\u0435 \u0443 \u043F\u043E\u0432\u0435\u0440\u0445\u043D\u043E\u0441\u0442\u0438 \u0441\u043E\u0441\u0442\u0430\u0432\u043B\u044F\u0435\u0442 \u0432 \u0441\u0440\u0435\u0434\u043D\u0435\u043C 0,6 \u043A\u041F\u0430 \u0438\u043B\u0438 6 \u043C\u0431\u0430\u0440 (1/170 \u043E\u0442 \u0437\u0435\u043C\u043D\u043E\u0433\u043E, \u0438\u043B\u0438 \u0440\u0430\u0432\u043D\u043E \u0437\u0435\u043C\u043D\u043E\u043C\u0443 \u043D\u0430 \u0432\u044B\u0441\u043E\u0442\u0435 \u043F\u043E\u0447\u0442\u0438 35 \u043A\u043C \u043E\u0442 \u043F\u043E\u0432\u0435\u0440\u0445\u043D\u043E\u0441\u0442\u0438 \u0417\u0435\u043C\u043B\u0438). \u0412\u044B\u0441\u043E\u0442\u0430 \u043E\u0434\u043D\u043E\u0440\u043E\u0434\u043D\u043E\u0439 \u0430\u0442\u043C\u043E\u0441\u0444\u0435\u0440\u044B \u0441\u043E\u0441\u0442\u0430\u0432\u043B\u044F\u0435\u0442 11,1 \u043A\u043C, \u043F\u0440\u0438\u043C\u0435\u0440\u043D\u0430\u044F \u043C\u0430\u0441\u0441\u0430 \u0430\u0442\u043C\u043E\u0441\u0444\u0435\u0440\u044B \u2014 2,5\u22C51016 \u043A\u0433 (\u0431\u043E\u043B\u0435\u0435 \u0447\u0435\u043C \u0432 200 \u0440\u0430\u0437 \u043C\u0435\u043D\u044C\u0448\u0435 \u0437\u0435\u043C\u043D\u043E\u0439). \u041C\u0430\u0440\u0441 \u0438\u043C\u0435\u0435\u0442 \u043E\u0447\u0435\u043D\u044C \u0441\u043B\u0430\u0431\u043E\u0435 \u043C\u0430\u0433\u043D\u0438\u0442\u043D\u043E\u0435 \u043F\u043E\u043B\u0435 (\u043F\u043E \u0441\u0440\u0430\u0432\u043D\u0435\u043D\u0438\u044E \u0441 \u0437\u0435\u043C\u043D\u044B\u043C) \u0438 \u0432 2,6 \u0440\u0430\u0437\u0430 \u0431\u043E\u043B\u0435\u0435 \u0441\u043B\u0430\u0431\u043E\u0435 \u043F\u043E \u0441\u0440\u0430\u0432\u043D\u0435\u043D\u0438\u044E \u0441 \u0437\u0435\u043C\u043D\u044B\u043C \u043F\u0440\u0438\u0442\u044F\u0436\u0435\u043D\u0438\u0435, \u0432\u0441\u043B\u0435\u0434\u0441\u0442\u0432\u0438\u0435 \u0447\u0435\u0433\u043E \u0441\u043E\u043B\u043D\u0435\u0447\u043D\u044B\u0439 \u0432\u0435\u0442\u0435\u0440 \u0432\u044B\u0437\u044B\u0432\u0430\u0435\u0442 \u0434\u0438\u0441\u0441\u0438\u043F\u0430\u0446\u0438\u044E \u0430\u0442\u043C\u043E\u0441\u0444\u0435\u0440\u043D\u044B\u0445 \u0433\u0430\u0437\u043E\u0432 \u0432 \u043A\u043E\u0441\u043C\u043E\u0441 \u0441\u043E \u0441\u043A\u043E\u0440\u043E\u0441\u0442\u044C\u044E \u043E\u043A\u043E\u043B\u043E 100 \u0433\u0440\u0430\u043C\u043C\u043E\u0432 \u0432 \u0441\u0435\u043A\u0443\u043D\u0434\u0443 (\u043C\u0435\u043D\u0435\u0435 9 \u0442\u043E\u043D\u043D \u0432 \u0434\u0435\u043D\u044C), \u0432 \u0437\u0430\u0432\u0438\u0441\u0438\u043C\u043E\u0441\u0442\u0438 \u043E\u0442 \u0442\u0435\u043A\u0443\u0449\u0435\u0439 \u0441\u043E\u043B\u043D\u0435\u0447\u043D\u043E\u0439 \u0430\u043A\u0442\u0438\u0432\u043D\u043E\u0441\u0442\u0438 \u0438 \u0440\u0430\u0441\u0441\u0442\u043E\u044F\u043D\u0438\u044F \u043E\u0442 \u0421\u043E\u043B\u043D\u0446\u0430."@ru ,
"Marte \u00E9 o quarto planeta a partir do Sol, e possui uma atmosfera muito diferente da atmosfera terrestre. Tem havido muito interesse no estudo de sua composi\u00E7\u00E3o desde a recente detec\u00E7\u00E3o de pequenas quantidades de metano, que poderia indicar alguma forma de vida em Marte."@pt ,
"\uD654\uC131\uC758 \uB300\uAE30\uB294 \uD0DC\uC591\uACC4\uC758 4\uBC88\uC9F8 \uD589\uC131\uC778 \uD654\uC131\uC744 \uB458\uB7EC\uC2F8\uACE0 \uC788\uB294 \uAE30\uCCB4\uCE35\uC744 \uC758\uBBF8\uD558\uBA70 \uB300\uBD80\uBD84\uC774 \uC774\uC0B0\uD654 \uD0C4\uC18C\uB85C \uAD6C\uC131\uB418\uC5B4 \uC788\uB2E4. \uD3C9\uADE0 \uAE30\uC555\uC740 \uC57D 600 \uD30C\uC2A4\uCE7C\uB85C \uC9C0\uAD6C\uC758 \uD574\uC218\uBA74 \uD3C9\uADE0 \uAE30\uC555\uC778 101.3 \uD0AC\uB85C\uD30C\uC2A4\uCE7C\uC758 0.6 % \uC815\uB3C4\uC774\uBA70, \uADDC\uBAA8\uACE0\uB3C4\uB294 \uC57D 11 km \uC815\uB3C4\uC774\uB2E4. \uC774\uB54C, \uD654\uC131\uC758 \uB300\uAE30 \uC9C8\uB7C9\uC740 25 \uD14C\uB77C\uD1A4(25\u00D71012\uD1A4)\uC73C\uB85C \uADDC\uBAA8\uACE0\uB3C4\uAC00 \uC57D 8.5 km\uC778 \uC9C0\uAD6C\uC758 \uB300\uAE30 \uC9C8\uB7C9\uC778 5148 \uD14C\uB77C\uD1A4(5148\u00D71012\uD1A4)\uC758 0.005 % \uBC16\uC5D0 \uB418\uC9C0 \uC54A\uB294\uB2E4. \uD654\uC131\uC758 \uAE30\uC555\uC740 \uACE0\uB3C4\uC5D0 \uB530\uB77C \uD070 \uCC28\uC774\uB97C \uBCF4\uC774\uB294\uB370, \uD654\uC131\uC5D0\uC11C \uAC00\uC7A5 \uB192\uC740 \uC9C0\uC5ED\uC778 \uC62C\uB9BC\uD478\uC2A4 \uC0B0\uC758 \uCD5C\uACE0\uBD09\uC5D0\uC11C\uB294 \uC57D 30 \uD30C\uC2A4\uCE7C \uC815\uB3C4\uACE0 \uAC00\uC7A5 \uB0AE\uC740 \uC9C0\uC5ED\uC778 \uD5EC\uB77C\uC2A4 \uBD84\uC9C0\uC5D0\uC11C\uB294 1,155 \uD30C\uC2A4\uCE7C \uC815\uB3C4\uB85C \uC5B4\uB514\uC11C\uB4E0\uC9C0 \uD654\uC131\uC758 \uAE30\uC555\uC740 \uC554\uC2A4\uD2B8\uB871 \uD55C\uACC4\uBCF4\uB2E4 \uD6E8\uC52C \uB0AE\uC544\uC11C \uC778\uAC04\uC774 \uD654\uC131\uC758 \uB300\uAE30\uC5D0 \uB9E8\uBAB8\uC73C\uB85C \uB178\uCD9C\uB41C\uB2E4\uBA74 \uC704\uD5D8\uD574\uC9C8 \uC218 \uC788\uB2E4."@ko ,
"The atmosphere of Mars is the layer of gases surrounding Mars. It is primarily composed of carbon dioxide (95%), molecular nitrogen (2.8%), and argon (2%). It also contains trace levels of water vapor, oxygen, carbon monoxide, hydrogen, and noble gases. The atmosphere of Mars is much thinner than Earth's. The average surface pressure is only about 610 pascals (0.088 psi) which is less than 1% of the Earth's value. The currently thin Martian atmosphere prohibits the existence of liquid water on the surface of Mars, but many studies suggest that the Martian atmosphere was much thicker in the past. The higher density during spring and fall is reduced by 25% during the winter when carbon dioxide partly freezes at the pole caps. The highest atmospheric density on Mars is equal to the density fo"@en ,
"L\u2019atmosph\u00E8re de Mars est la couche de gaz entourant la plan\u00E8te Mars. La pression au sol de l'atmosph\u00E8re martienne varie entre 30 Pa (0,03 kPa) au sommet d'Olympus Mons et 1 155 Pa (1,155 kPa) dans les profondeurs de Hellas Planitia. La pression moyenne est de 600 Pa (0,6 kPa soit 6 mbar, environ 170 fois moins que sur Terre) et sa masse totale est estim\u00E9e \u00E0 25 Tt (25 000 milliards de tonnes), soit environ 200 fois moins que l'atmosph\u00E8re terrestre ou encore le double de la masse combin\u00E9e de ses deux satellites, Phobos et D\u00E9imos."@fr ,
"\u0410\u0442\u043C\u043E\u0441\u0444\u0435\u0440\u0430 \u041C\u0430\u0440\u0441\u0430 \u2014 \u0433\u0430\u0437\u043E\u0432\u0430 \u043E\u0431\u043E\u043B\u043E\u043D\u043A\u0430, \u0449\u043E \u043E\u0442\u043E\u0447\u0443\u0454 \u043F\u043B\u0430\u043D\u0435\u0442\u0443 \u041C\u0430\u0440\u0441. \u0406\u0441\u0442\u043E\u0442\u043D\u043E \u0432\u0456\u0434\u0440\u0456\u0437\u043D\u044F\u0454\u0442\u044C\u0441\u044F \u0432\u0456\u0434 \u0437\u0435\u043C\u043D\u043E\u0457 \u0430\u0442\u043C\u043E\u0441\u0444\u0435\u0440\u0438 \u044F\u043A \u0437\u0430 \u0445\u0456\u043C\u0456\u0447\u043D\u0438\u043C \u0441\u043A\u043B\u0430\u0434\u043E\u043C, \u0442\u0430\u043A \u0456 \u0437\u0430 \u0444\u0456\u0437\u0438\u0447\u043D\u0438\u043C\u0438 \u043F\u0430\u0440\u0430\u043C\u0435\u0442\u0440\u0430\u043C\u0438. \u0422\u0438\u0441\u043A \u0431\u0456\u043B\u044F \u043F\u043E\u0432\u0435\u0440\u0445\u043D\u0456 \u0441\u0442\u0430\u043D\u043E\u0432\u0438\u0442\u044C 0,7-1,155 \u043A\u041F\u0430 (1/110 \u0432\u0456\u0434 \u0442\u0438\u0441\u043A\u0443 \u0432 \u0430\u0442\u043C\u043E\u0441\u0444\u0435\u0440\u0456 \u0417\u0435\u043C\u043B\u0456 \u043D\u0430 \u0440\u0456\u0432\u043D\u0456 \u043C\u043E\u0440\u044F, \u0449\u043E \u0434\u043E\u0440\u0456\u0432\u043D\u044E\u0454 \u0442\u0438\u0441\u043A\u0443 \u0432 \u0437\u0435\u043C\u043D\u0456\u0439 \u0430\u0442\u043C\u043E\u0441\u0444\u0435\u0440\u0456 \u043D\u0430 \u0432\u0438\u0441\u043E\u0442\u0456 \u043F\u043E\u043D\u0430\u0434 \u0442\u0440\u0438\u0434\u0446\u044F\u0442\u044C \u043A\u0456\u043B\u043E\u043C\u0435\u0442\u0440\u0456\u0432). \u041E\u0440\u0456\u0454\u043D\u0442\u043E\u0432\u043D\u0430 \u0442\u043E\u0432\u0449\u0438\u043D\u0430 \u0430\u0442\u043C\u043E\u0441\u0444\u0435\u0440\u0438 \u2014 110 \u043A\u043C. \u041F\u0440\u0438\u0431\u043B\u0438\u0437\u043D\u0430 \u043C\u0430\u0441\u0430 \u0430\u0442\u043C\u043E\u0441\u0444\u0435\u0440\u0438 \u2014 2,5\u00D7 1016 \u043A\u0433. \u041C\u0430\u0440\u0441 \u043C\u0430\u0454 \u0434\u0443\u0436\u0435 \u0441\u043B\u0430\u0431\u043A\u0435 \u043C\u0430\u0433\u043D\u0456\u0442\u043D\u0435 \u043F\u043E\u043B\u0435 (\u0443 \u043F\u043E\u0440\u0456\u0432\u043D\u044F\u043D\u043D\u0456 \u0437 \u0437\u0435\u043C\u043D\u0438\u043C), \u0456 \u0432 \u0440\u0435\u0437\u0443\u043B\u044C\u0442\u0430\u0442\u0456 \u0441\u043E\u043D\u044F\u0447\u043D\u0438\u0439 \u0432\u0456\u0442\u0435\u0440 \u043F\u043E\u0441\u0442\u0443\u043F\u043E\u0432\u043E \u00AB\u0437\u0434\u0443\u0432\u0430\u0454\u00BB \u0430\u0442\u043C\u043E\u0441\u0444\u0435\u0440\u0443 \u0432 \u043A\u043E\u0441\u043C\u043E\u0441 \u0437\u0456 \u0448\u0432\u0438\u0434\u043A\u0456\u0441\u0442\u044E 300 \u00B1 200 \u0442\u043E\u043D\u043D \u043D\u0430 \u0434\u0435\u043D\u044C (\u0437\u0430\u043B\u0435\u0436\u043D\u043E \u0432\u0456\u0434 \u043F\u043E\u0442\u043E\u0447\u043D\u0438\u0445 \u0441\u043E\u043D\u044F\u0447\u043D\u043E\u0457 \u0430\u043A\u0442\u0438\u0432\u043D\u043E\u0441\u0442\u0456 \u0442\u0430 \u0432\u0456\u0434\u0441\u0442\u0430\u043D\u0456 \u0432\u0456\u0434 \u0421\u043E\u043D\u0446\u044F.)"@uk ,
"Atmosf\u00E9ra Marsu je plynn\u00FD obal nach\u00E1zej\u00EDc\u00ED se okolo planety Mars. Je velmi \u0159\u00EDdk\u00E1, nen\u00ED schopn\u00E1 zadr\u017Eovat tepelnou v\u00FDm\u011Bnu mezi povrchem a okoln\u00EDm prostorem, co\u017E m\u00E1 za n\u00E1sledek velk\u00E9 tepeln\u00E9 rozd\u00EDly b\u011Bhem dne a noci."@cs ,
"\u0397 \u0391\u03C4\u03BC\u03CC\u03C3\u03C6\u03B1\u03B9\u03C1\u03B1 \u03C4\u03BF\u03C5 \u0386\u03C1\u03B7 \u03B1\u03C0\u03BF\u03C4\u03B5\u03BB\u03B5\u03AF\u03C4\u03B1\u03B9 \u03BA\u03C5\u03C1\u03AF\u03C9\u03C2 \u03B1\u03C0\u03CC \u03B4\u03B9\u03BF\u03BE\u03B5\u03AF\u03B4\u03B9\u03BF \u03C4\u03BF\u03C5 \u03AC\u03BD\u03B8\u03C1\u03B1\u03BA\u03B1. \u0397 \u03B1\u03C4\u03BC\u03BF\u03C3\u03C6\u03B1\u03B9\u03C1\u03B9\u03BA\u03AE \u03C0\u03AF\u03B5\u03C3\u03B7 \u03C3\u03C4\u03B7\u03BD \u03B5\u03C0\u03B9\u03C6\u03AC\u03BD\u03B5\u03B9\u03B1 \u03B5\u03AF\u03BD\u03B1\u03B9 \u03BA\u03B1\u03C4\u03AC \u03BC\u03AD\u03C3\u03BF \u03CC\u03C1\u03BF 600 \u03C0\u03B1\u03C3\u03BA\u03AC\u03BB \u03C0\u03BF\u03C5 \u03B9\u03C3\u03BF\u03CD\u03C4\u03B1\u03B9 \u03BC\u03B5 \u03C4\u03BF 0,6% \u03C4\u03B7\u03C2 \u03BC\u03AD\u03C3\u03B7\u03C2 \u0393\u03AE\u03B9\u03BD\u03B7\u03C2 \u03C0\u03AF\u03B5\u03C3\u03B7\u03C2 \u03C3\u03C4\u03BF \u03B5\u03C0\u03AF\u03C0\u03B5\u03B4\u03BF \u03C4\u03B7\u03C2 \u03B8\u03AC\u03BB\u03B1\u03C3\u03C3\u03B1\u03C2 \u03C4\u03C9\u03BD 101,3 \u03C7\u03B9\u03BB\u03B9\u03BF\u03C0\u03B1\u03C3\u03BA\u03AC\u03BB. \u0397 \u03C0\u03AF\u03B5\u03C3\u03B7 \u03BA\u03C5\u03BC\u03B1\u03AF\u03BD\u03B5\u03C4\u03B1\u03B9 \u03B1\u03C0\u03CC \u03C4\u03B7\u03BD \u03B5\u03BB\u03AC\u03C7\u03B9\u03C3\u03C4\u03B7 30 \u03C0\u03B1\u03C3\u03BA\u03AC\u03BB \u03C3\u03C4\u03B7\u03BD \u03BA\u03BF\u03C1\u03C5\u03C6\u03AE \u03C4\u03BF\u03C5 \u038C\u03C1\u03BF\u03C5\u03C2 \u038C\u03BB\u03C5\u03BC\u03C0\u03BF\u03C2 \u03C3\u03B5 \u03AD\u03C9\u03C2 \u03C0\u03AC\u03BD\u03C9 \u03B1\u03C0\u03CC 1.155 \u03C0\u03B1\u03C3\u03BA\u03AC\u03BB \u03C3\u03C4\u03B1 \u03B2\u03AC\u03B8\u03B7 \u03C4\u03B7\u03C2 \u0395\u03BB\u03BB\u03AC\u03C2 \u03A0\u03BB\u03B1\u03BD\u03AF\u03C4\u03B9\u03B1. \u0391\u03C5\u03C4\u03AE \u03B7 \u03C0\u03AF\u03B5\u03C3\u03B7 \u03B5\u03AF\u03BD\u03B1\u03B9 \u03C0\u03BF\u03BB\u03CD \u03C7\u03B1\u03BC\u03B7\u03BB\u03CC\u03C4\u03B5\u03C1\u03B7 \u03C4\u03B7\u03C2 \u03BF\u03C1\u03B9\u03B1\u03BA\u03AE\u03C2 \u0391\u03C1\u03BC\u03C3\u03C4\u03C1\u03BF\u03BD\u03B3\u03BA \u03B3\u03B9\u03B1 \u03C4\u03BF \u03B1\u03C0\u03C1\u03BF\u03C3\u03C4\u03AC\u03C4\u03B5\u03C5\u03C4\u03BF \u03B1\u03BD\u03B8\u03C1\u03CE\u03C0\u03B9\u03BD\u03BF \u03C3\u03CE\u03BC\u03B1. \u0397 \u0386\u03C1\u03B5\u03B9\u03B1\u03BD\u03AE \u03B1\u03C4\u03BC\u03BF\u03C3\u03C6\u03B1\u03B9\u03C1\u03B9\u03BA\u03AE \u03BC\u03AC\u03B6\u03B1 \u03C4\u03C9\u03BD 25 \u03C4\u03B5\u03C1\u03B1\u03C4\u03CC\u03BD\u03C9\u03BD \u03B5\u03AF\u03BD\u03B1\u03B9 \u03C3\u03C5\u03B3\u03BA\u03C1\u03AF\u03C3\u03B9\u03BC\u03B7 \u03BC\u03B5 \u03C4\u03B7\u03C2 \u0393\u03B7\u03C2 \u03C4\u03C9\u03BD 5148 \u03C4\u03B5\u03C1\u03B1\u03C4\u03CC\u03BD\u03C9\u03BD\u00B7 \u03BF \u0386\u03C1\u03B7\u03C2 \u03AD\u03C7\u03B5\u03B9 \u03BA\u03BB\u03AF\u03BC\u03B1\u03BA\u03B1 \u03CD\u03C8\u03BF\u03C5\u03C2 \u03AF\u03C3\u03B7 \u03BC\u03B5 11,1 \u03C7\u03BB\u03BC \u03BA\u03B1\u03B9 \u03B7 \u0393\u03B7 8,5 \u03C7\u03B9\u03BB\u03B9\u03CC\u03BC\u03B5\u03C4\u03C1\u03B1."@el ,
"L'atmosfera di Marte, a causa della bassa gravit\u00E0 del pianeta, \u00E8 estremamente rarefatta e completamente priva dei gas pi\u00F9 leggeri; la pressione rilevata dalle sonde automatiche inviate sul pianeta \u00E8 di circa 0,7\u20130,9 kPa nelle depressioni pi\u00F9 profonde (la pressione media dell'atmosfera terrestre, a titolo di paragone, \u00E8 di 101 kPa). Precedenti osservazioni dei transiti di Marte davanti alle stelle, effettuate dalla Terra, gi\u00E0 prima dell'era spaziale avevano suggerito una simile situazione."@it ;
rdfs:seeAlso dbr:Atmospheric_tide ,
dbr:Water_on_Mars ,
dbr:Dust_devil ,
dbr:Mineral_dust ,
dbr:Martian_polar_ice_caps ,
dbr:Orographic_lift ,
dbr:Atmospheric_escape ;
foaf:depiction ,
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@prefix dcterms: .
@prefix dbc: .
dbr:Atmosphere_of_Mars dcterms:subject dbc:Articles_containing_video_clips ,
dbc:Atmosphere_of_Mars ,
dbc:Planetary_atmospheres_of_the_Solar_System ,
dbc:Mars ;
dbo:abstract "L\u2019atmosph\u00E8re de Mars est la couche de gaz entourant la plan\u00E8te Mars. La pression au sol de l'atmosph\u00E8re martienne varie entre 30 Pa (0,03 kPa) au sommet d'Olympus Mons et 1 155 Pa (1,155 kPa) dans les profondeurs de Hellas Planitia. La pression moyenne est de 600 Pa (0,6 kPa soit 6 mbar, environ 170 fois moins que sur Terre) et sa masse totale est estim\u00E9e \u00E0 25 Tt (25 000 milliards de tonnes), soit environ 200 fois moins que l'atmosph\u00E8re terrestre ou encore le double de la masse combin\u00E9e de ses deux satellites, Phobos et D\u00E9imos. L'atmosph\u00E8re de Mars, en majorit\u00E9 compos\u00E9e de dioxyde de carbone (96 %), d'argon (1,93 %) et de diazote (1,89 %), contient des traces de dioxyg\u00E8ne, d'eau, et de m\u00E9thane. Elle est poussi\u00E9reuse pendant les temp\u00EAtes, conf\u00E9rant au ciel une couleur rouille lorsqu'elle est observ\u00E9e depuis la surface, et bleue lors des p\u00E9riodes d'accalmie. Les donn\u00E9es de Mariner 9, Mars Exploration Rovers et d'autres sondes indiquent qu'il s'agit de particules d'argile dont la taille m\u00E9diane est comprise entre 1,5 et 3 \u00B5m suivant les auteurs. Depuis la d\u00E9tection du m\u00E9thane, qui pourrait indiquer la pr\u00E9sence de vie sur Mars, l'int\u00E9r\u00EAt de l'\u00E9tude de la plan\u00E8te et de son atmosph\u00E8re s'est accru. Ce m\u00E9thane pourrait r\u00E9sulter d'un processus g\u00E9ochimique ou volcanique."@fr ,
"Atmosf\u00E9ra Marsu je plynn\u00FD obal nach\u00E1zej\u00EDc\u00ED se okolo planety Mars. Je velmi \u0159\u00EDdk\u00E1, nen\u00ED schopn\u00E1 zadr\u017Eovat tepelnou v\u00FDm\u011Bnu mezi povrchem a okoln\u00EDm prostorem, co\u017E m\u00E1 za n\u00E1sledek velk\u00E9 tepeln\u00E9 rozd\u00EDly b\u011Bhem dne a noci. Tlak na povrchu se pohybuje mezi 600 a 1 000 Pa (s extr\u00E9my 30 Pa na vrcholku Olympus Mons a\u017E 1 155 Pa v oblasti Hellas Planitia). Je to p\u0159ibli\u017En\u011B 100- a\u017E 150kr\u00E1t m\u00E9n\u011B ne\u017E na povrchu Zem\u011B; odpov\u00EDd\u00E1 to tlaku zhruba ve v\u00FD\u0161ce 30 km nad zemsk\u00FDm povrchem (pr\u016Fm\u011Brn\u00FD tlak na povrchu Zem\u011B je 101,3 kPa). Podobn\u011B jako na Zemi ale doch\u00E1z\u00ED k sez\u00F3nn\u00EDm zm\u011Bn\u00E1m v atmosf\u00E9\u0159e, jak se planeta k Slunci p\u0159ibli\u017Euje a oddaluje od n\u011Bj. V zim\u011B 25\u201330 % atmosf\u00E9rick\u00E9ho oxidu uhli\u010Dit\u00E9ho desublimuje na p\u00F3lech, zat\u00EDmco v l\u00E9t\u011B op\u011Bt sublimuje a vrac\u00ED se do atmosf\u00E9ry. Mars postupn\u011B v \u010Dase svou atmosf\u00E9ru ztr\u00E1c\u00ED, co\u017E je zp\u016Fsobov\u00E1no interakc\u00ED svrchn\u00EDch vrstev atmosf\u00E9ry se slune\u010Dn\u00EDm v\u011Btrem a kosmick\u00FDm z\u00E1\u0159en\u00EDm. Tyto interakce zp\u016Fsobuj\u00ED sr\u00E1\u017Eky molekul plyn\u016F tvo\u0159\u00EDc\u00EDch atmosf\u00E9ru s vysoce energetick\u00FDmi \u010D\u00E1sticemi. B\u011Bhem sr\u00E1\u017Eky dojde k roz\u0161t\u011Bpen\u00ED molekuly a jednotliv\u00E9 atomy (nap\u0159. vod\u00EDku) mohou b\u00FDt pak odtla\u010Deny dal\u0161\u00EDmi dopadaj\u00EDc\u00EDmi \u010D\u00E1sticemi z gravita\u010Dn\u00EDho p\u016Fsoben\u00ED planety do okoln\u00EDho vesm\u00EDru."@cs ,
"L'atmosfera de Mart \u00E9s relativament prima i est\u00E0 composta principalment de di\u00F2xid de carboni (95,32%). Hi ha hagut un inter\u00E8s en l'estudi de la seva composici\u00F3 des de la detecci\u00F3 de traces de met\u00E0, que pot indicar la pres\u00E8ncia de vida a Mart, per\u00F2 tamb\u00E9 pot ser produ\u00EFt per un proc\u00E9s geoqu\u00EDmic, l'activitat volc\u00E0nica o hidrotermal. La pressi\u00F3 atmosf\u00E8rica a la superf\u00EDcie de Mart varia de prop de 30 pascals (0,0044 psi) al cim d'Olympus Mons, a m\u00E9s de 1.155 pascals (0,1675 psi) en les profunditats de Hellas Planitia, amb una pressi\u00F3 mitjana a nivell de superf\u00EDcie de 600 pascals (0,087 psi), en comparaci\u00F3 amb la mitjana de la Terra al nivell del mar de 101,3 kilopascals (14,69 psi), i una massa total de 25 teratones, en comparaci\u00F3 amb els 5.148 teratones de la Terra. No obstant aix\u00F2, l'al\u00E7ada d'escala de l'atmosfera \u00E9s d'uns 11 quil\u00F2metres, una mica superior als 7 quil\u00F2metres de la Terra. L'atmosfera de Mart es compon d'un 95% de di\u00F2xid de carboni, 3% de nitrogen, 1,6% d'arg\u00F3, i cont\u00E9 traces d'oxigen, aigua i met\u00E0, amb una massa molar mitjana de 43,34 g/mol. L'atmosfera \u00E9s molt polsosa, donant al cel marci\u00E0 d'un color marr\u00F3 clar o ataronjat quan es veu de la superf\u00EDcie estant; les dades dels Rovers d'Exploraci\u00F3 de Mart indiquen que les part\u00EDcules de pols suspeses en l'atmosfera s\u00F3n m\u00E9s o menys 1,5 micr\u00F2metres de di\u00E0metre."@ca ,
"\u706B\u661F\u306E\u5927\u6C17\u306F\u3001\u91D1\u661F\u306E\u5927\u6C17\u3088\u308A\u3082\u9059\u304B\u306B\u5E0C\u8584\u3067\u3042\u308B\u304C\u3001\u540C\u69D8\u306B\u4E3B\u306B\u4E8C\u9178\u5316\u70AD\u7D20\u3067\u69CB\u6210\u3055\u308C\u3066\u3044\u308B\u3002\u751F\u547D\u306E\u5B58\u5728\u3092\u793A\u5506\u3059\u308B\u75D5\u8DE1\u91CF\u306E\u30E1\u30BF\u30F3\u304C\u691C\u51FA\u3055\u308C\u3066\u304B\u3089\u305D\u306E\u7D44\u6210\u306B\u518D\u3073\u95A2\u5FC3\u304C\u96C6\u307E\u3063\u3066\u3044\u305F\u304C\u3001\u30E1\u30BF\u30F3\u306F\u706B\u5C71\u3084\u71B1\u6C34\u5674\u51FA\u5B54\u3067\u3082\u751F\u6210\u3057\u3046\u308B\u3002 \u706B\u661F\u8868\u9762\u306E\u5927\u6C17\u5727\u306F\u3001\u5E73\u5747750\u30D1\u30B9\u30AB\u30EB\u3067\u3042\u308A\u3001\u5730\u7403\u306E\u6D77\u9762\u4E0A\u306E\u5E73\u5747\u3067\u3042\u308B101.3\u30AD\u30ED\u30D1\u30B9\u30AB\u30EB\u306E\u304A\u3088\u305D0.75%\u3001\u91D1\u661F\u306E\u5E73\u57479.3\u30E1\u30AC\u30D1\u30B9\u30AB\u30EB\u306E\u308F\u305A\u304B0.0065%\u3067\u3042\u308B\u3002\u30AA\u30EA\u30F3\u30DD\u30B9\u5C71\u306E\u9802\u4E0A\u306E30\u30D1\u30B9\u30AB\u30EB\u304B\u3089\u30D8\u30E9\u30B9\u5E73\u539F\u306E\u6700\u6DF1\u90E8\u3067\u306E1,155\u30D1\u30B9\u30AB\u30EB\u307E\u3067\u5E45\u304C\u3042\u308B\u3002\u5730\u7403\u306E\u5927\u6C17\u306E\u8CEA\u91CF\u306F5148\u30C6\u30E9\u30C8\u30F3\u3067\u3042\u308B\u306E\u306B\u6BD4\u3079\u3066\u3001\u706B\u661F\u306E\u5927\u6C17\u306E\u8CEA\u91CF\u306F25\u30C6\u30E9\u30C8\u30F3\u3067\u3042\u308B\u3002\u30B9\u30B1\u30FC\u30EB\u30CF\u30A4\u30C8\u306F\u3001\u5730\u7403\u306E\u7D046km\u306B\u5BFE\u3057\u3066\u3001\u706B\u661F\u306F\u7D0411km\u3067\u3042\u308B\u3002\u706B\u661F\u306E\u5927\u6C17\u306E\u7D44\u6210\u306F\u300195%\u304C\u4E8C\u9178\u5316\u70AD\u7D20\u30013%\u304C\u7A92\u7D20\u30011.6%\u304C\u30A2\u30EB\u30B4\u30F3\u3067\u3042\u308A\u3001\u9178\u7D20\u3001\u4E00\u9178\u5316\u70AD\u7D20\u3001\u6C34\u3001\u30E1\u30BF\u30F3\u3001\u305D\u306E\u4ED6\u306E\u6C17\u4F53\u306F\u75D5\u8DE1\u91CF\u3067\u3042\u308B\u3002\u5E73\u5747\u306E\u30E2\u30EB\u8CEA\u91CF\u306F43.34g/mol\u3068\u306A\u308B\u3002\u5927\u6C17\u306B\u306F\u975E\u5E38\u306B\u5875\u304C\u591A\u304F\u3001\u706B\u661F\u306E\u8868\u9762\u304B\u3089\u7A7A\u3092\u898B\u308B\u3068\u3001\u660E\u308B\u3044\u8336\u8272\u304B\u3089\u6A59\u8272\u306B\u898B\u3048\u308B\u3002\u30DE\u30FC\u30BA\u30FB\u30A8\u30AF\u30B9\u30D7\u30ED\u30EC\u30FC\u30B7\u30E7\u30F3\u30FB\u30ED\u30FC\u30D0\u30FC\u304B\u3089\u306E\u30C7\u30FC\u30BF\u306F\u3001\u5927\u6C17\u4E2D\u306B\u6D6E\u904A\u3059\u308B\u5875\u306E\u7C92\u5B50\u306F\u76F4\u5F84\u7D041.5\u03BCm\u3067\u3042\u308B\u3053\u3068\u3092\u793A\u5506\u3057\u305F\u3002"@ja ,
"Mars, planet ke-4 dari Matahari, memiliki atmosfer yang berbeda dengan atmosfer Bumi . Terdapat banyak ketertarikan dalam meneliti komposisinya sejak ditemukannya kandungan kecil metana, yang dapat menandai kehidupan di Mars."@in ,
"Mars atmosf\u00E4r \u00E4r f\u00F6rh\u00E5llandevis tunn och best\u00E5r huvudsakligen av koldioxid (95,32 procent), med mindre delar kv\u00E4ve och argon. Det \u00E4r intressant att studera dess sammans\u00E4ttning, eftersom uppt\u00E4ckt av sp\u00E5r av vissa \u00E4mnen, exempelvis metan, skulle kunna indikera att det funnits liv p\u00E5 Mars. Atmosf\u00E4rstrycket \u00E4r cirka 6,35 hektopascal, motsvarande mindre \u00E4n 1 procent av jordens lufttryck. Trycket \u00E4r dock mycket varierande, beroende p\u00E5 stora h\u00F6jdskillnader samt p\u00E5 grund av att m\u00E4ngder av koldioxid p\u00E5 vintern kondenseras och d\u00E5 bildar omfattande polarkalotter. Forskare tror att atmosf\u00E4ren var mycket tjockare f\u00F6r tre miljarder \u00E5r sedan. En tjockare atmosf\u00E4r skulle g\u00F6ra att planeten blev varmare. Mars var vid den tiden antagligen s\u00E5 varm att det fanns flytande vatten d\u00E4r. Rymdsonder har lokaliserat m\u00E5nga sp\u00E5r av vatten p\u00E5 Mars. F\u00F6r tre miljarder \u00E5r sedan var Mars en aktiv planet med vulkanutbrott och b\u00E4vningar. 2015 presenterade NASA bevis f\u00F6r att det \u00E4r solvinden i kombination med att Mars inte har n\u00E5got skyddande magnetf\u00E4lt som f\u00E5r planetens atmosf\u00E4r att f\u00F6rsvinna."@sv ,
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"Die Atmosph\u00E4re des Mars besitzt eine Gesamtmasse von etwa 2,5 \u00D7 1016kg.Sie ist sehr d\u00FCnn, ihre Dichte betr\u00E4gt ca. 1,2 % der Dichte der Erdatmosph\u00E4re. Der mittlere atmosph\u00E4rische Druck auf Nullniveau betr\u00E4gt ca. 6 hPa (0,006 Bar), 6,36 hPa (0,00636 Bar) am mittleren Radius mit jahreszeitlichen Schwankungen von 4,0 hPa (0,0040 Bar) bis 8,7 hPa (0,0087 Bar). Das sind nur 0,6 % des mittleren Luftdrucks auf der Erde mit 1013 hPa (1,013 Bar) und entspricht etwa dem Druck, der in der Stratosph\u00E4re der Erde in 32 km H\u00F6he herrscht.Die Schallgeschwindigkeit in einer H\u00F6he von 15 km betr\u00E4gt 230 m/s.Auf der Oberfl\u00E4che des Mars liegt die Schallgeschwindigkeit f\u00FCr niedrige Frequenzen bei 240 m/s, f\u00FCr hohe Frequenzen bei etwa 250 m/s. Der extrem niedrige atmosph\u00E4rische Druck liegt in der N\u00E4he des Tripelpunkts von Wasser. Das hei\u00DFt, fl\u00FCssiges Wasser kann auf der Marsoberfl\u00E4che nur in Tiefebenen (das sind haupts\u00E4chlich die Nordhalbkugel und Hellas Planitia) und nur bei hohen Temperaturen kurzzeitig f\u00FCr wenige Stunden existieren. Am tiefsten Punkt der Marsoberfl\u00E4che in Hellas Planitia erreicht der Druck maximal etwa 12 hPa (0,012 Bar). Das ist deutlich unter der Armstrong-Grenze von 63 hPa (0,063 Bar), bei der Wasser bei menschlicher K\u00F6rpertemperatur siedet, deshalb kann ein Mensch auf dem Mars nicht ohne einen Druckanzug oder eine Druckkabine \u00FCberleben. In ihrer chemischen Zusammensetzung besteht die Marsatmosph\u00E4re, wie auch die der Venus, haupts\u00E4chlich aus Kohlenstoffdioxid, in kleineren Mengen aber auch aus anderen Gasen wie Argon, Stickstoff und Sauerstoff. Im Jahre 2003 wurden auch Spuren von Methan in der Gash\u00FClle des Planeten nachgewiesen. Man konnte bisher nicht eindeutig erkl\u00E4ren, wie dieses Gas in die Atmosph\u00E4re gelangte. Obwohl die Atmosph\u00E4re des Mars so d\u00FCnn ist, ist der Himmel des Mars nicht schwarz. Wegen des hohen Staubanteils in der Atmosph\u00E4re wird das Licht stark gestreut. Der Taghimmel erscheint hell und Sterne sind nicht zu sehen. Die Farbe des Himmels w\u00E4hrend des Tages variiert von orangerot \u00FCber rosa und violett bis blau in der N\u00E4he der auf- und untergehenden Sonne."@de ,
"La atm\u00F3sfera de Marte est\u00E1 compuesta principalmente por di\u00F3xido de carbono (95%), nitr\u00F3geno (3%) y arg\u00F3n (1,6%), y contiene trazas de ox\u00EDgeno, agua y metano, siendo muy diferente a la atm\u00F3sfera de la Tierra. Recientemente ha habido mayor inter\u00E9s en el estudio de su composici\u00F3n por la detecci\u00F3n de peque\u00F1as cantidades de metano, que podr\u00EDan indicar la existencia de alguna forma de vida. La atm\u00F3sfera en Marte es ligera, y la presi\u00F3n atmosf\u00E9rica en la superficie var\u00EDa de 36,6 Pa (0,0366 kPa) en la cumbre del monte Olimpo a m\u00E1s de 1155 Pa (1,155 kPa) en las depresiones de Hellas Planitia con una presi\u00F3n media de la superficie de 600 Pa (0,600kPa), frente a la presi\u00F3n de 101300 Pa (101,3 kPa) terrestre. La atm\u00F3sfera de Marte es muy polvorienta, dando al cielo marciano un color amarillento cuando se ve desde la superficie. Los datos transmitidos por los veh\u00EDculos Mars Exploration Rovers indican que las part\u00EDculas en suspensi\u00F3n tiene alrededor de 1,5 micr\u00F3metros. La densidad atmosf\u00E9rica m\u00E1s alta en Marte es igual a la densidad que se encuentra a 35 km sobre la superficie de la Tierra. Existe una continua p\u00E9rdida de atm\u00F3sfera que escapa al espacio exterior. Se calcula que cada segundo se pierden entre 1 y 2kg de atm\u00F3sfera.\u200B\u200B"@es ,
"Marte \u00E9 o quarto planeta a partir do Sol, e possui uma atmosfera muito diferente da atmosfera terrestre. Tem havido muito interesse no estudo de sua composi\u00E7\u00E3o desde a recente detec\u00E7\u00E3o de pequenas quantidades de metano, que poderia indicar alguma forma de vida em Marte. A atmosfera marciana \u00E9 rarefeita, e a press\u00E3o atmosf\u00E9rica na superf\u00EDcie varia de 30 Pa (0,03 kPa) no pico do Olympus Mons para mais de 1 155 Pa (1,155 kPa) nas depress\u00F5es de Hellas Planitia, com uma press\u00E3o m\u00E9dia na superf\u00EDcie de 600 Pa (0,6 kPa), comparado \u00E0 press\u00E3o terrestre de 101,3 kPa. A atmosfera de Marte consiste em 95% de di\u00F3xido de carbono, 3% nitrog\u00EAnio, 1,6% arg\u00F4nio, e ainda tra\u00E7os de oxig\u00EAnio, \u00E1gua, e metano. A atmosfera de Marte \u00E9 bastante empoeirada, dando ao c\u00E9u marciano uma cor amarelada quando vista da superf\u00EDcie; dados da Mars Exploration Rovers indicam que part\u00EDculas suspensas possuem aproximadamente 1,5 micr\u00F4metros."@pt ,
"\u706B\u661F\u7684\u5927\u6C23\u5C64\uFF0C\u81EA\u5F9E\u706B\u661F\u767C\u73FE\u5C11\u91CF\u7532\u70F7\u4EE5\u4F86\uFF0C\u95DC\u65BC\u5176\u5982\u4F55\u7D44\u6210\u7684\u7814\u7A76\u8D8A\u4F86\u8D8A\u53D7\u5230\u95DC\u6CE8\uFF0C\u56E0\u70BA\u9019\u53EF\u80FD\u662F\u706B\u661F\u751F\u547D\u5B58\u5728\u7684\u8DE1\u8C61\uFF1B\u4E0D\u904E\u9019\u4E5F\u53EF\u80FD\u662F\u7531\u4F5C\u7528\u3001\u706B\u5C71\u4F5C\u7528\u6216\u7B49\u7121\u6A5F\u65B9\u5F0F\u6240\u9020\u6210\u7684\u3002 \u706B\u661F\u7684\u5927\u6C23\u5C64\u76F8\u5C0D\u8F03\u8584\uFF0C\u5730\u8868\u6C23\u58D3\u4F4E\u81F3\u5967\u6797\u5E15\u65AF\u5C71\u9802\u768430\u5E15\u3001\u9AD8\u81F3\u5E0C\u81D8\u5E73\u539F\u4F4E\u9EDE\u76841155\u5E15\u3002\u706B\u661F\u8868\u9762\u7684\u5E73\u5747\u6C23\u58D3\u70BA6\u767E\u5E15\uFF0C\u76F8\u6BD4\u4E4B\u4E0B\u5730\u7403\u6C23\u58D3\u70BA1013\u767E\u5E15\uFF0C\u4E5F\u5C31\u662F\u8AAA\u706B\u661F\u5927\u6C23\u58D3\u529B\u4E0D\u5230\u5730\u7403\u7684\u767E\u5206\u4E4B\u4E00\u3002\u706B\u661F\u5927\u6C23\u7E3D\u8CEA\u91CF\u70BA25\u5146\u5678\uFF0C\u800C\u5730\u7403\u70BA5148\u5146\u5678\uFF0C\u91D1\u661F\u5247\u70BA48\u4EAC\u5678\u3002\u7136\u800C\u5B83\u7684\u5927\u6C23\u6A19\u9AD8\u70BA11\u516C\u91CC\uFF0C\u6BD4\u5730\u7403\u76847\u516C\u91CC\u7A0D\u5927\u3002\u706B\u661F\u5927\u6C23\u542B\u670995%\u7684\u4E8C\u6C27\u5316\u78B3\u30013%\u7684\u6C2E\u6C23\u30011.6%\u7684\u6C2C\u6C23\u3001\u4E9B\u5FAE\u7684\u6C27\u6C23\u3001\u6C34\u6C23\u548C\u7532\u70F7\uFF0C\u5E73\u5747\u5206\u5B50\u91CF\u70BA43.34\u3002\u5927\u6C23\u4E2D\u9084\u5145\u6EFF\u5F88\u591A\u5875\u57C3\uFF0C\u4F7F\u5F97\u5F9E\u706B\u661F\u5730\u8868\u4F86\u770B\u662F\u9EC3\u8910\u8272\u7684\u3002\u706B\u661F\u63A2\u6E2C\u6F2B\u904A\u8005\u7684\u8CC7\u6599\u6307\u51FA\uFF0C\u9019\u4E9B\u61F8\u6D6E\u5FAE\u5875\u7D041.5\u5FAE\u7C73\u5BEC\u3002"@zh ,
"L'atmosfera di Marte, a causa della bassa gravit\u00E0 del pianeta, \u00E8 estremamente rarefatta e completamente priva dei gas pi\u00F9 leggeri; la pressione rilevata dalle sonde automatiche inviate sul pianeta \u00E8 di circa 0,7\u20130,9 kPa nelle depressioni pi\u00F9 profonde (la pressione media dell'atmosfera terrestre, a titolo di paragone, \u00E8 di 101 kPa). Precedenti osservazioni dei transiti di Marte davanti alle stelle, effettuate dalla Terra, gi\u00E0 prima dell'era spaziale avevano suggerito una simile situazione. L'atmosfera appare ricca di polveri che le conferiscono una caratteristica colorazione arancione-marrone quando osservata dalla superficie del pianeta; i dati registrati dai Mars Exploration Rover indicano una dimensione media delle particelle sospese di circa 1,5 \u03BCm. L'estrema scarsit\u00E0 di ozono permette alle radiazioni ultraviolette solari, letali per ogni forma di vita conosciuta, di raggiungere la superficie."@it ,
"\u0410\u0442\u043C\u043E\u0441\u0444\u0435\u0440\u0430 \u041C\u0430\u0440\u0441\u0430 \u2014 \u0433\u0430\u0437\u043E\u0432\u0430 \u043E\u0431\u043E\u043B\u043E\u043D\u043A\u0430, \u0449\u043E \u043E\u0442\u043E\u0447\u0443\u0454 \u043F\u043B\u0430\u043D\u0435\u0442\u0443 \u041C\u0430\u0440\u0441. \u0406\u0441\u0442\u043E\u0442\u043D\u043E \u0432\u0456\u0434\u0440\u0456\u0437\u043D\u044F\u0454\u0442\u044C\u0441\u044F \u0432\u0456\u0434 \u0437\u0435\u043C\u043D\u043E\u0457 \u0430\u0442\u043C\u043E\u0441\u0444\u0435\u0440\u0438 \u044F\u043A \u0437\u0430 \u0445\u0456\u043C\u0456\u0447\u043D\u0438\u043C \u0441\u043A\u043B\u0430\u0434\u043E\u043C, \u0442\u0430\u043A \u0456 \u0437\u0430 \u0444\u0456\u0437\u0438\u0447\u043D\u0438\u043C\u0438 \u043F\u0430\u0440\u0430\u043C\u0435\u0442\u0440\u0430\u043C\u0438. \u0422\u0438\u0441\u043A \u0431\u0456\u043B\u044F \u043F\u043E\u0432\u0435\u0440\u0445\u043D\u0456 \u0441\u0442\u0430\u043D\u043E\u0432\u0438\u0442\u044C 0,7-1,155 \u043A\u041F\u0430 (1/110 \u0432\u0456\u0434 \u0442\u0438\u0441\u043A\u0443 \u0432 \u0430\u0442\u043C\u043E\u0441\u0444\u0435\u0440\u0456 \u0417\u0435\u043C\u043B\u0456 \u043D\u0430 \u0440\u0456\u0432\u043D\u0456 \u043C\u043E\u0440\u044F, \u0449\u043E \u0434\u043E\u0440\u0456\u0432\u043D\u044E\u0454 \u0442\u0438\u0441\u043A\u0443 \u0432 \u0437\u0435\u043C\u043D\u0456\u0439 \u0430\u0442\u043C\u043E\u0441\u0444\u0435\u0440\u0456 \u043D\u0430 \u0432\u0438\u0441\u043E\u0442\u0456 \u043F\u043E\u043D\u0430\u0434 \u0442\u0440\u0438\u0434\u0446\u044F\u0442\u044C \u043A\u0456\u043B\u043E\u043C\u0435\u0442\u0440\u0456\u0432). \u041E\u0440\u0456\u0454\u043D\u0442\u043E\u0432\u043D\u0430 \u0442\u043E\u0432\u0449\u0438\u043D\u0430 \u0430\u0442\u043C\u043E\u0441\u0444\u0435\u0440\u0438 \u2014 110 \u043A\u043C. \u041F\u0440\u0438\u0431\u043B\u0438\u0437\u043D\u0430 \u043C\u0430\u0441\u0430 \u0430\u0442\u043C\u043E\u0441\u0444\u0435\u0440\u0438 \u2014 2,5\u00D7 1016 \u043A\u0433. \u041C\u0430\u0440\u0441 \u043C\u0430\u0454 \u0434\u0443\u0436\u0435 \u0441\u043B\u0430\u0431\u043A\u0435 \u043C\u0430\u0433\u043D\u0456\u0442\u043D\u0435 \u043F\u043E\u043B\u0435 (\u0443 \u043F\u043E\u0440\u0456\u0432\u043D\u044F\u043D\u043D\u0456 \u0437 \u0437\u0435\u043C\u043D\u0438\u043C), \u0456 \u0432 \u0440\u0435\u0437\u0443\u043B\u044C\u0442\u0430\u0442\u0456 \u0441\u043E\u043D\u044F\u0447\u043D\u0438\u0439 \u0432\u0456\u0442\u0435\u0440 \u043F\u043E\u0441\u0442\u0443\u043F\u043E\u0432\u043E \u00AB\u0437\u0434\u0443\u0432\u0430\u0454\u00BB \u0430\u0442\u043C\u043E\u0441\u0444\u0435\u0440\u0443 \u0432 \u043A\u043E\u0441\u043C\u043E\u0441 \u0437\u0456 \u0448\u0432\u0438\u0434\u043A\u0456\u0441\u0442\u044E 300 \u00B1 200 \u0442\u043E\u043D\u043D \u043D\u0430 \u0434\u0435\u043D\u044C (\u0437\u0430\u043B\u0435\u0436\u043D\u043E \u0432\u0456\u0434 \u043F\u043E\u0442\u043E\u0447\u043D\u0438\u0445 \u0441\u043E\u043D\u044F\u0447\u043D\u043E\u0457 \u0430\u043A\u0442\u0438\u0432\u043D\u043E\u0441\u0442\u0456 \u0442\u0430 \u0432\u0456\u0434\u0441\u0442\u0430\u043D\u0456 \u0432\u0456\u0434 \u0421\u043E\u043D\u0446\u044F.)"@uk ,
"Atmosfera Marsa \u2013 pow\u0142oka gazowa otaczaj\u0105ca Marsa. Jest bardzo cienka i rozrzedzona w por\u00F3wnaniu z ziemsk\u0105, ci\u015Bnienie atmosferyczne wynosi od 30 Pa na wierzcho\u0142ku Olympus Mons do ponad 1155 Pa przy dnie Hellas Planitia. Sk\u0142ad atmosfery to g\u0142\u00F3wnie dwutlenek w\u0119gla (95,32%), azot (2,7%) i argon (1,6%). Pozosta\u0142e 0,38% stanowi\u0105 pierwiastki \u015Bladowe, w\u015Br\u00F3d kt\u00F3rych znajduje si\u0119 tak\u017Ce tlen. Uwa\u017Ca si\u0119, \u017Ce miliardy lat temu atmosfera Marsa by\u0142a g\u0119stsza i zawiera\u0142a wi\u0119cej tlenu ni\u017C ziemska."@pl ,
"\uD654\uC131\uC758 \uB300\uAE30\uB294 \uD0DC\uC591\uACC4\uC758 4\uBC88\uC9F8 \uD589\uC131\uC778 \uD654\uC131\uC744 \uB458\uB7EC\uC2F8\uACE0 \uC788\uB294 \uAE30\uCCB4\uCE35\uC744 \uC758\uBBF8\uD558\uBA70 \uB300\uBD80\uBD84\uC774 \uC774\uC0B0\uD654 \uD0C4\uC18C\uB85C \uAD6C\uC131\uB418\uC5B4 \uC788\uB2E4. \uD3C9\uADE0 \uAE30\uC555\uC740 \uC57D 600 \uD30C\uC2A4\uCE7C\uB85C \uC9C0\uAD6C\uC758 \uD574\uC218\uBA74 \uD3C9\uADE0 \uAE30\uC555\uC778 101.3 \uD0AC\uB85C\uD30C\uC2A4\uCE7C\uC758 0.6 % \uC815\uB3C4\uC774\uBA70, \uADDC\uBAA8\uACE0\uB3C4\uB294 \uC57D 11 km \uC815\uB3C4\uC774\uB2E4. \uC774\uB54C, \uD654\uC131\uC758 \uB300\uAE30 \uC9C8\uB7C9\uC740 25 \uD14C\uB77C\uD1A4(25\u00D71012\uD1A4)\uC73C\uB85C \uADDC\uBAA8\uACE0\uB3C4\uAC00 \uC57D 8.5 km\uC778 \uC9C0\uAD6C\uC758 \uB300\uAE30 \uC9C8\uB7C9\uC778 5148 \uD14C\uB77C\uD1A4(5148\u00D71012\uD1A4)\uC758 0.005 % \uBC16\uC5D0 \uB418\uC9C0 \uC54A\uB294\uB2E4. \uD654\uC131\uC758 \uAE30\uC555\uC740 \uACE0\uB3C4\uC5D0 \uB530\uB77C \uD070 \uCC28\uC774\uB97C \uBCF4\uC774\uB294\uB370, \uD654\uC131\uC5D0\uC11C \uAC00\uC7A5 \uB192\uC740 \uC9C0\uC5ED\uC778 \uC62C\uB9BC\uD478\uC2A4 \uC0B0\uC758 \uCD5C\uACE0\uBD09\uC5D0\uC11C\uB294 \uC57D 30 \uD30C\uC2A4\uCE7C \uC815\uB3C4\uACE0 \uAC00\uC7A5 \uB0AE\uC740 \uC9C0\uC5ED\uC778 \uD5EC\uB77C\uC2A4 \uBD84\uC9C0\uC5D0\uC11C\uB294 1,155 \uD30C\uC2A4\uCE7C \uC815\uB3C4\uB85C \uC5B4\uB514\uC11C\uB4E0\uC9C0 \uD654\uC131\uC758 \uAE30\uC555\uC740 \uC554\uC2A4\uD2B8\uB871 \uD55C\uACC4\uBCF4\uB2E4 \uD6E8\uC52C \uB0AE\uC544\uC11C \uC778\uAC04\uC774 \uD654\uC131\uC758 \uB300\uAE30\uC5D0 \uB9E8\uBAB8\uC73C\uB85C \uB178\uCD9C\uB41C\uB2E4\uBA74 \uC704\uD5D8\uD574\uC9C8 \uC218 \uC788\uB2E4. \uD654\uC131\uC758 \uB300\uAE30\uB294 96 %\uAC00 \uC774\uC0B0\uD654 \uD0C4\uC18C, 1.9 %\uAC00 \uC544\uB974\uACE4, 1.9 %\uAC00 \uC9C8\uC18C \uB4F1\uC73C\uB85C \uC774\uB8E8\uC5B4\uC838 \uC788\uC73C\uBA70, \uC18C\uB7C9\uC758 \uC0B0\uC18C\uC640 \uC77C\uC0B0\uD654 \uD0C4\uC18C, \uC218\uC99D\uAE30 \uB4F1\uB3C4 \uD3EC\uD568\uB418\uC5B4 \uC788\uB2E4. \uBAB0 \uC9C8\uB7C9\uC740 \uC57D 43.34 g/mol \uC815\uB3C4\uC774\uBA70, 2003\uB144\uC5D0 \uD654\uC131\uC5D0\uC11C \uBA54\uD0C4\uC758 \uD754\uC801\uC774 \uBC1C\uACAC\uB41C \uC774\uB798\uB85C \uD654\uC131\uC758 \uB300\uAE30\uC5D0 \uAD00\uD55C \uAD00\uC2EC\uC774 \uAE09\uC99D\uD588\uB294\uB370, \uADF8 \uC774\uC720\uB294 \uBA54\uD0C4\uC774 \uC0DD\uBA85\uCCB4\uC758 \uC874\uC7AC\uB97C \uC554\uC2DC\uD558\uAE30 \uB54C\uBB38\uC774\uC9C0\uB9CC \uD55C\uD3B8\uC73C\uB85C\uB294 \uBA54\uD0C4\uC774 \uADF8\uC800 \uD654\uC131\uC758 \uD654\uC0B0\uC774\uB098 \uC5F4\uC218\uC131 \uD65C\uB3D9 \uB4F1\uC758 \uC9C0\uC9C8\uD559\uC801 \uD65C\uB3D9\uC744 \uD1B5\uD574 \uC0DD\uC0B0\uB41C \uAC83\uC774\uB77C\uB294 \uCD94\uCE21\uB3C4 \uC788\uB2E4. \uD654\uC131\uC758 \uB300\uAE30\uB294 \uBA3C\uC9C0\uAC00 \uB9E4\uC6B0 \uB9CE\uC544\uC11C \uD45C\uBA74\uC5D0\uC11C \uD654\uC131\uC758 \uD558\uB298\uC744 \uBCF8\uB2E4\uBA74 \uBC1D\uC740 \uAC08\uC0C9\uC774\uB098 \uC605\uC740 \uC8FC\uD669\uC0C9 \uACC4\uC5F4\uC758 \uBD89\uC740 \uC0C9\uC73C\uB85C \uBCF4\uC778\uB2E4. \uD654\uC131 \uD0D0\uC0AC\uCC28\uC778 \uC624\uD37C\uD29C\uB2C8\uD2F0\uC640 \uC2A4\uD53C\uB9BF\uC774 \uC218\uC9D1\uD55C \uC815\uBCF4\uC5D0 \uC758\uD558\uBA74 \uB300\uAE30 \uC0C1\uACF5\uC5D0 \uD45C\uB958\uD558\uB294 \uBA3C\uC9C0 \uC785\uC790\uC758 \uD06C\uAE30\uAC00 1.5 \uB9C8\uC774\uD06C\uB85C\uBBF8\uD130\uC778\uB370, \uC0C8\uB86D\uAC8C \uB5A0\uC624\uB974\uACE0 \uC788\uB294 \uD658\uACBD \uBB38\uC81C\uC778 \uBBF8\uC138\uBA3C\uC9C0\uB97C \uBD84\uB958\uD558\uB294 \uAE30\uC900\uC5D0 \uB530\uB974\uBA74 \uD654\uC131 \uBA3C\uC9C0\uC758 \uD06C\uAE30\uB294 2.5 \uB9C8\uC774\uD06C\uB85C\uBBF8\uD130 \uC774\uD558\uB85C \uADF9\uBBF8\uC138\uBA3C\uC9C0 \uD639\uC740 \uCD08\uBBF8\uC138\uBA3C\uC9C0\uC5D0 \uD574\uB2F9\uD55C\uB2E4."@ko ,
"T\u00E1 go leor eolais againn ar atmaisf\u00E9ar agus aer\u00E1id Mharsa. T\u00E1 10% de thoirt an Domhain i Mars, agus 25% d\u00E1 achar dromchla. T\u00E1 atmaisf\u00E9ar ag Mars, ach t\u00E1 s\u00E9 f\u00EDorthana\u00ED. T\u00E1 me\u00E1nbhr\u00FA an atmaisf\u00E9ir ar dhromchla Mharsa timpeall ar 750 Pa, n\u00F3 thart ar 0.75% de ghn\u00E1thbhr\u00FA an atmaisf\u00E9ir ar dhroim an Domhain seo againn. \u00D3n taobh eile, t\u00E1 an t-atmaisf\u00E9ar seo ag tan\u00FA n\u00EDos maille n\u00E1 \u00E1r n-atmaisf\u00E9ar f\u00E9in ag dul suas \u00F3 dhromchla an phl\u00E1in\u00E9id. D\u00E9-ocsa\u00EDd charb\u00F3in go pr\u00EDomha at\u00E1 ann, N\u00EDtrigin at\u00E1 i 3% de, agus arg\u00F3n at\u00E1 i 1.6%. Fosta, t\u00E1 meat\u00E1n agus ocsaigin i l\u00E1thair, chomh maith le triathgh\u00E1is eile seachas an t-arg\u00F3n - is \u00E9 sin, neon, criopt\u00F3n agus xean\u00F3n, n\u00F3 n\u00EDl imtharraingt Mharsa in ann g\u00E1s chomh h\u00E9adrom le h\u00E9iliam a choinne\u00E1il \u00F3 \u00E9al\u00FA go dt\u00ED an sp\u00E1s. Ar an gc\u00FAis ch\u00E9anna, n\u00EDl hidrigin shaor le f\u00E1il in atmaisf\u00E9ar Mharsa ach an oiread. Is \u00E9 an phr\u00EDomhch\u00FAis le fuacht Mharsa an t-atmaisf\u00E9ar seo, n\u00F3, \u00F3s rud \u00E9 go bhfuil s\u00E9 chomh sc\u00E1inte sin, n\u00EDl s\u00E9 in ann teas a cheapadh n\u00E1 a choinne\u00E1il. C\u00E9 go bhfuil atmaisf\u00E9ar an phl\u00E1in\u00E9id chomh tana\u00ED sin, t\u00E1 cuid mhaith dusta ag foluain timpeall. Na sonra\u00ED a bhailigh na gl\u00E9asanna gluaisteacha taisc\u00E9ala\u00EDochta Spirit agus Opportunity ar dhromchla an phl\u00E1in\u00E9id le d\u00E9ana\u00ED, tugann siad le fios go bhfuil an dusta seo comhdh\u00E9anta as gr\u00E1inn\u00EDn\u00ED at\u00E1 thart ar 1.5 micrim\u00E9adar (1.5 m\u00EDli\u00FA cuid de mhillim\u00E9adar) trasna. Sa bhliain 2003, d'aithin teileasc\u00F3ip th\u00EDos ar an Domhan go raibh meat\u00E1n le f\u00E1il in atmaisf\u00E9ar Mharsa, agus dealra\u00EDonn s\u00E9 gur dheimhnigh an taisc\u00E9ala\u00ED Mars Express Orbiter an breathn\u00FA seo i M\u00ED na M\u00E1rta 2004. Tugann na tortha\u00ED tomhais le fios go bhfuil dl\u00FAs an mheat\u00E1in in atmaisf\u00E9ar Mharsa thart ar aon bhilli\u00FAn\u00FA cuid d\u00E9ag (11 pbb). C\u00FAis suntais \u00E9 an meat\u00E1n sin, n\u00F3 t\u00E1 an meat\u00E1n chomh h\u00E9agobhsa\u00ED mar gh\u00E1s is nach mbeadh s\u00E9 ann murach go bhfuil foinse \u00E9igin \u00E1 shol\u00E1thar taobh istigh den phl\u00E1in\u00E9ad. N\u00EDl s\u00E9 scaipthe go cothrom tar \u00E9is an phl\u00E1in\u00E9id, ach an oiread. Mar sin, caithfidh s\u00E9 go bhfuil s\u00E9 \u00E1 scaoileadh saor in \u00E1iteanna \u00E1irithe, agus is \u00ED an cheist mh\u00F3r a chuireann na saineolaithe orthu f\u00E9in, ar nd\u00F3igh, an bhfuil beatha de chine\u00E1l \u00E9igin - cos\u00FAil leis na miocrorg\u00E1naigh airc\u00E9acha ar a dtugtar meat\u00E1naigin\u00ED - ag t\u00E1irgi\u00FA an mheat\u00E1in seo. Maidir le saintr\u00E9ithe eile an atmaisf\u00E9ir, b\u00EDonn siad claochlaitheach go leor. Sa gheimhreadh, nuair at\u00E1 an chaidhp pholach f\u00E1gtha i ndorchadas, \u00E9ir\u00EDonn an dromchla chomh fuar is a chuireann s\u00E9 an d\u00E9-ocsa\u00EDd charb\u00F3in san atmaisf\u00E9ar ag sioc s\u00EDos. Is f\u00E9idir d'oiread is 25 % den atmaisf\u00E9ar iomp\u00FA ina oighear tirim. Le teacht an earraigh agus an tsolais, iomp\u00F3idh an leac oighir ina g\u00E1s ar\u00EDs. Tabhair faoi deara nach le\u00E1nn an t-oighear d\u00ED-ocsa\u00EDde carb\u00F3in - sin \u00E9 an ch\u00FAis a dtugtar oighear tirim air - n\u00F3 is dual di n\u00E9al\u00FA ina g\u00E1s sula sroichfear an le\u00E1phointe. N\u00ED f\u00E9idir di bheith ina sreabh\u00E1n (leacht) ach faoi bhr\u00FA an-mh\u00F3r, rud nach bhfuil le f\u00E1il faoi atmaisf\u00E9ar tana\u00ED Mharsa. Mar sin, le teacht an ts\u00E9as\u00FAir the, n\u00E9ala\u00EDonn an d\u00ED-ocsa\u00EDd charb\u00F3in go sciobtha de dhromchla na caidhpe pola\u00ED, agus cuireann an pr\u00F3iseas seo gaotha m\u00F3ra millteanacha ag s\u00E9ideadh - is f\u00E9idir do stoirm den chine\u00E1l seo luas ceithre ch\u00E9ad cilim\u00E9adar in aghaidh uair an chloig (400 km/h) a bhaint amach. Ansin, crutha\u00EDtear scamaill at\u00E1 comhdh\u00E9anta as criostail bheaga oighir (is \u00E9 sin, oighear uisce, seachas oighear tirim). Chuirfid\u00EDs i gcuimhne duit cine\u00E1lacha \u00E1irithe scamaill a d'fheicfe\u00E1 ar an sp\u00E9ir anseo ar an Domhan. N\u00EDltear r\u00F3chinnte, an bhfuil aer\u00E1id Mharsa ag dul i bhfuacht n\u00F3 ag t\u00E9amh. T\u00E1 an dara bh'fh\u00E9idir ann: sna blianta 2002-2005, th\u00E1inig crapadh ar an gcaidhp pholach theas i ngach samhradh i gcompar\u00E1id leis an mbliain roimhe sin, agus n\u00ED raibh an geimhreadh in ann an crapadh seo a stopadh. Tugann an fhorbairt seo le fios go bhfuil Mars ag t\u00E9amh. Ina dhiaidh sin f\u00E9in, t\u00E1 s\u00E9 n\u00EDos fuaire ar Mhars inniu n\u00E1 mar a bh\u00ED thiar sna seacht\u00F3id\u00ED, nuair a thuirling an d\u00E1 Viking ansin."@ga ,
"\u0410\u0442\u043C\u043E\u0441\u0444\u0435\u0440\u0430 \u041C\u0430\u0440\u0441\u0430 \u2014 \u0433\u0430\u0437\u043E\u0432\u0430\u044F \u043E\u0431\u043E\u043B\u043E\u0447\u043A\u0430, \u043E\u043A\u0440\u0443\u0436\u0430\u044E\u0449\u0430\u044F \u043F\u043B\u0430\u043D\u0435\u0442\u0443 \u041C\u0430\u0440\u0441. \u0421\u0443\u0449\u0435\u0441\u0442\u0432\u0435\u043D\u043D\u043E \u043E\u0442\u043B\u0438\u0447\u0430\u0435\u0442\u0441\u044F \u043E\u0442 \u0437\u0435\u043C\u043D\u043E\u0439 \u0430\u0442\u043C\u043E\u0441\u0444\u0435\u0440\u044B \u043A\u0430\u043A \u043F\u043E \u0445\u0438\u043C\u0438\u0447\u0435\u0441\u043A\u043E\u043C\u0443 \u0441\u043E\u0441\u0442\u0430\u0432\u0443, \u0442\u0430\u043A \u0438 \u043F\u043E \u0444\u0438\u0437\u0438\u0447\u0435\u0441\u043A\u0438\u043C \u043F\u0430\u0440\u0430\u043C\u0435\u0442\u0440\u0430\u043C. \u0414\u0430\u0432\u043B\u0435\u043D\u0438\u0435 \u0443 \u043F\u043E\u0432\u0435\u0440\u0445\u043D\u043E\u0441\u0442\u0438 \u0441\u043E\u0441\u0442\u0430\u0432\u043B\u044F\u0435\u0442 \u0432 \u0441\u0440\u0435\u0434\u043D\u0435\u043C 0,6 \u043A\u041F\u0430 \u0438\u043B\u0438 6 \u043C\u0431\u0430\u0440 (1/170 \u043E\u0442 \u0437\u0435\u043C\u043D\u043E\u0433\u043E, \u0438\u043B\u0438 \u0440\u0430\u0432\u043D\u043E \u0437\u0435\u043C\u043D\u043E\u043C\u0443 \u043D\u0430 \u0432\u044B\u0441\u043E\u0442\u0435 \u043F\u043E\u0447\u0442\u0438 35 \u043A\u043C \u043E\u0442 \u043F\u043E\u0432\u0435\u0440\u0445\u043D\u043E\u0441\u0442\u0438 \u0417\u0435\u043C\u043B\u0438). \u0412\u044B\u0441\u043E\u0442\u0430 \u043E\u0434\u043D\u043E\u0440\u043E\u0434\u043D\u043E\u0439 \u0430\u0442\u043C\u043E\u0441\u0444\u0435\u0440\u044B \u0441\u043E\u0441\u0442\u0430\u0432\u043B\u044F\u0435\u0442 11,1 \u043A\u043C, \u043F\u0440\u0438\u043C\u0435\u0440\u043D\u0430\u044F \u043C\u0430\u0441\u0441\u0430 \u0430\u0442\u043C\u043E\u0441\u0444\u0435\u0440\u044B \u2014 2,5\u22C51016 \u043A\u0433 (\u0431\u043E\u043B\u0435\u0435 \u0447\u0435\u043C \u0432 200 \u0440\u0430\u0437 \u043C\u0435\u043D\u044C\u0448\u0435 \u0437\u0435\u043C\u043D\u043E\u0439). \u041C\u0430\u0440\u0441 \u0438\u043C\u0435\u0435\u0442 \u043E\u0447\u0435\u043D\u044C \u0441\u043B\u0430\u0431\u043E\u0435 \u043C\u0430\u0433\u043D\u0438\u0442\u043D\u043E\u0435 \u043F\u043E\u043B\u0435 (\u043F\u043E \u0441\u0440\u0430\u0432\u043D\u0435\u043D\u0438\u044E \u0441 \u0437\u0435\u043C\u043D\u044B\u043C) \u0438 \u0432 2,6 \u0440\u0430\u0437\u0430 \u0431\u043E\u043B\u0435\u0435 \u0441\u043B\u0430\u0431\u043E\u0435 \u043F\u043E \u0441\u0440\u0430\u0432\u043D\u0435\u043D\u0438\u044E \u0441 \u0437\u0435\u043C\u043D\u044B\u043C \u043F\u0440\u0438\u0442\u044F\u0436\u0435\u043D\u0438\u0435, \u0432\u0441\u043B\u0435\u0434\u0441\u0442\u0432\u0438\u0435 \u0447\u0435\u0433\u043E \u0441\u043E\u043B\u043D\u0435\u0447\u043D\u044B\u0439 \u0432\u0435\u0442\u0435\u0440 \u0432\u044B\u0437\u044B\u0432\u0430\u0435\u0442 \u0434\u0438\u0441\u0441\u0438\u043F\u0430\u0446\u0438\u044E \u0430\u0442\u043C\u043E\u0441\u0444\u0435\u0440\u043D\u044B\u0445 \u0433\u0430\u0437\u043E\u0432 \u0432 \u043A\u043E\u0441\u043C\u043E\u0441 \u0441\u043E \u0441\u043A\u043E\u0440\u043E\u0441\u0442\u044C\u044E \u043E\u043A\u043E\u043B\u043E 100 \u0433\u0440\u0430\u043C\u043C\u043E\u0432 \u0432 \u0441\u0435\u043A\u0443\u043D\u0434\u0443 (\u043C\u0435\u043D\u0435\u0435 9 \u0442\u043E\u043D\u043D \u0432 \u0434\u0435\u043D\u044C), \u0432 \u0437\u0430\u0432\u0438\u0441\u0438\u043C\u043E\u0441\u0442\u0438 \u043E\u0442 \u0442\u0435\u043A\u0443\u0449\u0435\u0439 \u0441\u043E\u043B\u043D\u0435\u0447\u043D\u043E\u0439 \u0430\u043A\u0442\u0438\u0432\u043D\u043E\u0441\u0442\u0438 \u0438 \u0440\u0430\u0441\u0441\u0442\u043E\u044F\u043D\u0438\u044F \u043E\u0442 \u0421\u043E\u043B\u043D\u0446\u0430. \u041D\u0435\u0441\u043C\u043E\u0442\u0440\u044F \u043D\u0430 \u0432\u044B\u0441\u043E\u043A\u0443\u044E \u0440\u0430\u0437\u0440\u0435\u0436\u0435\u043D\u043D\u043E\u0441\u0442\u044C, \u0432 \u0430\u0442\u043C\u043E\u0441\u0444\u0435\u0440\u0435 \u041C\u0430\u0440\u0441\u0430 \u0432\u043E\u0437\u043C\u043E\u0436\u043D\u044B \u0438 \u043E\u0441\u0443\u0449\u0435\u0441\u0442\u0432\u043B\u0435\u043D\u044B \u043F\u043E\u043B\u0451\u0442\u044B \u0438\u0441\u043A\u0443\u0441\u0441\u0442\u0432\u0435\u043D\u043D\u044B\u0445 \u0430\u043F\u043F\u0430\u0440\u0430\u0442\u043E\u0432."@ru ,
"The atmosphere of Mars is the layer of gases surrounding Mars. It is primarily composed of carbon dioxide (95%), molecular nitrogen (2.8%), and argon (2%). It also contains trace levels of water vapor, oxygen, carbon monoxide, hydrogen, and noble gases. The atmosphere of Mars is much thinner than Earth's. The average surface pressure is only about 610 pascals (0.088 psi) which is less than 1% of the Earth's value. The currently thin Martian atmosphere prohibits the existence of liquid water on the surface of Mars, but many studies suggest that the Martian atmosphere was much thicker in the past. The higher density during spring and fall is reduced by 25% during the winter when carbon dioxide partly freezes at the pole caps. The highest atmospheric density on Mars is equal to the density found 35 km (22 mi) above the Earth's surface and is \u22480.020 kg/m3. The atmosphere of Mars has been losing mass to space since the planet's core slowed down, and the leakage of gases still continues today. The atmosphere of Mars is colder than Earth's. Owing to the larger distance from the Sun, Mars receives less solar energy and has a lower effective temperature, which is about 210 K (\u221263 \u00B0C; \u221282 \u00B0F). The average surface emission temperature of Mars is just 215 K (\u221258 \u00B0C; \u221273 \u00B0F), which is comparable to inland Antarctica. The weaker greenhouse effect in the Martian atmosphere (5 \u00B0C (9.0 \u00B0F), versus 33 \u00B0C (59 \u00B0F) on Earth) can be explained by the low abundance of other greenhouse gases. The daily range of temperature in the lower atmosphere is huge due to the low thermal inertia; it can range from \u221275 \u00B0C (\u2212103 \u00B0F) to near 0 \u00B0C (32 \u00B0F) near the surface in some regions. The temperature of the upper part of the Martian atmosphere is also significantly lower than Earth's because of the absence of stratospheric ozone and the radiative cooling effect of carbon dioxide at higher altitudes. Dust devils and dust storms are prevalent on Mars, which are sometimes observable by telescopes from Earth, and in 2018 even with the naked eye as a change in colour and brightness of the planet. Planet-encircling dust storms (global dust storms) occur on average every 5.5 Earth years (every 3 Martian years) on Mars and can threaten the operation of Mars rovers. However, the mechanism responsible for the development of large dust storms is still not well understood. It has been suggested to be loosely related to gravitational influence of both moons, somewhat similar to the creation of tides on Earth. The Martian atmosphere is an oxidizing atmosphere. The photochemical reactions in the atmosphere tend to oxidize the organic species and turn them into carbon dioxide or carbon monoxide. Although the most sensitive methane probe on the recently launched ExoMars Trace Gas Orbiter failed to find methane in the atmosphere over the whole of Mars, several previous missions and ground-based telescope detected unexpected levels of methane in the Martian atmosphere, which may even be a biosignature for life on Mars. However, the interpretation of the measurements is still highly controversial and lacks a scientific consensus."@en ,
"\u0397 \u0391\u03C4\u03BC\u03CC\u03C3\u03C6\u03B1\u03B9\u03C1\u03B1 \u03C4\u03BF\u03C5 \u0386\u03C1\u03B7 \u03B1\u03C0\u03BF\u03C4\u03B5\u03BB\u03B5\u03AF\u03C4\u03B1\u03B9 \u03BA\u03C5\u03C1\u03AF\u03C9\u03C2 \u03B1\u03C0\u03CC \u03B4\u03B9\u03BF\u03BE\u03B5\u03AF\u03B4\u03B9\u03BF \u03C4\u03BF\u03C5 \u03AC\u03BD\u03B8\u03C1\u03B1\u03BA\u03B1. \u0397 \u03B1\u03C4\u03BC\u03BF\u03C3\u03C6\u03B1\u03B9\u03C1\u03B9\u03BA\u03AE \u03C0\u03AF\u03B5\u03C3\u03B7 \u03C3\u03C4\u03B7\u03BD \u03B5\u03C0\u03B9\u03C6\u03AC\u03BD\u03B5\u03B9\u03B1 \u03B5\u03AF\u03BD\u03B1\u03B9 \u03BA\u03B1\u03C4\u03AC \u03BC\u03AD\u03C3\u03BF \u03CC\u03C1\u03BF 600 \u03C0\u03B1\u03C3\u03BA\u03AC\u03BB \u03C0\u03BF\u03C5 \u03B9\u03C3\u03BF\u03CD\u03C4\u03B1\u03B9 \u03BC\u03B5 \u03C4\u03BF 0,6% \u03C4\u03B7\u03C2 \u03BC\u03AD\u03C3\u03B7\u03C2 \u0393\u03AE\u03B9\u03BD\u03B7\u03C2 \u03C0\u03AF\u03B5\u03C3\u03B7\u03C2 \u03C3\u03C4\u03BF \u03B5\u03C0\u03AF\u03C0\u03B5\u03B4\u03BF \u03C4\u03B7\u03C2 \u03B8\u03AC\u03BB\u03B1\u03C3\u03C3\u03B1\u03C2 \u03C4\u03C9\u03BD 101,3 \u03C7\u03B9\u03BB\u03B9\u03BF\u03C0\u03B1\u03C3\u03BA\u03AC\u03BB. \u0397 \u03C0\u03AF\u03B5\u03C3\u03B7 \u03BA\u03C5\u03BC\u03B1\u03AF\u03BD\u03B5\u03C4\u03B1\u03B9 \u03B1\u03C0\u03CC \u03C4\u03B7\u03BD \u03B5\u03BB\u03AC\u03C7\u03B9\u03C3\u03C4\u03B7 30 \u03C0\u03B1\u03C3\u03BA\u03AC\u03BB \u03C3\u03C4\u03B7\u03BD \u03BA\u03BF\u03C1\u03C5\u03C6\u03AE \u03C4\u03BF\u03C5 \u038C\u03C1\u03BF\u03C5\u03C2 \u038C\u03BB\u03C5\u03BC\u03C0\u03BF\u03C2 \u03C3\u03B5 \u03AD\u03C9\u03C2 \u03C0\u03AC\u03BD\u03C9 \u03B1\u03C0\u03CC 1.155 \u03C0\u03B1\u03C3\u03BA\u03AC\u03BB \u03C3\u03C4\u03B1 \u03B2\u03AC\u03B8\u03B7 \u03C4\u03B7\u03C2 \u0395\u03BB\u03BB\u03AC\u03C2 \u03A0\u03BB\u03B1\u03BD\u03AF\u03C4\u03B9\u03B1. \u0391\u03C5\u03C4\u03AE \u03B7 \u03C0\u03AF\u03B5\u03C3\u03B7 \u03B5\u03AF\u03BD\u03B1\u03B9 \u03C0\u03BF\u03BB\u03CD \u03C7\u03B1\u03BC\u03B7\u03BB\u03CC\u03C4\u03B5\u03C1\u03B7 \u03C4\u03B7\u03C2 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\u03BA\u03B1\u03C4\u03B1\u03B9\u03B3\u03AF\u03B4\u03B1\u03C2 \u03C3\u03C4\u03B1 \u03BC\u03AD\u03C3\u03B1 \u03C4\u03BF\u03C5 \u03BC\u03AE\u03BD\u03B1. \u03A4\u03B7\u03BD 1\u03B7 \u0399\u03BF\u03C5\u03BD\u03AF\u03BF\u03C5 2018, \u03BF\u03B9 \u03B5\u03C0\u03B9\u03C3\u03C4\u03AE\u03BC\u03BF\u03BD\u03B5\u03C2 \u03C4\u03BF\u03C5 NASA \u03B1\u03BD\u03AF\u03C7\u03BD\u03B5\u03C5\u03C3\u03B1\u03BD \u03AF\u03C7\u03BD\u03B7 \u03B1\u03BC\u03BC\u03BF\u03B8\u03CD\u03B5\u03BB\u03BB\u03B1\u03C2 \u03C3\u03C4\u03BF\u03BD \u0386\u03C1\u03B7, \u03C0\u03BF\u03C5 \u03AF\u03C3\u03C9\u03C2 \u03B4\u03C5\u03C3\u03C7\u03B5\u03C1\u03AC\u03BD\u03B5\u03B9 \u03C4\u03BF \u03C4\u03C1\u03BF\u03C6\u03BF\u03B4\u03BF\u03CD\u03BC\u03B5\u03BD\u03BF \u03BC\u03B5 \u03B7\u03BB\u03B9\u03B1\u03BA\u03AE \u03B5\u03BD\u03AD\u03C1\u03B3\u03B5\u03B9\u03B1 \u03C1\u03CC\u03B2\u03B5\u03C1 \u0395\u03C5\u03BA\u03B1\u03B9\u03C1\u03AF\u03B1, \u03B5\u03BC\u03C0\u03BF\u03B4\u03AF\u03B6\u03BF\u03BD\u03C4\u03B1\u03C2 \u03C4\u03B7 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\u0391\u03BC\u03B5\u03C1\u03B9\u03BA\u03AE \u03BA\u03B1\u03B9 \u03B7 \u03A1\u03C9\u03C3\u03AF\u03B1 \u03BC\u03B1\u03B6\u03AF (1/4 \u03C4\u03BF\u03C5 \u03C0\u03BB\u03B1\u03BD\u03AE\u03C4\u03B7). \u03A4\u03B7\u03BD 13 \u0399\u03BF\u03C5\u03BD\u03AF\u03BF\u03C5, \u03C4\u03BF \u03C1\u03CC\u03B2\u03B5\u03C1 \u0395\u03C5\u03BA\u03B1\u03B9\u03C1\u03AF\u03B1 \u03B1\u03BD\u03B1\u03C6\u03AD\u03C1\u03B8\u03B7\u03BA\u03B5 \u03CC\u03C4\u03B9 \u03B1\u03BD\u03C4\u03B9\u03BC\u03B5\u03C4\u03C9\u03C0\u03AF\u03B6\u03B5\u03B9 \u03C3\u03BF\u03B2\u03B1\u03C1\u03AC \u03C0\u03C1\u03BF\u03B2\u03BB\u03AE\u03BC\u03B1\u03C4\u03B1 \u03B5\u03C0\u03B9\u03BA\u03BF\u03B9\u03BD\u03C9\u03BD\u03AF\u03B1\u03C2 \u03BB\u03CC\u03B3\u03C9 \u03C4\u03B7\u03C2 \u03B1\u03BC\u03BC\u03BF\u03B8\u03CD\u03B5\u03BB\u03B1\u03C2 \u03C3\u03B5 \u03C4\u03B7\u03BB\u03B5\u03B4\u03B9\u03AC\u03C3\u03BA\u03B5\u03C8\u03B7. \u03C4\u03BF\u03BD \u0399\u03BF\u03CD\u03BB\u03B9\u03BF 2018, \u03BF\u03B9 \u03B5\u03C1\u03B5\u03C5\u03BD\u03B7\u03C4\u03AD\u03C2 \u03B4\u03AE\u03BB\u03C9\u03C3\u03B1\u03BD \u03CC\u03C4\u03B9 \u03B7 \u03BC\u03B5\u03B3\u03B1\u03BB\u03CD\u03C4\u03B5\u03C1\u03B7 \u03B5\u03BD\u03B9\u03B1\u03AF\u03B1 \u03C0\u03B7\u03B3\u03AE \u03C7\u03CE\u03BC\u03B1\u03C4\u03BF\u03C2 \u03C3\u03C4\u03BF\u03BD \u03C0\u03BB\u03B1\u03BD\u03AE\u03C4\u03B7 \u0386\u03C1\u03B7 \u03C0\u03C1\u03BF\u03AD\u03C1\u03C7\u03B5\u03C4\u03B1\u03B9 \u03B1\u03C0\u03CC \u03C4\u03BF \u03A3\u03C7\u03B7\u03BC\u03B1\u03C4\u03B9\u03C3\u03BC\u03CC \u039C\u03AD\u03B4\u03BF\u03C5\u03C3\u03B1 \u03A6\u03CC\u03C3\u03C3\u03B1. \u03A4\u03B7\u03BD 7 \u0399\u03BF\u03C5\u03BD\u03AF\u03BF\u03C5 2018, \u03C4\u03BF NASA \u03B1\u03BD\u03B1\u03BA\u03BF\u03AF\u03BD\u03C9\u03C3\u03B5 \u03C0\u03B5\u03C1\u03B9\u03BF\u03B4\u03B9\u03BA\u03AE, \u03B5\u03C0\u03BF\u03C7\u03B9\u03B1\u03BA\u03AE \u03BC\u03B5\u03C4\u03B1\u03B2\u03BF\u03BB\u03AE \u03C3\u03C4\u03B1 \u03B5\u03C0\u03AF\u03C0\u03B5\u03B4\u03B1 \u03B1\u03C4\u03BC\u03BF\u03C3\u03C6\u03B1\u03B9\u03C1\u03B9\u03BA\u03BF\u03CD \u03BC\u03B5\u03B8\u03B1\u03BD\u03AF\u03BF\u03C5."@el ;
dbo:wikiPageWikiLink dbr:Zirconia ,
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,
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,
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,
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dbr:Carbon-13 ,
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dbr:Medusae_Fossae_Formation ,
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dbr:Mars ,
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,
dbr:Astrobiology ,
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dbr:Seasonal_flows_on_warm_Martian_slopes ,
dbr:Extreme_ultraviolet ,
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dbc:Mars ,
,
dbr:Pyrite ,
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dbr:Life_on_Mars ,
dbr:High_Resolution_Imaging_Science_Experiment ,
dbr:Carbon_monoxide ,
,
dbr:Opportunity_mission_timeline ,
dbr:NASA_Goddard_Space_Flight_Center ,
dbr:Robert_Zubrin ,
dbr:Carbon_dioxide ,
dbr:Olivine ,
dbr:Turbopause ,
dbr:Herschel_Space_Observatory ,
dbr:In_situ_resource_utilization ,
,
,
,
,
,
dbr:Global_equivalent_layer ,
,
,
,
dbc:Planetary_atmospheres_of_the_Solar_System ,
,
,
dbr:Electrolysis ,
,
,
dbc:Atmosphere_of_Mars ,
dbr:Late_Heavy_Bombardment ,
dbr:Design_Reference_Mission ,
,
,
dbr:Effective_temperature ,
dbr:Thermosphere ,
dbr:Hydroxyl_radical ,
dbr:Spirit_rover ,
dbr:Crustal_magnetism ,
dbr:Climate_of_Mars ,
dbr:Terraforming_of_Mars ,
dbr:William_Rutter_Dawes ,
dbr:Atmospheric_escape ,
dbr:Arsia_Mons ,
,
dbr:Ozone_layer ,
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dbr:Methane ,
dbr:Atmosphere_of_Jupiter ,
dbr:Philosophical_Transactions_of_the_Royal_Society ,
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dbr:Scale_height ,
dbr:Dust_devil ,
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,
dbr:Rocket_fuel ,
dbr:Martian_soil ,
dbr:MAVEN ,
dbr:Noble_gas ,
dbr:Lick_Observatory ,
,
dbr:Atmospheric_pressure ,
dbr:Atomic_oxygen ,
dbr:Faint_young_Sun_paradox ,
,
dbr:Ozone ,
dbr:William_Herschel ,
,
dbr:Audio_frequency ,
dbr:InSight ,
dbr:Aerobraking ,
dbr:Hydrogen ,
dbr:Greenhouse_effect ,
dbr:Goddard_Space_Flight_Center ,
dbr:Mars_MetNet ,
dbr:Biosignature ,
dbr:Interplanetary_contamination ,
dbr:Dust_storm .
@prefix dbp: .
@prefix dbt: .
dbr:Atmosphere_of_Mars dbp:wikiPageUsesTemplate dbt:Sub ,
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dbt:Merge_from ,
dbt:Cite_web ,
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dbt:Mars ,
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dbo:wikiPageExternalLink ,
.
@prefix ns12: .
dbr:Atmosphere_of_Mars dbo:wikiPageExternalLink ns12:methane_mars_atmosphere_frascati ,
,
,
.
@prefix ns13: .
dbr:Atmosphere_of_Mars dbo:wikiPageExternalLink ns13:methane_mars_atmosphere_frascati ,
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"2012-11-18"^^xsd:date ,
dbr:Argon ,
"2018-06-06"^^xsd:date ,
"Molecular nitrogen"@en ,
"2012-11-25"^^xsd:date ,
dbr:Carbon_dioxide ;
owl:sameAs ,
,
,
,
,
,
,
.
@prefix dbpedia-pl: .
dbr:Atmosphere_of_Mars owl:sameAs dbpedia-pl:Atmosfera_Marsa .
@prefix dbpedia-it: .
dbr:Atmosphere_of_Mars owl:sameAs dbpedia-it:Atmosfera_di_Marte ,
,
dbr:Atmosphere_of_Mars ,
,
,
,
,
,
.
@prefix dbpedia-id: .
dbr:Atmosphere_of_Mars owl:sameAs dbpedia-id:Atmosfer_Mars ,
,
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dbr:Atmosphere_of_Mars owl:sameAs dbpedia-simple:Atmosphere_of_Mars ,
,
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,
,
,
,
.
@prefix wikidata: .
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,
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dbr:Atmosphere_of_Mars owl:sameAs yago-res:Atmosphere_of_Mars ,
,
,
,
,
,
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@prefix dbpedia-ca: .
dbr:Atmosphere_of_Mars owl:sameAs dbpedia-ca:Atmosfera_de_Mart .
@prefix dbpedia-pt: .
dbr:Atmosphere_of_Mars owl:sameAs dbpedia-pt:Atmosfera_de_Marte .
@prefix gold: .
dbr:Atmosphere_of_Mars gold:hypernym dbr:Layer .
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dbr:Atmosphere_of_Mars prov:wasDerivedFrom ;
foaf:isPrimaryTopicOf wikipedia-en:Atmosphere_of_Mars ;
dbp:captionAlign "center"@en ;
dbp:header "Dust storms on Mars"@en ,
"Principal components of the Martian atmosphere"@en ;
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dbp:footer "Locations of lander and rovers are noted"@en .
@prefix dbd: .
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18 ,
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dbr:Viking_lander_biological_experiments dbo:wikiPageWikiLink dbr:Atmosphere_of_Mars .
dbo:wikiPageWikiLink dbr:Atmosphere_of_Mars .
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