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Topic: Arandas crater

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	Craters
		IMPACT CRATERS, which occur almost everywhere on the Martian surface, are significant because the number of impact craters per unit area area gives an indication of the relative ages of different parts of the surface.
		Crater densities low enough to suggest significantly higher rates of resurfacing are found only in the polar regions, around some volcanoes, and very locally in other areas.
		The general surface layer of debris has been removed everywhere except around craters where ejecta have armored the surface against the wind, with the result that most craters are surrounded by a platform composed of remnants of the debris blanket.
	www.lindbergh.k12.mo.us /mars/VOViews/CRATERS.HTM (709 words)

	ch7
		Although buried by Yuty ejecta, a pre-Yuty crater close to the rim is clearly visible, indicating that the ejecta deposit is thin.
		This crater is close to Kasei Vallis, the edge of which is marked by an escarpment in the northwest corner of the image.
		A cluster of craters at the top of the frame strongly resembles a group of volcanic cones but is probably part of the impact crater continuum.
	history.nasa.gov /SP-441/ch7.htm (1261 words)

	Chapter 6 - The Solar System
		All ages and size of craters can be seen, ranging from fresh craters with sharply defined rims to older craters which have been filled by some free-flowing material, to the oldest craters where only a few segments of the rim remain visible through the cover of material and recent meteoroids.
		In some of the older craters it is possible to observe that the rounded floor of the newly-formed crater has been gradually filled to form a flat plateau within the crater walls, and it is common for this material to be the same dark material as the Marias.
		On the edge of the Kassi Vallis on the western side of Mars is an impact crater with a diameter of 18km.
	www.dinox.org /book/chap6.htm (4712 words)

	ch11-2
		Scientists think that the caldera-the crater formed by the collapse of the central part of the volcano-of a patera is the result of simultaneous lifting and collapsing of the sides of the volcano, probably repeated many times over a long period.
		The impact melts the ground ice and lubricates the [ejecta] that is thrown out of the crater so when it lands on the ground it flows away from the crater in a debris flow and forms the characteristic features we have observed.
		Craters on the moon and Mercury typically had a coarse, disordered texture close to the rim that became finer farther out, grading almost imperceptibly into dense fields of secondary craters.
	www.hq.nasa.gov /office/pao/History/SP-4212/ch11-2.html (3527 words)

	Comparative Geology: Earth and Mars
		The student compares impact craters, shield volcanoes, faults, river deltas, and drainage basin features on Earth and Mars by writing a short paragraph distinguishing the characteristics for each set of features.
		Impact Craters (3-D) Arandas is an example of a martian crater with fluidized ejecta deposits, a distinguishing characteristic of rampart craters.
		Meteor Crater formed roughly 50,000 years ago when a 30-meter-wide iron-rich meteor weighing 100,000 tons struck the Arizona desert at an estimated 20 kilometers per second.
	www.astro.washington.edu /labs/clearinghouse150/labs/Mars/comgeol.html (1247 words)

	Untitled Document (Site not responding. Last check: 2007-10-26)
		The floor of the crater is occupied by a central peak and a crater.
		The next image is of the crater Arandas, it again has an ejecta blanket with multiple lobes.
		A rille descending from the tholus crater has formed a small delta on the floor of the crater.
	faculty.sulross.edu /jlwstark/planet/planet49.html (183 words)

	List of craters on Mars - Wikipedia, the free encyclopedia
		There are hundreds of thousands of craters on Mars, but only some of them have names.
		Here is a list of named Martian craters.
		Martian craters are named after famous scientists and science fiction authors, or after towns (with a population of less than 100,000) on Earth.
	en.wikipedia.org /wiki/List_of_craters_on_Mars (87 words)

	Final Gallery
		The Arandas crater is more complex than the Meteor crater; it features a terraced rim, which is thought to have formed from the outward movement of âsoftâ terrain over millions of years.
		Mars also contains many pit craters, which are craters that contain central, peak-like structures, which are thought to have formed from large peaks in existence before meteor impact.
		Approximately 30% of all craters with central formations on the surface of Mars are pit craters.
	aerospacescholars.jsc.nasa.gov /has/Students/finalGall.cfm?id=215 (1338 words)

	3. Double Lobe Rampart (Site not responding. Last check: 2007-10-26)
		Arandas, the 24.5-km-multilobate crater seen in this image, is located in the mottled terrain, a region near the martian north pole where craters are typically surrounded by bright halos of material.
		To the right of the crater is an example of the polygonal terrain, the origin of which has been variously attributed to ice, volcanism, and tectonism.
		Crater at 42.53° N, 14.97° W; Viking Orbiter frame 673B52
	www.lpi.usra.edu /publications/slidesets/stones/slide_3.html (107 words)

	The Guinnes of
		This shows a composite of several Mariner 9 photographs that reveal the summit craters and the cliff at the base of the huge pile of lava.
		At left, a fresh young crater about 30 km across, in Lunae Planum, is near a dry river channel running alongside a cliff in possible lava flows (Kasei Valley).
		Photographed 22 July 1976 by the Viking 1 orbiter at 43°N latitude, 15° longitude, Arandas is about 25 km in diameter.
	www.pianeta-marte.it /marte_in_cifre/english_guinnes_of_mars.htm (979 words)

	[No title] (Site not responding. Last check: 2007-10-26)
		Jupiter Ganymede Amset -14.4 178.8 -14.6 -14.3 178.6 178.9 W 10.9 Africa Egypt JG-08 I-1536 Adopted by IAU General Assembly 1997 A circular depression Crater, craters One of the four gods of the dead, son of Horus.
		Mars Mars Arandas 42.7 15.1 42.5 43.0 14.8 15.4 W 25.1 North America Mexico MC-04 I-2574 Adopted by IAU General Assembly 1976 A circular depression Crater, craters Town in Mexico.
		Mars MarsE Arandas 42.4 344.9 42.177 42.676 345.2 344.6 E 25.1 North America Mexico MC-04 I-2574 Adopted by IAU General Assembly 1976 A circular depression Crater, craters Town in Mexico.
	planetarynames.wr.usgs.gov /jsp/AllDataExcelText.jsp (22652 words)

	[No title]
		The diameter of the crater is 120 kilometers.
		445; Figure 27.2 Craters and structures of impact origin are conspicuous in this Apollo 8 view of the lunar surface.
		The dark circular “seas” are themselves basalt filled impact basins and rays of ejected material are visible radiating from the small crater near the top of the picture.
	www.geop.itu.edu.tr /~emine/jef431e/lec-week-2.doc (1255 words)

	ch10-7 (Site not responding. Last check: 2007-10-26)
		Because of defects in some of the B-2 photos and an atmospheric haze that had obscured the surface, the interpreters were cautious in their estimates of the dunes in that zone.
		Some felt that the B-2 craters and ejecta blocks, being smaller than those in B-3, were better covered by B-2's bigger dunes and that B-3's smaller dunes might not cover the ejecta from the larger craters there as well.
		In the region of the crater Mie, it was hard to project what size blocks could be anticipated.
	solarviews.com /history/SP-4212/ch10-7.html (3688 words)

	ch11
		Projections on or near the horizon may be rims of distant craters.
		Some of the rocks appear to be undercut on one side and partially buried by drifting sand on the other.
		The boulders littering the scene were probably imposed, either as broken lava flows or as ejected boulders from a nearby crater.
	www.hq.nasa.gov /pao/History/SP-4212/ch11.html (12773 words)

	[No title]
		M M Airy-0 5.1S 0.0W 0.5 EU GB MC20 I2532 5 2003 172 AA Small crater within crater Airy that defines zero degrees longitude on Mars.
		M ME Arandas 42.4N 344.9E 25.1 NA ME MC4 I2574 5 1976 36 AA Town in Mexico.
		M M Arandas 42.7N 15.1W 25.1 NA ME MC4 I2574 5 1976 36 AA Town in Mexico.
	planetarynames.wr.usgs.gov /alph_excel.txt (10256 words)

	[No title] (Site not responding. Last check: 2007-10-26)
		M M Airy-0 -5.1 0.0 0.0 0.0 0.0 0.0 W 0.5 EU GB MC-20 I-2532 5 2003 172 AA Small crater within crater Airy that defines zero degrees longitude on Mars.
		M M Arandas 42.7 15.1 42.5 43.0 14.8 15.4 W 25.1 NA ME MC-04 I-2574 5 1976 36 AA Town in Mexico.
		M ME Arandas 42.4 344.9 42.2 42.7 345.2 344.6 W 25.1 NA ME MC-04 I-2574 5 1976 36 AA Town in Mexico.
	planetarynames.wr.usgs.gov /jsp/AllDataPlainText.jsp (19085 words)

	Science Fair Projects - List of craters on Mars
		Science Fair Projects - List of craters on Mars
		Or else, you can start by choosing any of the categories below.
		Martian craters are named after famous scientists and science fiction authors, or after towns on Earth.
	www.all-science-fair-projects.com /science_fair_projects_encyclopedia/List_of_craters_on_Mars (215 words)

	Gazetter of Mars
		Buried Mid-Latitude Craters (Released 17 December 2003) The image is located near 28.4N, 317.5W.in northeastern Arabia Terra.
		Exhumed Crater with Slope Streaks (Released 15 December 2003)The image is located near 20.9N, 320.7W, and shows a crater in Arabia Terra.
		Exhuming Crater in Northeast Arabia (Released 03 December 2003)
	www.lindoponline.com /alphastro/solar_system/mars/a.html (344 words)

	Tequila
		There are an estimated 100 million Agave tequilana plants in the area, and the approximately 40,000 hectares of cultivated agaves produce no less than 50 million litres of tequila each year.
		To qualify as genuine Tequila, the drink has to be manufactured in one of two municipalities, either that of Tequila or that of Arandas to the northeast of Guadalajara.
		Conoissoeurs argue long and loud as to which is the better product.
	www.mexconnect.com /mex_/travel/tonysarticles/tequila.html (993 words)

	Facts about list of craters on mars (Site not responding. Last check: 2007-10-26)
		Here is a list of Martian craters with their own names:
		Some articles mentioning "list of craters on mars":
		Crater: Articles on Crater (current) from Fablis Online Encyclopedia
	www.supercrawler.com /Facts/list_of_craters_on_mars.html (125 words)

	Fototek:Viking_Orbiter
		Designation of purported drowned continent south of India; also relates to lemur monkeys found on Madagascar and Sunda islands
		Name given to the crater that fills most of the famous picture No. 11 taken by Mariner IV in 1965
		Carl H.; German astronomer (1851-1925); same crater as above
	fototek.geol.u-psud.fr /viking_orbiter/nomenclature.php (849 words)

	Cruz Family Genealogy Forum (Page 2)
		Re: Cruz Marcelino - Arandas, Jalisco - 1900 - Ruben Medina De La Cruz Guardiola 4/30/01
		Re: Cruz Marcelino - Arandas, Jalisco - 1900 - Art Magon 4/30/01
		Re: Esperidion Cruz descendants please reply - John Crater 10/13/00
	genforum.genealogy.com /cgi-bin/redirect.cgi?cruz::382.html (2220 words)

	Arandas crater (Site not responding. Last check: 2007-10-26)
		Click here to zoom out to the map location of area southwest of Jen crater
		The map below is (being) generated on the fly by the USGS site in Flagstaff.
		At present, the Roving Mouse site can't afford the disk space to cache all feature maps.
	www.roving-mouse.com /planetary/Mars/Atlas/features/xmaps/a/arandas-F1.html (46 words)

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		Discover the beauty and excitement of wildlife viewing in vehicles and on foot in
		, Ngorongoro Crater and the endless plains of the Serengeti.
		As you meet new friends in modern Mto Wa Mbu village, join in the welcoming dance at a traditional Maasai homestead and meet Zinjanthropus, one of the earliest fossils of man at
	www.houstonzoo.org /Index.asp?page_ID=320&skip_frames=&site_ID=2 (10089 words)

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