Lunar Features Because the moon spans 3476 kilometers, about a quarter the diameter of Earth, and lies only a quarter million miles away, it exhibits a wealth of detail in a small telescopes and binoculars. Both will reveal the Moon's desolate landscape punctuated by bright highlands, dark plains, and rayed craters. At every phase except when full, you'll notice that the lunar globe is divided by the terminator, the line separating the Moon's bright, sunlit side from the side hidden in shadow. Here is where surface features stand out best. Seen in a small telescope or high-power binoculars, the landscape near the terminator stands out in bold contrast and detail. The terrain looks very rough near the terminator because here the Sun is near the lunar horizon. Thus every low hill casts a long, black shadow that creates an exaggerated impression of height. The term 'meteorite impact' is used to describe the process of surface bombardment by cosmic objects. The objects themselves are variously referred to as impactors or 'projectiles'. The impact process is explosive, impacting the surface at more than 20 km/sec (45,000 mi/hour). Upon impact, the impactor vaporizes and the planetary or lunar material is compressed and is tossed out of the target area, piling up around the hole with the bottom of the crater lower than the original ground surface with the piled up material on the rim higher. PART I: SIZE OF LUNAR FEATURES To determine the size of any lunar feature you must first determine the scale of the photograph. Using a ruler, measure the diameter of the Moon (Image #1) to the nearest millimeter. The moon’s actual diameter is known to be 3476 km. Determine the scale of your photograph in km/mm. Diameter of lunar image = __________ mm Scale of Image #1 = __________ km/mm To determine the magnification of Image #2 measure the distance from the centers of the craters Plato and Cassini on Image #1 and Image #2. From these measurements determine the magnification of Image #2. Distance Image #1 = __________ mm Distance Image #2 = __________ mm Magnification = ________ __ times The surface features on the full image are blurry making accurate measurements difficult. By knowing the scale of the lunar image and the magnification of the inset (Image #2), you can now calculate the diameters of the two craters, Plato and Cassini with greater accuracy as they appear in Image #1. Compare your results with the known diameters of the two craters (Google it!) Crater Measured Diameter Image #2 (mm) Calculated Diameter Image #1 (mm) Calculated Diameter (km) Actual Diameter (km) Plato Cassini 5 Height of Lunar Features The height of a certain lunar feature such as mountains or craters can be calculated by analyzing the length of their shadows. In the figure below you are viewing the moon from above one of its poles. S M sunlight T B C In this diagram MB represents the height of a surface feature, such as a mountain, BC is the moon’s radius, MS is the length of the shadow as seen from Earth, and BT is the distance of the mountain from the terminator. Notice that each of the two triangles are right triangles so that the ratios of the sides are equal. So that: MB BT = MS (Equation 1) BC Since we are interested in the height of the surface feature, rearranging results in: (MS) (BT) MB = (Equation 2) BC Remembering your algebra, we must know all of the terms on the right hand side of the equation to determine the height of the crater. BC is the Moon’s radius, which is known (from Part I) and BT, the distance of the mountain from the terminator can be measured from the full lunar photograph (Image #1). The length of the shadows (MS) is difficult to measure from the full lunar photograph, but can be determined by measuring the shadow on the enlarged image and scaling it to the size of Image #1. Now you have all the needed information to calculate the height of a lunar feature. 1. The mountains Mons Piton and Mons Pico have been identified on the magnified lunar photograph. Measure the length of their shadows on the magnified image (Image #2) and from this determine the length of the shadows (MS) on the full image (Image #1) using the scale of the enlarged photo. 2. Measure the distance from the mountain’s center to the terminator from Image #1. (BT) 3. Use Equation 2 to calculate the height of the mountain (in millimeters) as it appears in Image #1. Use the scale of Image #1 to determine the calculated height of the mountain (in kilometers). 4. Compare your answers with the known heights (Google it!) Feature Distance to Terminator (BT) (mm) Moon’s Radius (BC) (mm) Length of Shadow (MS) (mm) Height (MB) (mm) Calculated Height (MB) (km) Known Height (km) Mons Pico Mons Piton 6 Image #1: Lunar Surface at 1st Quarter Image #2: Magnified Portion Crater Plato Mons Pico Crater Cassini Mons Piton 7
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