First science results from the MESSENGER Mercury flyby
The MESSENGER mission held a press conference this morning to describe the first, preliminary conclusions from the first Mercury flyby. I'd say that the overarching conclusion is: MESSENGER will produce an absolutely fantastic data set. What we've seen so far is just a taste of what's to come. I wrote up a detailed story on the Mercury science results with lots of pictures here. I have to hand it to the MESSENGER team: they didn't pull any punches when it came to the science. I liked that but it did make it a bit challenging to get my story finished today -- it took a lot of effort to work through all those details and try to find ways to explain the science. In the end, I didn't have time to post it until after I put the baby to bed tonight. And almost none of what was presented today made it into the Associated Press story on the flyby (except the "spider" -- read my story to see what that is).
Among the many images that they released today was a color view of the departing shot of Mercury, the side that was mostly unseen by Mariner 10. Like the approach view that they released last week, it was a false-color view, showing information from the violet to the infrared, a bit broader than the spectrum to which human eyes are sensitive. I brought the image into Photoshop and cranked up the saturation to show just how much information is waiting to be pulled out of this data set. Based on all these garish colors the geologists on the team will start mapping the globe, figuring out which areas are covered with materials similar to those found in other areas, figuring out which stuff is fresh and which stuff has been exposed to space weathering for a long time, and figuring out some spots where they want to make absolutely sure MESSENGER gets some really high-resolution views.
NASA / JPL / CIW / Emily Lakdawalla
The image at left represents a false color view of Mercury captured by MESSENGER as it sped away from its first encounter with the planet on January 14, 2008. The image is composed of three captured through filters with wavelengths of 1000, 700, and 430 nanometers (infrared, red, and violet), covering a wider range of the electromagnetic spectrum than human eyes can see. The image on the right is the same, but the saturation of its colors has been severely enhanced. The garish colors pick out interesting compositional differences across the surface. Fresh craters and their rays show up as bright blue. The Caloris impact basin appears deep orange, surrounded by a dark red ringl craters in its interior have deep purple rims. To the south, near Mercury's limb, a violet stain surrounds the crater Tolstoj, which, like Caloris, has an orange interior. These color differences hint at compositional differences, but exactly how the composition differs is not yet known.
I've gotten several emails from people complaining about how they haven't released a "true color" view yet. I think that one reason that they haven't is that Mercury is kind of underwhelming when seen in "true color," nearly gray in its appearance, like the Moon. You don't gain a lot of understanding of Mercury when you view it in "true color." Another reason is that calibrating space cameras is a tricky thing; they don't even know yet exactly how to manipulate the contributions of different-color-filter images to produce something that simulates what the human eye would see if they were there.
However, if you're resourceful, and if you're not constrained by the desire to be scientifically exact about how you process an image, you can achieve a pretty good approximation of a true-color view of Mercury from the data that's already been released. Eric Landreneau sent me these two versions of the released views, with their colors manipulated so that they approximate the colors that you might see if you were there.
NASA / JHUAPL / CIW / Eric Landrenau
MESSENGER approaches Mercury
To oversimplify the process he used to create these images: Eric reasoned that, given the fairly smoothly sloping spectrum released by the MASCS team, you can take the extended-spectrum (infrared to violet) images released by the MESSENGER team and compute new images that approximate the red-green-blue range that our eyes can see. I'm not going to get more detailed than that; for a little more insight into how you might go about doing this, you can read the Wikipedia entry on CIE color space.
Finally, I'll post a couple of notes from today's press conference that didn't make it into my story. One of the press questions at the end was from a tiny local radio station who said that he knew he was being listened to by an audience of schoolkids; what would the science panel say to those kids? One panelist, Bob Strom, talked briefly about how much of a "turn-on" science was, which was a bit awkward; but, with a couple more minutes to think, Sean Solomon really stepped up. Here's what he said, which is, I think, a good message to deliver to high school kids, or college kids, kids old enough to realize they almost certainly will not be astronauts (just like, with only rare exceptions, they almost certainly will not be professional sports players or movie stars or President): there's many different ways to contribute to space exploration, many different challenges you can attempt to meet, depending upon your own strengths and inclination:
Space exploration is a lot more than space science. We're flying a spacecraft that owes its origin and livelihood to hundreds of engineers and technicians who designed it, who worried about how it would survive so close to the Sun, how it would survive radiation, how it would live for nearly 8 years, how it would communicate its scientific findings back to the Earth, how it would get launched, how it would find its way billions of miles, 15 times around the Sun, to get into Mercury orbit 6 and a half years following its launch. There are a lot of ways to contribute to space exploration. Science is one of them. The engineering of building, operating, and maintaining spacecraft is a terrific field, and we [gesturing to the panel] would not be up here if we did not have an outstanding team of engineers who put this spacecraft together and keep it going.
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