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A New Atlas?
Lat: 8.86°S, Long: 61°E, Diam: 131.98 km, Depth: 4.5 km, Rükl: 49,
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LPOD|Photo Gallery images
Lunar Orbiter Images
LANGRENUS.--This noble circumvallation, the most northerly of the meridional chain of immense walled-plains, extending for more than 600 miles from near the equator to S. lat. 40 deg., would, but for its propinquity to the limb, rank with
(which in many respects it resembles) among the most striking objects on the surface of the moon. Its length is about 90 miles from N. to S., and its breadth fully as much. In shape it approximates very closely to that of a foreshortened regular hexagon. The walls, which at one point on the W. rise to an altitude of nearly 10,000 feet, are continuous, except on this side, where they are broken by the interference of an irregular depression, and on the extreme S., where they are intersected by cross-valleys. Within, the terraces are remarkably distinct, and the intervening valleys strongly marked. The brilliant compound central mountain rises at its loftiest peak to a height of more than 3000 feet. On the N. of it is an obscure circular
ring, which may possibly merely represent a fortuitous combination of ridges, though it has all the appearance of a modified ring-plain. On the Mare, some distance N.W. of the formation, is a group of three ring-plains, with two small craters (associated with a ridge) on the N. of them. Two of the more easterly of these objects have prominent central mountains, and the third a very dark interior. At least three bright streaks originate on the W. flank of Langrenus, which, diverging widely, traverse the
[FLATTENINGS ON THE MOON'S EASTERN LIMB. --About thirty years ago, the Rev. Henry Cooper Key
to certain flattenings which he had noted on the E. limb, which are very apparent under favourable conditions of libration. Their position cannot be closely defined, but the principal deviation from circularity extends from about S. lat. 10 deg. to the region on the limb opposite the S. border of the
Depth data from
Kurt Fisher database
Pike, 1976: 4.5 km
Westfall, 2000: 4.5 km
Viscardy, 1985: 2.6 km
Cherrington, 1969: 4.93 km
Central peak composition
: GNTA1, AN & T (
Tompkins & Pieters, 1999
Central peak height
Alpha: 3.5 km
Beta: 3.0 km
Exterior impact melt deposits most extensive to SSE, max of ~50 km beyond rim. Most extensive ejecta, rays and secondary craters to the SSE, and topographically lowest rim crest to SSW and NW (
Hawke and Head, 1977
ALPO list of bright ray craters
are on the
ALPO list of banded craters
Langrenus C, FF, M
are thermal anomaly craters, implying youthful ages -
Moore et al, 1980
According to the book
Apollo 14 Preliminary Science Report
, there should be a color anomaly in Langrenus. Page 275: “A distinct rusty color is evident in one of a group of smooth bulbous domes with single or multiple furrows at or near the crests” (on the eastern wall of Langrenus).
TSI = 35, CPI = 20, FI = 25; MI =80
Smith and Sanchez, 1973
A small "overlooked"
chain of secondary craters
between Vendelinus and Langrenus was imaged by Joseph H.C. Liu and published in the Summer 2006 issue of Selenology: Journal of the American Lunar Society.
Possible TLP (Transient Lunar Phenomenon) in
, observed by the French astronomer
on December the 30th, 1992. Mentioned in the book
by W.P.Sheehan and T.A.Dobbins (2001).
Jun 6, 2014
Michael Florent van Langren
(circa 1600 – 1675), a Belgian astronomer and cartographer. Van Langren is noted for publishing in 1645
which is generally regarded as the first map to assign names to the features on the Moon visible through a telescope. Van Langren's nomenclature was a mix of generic Latin terms, names of current and ancient scientists and philosophers, and the names of contemporary royalty assigned to prominent features in capital letters. Two years later,
' much more influential lunar survey supplanted Van Langren's system with a completely different set of terrestrial-analog geographic names. However, in later years Hevelius's proposals were themselves largely replaced by a system, close to Van Langren's, introduced by
in 1651. Riccioli re-used many of Van Langren's scientist and philosopher names (although almost never for the same features) as well as his system of calling the dark areas "mare" (one of the few features embraced by Hevelius) and the bright areas "terra", but again with different names.
The names that appear on Van Langren's engraving are listed in Appendix D (pages 195-200) of
's book, along with, in earlier appendices, the somewhat different names appearing on a manuscript version and the slight changes made in various "states" of the final engraving. Whitaker's list includes what he feels are the modern identities of the features named, although there must, of course, be much uncertainty about what Van Langren intended to represent by some of the minor markings.
, Van Langren named the present crater "
" (after himself, one assumes).
modified the name to "
" in 1651. It has not been changed since. According to the Appendices in
, this is one of the
in continuous use at a given location.
is also one of the very few instances in which a map maker has named a specific feature after himself and that choice has been honored by later map makers.
is perhaps the only other example.
A Penchant for Names
Four in a Row
Dark Rays, Dark Streaks
: Aged ray system.
Apollo Over the Moon
, Chapter 5: Craters (
), Figure 169.
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