File:Schubert and Chekhov craters EW0228589220G.png

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Summary

Description
English: Date acquired: October 31, 2011

Image Mission Elapsed Time (MET): 228589200, 228589220, 228589204 Image ID: 956051, 956056, 956052 Instrument: Wide Angle Camera (WAC) of the Mercury Dual Imaging System (MDIS) WAC filters: 9, 7, 6 (996, 748, 433 nanometers) in red, green, and blue Center Latitude: -37.80° Center Longitude: 303.8° E Resolution: 655 meters/pixel Scale: Scene is approximately 700 km (435 miles) across Incidence Angle: 71.1° Emission Angle: 15.9° Phase Angle: 86.8°

Of Interest: Two prominent basins, Chekhov at the upper left and Schubert at lower right, are both just under 200 km in diameter but have very different appearances. Chekhov has a prominent peak ring and its older age is reflected in the numerous craters that have battered its rim and floor. Schubert's floor is smooth with only a hint of its peak ring peeking through.

This image was acquired as a high-resolution targeted observation. Targeted observations are images of a small area on Mercury's surface at resolutions much higher than the 250-meter/pixel (820 feet/pixel) morphology base map or the 1-kilometer/pixel (0.6 miles/pixel) color base map. It is not possible to cover all of Mercury's surface at this high resolution during MESSENGER's one-year mission, but several areas of high scientific interest are generally imaged in this mode each week.
Date
Source A TALE OF TWO BASINS
Author NASA/Johns Hopkins University Applied Physics Laboratory/Carnegie Institution of Washington

Licensing

Public domain This file is in the public domain in the United States because it was solely created by NASA. NASA copyright policy states that "NASA material is not protected by copyright unless noted". (See Template:PD-USGov, NASA copyright policy page or JPL Image Use Policy.)
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current03:38, 15 January 2020Thumbnail for version as of 03:38, 15 January 20201,328 × 1,255 (4.78 MB)JstubyUser created page with UploadWizard
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