Tuesday, July 6, 2010

Reiner Gamma Region of Interest

The heart of the region of interest in the Reiner Gamma swirl. Astronauts exploring this region will address longstanding questions about the origins of this distinctive natural feature. Image width is 510 m [NASA/GSFC/Arizona State University]. View larger image


First identified by early astronomers during the Renaissance, the Reiner Gamma formation has been a subject of powerful scientific study for almost five decades and is one of the maximum-priority targets for future human lunar exploration. Reiner Gamma is one of the most idiosyncratic natural features on the Moon. This striking, tadpole-shaped swirl has a considerably higher reflectance than the surrounding mare basalts.

WAC monochrome context image of the Reiner Gamma swirl. Arrow indicates approximate location of NAC detail above. Image M117874527M; scene width approximately 80 km [NASA/GSFC/Arizona State University]. View larger image

Several LROC Featured Images have shown stunning new images of the swirls near Mare Ingenii which are similar to the swirls of Reiner Gamma. Reiner Gamma, however, is the "prototypical" lunar swirl.

A concept that comes up frequently in lunar science is "space weathering." This term is used to describe a suite of natural processes (including micrometeoroid impacts and exposure to the solar wind) that can alter the spectral properties of lunar surface materials. Since the reflectance of the lunar surface within the Reiner swirl is so diverse from the surrounding mare, some process may have altered the space weathering defenselessness of the swirl materials. There are several theories to account for the existence of the Reiner Gamma swirl. Results from previous lunar missions (including Lunar Prospector) have indicated that the swirl region has an elevated magnetic field, so it's probable that an event hundreds of millions of years ago modified the magnetic properties of the surface materials, deflecting the solar wind and changing how the reflectance is customized by space weathering. Some investigators have proposed that the coma of a comet - streaking in just above the surface - interacted with the lunar surface, changing the surface properties to the degree where the Reiner Gamma swirl could persist for millions of years.

However, based on the available data, we just don't know for sure! That's not a bad thing; if we knew all the answers to all of these interesting problems, we wouldn't ever need to explore! We will not know what caused the swirls of the Reiner Gamma formation until human explorers return to this region to do the fieldwork and collect the samples that will enable us to answer this essential scientific question.

Plan your own adventure to the mysterious swirls of Reiner Gamma! Think about where you would go to answer these scientific questions!

However, based on the available data, we just don't know for sure! That's not a bad thing; if we knew all the answers to all of these fascinating problems, we wouldn't ever need to explore!

To Learn More Visit http://www.nasa.gov/mission_pages/LRO/multimedia/lroimages/lroc-reinergamma-20100629.html



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