<p><BR/>Replying to:<BR/><DIV CLASS='Discussion_PostQuote'>Just niggles really, but, is the Moon's gravity strong enought to attract meteors, perpendicularly, to its surfrace? Why isn't there evidence of some meteors coming in at angle, hitting the surface with a glancing (scooping) blow?<br /> Posted by JackronRM</DIV></p><p>Actually, there is:</p><span style="font-family:Times" class="Apple-style-span"><font face="Times New Roman"><span style="font-style:italic" class="Apple-style-span"><span style="font-size:x-small" class="Apple-style-span">Careful </span></span></font><font face="Verdana"><span style="font-style:italic" class="Apple-style-span"><span style="font-size:x-small" class="Apple-style-span">–</span></span></font><font face="Times New Roman"><span style="font-style:italic" class="Apple-style-span"><span style="font-size:x-small" class="Apple-style-span"> while most craters are circular or close to it, a few aren't. There are oblong craters, stretched-looking distorted craters, scalloped craters, even square craters. The reasons for non-circular craters include the degradation or modification of the crater with age, the material strength of the target compared to the energy of the impact, and, yes, the angle of impact.<br /><br />Earth is a hugely active planet, with erosion by wind and water, volcanoes, and tectonic movement working to modify, subduct, bury, and destroy craters relatively rapidly by geological standards </span></span></font><font face="Verdana"><span style="font-style:italic" class="Apple-style-span"><span style="font-size:x-small" class="Apple-style-span">–</span></span></font><font face="Times New Roman"><span style="font-style:italic" class="Apple-style-span"><span style="font-size:x-small" class="Apple-style-span"> which is to say, over tens to hundreds of millions of years. The process is different on worlds with no atmosphere. On the moon, for example, volcanism has had a role in erasing and degrading craters. The mare on the moon are enormous impact basins flooded by basaltic lava, erasing all traces of previous craters. On older surfaces already saturated with craters, later impacts modify or erase earlier ones. Micrometeorites "soften" the sharp features of craters. Tectonism on airless worlds is uncommon, but on the icy satellites of Jupiter, viscous relaxation of craters and tidal forces have modified and erased craters.<br /><br />Your intuition that most impacts aren't perpendicular is spot on </span></span></font><font face="Verdana"><span style="font-style:italic" class="Apple-style-span"><span style="font-size:x-small" class="Apple-style-span">– </span></span></font><font face="Times New Roman"><span style="font-style:italic" class="Apple-style-span"><span style="font-size:x-small" class="Apple-style-span">in fact, perpendicular impacts are rare. In a large sampling of potential impactors, which can come from anywhere in the sky, the average impact angle is around 45 degrees. The spread of impact angles isn't entirely random due to gravity well effects and the fact that most bodies in the solar system orbit the sun and each other within a plane called the ecliptic, but it's close enough for this discussion.<br /><br /></span></span></font></span><p><span style="font-family:TimesNewRoman" class="Apple-style-span"><span style="font-style:italic" class="Apple-style-span"><span style="font-size:x-small" class="Apple-style-span">Impact angle has an influence on the shape of a crater, but the effect is small except when the angle is shallow, typically less than 20 degrees. When the impact angle is less than 10 degrees, crater distortion is quite pronounced. Because of the minimal variation in crater shape above 20 degrees, we have to look to other features to deduce more about the impact. Specifically, if the crater is large enough to be "complex" (rather than a simple bowl shape) we can look at interior structures such as the central peak or peak-ring in craters that have them and, outside the crater itself, at the ejecta (the debris that gets thrown out of an impact crater).</span></span></span><span style="font-style:italic" class="Apple-style-span"><span style="font-size:x-small" class="Apple-style-span"> </span></span></p><p><span style="font-family:TimesNewRoman" class="Apple-style-span"><span style="font-style:italic" class="Apple-style-span"><span style="font-size:x-small" class="Apple-style-span">For small, "simple" craters (under 4 km diameter on Earth, under 15 km on the moon, for example), the basic bowl-and-rim shape is characteristically circular except when the impact angle is less than 20 degrees, in which case you start seeing some aberration in the up-field (the direction the impactor was coming from) and down-field parts of the rim. When the impact angle is lower still, the entire crater becomes elongated. At near-grazing angles you can even have multiple craters. A very low angle impact crater can look like a butterfly, where ejecta sprays out almost perpendicularly to the impact direction, as in this example from the Hesperia Planum region of Mars:</span></span></span></p><p>http://www.esa.int/esaMI/Mars_Express/SEMZLM8A9HE_0.html</p><span style="font-family:TimesNewRoman" class="Apple-style-span"><span style="font-size:x-small" class="Apple-style-span"><span style="font-style:italic" class="Apple-style-span">Craters from shallow impacts can even look like a skipped stone on a pond (this may form due to the first impact fracturing the incoming body into multiple pieces, which each form their own crater down range). Craters Messier and Messier A on the moon, seen here:<br /></span></span></span><p><br /> <img src="http://sitelife.space.com/ver1.0/Content/images/store/3/7/73f7cdc8-f411-4aad-87ea-9c9dd7c14489.Medium.gif" alt="" /> </p><br /> <img src="http://sitelife.space.com/ver1.0/Content/images/store/7/13/57f38e05-db5a-4fd4-8d91-96e80b563ed8.Medium.jpg" alt="" /> <div class="Discussion_UserSignature"> </div>