The Edge of Mercury, Moody and Gray

The entire universe in blog form
June 26 2013 10:30 AM

Mercury’s Limb

Mercury from MESSENGER.
The crater-laden surface of Mercury, as seen by the Sun-blasted Messenger spacecraft. Click to hermesenate.

Photo by NASA/Johns Hopkins University Applied Physics Laboratory/Carnegie Institution of Washington

I haven’t posted a dramatic picture of Mercury from the Messenger (MErcury Surface, Space ENvironment, GEochemistry, and Ranging) spacecraft in a long time—not since I moved to Slate, certainly—and I really like this new one, shown above. This is the limb, or apparent edge, of the planet seen near the planet’s south pole from the orbiting spacecraft.

Phil Plait Phil Plait

Phil Plait writes Slate’s Bad Astronomy blog and is an astronomer, public speaker, science evangelizer, and author of Death From the Skies!  

Funny how much it superficially looks like the Moon. Both are airless and rocky, so the color and cratering are similar. But even if you woke me out of a cold sleep, I could tell you that’s not the Moon. I don’t know why, exactly: I’m familiar enough with the Moon’s surface but not so much that I could recognize any random spot.


But even so, these features are just different. The contrast is different than on the Moon, and the crater sizes don’t seem to have the same distribution. Ignoring the craters, the surface also seems flatter than the Moon's, which is littered with hills and mountain chains and hummocks.

This shot of Mercury does show some neat features. The crater with rays, those liner streaks, is probably the most obvious. That’s Han Kan, a 50-kilometer (30-mile) wide impact crater. Rays are formed when plumes of material shoot out from the impact site and settle onto the surface. They wear away with time (erosion from micrometeorites, impact from the solar wind, and even the thermal stress of the extreme temperature difference between day and night contributes to that), so seeing a rayed crater indicates relative youth.

You can also see a couple of double-walled craters, like a crater in a crater. That sometimes forms in larger impacts, though the exact physics isn’t completely understood. (It’s hard to model a gigantic hypervelocity impact when you’re not exactly sure what all the physical processes going on happen to be.) The one just below center is Bach—here’s a shot of it looking straight down—and a little to the north is Cervantes. You can spot more of them, too, if you look around. It helps to have an atlas.

Mercury is a very hard planet to observe from Earth; its orbit around the Sun is smaller, so it never gets very far from the star. That means it’s only up at dawn and dusk, so you don’t get much time to view it before either it sets or the Sun rises. You’re also always looking near our horizon, through our thick air, distorting and dimming the view. In other words, there’s nothing like being there.

We’ve sent probes to the smallest planet in the past, but they were all “fly-by” missions; Messenger was the first to orbit. It’s been an amazing beast, withstanding the heat and radiation of the Sun for years—it went into orbit around Mercury in March 2011 after several years of travel to get there. The primary mission ended in 2012, but it was extended a year, and hopefully it will be extended again; we’re still awaiting word if it will get more time.

Obviously, I hope it does. Mercury is a fascinating little world, so familiar yet so strange. It’s certainly worth taking more time to get a closer look.



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