In southeastern Mongolia, roughly halfway between Ulaanbaatar and Beijing, lies an ancient crater. Tabun Khara Obo (sometimes spelled with hyphens) was first identified as a probable impact crater in 1976, although confirmation of the hypothesis only occurred decades later. Drilling at the site in 2008 revealed rock features consistent with high-speed impacts such as those caused by meteorites.
The Advanced Land Imager (ALI) on NASA’s Earth Observing-1 (EO-1) satellite acquired this true-color image on August 28, 2009. Sunlight shines from the southeast, leaving the northern and western slopes in shadow. The crater’s rim rises some 20 to 30 meters (65 to 100 feet) above the crater bottom. The crater occurs on a block of Proterzoic rock more than 600 million years old, but the crater’s age—which may be considerably younger—has not yet been identified.
The dark, irregularly shaped area in the lower right corner of the image results from vegetation, likely occurring along a river channel. For the most part, the scene shows an earth-toned, arid landscape.
NASA image created by Jesse Allen, using EO-1 ALI data provided courtesy of the NASA EO-1 Team. Caption by Michon Scott.
Acquired on August 28, 2009, this true-color image shows the Tabun Khara Obo in southeastern Mongolia. Sunlight shines from the southeast, leaving the crater’s northern and western slopes in shadow.
Anderson, P., Ochirbat, M. (2004). The Tavan Har Impact Crater, eastern Gobi, Mongolia: A study of impact related features, Seventeenth Annual Keck Research Symposium in Geology Proceedings. Keck Geology Consortium, Northfield, MN.
Earth Impact Database. Tabun-Khara-Obo. Planetary and Space Science Centre, University of New Brunswick. Accessed September 4, 2009.
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.
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.
Acquired October 10, 2007, this false-color image shows Chiyli Crater in western Kazakhstan. Vegetation appears red, and clings primarily to riverbanks near the crater. Sunlight illuminates south-facing slopes, including the central peak of the crater.