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1 References  





2 See also  














Labeatis Fossae: Difference between revisions






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|naming=a previously named feature at 30N, 75W

|naming=a previously named feature at 30N, 75W

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'''Labeatis Fossae''' is large trough in the [[Lunae Palus quadrangle]] of [[Mars]], located at 25.5° N and 84.1° W. It is 1,560.0&nbsp;km long and was named after a previously named feature at 30N, 75W.<ref>http://planetarynames.wr.usgs.gov</ref>

'''Labeatis Fossae''' is a large trough in the [[Lunae Palus quadrangle]] of [[Mars]], located at 25.5° N and 84.1° W. It is 1,560.0&nbsp;km long and was named after a previously named feature at 30N, 75W.<ref>http://planetarynames.wr.usgs.gov</ref>



The term "fossae" is used to indicate large troughs when using geographical terminology related to Mars. Troughs, sometimes also called [[graben]]s, form when the crust is stretched until it breaks, which forms two breaks with a middle section moving down, leaving steep cliffs along the sides. Sometimes, a line of pits form as materials collapse into a void that forms from the stretching.<ref>[http://www.msss.com/mars_images/moc/2004/01/29/index.html Mars Global Surveyor MOC2-620 Release]</ref>

The term "fossae" is used to indicate large troughs when using geographical terminology related to Mars. Troughs, sometimes also called [[graben]]s, form when the crust is stretched until it breaks, which forms two breaks with a middle section moving down, leaving steep cliffs along the sides. Sometimes, a line of pits form as materials collapse into a void that forms from the stretching.<ref>[http://www.msss.com/mars_images/moc/2004/01/29/index.html Mars Global Surveyor MOC2-620 Release]</ref>


Revision as of 09:44, 1 July 2018

Template:Infobox feature on Mars Labeatis Fossae is a large trough in the Lunae Palus quadrangleofMars, located at 25.5° N and 84.1° W. It is 1,560.0 km long and was named after a previously named feature at 30N, 75W.[1]

The term "fossae" is used to indicate large troughs when using geographical terminology related to Mars. Troughs, sometimes also called grabens, form when the crust is stretched until it breaks, which forms two breaks with a middle section moving down, leaving steep cliffs along the sides. Sometimes, a line of pits form as materials collapse into a void that forms from the stretching.[2]


References

See also


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    This page was last edited on 1 July 2018, at 09:44 (UTC).

    This version of the page has been revised. Besides normal editing, the reason for revision may have been that this version contains factual inaccuracies, vandalism, or material not compatible with the Creative Commons Attribution-ShareAlike License.



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