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	Lade (crater) - Wikipedia, the free encyclopedia
		Lade is the remains of a lunar crater that has been flooded by lava.
		To the north is Godin crater, and in the south-southeast is the worn, lava-flooded Saunder crater.
		The surviving crater wall is worn and somewhat hexagonal in outline.
	en.wikipedia.org /wiki/Lade_(crater) (175 words)

	Louis Godin - Wikipedia, the free encyclopedia
		Louis Godin (February 28, 1704 - September 11, 1760) was a French astronomer.
		Godin was a member with Charles Marie de La Condamine and Pierre Bouguer of the expedition sent to Peru in 1735 to determine the length of a degree of the meridian in the neighbourhood of the equator.
		This would also determine whether the earth's diameter were greater at the equator than at the poles, as had been conjectured by Isaac Newton.
	en.wikipedia.org /wiki/Louis_Godin (231 words)

	Agrippa (crater) - TheBestLinks.com - Crater, Latitude, Longitude, Kilometer, ... (Site not responding. Last check: 2007-10-13)
		Agrippa is a lunar impact crater that is located at the southeast edge of the Mare Vaporum.
		It is located to the north of the Godin crater, and the irregular Tempel crater formation lies just to the east.
		The crater is associated with a ray system that extends for a distance of about 270 kilometers.
	www.thebestlinks.com /Agrippa___28__crater__29__.html (195 words)

	Hitchhiker's Guide to Rukl Chart 34
		It often appears like a crater chain in the telescope, but lunar photogeologists say the "craters" are collapse pits, where the wall of the rille has fallen in.
		The crater midway along the rille is a true crater.
		From the crater the prominent Hyginus Rille extends east-southeast toward the camera and northwest toward the Sea of Vapors.
	www.shallowsky.com /moon/rukl34.html (828 words)

	LPOD lunar photo of the day » 2006 » February
		Agrippa (above) and Godin are rarely imaged craters in plain view near the lunar center of face.
		Godin has no floor, its entire interior is covered with material that slid down the walls and piled up as wide and high terraces.
		Landslides occur when complex craters are formed as part of the accommodation to the removal of rock from the crater center.
	www.lpod.org /?m=20060217 (336 words)

	Dembowski (crater) - TheBestLinks.com - Crater, Latitude, Longitude, Polygon, ... (Site not responding. Last check: 2007-10-13)
		Dembowski (crater) - TheBestLinks.com - Crater, Latitude, Longitude, Polygon,...
		To the east are the Agrippa and Godin craters, and to the southwest is Rhaeticus crater.
		The surviving western half of the rim is polygonal in shape, and the ends are broken; forming rises in the surface.
	www.thebestlinks.com /Dembowski___28__crater__29__.html (188 words)

	Lunar Images with Maksutov-Cassegrain
		Craters Aristarchus (bright) and Herodotus, Vallis Schroteri 160 km long valley, Rupes Toscanelli to left, flooded crater Prinz at upper left.
		Crater Cassini at center with the lone summit of Piton brilliantly lit by the rising sun.
		Craters Watt, Steinheil and Janssen, upper right, along with the Rheita Valley are clearly visible along the morning terminator.
	www.fortunecity.com /victorian/canterbury/222/maksutov.htm (522 words)

	Lake County Astronomical Society NightTimes
		Despite the hundreds of years during which the moon has been observed through telescopes and via more recent close views from space vehicles, observational data is still needed to test the theories of the origin of bright rays and their nature.
		And if you observed the craters when their rays could not be seen, that is also of great importance since it'll help determine when the rays are not visible.
		Other things to be noted are the association of rays with linear arrangements of craterlets, the divergence of rays from points other than the center of the 'parent' crater, and their becoming visible only at some distance from the point of origin.
	www.bpccs.com /lcas/Articles/moonrays.htm (1060 words)

	22mai1999ang
		Caucasus, Montes [39N; 9E] - It is the prolongation of the chain of the Apennines from which it is separated by a " strait " from 50 km connecting the sea of Showers to the sea of Serenity.
		The Eudoxe crater, with the massive walls, seems to be the twin of Aristote.
		The Caucasus extends on approximately 520 km, of the above-mentioned strait, to the Eudoxe crater.
	www.astrosurf.com /couic-cam/lune22mai1999ang.htm (1333 words)

	No title
		Following Gene Shoemaker's analysis in the late 1950s we now know that crater rays are pulverized ejecta widely dispersed from craters formed by high speed impact and mixed with local material gardened by such ejecta.
		The two most important recent studies are The Origin of Lunar Crater Rays by Hawke and colleagues, and Optical Maturity of Ejecta from Large Rayed Lunar Craters by Grier and colleagues.
		Although there are obviously many rayed craters, lists of crater ray systems are not as common as they were 100 years ago.
	www.lpod.org /cwm/DataStuff/rays.htm (533 words)

	Observing log for BAA/ALPO members for April 2003 (Site not responding. Last check: 2007-10-13)
		The crater floor looked uniformly dark at first, but on closer observation, particularly under lower powers where contrast was greater, variations in albedo and light intensity could be seen.
		Near the center of the crater floor a vague circular spot, slightly lighter than the surrounding areas, could be occasionally barely glimpsed or suspected.
		In the southwest corner of the crater floor a narrow arc like line could be seen projecting into the interior of the crater from the margin of the dark floor.
	www.cs.nott.ac.uk /~acc/Lunar/2003dec.htm (6852 words)

	Bouguer biography
		La Condamine was a member of the same expedition and its third scientific member was the leader of the expedition Louis Godin.
		Godin began to work on his own while Bouguer worked with La Condamine.
		Bouguer was the first to attempt to measure the density of the Earth using the deflection of a plumb line due to the attraction of a mountain.
	www-history.mcs.st-and.ac.uk /Biographies/Bouguer.html (670 words)

	AGRIPPA (Site not responding. Last check: 2007-10-13)
		DAVID O. "AGRIPPA: A fine crater 30 miles in diameter not far from Hyginus, near the border of the Mare Vaporum.
		No reports have been made when crater is located in the Earthshine region of the Moon.
		When examining this close up photograph taken by the Clementine space craft the crater floor does seem to exhibit a great number of domes on the western floor.
	www.ltpresearch.org /agrippa1.htm (314 words)

	NexStar 50 Lunar Club Observation Log - Douglas E. Johnson
		Date Observed: 9/14/05 10:02 PM Comments: Small, circular crater just west of the Riphaeus Mountains on the eastern edge of Ocean Procellarum directly east of crater Hansteen with the intervening mare between the two devoid of features, approximately mid-way between craters Kepler and Gassendi.
		While it is nice to speculate that 5 monks may have described its origin from a meteorite in 1178, the current evidence suggests what they saw was most likely due to their witnessing a meter (Beta Taurid meteor) burning up in a trajectory that was limited to their field of view.
		Date Observed: 8/10/05 9:30 PM Comments: Large, well-defined crater- the 1st of a chain of three (Theophilus, Cyrillis, Catharina) lying at the western junction of Mare Nectaris and Sinus Asperitatis- with prominent terraced walls, smooth floor and prominent central peaks.
	www.nexstarsite.com /NS50ClubLogs/JohnsonDouglasLunar.htm (1690 words)

	THE FIRMAMENT: Moon - craters, mountains, mares, rilles (Site not responding. Last check: 2007-10-13)
		Mare Frigoris and the craters Plato, Aristoteles and Eudoxus.
		The Luna 2 probe crushed on the slope of the Autolycus crater on 14 September 1959.
		In the vast area of Mare Fecunditatis is the well-known pair of craters Messier and Messier A, which is the centre fo two bright rays radiating to the West.
	www.madpc.net /~firmament/images/moon/moon_details/moon_details.html (5144 words)

	Early life on Earth
		If true, impact craters could represent some of the best sites to look for signs of past or present life on Mars and other planets.
		Lakes accumulate sediments, the layers of which are a geological archive of the time after the crater formed.
		Impact craters of that age were long ago erased on Earth by erosion, volcanic resurfacing and plate tectonics.
	www.theallineed.com /ecology/06010313.htm (618 words)

	[No title] (Site not responding. Last check: 2007-10-13)
		The central area of the lunar surface is seen in the photograph taken on August 7, 1966 with the
		are Godin and Agrippa, with the latter being the larger at 28 miles in diameter.
		the left is the almost fully shadowed crater Menelaus at 20 miles in diameter.
	www.w7ftt.net /moon7.html (185 words)

	[No title]
		Frequently small craters are found on the summits of these elevations, but more often on their flanks and near their base.
		Its crest is broken on the E. by a large brilliant crater, and its continuity is interrupted on the N. by a formation resembling a large double crater, which is associated with a number of low rounded banks and ridges extending some distance towards the N.W., and breaking the continuity of the _glacis_.
		There is a conspicuous crater on the N.W. side of the floor, and a curious square enclosure, with a crater on its W. border, abutting on the N.E. wall.
	www2.cddc.vt.edu /gutenberg/1/7/7/1/17712/17712.txt (17667 words)

	Observing log for BAA
		The floor of Herodotus was mostly shadow filled with the shadow of a prominent rim peak reaching across the crater floor to the sunlit west wall.
		On the inside margin of the western side of the crater was a dark but not absolutely fl shadow, the rest of the crater appeared to be a featureless, moderately bright crescent.
		The crater floor was variably shaded as well, being darker in the south than in the north.
	www.ltpresearch.org /feb05observing_log_for_baa.htm (3387 words)

	Observing log for BAA/ALPO members for April 2003 (Site not responding. Last check: 2007-10-13)
		Running along the southwest edge of the crater floor was what appeared to be a ridge and on the east side of the crater floor appeared to be a hill to the north of which was a less elevated plateau.
		Three of the spots were located in the southwest part of the crater and a fourth in the north central part of the floor of Julius Caesar.
		No other craters seem to have this tonight so don't think it was a telescope/observer artifact, but have not checked the imagery to see if this is a normal feature.
	www.cs.nott.ac.uk /~acc/Lunar/2003mar.htm (8407 words)

	Oh, l'Amour
		But it's definitely a good thing that Dunckel and Godin are so in touch with their feelings, because their sensations — more important, their instincts — are key to making their best music.
		And more recently, Godin bought a lesson on tape from a French protégé of Atkins in order to take his fingerpicking to the next level.
		Onstage, Dunckel and Godin's live setup includes a Fender Rhodes, a Moog Minimoog Voyager, a Korg MS-20, a Clavia Nord Lead, an ARP Solina String Ensemble, an organ through an Electro-Harmonix delay box and a little Boss SP-202 sampler.
	remixmag.com /artists/remix_oh_lamour (2728 words)

	Perth Penguinista: 01/2006
		However, the craters in the chain are often all of a size.
		The uniform physical properties and bedding of these layers might indicate that they were originally deposited in a lake (it is possible that the crater was at the bottom of a much larger lake, filling Schiaparelli Basin); alternatively, the layers were deposited by settling out of the atmosphere in a dry environment.
		These are often described as “rebounds”, but the geologists are pretty sure that the Chicxulub crater — also blamed for the lack of living dinosaurs — is an impact crater, and the rock structure under that is a mess, not the neatly deposited, even, symmetrical layers we see here with no evidence of underlying chaos.
	leonbrooks.blogspot.com /2006_01_01_leonbrooks_archive.html (6815 words)

	Copernicus (Site not responding. Last check: 2007-10-13)
		The large crater Copernicus comes into view when the moon is about 9 days old.
		The two craters above Copernicus are Reinhold and Lansberg, while at the right-hand edge, Kepler, with its system of bright rays is visible.
		The pair of large craters above (south) of Manilus are Godin (top) and Agrippa (below).
	www.montgomerycollege.edu /faculty/~mclark/public_html/copern.htm (262 words)

	Rags' Soapbox: Tanzania Part 2 - Safari
		The crater is actually a caldera formed from the implosion of a volcano millions of years ago.
		The crater teems with wildlife and has a high density of all sorts of animals.
		All in all, the crater was nice but it was too crowded for us compared to the more open Serengeti.
	www.ragsgupta.com /weblog/2005/07/tanzania_part_2.html (1549 words)

	Traffick: December 19, 2004: Search Engine Enlightenment \| RSS: traffick.com/atom.xml
		If I had to boil it down to one takeaway, it would be Godin's urgings in Free Prize Inside to focus on "going to the edge" in developing new products, services, and features.
		Godin is capable of ripping off hundreds of examples on command.
		Maybe the TV-industrial complex isn't quite dead as Godin argues, but it's certain that the role of advertising is rapidly changing.
	www.traffick.com /blog/archive/2004_12_19_archive.asp (2442 words)

	Observing log for BAA/ALPO members for April 2003 (Site not responding. Last check: 2007-10-13)
		The southwest inner wall was barely visible at the start of the observing period but had brightened noticeably by the end of the session.
		The rest of the interior of the crater was in fl shadow.
		To the north of the shadowed crater wall was a fairly bright, nearly closed ring that almost looked craterlike itself.
	www.cs.nott.ac.uk /~acc/Lunar/2005feb.htm (5706 words)

	La_Condamine biography
		Bouguer was a member of the same expedition and its third scientific member was the leader of the expedition Louis Godin.
		In 1741 Bouguer discovered a small error in their joint measurements and these two fell out when Bouguer refused to allow La Condamine to recheck the results.
		The last survivor of the expedition, La Condamine, who was a less gifted astronomer than Godin and a less reliable mathematician than Bouguer often received the major part of the credit, probably because of his amiable nature and his talent as a writer.
	www-groups.dcs.st-and.ac.uk /~history/Biographies/La_Condamine.html (474 words)

	Manilus
		On the shore of Mare Vaporum, near Mare Serenitatis lies a very defined crater, about 40 km across, with a good central peak.
		This is Manilus, and its distinictivness makes it a very useful starting off point for navigating the central regions of the Moon.
		To the left, on the edge of Mare Serenitatis is another bright crater, Menelaus, while directly above are Godin and Agrippa.
	www.montgomerycollege.edu /faculty/~mclark/public_html/man.htm (80 words)

	Marek Cichanski; 6/7/2003: The Moon from the Breakfast Nook
		Can't tell the relative ages of Nasireddin and Miller to its north - the two craters are perfectly tangent to each other.
		Floor of crater Plato, at N rim of Mare Imbrium, is fully shaded.
		Craters Birt and Birt A appear to be quite tall-walled, due to the shallow angle of illumination.
	observers.org /reports/2003.06.07.html (818 words)

	EirePreneur: May 8, 2005 - May 14, 2005
		However, after processing the Mapproxy satellite map in GIMP using a simple NEON Edge-Detect filter we were left with this view which appears to show traces of the eastern crater wall.
		I was a litte concerned that the 8 metre (ish) accuracy of my Garmin Geko 201 GPS receiver would be 'exposed' when mapping on a small scale but as the screenshot indicates it did perfectly well in mapping Newcastlewest on a small scale.
		As the reviews for Seth Godin's new book start trickling in he decides to post his list of 'what every good marketer knows'.
	eirepreneur.blogs.com /eirepreneur/2005/week19 (1623 words)

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