To install click the Add extension button. That's it.

The source code for the WIKI 2 extension is being checked by specialists of the Mozilla Foundation, Google, and Apple. You could also do it yourself at any point in time.

4,5
Kelly Slayton
Congratulations on this excellent venture… what a great idea!
Alexander Grigorievskiy
I use WIKI 2 every day and almost forgot how the original Wikipedia looks like.
What we do. Every page goes through several hundred of perfecting techniques; in live mode. Quite the same Wikipedia. Just better.
.
Leo
Newton
Brights
Milds

From Wikipedia, the free encyclopedia

Crater characteristics
PlanetVenus
Coordinates12°30′N 57°12′E / 12.5°N 57.2°E / 12.5; 57.2
QuadrangleSedna Planitia
Diameter270 km
EponymMargaret Mead

Mead is an impact crater on Venus named in honor of the cultural anthropologist Margaret Mead.

Mead crater is the largest impact crater on Venus, with a diameter of 280 km (174 miles).[1] The crater has an inner and an outer ring and a small ejecta blanket surrounding the outer ring. Mead crater is relatively shallow (likely due to viscous relaxation[2] and infilling) and crater floor looks very similar in morphology to the surrounding plain.

Mead is classified as a multi-ring crater with its innermost, concentric scarp being interpreted as the rim of the original crater cavity. No inner peak-ring of mountain massifs is observed on Mead. The presence of hummocky, radar-bright crater ejecta crossing the radar-dark floor terrace and adjacent outer rim scarp suggests that the floor terrace is probably a giant rotated block that is concentric to, but lies outside, the original crater cavity. The flat, somewhat brighter inner floor of Mead is interpreted to result from considerable infilling of the original crater cavity by impact melt and/or by volcanic lavas. To the southeast of the crater rim, emplacement of hummocky ejecta appears to have been impeded by the topography of preexisting ridges, thus suggesting a very low ground-hugging mode of deposition for this material.[3]

References

  1. ^ Herrick; Sharpton (1996). "Geologic history of the Mead impact basin, Venus". Geology. 24 (1): 11–14. Bibcode:1996Geo....24...11H. doi:10.1130/0091-7613(1996)024<0011:GHOTMI>2.3.CO;2.
  2. ^ Karimi; Dombard (2017). "Studying lower crustal flow beneath Mead basin: Implications for the thermal history and rheology of Venus". Icarus. 282: 34–39. Bibcode:2017Icar..282...34K. doi:10.1016/j.icarus.2016.09.015.
  3. ^ Catalog Page for PIA00148

External links


This page was last edited on 24 February 2022, at 04:24
Basis of this page is in Wikipedia. Text is available under the CC BY-SA 3.0 Unported License. Non-text media are available under their specified licenses. Wikipedia® is a registered trademark of the Wikimedia Foundation, Inc. WIKI 2 is an independent company and has no affiliation with Wikimedia Foundation.