Saturday 20 May 2017

Canyons on Charon



This week’s image shows a canyon system on Charon, the largest moon of Pluto. This is a very interesting solar system body, as it is only recently that we have gotten a good look at its surface. This image comes from the New Horizons probe which visited the Pluto system in 2015. New Horizons has provided us with a huge amount of data about these small worlds, which will keep planetary scientists busy for years to come, however it had relatively little time to observe the Pluto system, as it never went into orbit around either Pluto or Charon. All of the images were recorded during a brief flyby, and so the observations had to be carefully planned in order to maximise the amount of information acquired. The distance to the Pluto system means that follow up observations aren’t likely any time soon. New Horizons is still operational, and will go on to examine other objects in the Kuiper Belt, however it will be decades before another spacecraft can reach Pluto, even if one were sent in the next few years. 



Charon is one of several small objects to orbit Pluto, but stands out due to its large size. It is almost half the size of Pluto, making it one of the largest moons relative to the planet it orbits, it is likely that it evolved independently of Pluto and was later captured by it. The full image shows how large this canyon is relative to the size of the moon. It is one of several canyons which scar the surface of this moon, another canyon can be seen in teh image below, but this one was imaged at an oblique angle, showing how deeply it cuts into the surface of Charon. NASA’s description of this image notes that this canyon seems to be 9 km deep in places, and that its cliffs might be the tallest in the solar system. 

In their description of the first image the new Horizons team note that this canyon lies on the boundary between the highlands to the top of the image and a large plain to the south. Both terrains are heavily cratered, and this highlights something very interesting about this small moon, which makes it very different to the dwarf planet it orbits; Charon is heavily cratered, whereas Pluto is not. 

Pluto has large regions with very few impact craters. Charon on the other hand is pitted with craters, and looks much more like Mercury or Earth’s Moon. This striking contrast is quite surprising. Since both objects are in close proximity they would be expected to be hit by the same number of meteorites and have the same density of craters. The fact that this is not the case indicates that Pluto has a surprisingly young surface. The icy surface of Pluto has clearly been resurfaced regularly, and this suggests that the planet could be far more active than expected given that it is so small, and so wouldn’t be expected to retain much heat. Precisely why Pluto is so active remains to be determined, but it makes these small planets quite an intriguing target for future missions. New Horizons’ observations definitely raised as many questions as they answered. 

Image Credits
 NASA/JHUAPL/SwRI
NASA/JHUAPL/SwRI

Further reading
Differences between Pluto and Charon

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