The latest featured image from NASAs MESSENGER spacecraft, soon to complete its first year in orbit around Mercury, shows the central peak of the 78-mile (138-km) wide crater Eminescu surrounded by more of those brightly-colored surface features dubbed hollows. Actually tinted a light blue color, hollows may be signs of an erosion process unique to Mercury because of its composition and close proximity to the Sun.
First noted in September of last year, hollows have now been identified in many areas across Mercury. They showed up in previous images as only bright spots, but once MESSENGER established orbit in March of 2011 and began high-resolution imaging of Mercurys surface it became clear that these features were something totally new.
The lack of craters within hollows seems to indicate that they are relatively young features. In fact, they may be part of a process that continues even now.
Analysis of the images and estimates of the rate at which the hollows may be growing led to the conclusion that they could be actively forming today, said David Blewett of the Johns Hopkins University Applied Physics Laboratory (APL).
One hypothesis is that the hollows are formed by the sublimation of subsurface material exposed during the creation of craters, around which they are most commonly seen. Being so close to the Sun (29 million miles/46 million km at closest) and lacking a protective atmosphere like Earths, Mercury is constantly being scoured by the powerful solar wind. This relentless stream of charged particles may literally be sandblasting exposed volatile materials off the planets surface!
The image above shows an area approximately 41 miles (66 km) across. It has been rotated to enhance perspective; see the original image and caption here.
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