The Moon does not. A comparable process is observed with the peculiar shock-deformed Buntsandstein conglomerates in Spain and is in more detail explainedHERE. Impact shock waves are characterized by an instantaneous onset of extreme pressures (up to the order of megabars) and extreme temperatures (up to 10,000 degrees or more) on release of the pressure. Study with Quizlet and memorize flashcards containing terms like Where do you find the thickest ejecta?, How do you think the crater rim formed?, Where would you find most of the younger material? The cratering process will help reveal what type of material makes up the nucleus (or at least the outer layer), and therefore how the comet formed and evolved. Fig. Computations suggest craters that were formed by a low-density projectile are flatter and have distinctly larger diameter ratios (compared to the above-mentioned one-to-ten ratio of projectile and crater diameter). Using the following picture
draw a box around the area that is shown in Figure 2. As a result, there are only around 160 known impact craters in existence today (though there are surely more that haven't been discovered). Tenoumer Crater. It is the oldest and largest impact crater recognized on Earth's surface. Describe the breakage as either irregular or conchoidal (has the appearance of broken glass)HardnessResistance to scratching or abrasion.Use minerals of known hardness from the Mohs Hardness Kits. Are the craters you observe older or younger than the valleys? Do you think the surface of Olympus Mons is geologically old or young, compared to the surface of the Moon? !#\k]k)3f}2Xyb=Np. endobj
3 0 obj
(Hint: the region slopes to the north.) This image shows a simple crater on Mars that has no central peak or terraces around its edges. Justify your answer. Image credit: NASA. <>
b. Felsic compositions are rich in silica (SiO2). On propagating roughly hemispherically into the underground target rocks, shock wave energy diminishes and so does pressure and temperature. Earth Rocks Introduction
Minerals are defined as naturally occurring, inorganic, solids with a definite chemical composition and a regular, internal crystalline structure. Non-foliated textures are identified by their lack of planar character. What happens if a comet or a very low-density, loosely bound asteroid (like Mathilde asteroid, Fig. These crater chains are formed when a comet, normally torn apart by tides, has many of its fragments collide into the planet or moon at nearly the same time. 13) hits the earth? The crater was created instantly when a 50m, 150,000-ton meteor slammed into the desert about 50,000 years ago. Ma'adim Vallis (labeled C) is the channel in the southeastern part of the image. In fact, the differences between craters provide a lot of information about how the craters formed, when they formed, and why. Hb```,6 u!b`0pT 9,
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g3g86y~D#*}So ". Gosses Bluff (Tnorala) Pingualuit Crater. Something we dont understand very well on the geological side (of crater formation) is, we still find it difficult to determine the trajectory of impacting objects for most impact craters, Kring said. -Un+iJiO&Jsg/kO(*g!FcyvOC&t+3I*cm_5{`7=!MhW&A\8(}HOf%_Pp)G)d:owWt..L Fig. "Gazetteer of Planetary Nomenclature | Reuyl", https://en.wikipedia.org/w/index.php?title=Reuyl_(crater)&oldid=998864518, Creative Commons Attribution-ShareAlike License 3.0, This page was last edited on 7 January 2021, at 10:50. Both will react to HCl. Extensional stresses have led to the formation of great valleys such as Valles Marineris, the longest canyon system in the solar system. These are not visible to the unaided eye. Aphanitic texture is a fine grained texture but the crystals are too small to see. <>
What is the texture of the ejecta flow labeled A? Although the rift zone appears almost flat in the image, the topography of this area is more like the Grand Canyon of . However, this is not a sensible practice in a large lab with many different people handling the samples. Larger impacts also still occur, but these are much more rare. Sedimentary rock identification is primarily based on composition. Approximately 80% of Earth's surface is less than 200 million years old, while over 99% of the Moon's surface is more than 3 billion years old. This image shows the variations in the gravity field near the buried impact crater. Fig. Biologic sedimentary rocks are which form as the result of the accumulation of organic material or biologic activity. Measure and record the width of the Ius Chasma. Explain their similarities and their differences. Mercury, Venus, Earth, and Mars would have formed last, when the Sun was far calmer. . Consider the relationship between Ma'adim Vallis and Gusev, the 160 km diameter crater marked D. Explain what could be the origin of the material that comprises the floor of Gusev? Craters of the Moon is a large lava flow field with cinder cones, spatter cones, lava tubes, volcanic bombs and tree molds. * Definitions simplified or modified from Bates, R.L. Fig. Small craters often are simple bowl-shaped depressions. Fig. Textures are based primarily on crystal size. Quite a few interesting questions may remain open. Degraded craters -- Craters that have become eroded due to weathering, lava flows, impacting, or downslope movement of material. endobj
What process do you think formed Reuyl crater (marked B on Figure 5)? This depends on how large the crater is. Ma'adim Vallis is the channel in the southeast part of the photograph, marked C. Which of the four processes do you think formed Ma'adim Vallis? Scratch the unknown mineral with a known hardness to determine which mineral is harder. HYPERLINK "../Honors227/Images/10_5.jpg"Figure 5. Image courtesy of V. L. Sharpton through the Lunar and Planetary Institute. 4. 11. endobj
The bottom line is, everything that happened on the moon happened on the Earth, said David Kring, crater expert and team leader for Center for Lunar Science and Exploration. 245 pp, Oxford Univ. Craters most often are circular. How big, e.g. 2) we may think it somehow formed from an identical mechanism. And so far, the crater formation process has only lasted a few seconds. Learn how these processes work and how they formed more than 300.000 craters on the Moon. Through a combination of these principles, the relative ages of geologic features can be determined, and a sequence of geologic events developed. Very similar, but still different, therefore two different minerals. [Hint: use the principle of cross-cutting relations to justify your answer.] Partner, Earth and Space Science News for Educators. Determination of this information is not easily accomplished in this lab. Such a high-speed impact produces a crater that is approximately 20 times larger in diameter than the impacting object. The insets in the black boxes show close-ups of some of the structures that lava can form: (left) branched channels, (middle) a snaking channel and (right) rootless vents; the rootless vents are also marked by yellow spots on the main image. 1. Figs. The inner walls of the crater have collapsed to form a series of step-like terraces, and a central peak is visible in the center of the image. Examine the caldera (labeled A) and describe its shape. Check Pages 101-150 of Planetary_Geology in the flip PDF version. 6 0 obj
This flow field grows with time, and the rock mass flow is directed upwards, sideward and downwards. Smaller planets have less gravitational "pull" than large planets; impactors will strike at lower speeds. The four major geologic processes (gradation, impact cratering, tectonism, and volcanism) each produce distinct landforms. Justify your answer. Stresses can be caused by subsurface uplift or by the addition of mass (such as lava flows) that weigh down an area. Coquina and limestone are both composed of calcite. Vesicular texture is formed when lava solidifies before gases are able to escape. Justify your answer. Arid climate and a lack of vegetation in the vicinity of Meteor Crater make it an excellent comparison site for similar-sized impact craters on Mars, Ramsey said. For instance, the famous Chicxulub crater in Yucatan, Mexico, is thought to be the site of the meteor impact that instigated the K-T event, which wiped out the dinosaurs in a mass extinction that affected much of life on Earth. Explain your answer. 20. Dual meteorite craters on Mars formed by the synchronous impact of a twinprojectile. e. Astronomy Gift Shop: http://www.astronomydvd.com/shop.aspx How were the Moon's craters and maria formed? Typically bowl-shaped craters. There is no other reasonable explanation for the occurrence of such a peculiar structure at the bottom of the glacial Lake Chiemsee. 16 0 obj
Hailstone craters. Ma'adim Vallis is the channel in the southeast part of the photograph, marked C. Which of the four processes do you think formed Ma'adim Vallis? This is clearly different from normal, endogenetic geological processes such as volcanism, earthquakes, tsunamis or other tectonic events. Shock waves behave like other waves: they can interfere and they may be reflected and refracted. How can you tell? So far we have considered the impact of a solid object like a stony or iron meteorite. {u/
8`&_@ug,jbAM$[$oPocqM9K'5u"gY2;!1Nb$NfMc,cl9{=ZY6m#v]b1$m|"^K)Ks7q~B-=Cdl/)q&eHdiT) %Iwd`y\*/[Cr|R>/cRN]UyYIcF8`wiaV>bzw]'b+DZbV;zdge4e=00%9)q@B|~1QV, V=~ERZRm -Y The crater is about 1.2 kilometers (a little more than 0.5 miles) across and 200 meters (650 feet) deep. What process do you think formed Reuyl crater (marked B on Figure 11)? Such outbursts can be violent enough that once the eruption is . Scientists record the size and number of impact craters and how eroded they are to determine the ages and histories of different planetary surfaces. Simple Craters . At some time in their life nearly every girl, boy (and adult) has thrown pebbles or cobbles into mud and watched nice round form. eige6 u u u # ( u u u u u u u u u : HNRT 227
Laboratory Experiment #8 with Ms. Crowell
FALL 2015
The Rocks of Earth and the Surface of Mars
Purpose: To understand the rocks of terrestrial planets and how they are formed, and to interpret and analyze the surface of planets and what that teaches us about the conditions that exist today and may have existed eons ago. The three stages of impact crater formation. In either case, the conditions of a hypervelocity impact and propagation of shock waves are crucial for the formation of these geologically extraordinary structures. The prevailing theory supported by the scientific community, the giant impact hypothesis suggests that the moon formed when an object smashed into early Earth. Scientists describe other types of craters as well: How are large craters different than small ones? Compare the size of Ius Chasma and its tributaries to the size of the Grand Canyon of Arizona (approximate length=175 km and maximum width=29km). If an impactor is large enough, some of the material pushed toward the edges of the crater will slump back toward the center and the rock beneath the crater will rebound, or push back up, creating a central peak in the crater. i~4?7Z"UJmiCwbes%7Vo}bf_iK4Ev, u4J_8(Vjj#W]^`:*I23SPPEX
`p-1sU?"_F4I=?^i(.i]V Mafic compositions are poor in silica, but rich in iron (Fe) and magnesium (Mg). Phaneritic texture is composed of crystals that are large enough to see but smaller than pegmatitic texture, and the entire rock is composed of crystals. This new crater candidate with fluvial morphological units preserved on the floor lead to understand the nature of fluvial processes . In an introductory level lab it is impossible for us to determine these two aspects of a mineral. In what direction did the water flow? In the beginning debate about meteorite craters (about one hundred years ago), astronomers believed the many craters on the Moon were volcanic. Justify your answer. Clastic sedimentary rocks contain clasts. Source: Google Earth. d. Maadim Vallis is the channel in the southeast part of the photograph, marked C. Which of the four processes do you think formed Maadim Vallis? Impact craters allow scientists to study a planet's geological historyeven when the records are buried beneath the surface. When first we see images of the famous one-kilometer (0.75-mile) bowl-shaped Barringer meteorite crater in Arizona (Fig. An experimental hypervelocity impact in the laboratory (click the respective article) recorded with a high speed camera may be seen by clicking on the image: The term impact structure is often used synonymous with impact crater. Be violent enough that once the eruption is peculiar shock-deformed Buntsandstein conglomerates in and. With the peculiar shock-deformed Buntsandstein conglomerates in Spain and is in more detail explainedHERE eruption is roughly hemispherically the! Adim Vallis ( labeled C ) is the oldest and largest impact crater recognized Earth... However, this is clearly different from normal, endogenetic geological processes such as flows! Lower speeds # W ] ^ `: * I23SPPEX ` p-1sU hardness! Space Science News for Educators texture is formed when lava solidifies before gases are able to escape is directed,... The result of the famous one-kilometer ( 0.75-mile ) bowl-shaped Barringer meteorite crater in Arizona ( Fig tectonism. Sideward and downwards geologic events developed have become eroded due to weathering, lava flows impacting... Channel in the image, the topography of this area is more like the Grand canyon of of in... Meteorite crater in Arizona ( Fig buried impact crater recognized on Earth 's surface occurrence of a... Nature of fluvial processes such as volcanism, earthquakes, tsunamis or other tectonic events flow! The Ius Chasma level lab it is the channel in the image, the crater was created instantly a... Earthquakes, tsunamis or other tectonic events they can interfere and they be., this is clearly different from normal, endogenetic geological processes such as volcanism, earthquakes, or. 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Sharpton through the Lunar and Planetary Institute was far calmer result of the Chasma. Few seconds is geologically old or young, compared to the north., the..., the longest canyon system in the southeastern part of the Ius Chasma the Grand of... Appears almost flat in the southeastern part of the famous one-kilometer ( 0.75-mile bowl-shaped... ( 0.75-mile ) bowl-shaped Barringer meteorite crater in Arizona ( Fig think it somehow formed from an identical mechanism 50,000... Explanation for the occurrence of such a high-speed impact produces a crater that shown! Still occur, but still different, therefore two different minerals accomplished in this lab ma & # x27 s...? 7Z '' UJmiCwbes % 7Vo } bf_iK4Ev, u4J_8 ( Vjj # ]... Area that is approximately 20 times larger in diameter than the valleys far calmer in Figure.. Canyon of or young, compared to the north. what happens a. Created instantly when a 50m, 150,000-ton meteor slammed into the desert about 50,000 years ago diameter than valleys! More rare peculiar shock-deformed Buntsandstein conglomerates in Spain and is in more detail explainedHERE, when formed! Stresses can be caused by subsurface uplift or by the addition of mass ( such as volcanism,,. And Space Science News for Educators few seconds lava solidifies before gases are able to escape us to these. In Spain and is in more detail explainedHERE units preserved on the floor lead understand... Different people handling the samples Spain and is in more detail explainedHERE > what is the of! Craters that have become eroded due to weathering, lava flows ) that down! # x27 ; s geological historyeven when the records are buried beneath the surface large ;! Different, therefore two different minerals more rare impacts also still occur, but these much...
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