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	<id>https://enciklopedija.cc/index.php?action=history&amp;feed=atom&amp;title=Messina_Chasmata</id>
	<title>Messina Chasmata - Povijest promjena</title>
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	<updated>2026-09-01T00:07:07Z</updated>
	<subtitle>Povijest promjena ove stranice na wikiju</subtitle>
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	<entry>
		<id>https://enciklopedija.cc/index.php?title=Messina_Chasmata&amp;diff=788753&amp;oldid=prev</id>
		<title>Bot1: Automatski uvoz s hrwiki (zadnjih 72 sati)</title>
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		<updated>2026-08-24T09:59:45Z</updated>

		<summary type="html">&lt;p&gt;Automatski uvoz s hrwiki (zadnjih 72 sati)&lt;/p&gt;
&lt;p&gt;&lt;b&gt;Nova stranica&lt;/b&gt;&lt;/p&gt;&lt;div&gt;{{značajka na astronomskom objektu&lt;br /&gt;
|name = Messina Chasmata&lt;br /&gt;
|image = PIA00039 Titania.jpg&lt;br /&gt;
|caption = Messina Chasmata je blizu središta ove slike Titanije snimljene letjelicom &amp;#039;&amp;#039;[[Voyager 2]]&amp;#039;&amp;#039;.&lt;br /&gt;
|type = Chasm system&lt;br /&gt;
|location = Titania&lt;br /&gt;
|length = ~{{convert|1492|km|mi|abbr=on}}&amp;lt;ref name=&amp;quot;gpn&amp;quot;/&amp;gt;{{efn|Duljina je označena pod &amp;quot;diameter&amp;quot; u GPN bazi podataka.}}&lt;br /&gt;
|depth = &lt;br /&gt;
|coordinates = {{coord|33.30|S|25.00|W|globe:titania_type:landmark|display=inline,title}}&lt;br /&gt;
|coordinates_footnotes = &amp;lt;ref name=&amp;quot;gpn&amp;quot;/&amp;gt;&lt;br /&gt;
|discoverer = &amp;#039;&amp;#039;[[Voyager 2]]&amp;#039;&amp;#039;&lt;br /&gt;
|naming =  &lt;br /&gt;
|eponym = lokacija u [[William Shakespeare|Shakespeareovoj]] komediji [[Mnogo vike ni za što]].&amp;lt;ref name=&amp;quot;gpn&amp;quot;/&amp;gt;&lt;br /&gt;
}}&lt;br /&gt;
[[slika:Titania (moon) labeled.jpg|mini|lijevo|300px|Slika Titanije s oznakama, Messina Chasmata je na sredini ruba desno]]&lt;br /&gt;
&amp;#039;&amp;#039;&amp;#039;Messina Chasmata&amp;#039;&amp;#039;&amp;#039; najveći je [[Klanac|kanjon]] na površini Uranovog mjeseca [[Titanija (mjesec)|Titanije]].&lt;br /&gt;
&lt;br /&gt;
Ovaj 1492 km dug kanjon uključuje dva [[Rasjed|normalna rasjeda]] koji se protežu u smjeru sjeverozapad-jugoistok, a koji su omeđivali spušteni blok kore tvoreći strukturu nazvanu [[tektonski rov]].&amp;lt;ref name=&amp;quot;Smith Soderblom et al. 1986&amp;quot; /&amp;gt; Tektonski rov presijeca udarne kratere, što vjerojatno znači da je nastao u relativno kasnoj fazi evolucije satelita,&amp;lt;ref name=&amp;quot;Plescia 1987&amp;quot;/&amp;gt; kada se unutrašnjost Titanije proširila i njezina ledena kora je kao rezultat toga napukla.&amp;lt;ref name=&amp;quot;Croft 1989&amp;quot; /&amp;gt; Messina Chasmata ima samo nekoliko superponiranih kratera, što također implicira da je relativno mlada.&lt;br /&gt;
&lt;br /&gt;
Kanjon je prvi put snimio &amp;#039;&amp;#039;[[Voyager 2]]&amp;#039;&amp;#039; u siječnju 1986.&amp;lt;ref name=&amp;quot;Smith Soderblom et al. 1986&amp;quot; /&amp;gt;&lt;br /&gt;
&lt;br /&gt;
== Ime ==&lt;br /&gt;
Kanjon je nazvan po lokaciji u komediji [[William Shakespeare|Williama Shakespearea]] [[Mnogo vike ni za što]].&amp;lt;ref name=&amp;quot;gpn&amp;quot;/&amp;gt;&lt;br /&gt;
&lt;br /&gt;
== Bilješke ==&lt;br /&gt;
{{Bilješke}}&lt;br /&gt;
&lt;br /&gt;
== Izvori ==&lt;br /&gt;
&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;ref name=&amp;quot;Croft 1989&amp;quot;&amp;gt;&lt;br /&gt;
{{cite conference&lt;br /&gt;
| last = Croft&lt;br /&gt;
| first = S.K.&lt;br /&gt;
|date=March 1989&lt;br /&gt;
| title = New Geologic Maps of the Uranian Satellites Titania, Oberon, Umbriel and Miranda&lt;br /&gt;
| publisher = Lunar and Planetary Sciences Institute, Houston&lt;br /&gt;
| work = Proceeding of Lunar and Planetary Sciences&lt;br /&gt;
| volume = 20&lt;br /&gt;
| page = 205C&lt;br /&gt;
| bibcode = 1989LPI....20..205C&lt;br /&gt;
}}&lt;br /&gt;
&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;ref name=&amp;quot;Smith Soderblom et al. 1986&amp;quot;&amp;gt;&lt;br /&gt;
{{cite journal&lt;br /&gt;
 | last1 = Smith| first1 = B. A.| last2 = Soderblom| first2 = L. A.| last3 = Beebe| first3 = A.&lt;br /&gt;
 | last4 = Bliss| first4 = D.| last5 = Boyce| first5 = J. M.| last6 = Brahic| first6 = A.&lt;br /&gt;
 | last7 = Briggs| first7 = G. A.| last8 = Brown| first8 = R. H.| last9 = Collins| first9 = S. A.&lt;br /&gt;
 | date = 1986-07-04&lt;br /&gt;
 | title = Voyager 2 in the Uranian System: Imaging Science Results&lt;br /&gt;
 | url = https://zenodo.org/record/1230972&lt;br /&gt;
 | journal = Science| volume = 233| issue = 4759| pages = 43–64&lt;br /&gt;
 | pmid = 17812889| bibcode = 1986Sci...233...43S| s2cid = 5895824&lt;br /&gt;
 | doi = 10.1126/science.233.4759.43&lt;br /&gt;
 | ref = {{sfnRef|Smith Soderblom et al.|1986}}&lt;br /&gt;
}}&lt;br /&gt;
&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;ref name=&amp;quot;Plescia 1987&amp;quot;&amp;gt;&lt;br /&gt;
{{cite journal&lt;br /&gt;
 | doi = 10.1029/JA092iA13p14918&lt;br /&gt;
 | last = Plescia| first = J. B.&lt;br /&gt;
 | date = 1987-12-30&lt;br /&gt;
 | title = Cratering history of the Uranian satellites: Umbriel, Titania and Oberon&lt;br /&gt;
 | journal = Journal of Geophysical Research&lt;br /&gt;
 | issn = 0148-0227| volume = 92| issue = A13&lt;br /&gt;
 | pages = 14,918–14,932&lt;br /&gt;
 | bibcode = 1987JGR....9214918P&lt;br /&gt;
}}&lt;br /&gt;
&amp;lt;/ref&amp;gt;&lt;br /&gt;
}}&lt;br /&gt;
&lt;br /&gt;
[[Kategorija:Kanjoni]]&lt;br /&gt;
[[Kategorija:Površinske značajke Titanije]]&lt;/div&gt;</summary>
		<author><name>Bot1</name></author>
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