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View of the Steven F. Udvar-Hazy Center tower at sunset

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Bob Hoover Gives an Air Show Performance

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Images of Mercury from MESSENGER Spacecraft

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  • Two perspectives of the surface of Mercury show that tectonic landforms called lobate scarps (rising of land) are visible in large and small forms on the planet.
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    MESSENGER confirmed that the contraction of Mercury resulted in a global array of lobate scarps, tectonic landforms that are the surface expression of thrust faults.  Enterprise Rupes is the Goliath of lobate scarps on Mercury (top, white arrows). At about 1000 km long, comparable in length to Earth’s San Andreas fault, and with over 3 km of relief it is the largest lobate scarp on Mercury.  Images obtained after MESSENGER’s altitude was lowered during the last phase of its mission have revealed a population of small fault scarps (bottom, white arrows) that can be more than an order of magnitude smaller in size than their larger counterparts.  These small scarps are less than 10 km in length and have only tens of meters of relief.  They are comparable in size and morphology to small fault scarps imaged on the Moon by the Lunar Reconnaissance Orbiter.

  • Two perspectives of the surface of Mercury show that tectonic landforms called lobate scarps (rising of land) are visible in large and small forms on the planet.

Credit:

<p>NASA/Johns Hopkins University Applied Physics Laboratory/Carnegie Institution of Washington/Smithsonian Institution</p>

Source:

NASA/Johns Hopkins University Applied Physics Laboratory/Carnegie Institution of Washington/Smithsonian Institution

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NASA/Johns Hopkins' Applied Physics Laboratory

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Contact NASA/Johns Hopkins' Applied Physics Laboratory

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Open daily 10:00 am – 5:30 pm

National Air and Space Museum

National Air and Space Museum 650 Jefferson Drive SW
Washington, DC

202-633-2214

Free Timed-Entry Passes Required

Steven F. Udvar-Hazy Center

Steven F. Udvar-Hazy Center 14390 Air and Space Museum Parkway
Chantilly, VA 20151

703-572-4118

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