List of largest rifts, canyons and valleys in the Solar System

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Following are the longest, widest, and deepest rifts and valleys in various worlds of the Solar System.

Contents

List

WorldRift/ValleyLengthMax. widthMax. depthNotes
Venus Baltis Vallis A lava channel
Earth Atlantic Ocean Length taken to be that of the Mid-Atlantic Ridge. (The ridge also has a secondary rift valley running its length.) The width is an average taken along the spreading ridges (Georgia–Senegal, Brazil – Bight of Benin, etc.). The greatest depth is the Romanche Trench. (The Puerto Rico Trench is not part of the rift system.)
Great Rift Valley Width and depth are those of the Red Sea Rift, discounting continental shelves < 200 m deep. (These may not be the extremes of the whole rift system.) Length of the Red Sea section 2,250 km (1,400 mi).
Canadian Arctic Rift System A northwesterly continuation of the Mid-Atlantic Ridge.
West Antarctic Rift System
Midcontinent Rift System Width & depth Isle RoyaleKeweenaw Peninsula; may not be widest point.
Grand Canyon
Colca Canyon
Cotahuasi Canyon
Moon Vallis Snellius Width assumed to be approx. that of Vallis Rheita
Mars Valles Marineris
Kasei Valles
Tiu Valles
Ares Vallis
Vesta equatorial channelsLength may be as much as the 1790-km circumference of Vesta
Divalia Fossa ≈ 22 kmCompression fracture from Rheasilvia
Saturnalia Fossa ≈ 39 km365 km visible at one point; rest in northern shadow.
Compression fracture from
Veneneia.
Europa  ? ?Moon of Jupiter
Tethys Ithaca Chasma Moon of Saturn. Ithaca span approx. 75% the circumference of the Moon.
Charon Argo Chasma 700 km (430 mi)?9 km (6 mi)Moon of Pluto. Part of a belt of grabens that span most of the circumference of the moon. Only a section was seen on limb of Charon and so exact length uncertain. Not yet officially named. [1]
Caleuche Chasma 400 km (250 mi) ?13 km (8.1 mi)Depth estimated in the range 10–16 km (6.2–9.9 mi). [2]
Miranda tectonic grabens20 km10-20 kmExtensive series of grabens and scarps that cover most of the moon.
Titania Messina Chasma 1492 km (900 mi)50 km (30 mi)2-5 kmGeologically young belt of grabens that cut through craters. Bright, icy material exposed on canyon walls.
Pluto Sleipnir Fossa 580 km (360 mi)5-10 km≈3 km (2 mi)One of the six extensional "spider" fractures, cuts through Tartarus Dorsa . Not yet officially named.
Lowell Regio canyons≈200 km (120 mi)75 km (45 mi)≈3-4 kmA series of canyons found very close to the north pole. Not yet officially named.

See also

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References

  1. Keeter, Bill (2016-06-23). "A 'Super Grand Canyon' on Pluto's Moon Charon". NASA. Retrieved 2017-08-14.
  2. Schenk, Paul Michael; Beyer, Ross A.; McKinnon, William B.; Moore, Jeffrey M.; Spencer, John R.; White, Oliver L.; Singer, Kelsi; Umurhan, Orkan M.; Nimmo, Francis; Lauer, Tod R.; Grundy, William M.; Robbins, Stuart; Stern, S. Alan; Weaver, Harold A.; Young, Leslie A.; Smith, K. Ennico; Olkin, Cathy (2018). "Breaking up is hard to do: Global cartography and topography of Pluto's mid-sized icy Moon Charon from New Horizons". Icarus. 315: 124–145. Bibcode:2018Icar..315..124S. doi:10.1016/j.icarus.2018.06.010. ISSN   0019-1035. S2CID   125833113.