Serpentine Ridge

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Serpentine Ridge

(informal name)

Lat: 25°N, Long: 25°E, Length: 500 km, Height: km, [/R%C3%BCkl%2024 Rükl: 24]

Table of Contents

[#Serpentine Ridge Serpentine Ridge]
[#Serpentine Ridge-Images Images]
[#Serpentine Ridge-Maps Maps]
[#Serpentine Ridge-Description Description]
[#Serpentine Ridge-Description: Elger Description: Elger]
[#Serpentine Ridge-Additional Information Additional Information]
[#Serpentine Ridge-Nomenclature Nomenclature]
[#Serpentine Ridge-LPOD Articles LPOD Articles]
[#Serpentine Ridge-Bibliography Bibliography]
external image normal_Serpentine_Ridge_CLA-C4_LTVT.jpg
Consolidated Lunar Atlas plate C4 The "Serpentine Ridge" is the long series of mare ridges extending from "A" to "B".

Images

LPOD Photo Gallery Lunar Orbiter Images Apollo Images

  • The Serpentine Ridge ([/Dorsa%20Smirnov Dorsa Smirnov]) was frequently photographed during the missions of Apollo 15 and Apollo 17. - DannyCaes DannyCaes Apr 30, 2010


Maps

([/LAC%20zone LAC zone] 42B3) LAC map Geologic map LM map

Description


Description: Elger

([/IAU%20Directions IAU Directions]) [/Mare%20Serenitatis Mare Serenitatis] ... includes besides one of the longest and loftiest (ridges) on the moon's visible surface -- the great serpentine ridge, first drawn and described nearly a hundred years ago by the famous selenographer, Schroter of Lilienthal. Originating at a little crater under the north-west wall of great ring-plain [/Posidonius Posidonius], it follows a winding course across the Mare toward the south, throwing out many minor branches, and ultimately dies out under a great rocky promontory--the [/Promontorium%20Archerusia Promontory Acherusia], at the eastern termination of the [/Montes%20Haemus Haemus range]. A comparatively low power serves to show the curious structural character of this immense ridge, which appears to consist of a number of corrugations and folds massed together, rising in places, according to Neison, to a height of 700 feet and more.

Additional Information


Nomenclature

  • Drawn by [/Johann%20Schr%C3%B6ter Johann Schröter] ([/Whitaker Whitaker], Fig. 67, p. 104 -- Schröter's Plate X, observed on November 17, 1789 at 10:10 pm local time). On page 185 of the first volume of his book, Schröter refers to the ridge as a "fortlaufende Bergader" ("fortlaufende" = continuous; "Berg" = mountain; "Ader" = vein, as in coal mining) connecting [/Plinius Plinius] and [/Posidonius Posidonius]. At the bottom of the page he further describes it as "schlangenformig" ("schlangen" = snake/serpent).
  • Various English observer's picked up on Schröter's descriptive term. For example, on page 180 of an 1868 edition of the Astronomical register, [/Birt Birt] refers to "the well-known serpentine ridge of Schröter." However, like ""Bergader", the term "serpentine" was also used with some indifference as a descriptive term. For example, in various publications [/Elger Elger] refers to "the great Serpentine ridge", but there is little other than the extra adjective "great" to distinguish this from Elger's serpentine ridges in Mare Frigoris and near Langrenus.
  • Although this feature was drawn on the maps of [/Blagg%20and%20M%C3%BCller Blagg and Müller], it was not named by them. Several features along it did have IAU-approved names: Posidonius Gamma (the elevated region around [/Posidonius Posidonius] Y -- regarded as a "crater cone"), the crater [/Very Very] (Le Monnier B), and [/Bessel Bessel] Alpha (an elevated point to the south of [/Very Very] which no longer has an official name).
  • In the modern [/IAU%20nomenclature IAU nomenclature], the Serpentine Ridge corresponds to [/Dorsum%20Nicol Dorsum Nicol], portions of [/Dorsa%20Lister Dorsa Lister], [/Dorsa%20Smirnov Dorsa Smirnov], and an unnamed northward extension of that ridge ending near [/Posidonius Posidonius] F.


LPOD Articles

A Glorious Serpentine Ridge

Bibliography




This page has been edited 1 times. The last modification was made by - tychocrater tychocrater on Jun 13, 2009 3:24 pm - afx3u2