Category Archives: New Horizons mission

Announcing Charon’s Dark Pole

What’s Causing THAT?

These recent images show the discovery of significant surface details on Pluto’s largest moon, Charon. They were taken by the New Horizons Long Range Reconnaissance Imager (LORRI) on June 18, 2015. The image on the left is the original image, displayed at four times the native LORRI image size. After applying a technique that sharpens an image (called “deconvolution”), details become visible on Charon, including a distinct dark pole. Deconvolution can occasionally introduce “false” details, so the finest details in these pictures will need to be confirmed by images taken from closer range in the next few weeks. Credits: NASA/Johns Hopkins University Applied Physics Laboratory/Southwest Research Institute

As the New Horizons spacecraft gets closer to Pluto, we are seeing more detailed images of this world and its companion, Charon. The latest ones, taken with the LORRI instrument onboard the spacecraft, show what looks like a darkened pole on Charon, a somewhat lighter region below it, and some bright regions along the limb. “Fascinating” as Mr. Spock would say. But, what is happening at Charon to make it look like that? The final answer is a couple of weeks away, so let’s talk about how we figure out what’s happening at a world (planet, dwarf planet, moon, asteroid, or comet) from images of it.

An artist’s conception of Charon (with Pluto in the background). The plumes and brighter spots depicted on Charon’s “left side” are thought to be created as water (with some ammonia hydrate mixed in) “erupts” from deep beneath the surface. The material sprays out through cracks in the icy crust, immediately freezes and snows crystalline ice down onto the surface, creating a water-ammonia hydrate ice field. Such fields were detected and studied using the near-infrared imager on Gemini North. (This composite image includes Pluto and Charon models (enhanced), courtesy of Software Bisque. www.seeker3d.com, with plumes and ice fields added by Mark C. Petersen, Loch Ness Productions. Star field from DigitalSky 2, courtesy Sky-Skan, Inc.)

As in all other aspects of planetary science, you have to look for processes on the world you’re studying to understand how they affect the surface of that place. For example, if you were approaching Earth and were still quite a ways away as you came in to assume a standard orbit (Mr. Sulu), you’d likely notice the poles, the bluish color, and the darker areas that indicate land masses. The existence of ice at the poles tells you something about the climate and temperature in those regions. The bluish water in a liquid state tells you that conditions are good enough to permit liquid water. And, the land masses have many messages of their own, from the signatures of volcanoes to the ongoing (and long-term) deformation of the surface due to plate tectonics. What you see on Earth, even at the most cursory level — and at Pluto and Charon — are all caused by complex interactions comprising chemical reactions, atmospheric mixing, and actions going on below the surface.

So, with that in mind, what’s going on at Charon? I wish I could tell you for sure. But, it looks really, really interesting! Now that we’re seeing a great variety of surface features (or, as the scientists call it, “terrain types”) it’s a hint that Charon is not just a frozen dead world. A dark terrain could indicate some sort of chemical interaction as sunlight hits specific ices on the surface. That normally happens with methane-rich ice, which Charon doesn’t appear to have much (if any) of. Instead, it has been measured to be mostly water and nitrogen ice.

However, I suspect there’s more going on at Charon than meets the eye.

A few years ago, we created a graphic “approximation” of Charon for a project with Gemini Observatory. We had to guess at what the surface looked like. You can see that, even in 2007, we had an idea that there’d be darker areas on an already darkish object. The real interesting bit was that astronomers using Gemini telescope had spotted what looked like evidence for geyser-like activity on Charon. I will be really interested to see if New Horizons finds that same evidence and confirms such activity. If it does, then we’re looking at a dynamic world with an interior that is forcing mixtures of ammonia hydrates (ammonia mixed with water) and water crystals onto the surface.  And, THAT’s cool.

I don’t know why Charon has a dark pole, yet. I suspect that the New Horizons mission team members don’t YET know for sure. They’re likely going through all the ideas en masse, and once they have more data, we’ll all know what’s ticking inside this little world.

Dust in Space!

A Student-built Instrument is Teaching us about Dust in Space

When I went back to school to pursue graduate studies, I applied for on-campus jobs related to my interests in astronomy and planetary science. One I applied for was a student-controlled mission, the other was a place on a research team where I would eventually work with Hubble Space Telescope data. I got the second one, which turned out to be a real turning point in my career studying astronomy as well as being a science writer.

The location of the Venetia Burney Student Dust Counter onboard New Horizons. Courtesy NASA/APL/New Horizons

The school was the University of Colorado, which is the premier place to be if you want to work on space missions as an undergraduate or a grad student. I’m often meet CU grads at NASA and other institutions who got their start working on some mission or another while at the university. Which brings me to the latest student-run effort: the Venetia Burney Student Dust Counter (SDC) onboard the New Horizons mission on it’s way to an encounter with dwarf planet Pluto. It was designed, built, and is run by students. It’s named for Venetia Burney Phair, a British woman who, as a young girl, sent in the name “Pluto” for Clyde Tombaugh’s newly discovered planet back in 1930.

Dr. Mihayl Horanyi (University of Colorado) presents Mrs. Venetia Burney Phair with a plaque dedicating the Student Dust Counter in her name. Courtesy NASA/APL/New Horizons

As the spacecraft swoops through the solar system, the SDC gathers dust, literally. The impacts of the dust on the detector tell the mission scientists something about the sizes and distribution (how much dust there is in given areas of the solar system) of particles along the mission trajectory.

To understand why this counter is important, let’s look at dust in the solar system in general. We find it everywhere, spread throughout interplanetary space. It’s more dense in some places (such as ring systems or along comet orbits) than in others, and its presence tells us something about what’s been happening in that area of the solar system. Comets spread dust as they warm up near the Sun, and asteroids generate dust as they orbit. Collisions are great creators of dust, particularly impacts between asteroids, asteroids onto planet surfaces,  and collisions between small bodies in the outer solar system. Interstellar dust comes zipping through our neighborhood; it can collide with comets, asteroids, and other objects, sending dust out to interplanetary space, too. Our solar system continues to be a busy place, even down to the production of dust!

Astronomers know more about the dust in the inner parts of the solar system, largely because there have been more missions swooping through this part of the neighborhood. What we don’t have a lot of knowledge about is the dust environment in the outer solar system. In particular, we need to know more about the dust in the Kuiper Belt region: what’s its made of and where it comes from.

This is where the SDC comes in very handy. It has been counting dust ever since just after launch, making the first-ever measurements of very small grains of dust (called sub-micron-sized particles), along its route, and will continue to do so as the spacecraft continues through the Kuiper Belt (where Pluto orbits). The major idea behind this experiment is to measure how the distribution of dust changes through the solar system, which the SDC is doing very well. It’s the first (and so far only) dust detector to be flown out to such a distant realm (beyond the outer gas giants, and is giving the mission scientists a more complete look at dust production and dust “transport” through the solar system than they’ve ever had before.

What tickles me is that students are doing this project, in a grand tradition that I was (and am) proud to be part of at my alma mater. There have been research papers generated by the students and scientists attached to the mission, and there will be more. All in all, it’s already a great success story for the New Horizons mission.

Keep up with the latest news about the New Horizons mission on the mission web page and keep checking back. Flyby date with Pluto is a month away! There’s a LOT more cool stuff to come!