In northern Brazil, underneath tropical savanna vegetation, lies the evidence of an ancient collision. Roughly 220 million years ago, geologists estimate, a meteorite struck Earth here. Despite its age, Serra da Cangalha remains Brazil’s best-preserved impact crater, resting upon largely undisturbed sediments laid down some 300 million years ago.
The Advanced Spaceborne Thermal Emission and Reflection Radiometer (ASTER) on NASA’s Terra satellite took this picture of Serra da Cangalha on June 23, 2006. In this simulated-true-color image, varying shades of green define the local cerrado landscape—a mix of savanna and riparian forest (forests along a river or stream). Occasional patches of purple-gray indicate bare ground. Regardless of the overlying vegetation, the crater’s structure remains obvious, showing a series of concentric rings. The crater’s diameter is roughly 13 kilometers (8 miles), and its innermost bowl is rimmed by rocks rising 420 meters (about 1,380 feet) above the surrounding land. The crater walls cast shadows on the nearby landscape.
Serra da Cangalha’s status as an impact crater took some time to be established. That it might be such a structure was first proposed based on several factors: its circular shape, the absence of carbonate or salt layers in nearby sediments, which would suggest a salt dome, and the fact no volcanic rocks appeared in a drill core from the crater itself. Even more definitive signs of an impact appeared in the form of shatter cones—conical-shaped, grooved rocks known only to appear in impact craters. Blocks of fossil wood have also been found in the crater’s central uplift area.
NASA image created by Jesse Allen, using data provided courtesy of NASA/GSFC/METI/ERSDAC/JAROS,
and U.S./Japan ASTER Science Team. Caption by Michon Scott.
Roughly 220 million years ago, geologists estimate, a meteorite struck Earth here. Despite its age, Serra da Cangalha remains Brazil’s best-preserved impact crater, resting upon largely undisturbed sediments laid down some 300 million years ago.
Spider Crater rests in a depression some 13 by 11 kilometers (8 by 7 miles) across. Meteorite craters often have central areas of uplift, and Spider Crater fits this pattern. Spider Crater sits in a depression and has a central uplift area characteristic of impact craters, it shows extreme differences in erosion, giving it a unique appearance.
Deep in the Sahara Desert lies a crater. Nearly a perfect circle, it is 1.9 kilometers (1.2 miles) wide, and sports a rim 100 meters (330 feet) high. Modern geologists long debated what caused this crater, some of them favoring a volcano. But closer examination of the structure revealed that the crater’s hardened “lava” was actually rock that had melted from a meteorite impact.
Wolfe Creek Crater is the second largest crater in the world from which meteorite fragments have been collected. Because of its excellent preservation, the crater clearly shows the classic features that result from a large meteorite striking the Earth.