Surprises from Mercury
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January 30, 2008: After a journey of more than 2 billion miles and three and a half years, NASA's MESSENGER spacecraft flew by Mercury on Jan. 14, 2008, and it has beamed back some surprises.
"This flyby allowed us to see a part of the planet never before viewed by spacecraft, and our little craft has returned a gold mine of exciting data," said Sean Solomon, MESSENGER's principal investigator at the Carnegie Institution of Washington. The spacecraft's cameras and other sensors collected more than 1,200 images and made the first up-close measurements of Mercury since Mariner 10 visited the planet in the mid-1970s.
Above: The "Spider crater" located on the floor and near the center of Mercury's giant Caloris basin. [Larger image] [More]
Researchers once thought Mercury to be much like Earth's moon, but MESSENGER has found many differences. For instance, unlike the moon, Mercury has huge cliffs with structures snaking hundreds of miles across the planet's face. The spacecraft also revealed impact craters that appear very different from lunar craters. One particularly curious crater has been dubbed "The Spider."
"The Spider has a crater near its center, but whether that crater is related to the original formation or came later is not clear at this time," said James Head, science team co-investigator at Brown University, Providence, R.I.
When Mariner 10 flew by Mercury in the 1970s, it saw only a portion of Caloris basin. Now that MESSENGER has shown scientists the basin's full extent, its diameter has been revised upward from the Mariner 10 estimate of 800 miles to perhaps as large as 960 miles from rim to rim. Researchers already knew that Caloris was one of the largest impact craters in the solar system; MESSENGER has shown it is even bigger than they thought!
Right: During the Jan. 14th flyby, MESSENGER made the first measurements of Mercury's magnetospheric plasma. Click to play a movie of data recorded by the spacecraft's Fast Imaging Plasma Spectrometer (FIPS). [Movie] [More]
MESSENGER's suite of instruments also detected ultraviolet emissions from sodium, calcium and hydrogen in Mercury's exosphere. (An exosphere is a super-low-density atmosphere probably formed, in this case, from atoms sputtering off Mercury's surface. The sputtering may be caused by contact with hot plasma trapped in Mercury's magnetic field.) MESSENGER encountered Mercury's sodium-rich exospheric "tail" which extends more than 25,000 miles from the planet and also discovered a hydrogen tail of similar dimensions.
"We should keep this treasure trove of data in perspective," said project scientist Ralph McNutt of the Applied Physics Laboratory, Laurel, Md. "With two flybys to come and an intensive orbital mission to follow, we are just getting started to go where no one has been before."
Editor: Dr. Tony Phillips | Credit: Science@NASA
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MESSENGER mission home page
MESSENGER Press Conference Multimedia Page
Mercury Flyby Sets Stage for Discovery (Science@NASA)
Mercury flyby gallery
The MESSENGER project is the seventh in NASA's Discovery Program of low-cost, scientifically focused space missions. The Applied Physics Laboratory designed, built and operates the spacecraft and manages the mission for NASA. MESSENGER stands for MErcury Surface, Space ENvironment, GEochemistry and Ranging.
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