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Headshot of Emily Lakdawalla

Pluto and Charon spin among the stars

Posted by Emily Lakdawalla

16-06-2015 20:10 CDT

Topics: trans-neptunian objects, New Horizons, pretty pictures, Pluto, amateur image processing, Charon, dwarf planets beyond Neptune, many worlds, animation

I've spent a happy couple of days playing with raw data downloaded from the New Horizons website. Before I wander into lengthy descriptions of what you can and can't do with these photos, I thought I'd share the result of my work. This animation consists of images of Pluto and Charon and background stars taken between June 1 and June 15. For this animation, I chose to align things on background stars. That makes Pluto and Charon whirl and dance about their mutual barycenter, a point that drifts slightly to the right with respect to the background stars as New Horizons approaches them.

In this animation, first you see just the images at the brightness at which they were posted to the Web. Then I brighten the images, which washes out all the detail on Pluto but which reveals some background stars. Then I overlay an image from the ESO Digital Sky Survey to show you how many more stars (and dust clouds) there are in this region of space, unseen in the short exposures that the New Horizons LORRI camera takes to image Pluto and Charon. As far as I can tell, other moons like Nix and Hydra are not yet visible in these full-resolution LORRI images.

Pluto and Charon spin among the stars (as of June 15, 2015)

NASA / JHUAPL / SwRI / Emily Lakdawalla

Pluto and Charon spin among the stars (as of June 15, 2015)
Faint stars in the background of raw images from New Horizons allow the images to be aligned, giving us a sense of New Horizons' changing view on Pluto and Charon as it approaches the dancing pair. Images were taken between June 1 and 15, 2015. More information in this blog entry.

So how did I get to this animation? I began with data off of the New Horizons website. New Horizons took these photos from a variety of distances. More challenging, the spacecraft usually rotates in the time between imaging sessions, so "up" (or celestial north, or whatever reference direction you want to use) is in a different orientation for each set of pictures. You can see that just animating sequential photos into a GIF produces something pretty jerky.

Herky jerky Pluto approach images

NASA / JHUAPL / SwRI

Herky jerky Pluto approach images

Another challenge with these images is that they have experienced an automatic exposure adjustment and are saved in JPEG format, which does some nasty things to the quality of the data. In particular, those faint background stars can be very hard to find among all the JPEG artifacts. Here is what a fainter star looks like. It should be a fuzzy roundish dot, but instead it's a misshapen splat with lots of bright and dark pixels located well away from the star. (It also looks like there are creepers in the background. Those are the evil JPEG spirits. Kidding.)

Enlargement of a JPEGged star

Fortunately for us, most of the time New Horizons takes more than one photo each time it observes Pluto and Charon. By taking several photos with slight pointing differences between them, the New Horizons team can produce "super-resolution" images showing details finer than one pixel. They do this with losslessly compressed data from the spacecraft. That's why their processed image releases look so much nicer than anything an amateur can produce with raw data. A lot of the fine detail is lost with the JPEG compression of the public images. This is no accident; it's a way for the mission to share all the images nearly as soon as they arrive on Earth, allowing the public to enjoy the view, while substantially reducing the images' scientific quality, to prevent the team from being "scooped." We can't recover this lost detail from the raw JPEGs, but at least we can use the multiple exposures to reduce the JPEG compression artifacts. (The detail is "lost" to us for now, but not forever; the New Horizons team has it, and they will give it all to us when they archive the data in the Planetary Data System eventually.)

So here are the steps it took to make the animation:

  • Download all the data and put all the images into a single Photoshop file
  • Sort each observation into folders
  • Enlarge the images 4x
  • Align all the images within observations precisely on each other
  • Average the images within each observation together, producing a single image for each observation
  • Reduce the images by 2x (leaving them at twice their original resolution)
  • Grab a piece of the Digital Sky Survey covering the same region of space (thanks to Alex Parker for the pointers here)
  • Resize the DSS image to match the resolution of the LORRI images
  • Rotate the LORRI images to align them to background stars

The resulting animation is fun, but it's not the only thing I can do with my aligned data set. By aligning the images on the background stars, I rotated them all into a common orientation. That means I can now make a continuous animation of Charon spinning around Pluto. I have to sort them into rotational order, and I have to resize the images to account for the varying distance between New Horizons and Pluto, and then I have to align them all on Pluto. Et voila:

Pluto and Charon rotation sequence

NASA / JHUAPL / SwRI / Emily Lakdawalla

Pluto and Charon rotation sequence
This animation contains 15 images captured between June 1 and 15. The images have been resized to account for the changing distance between New Horizons and the Pluto system during that time, which ranged from 50 to 35 million kilometers.

Now, what else can I do with these images? Hey, I can align it on Charon instead, because why should Pluto have all the fun?

Pluto and Charon rotation sequence, centered on Charon

NASA / JHUAPL / SwRI / Emily Lakdawalla

Pluto and Charon rotation sequence, centered on Charon
This animation contains 15 images captured between June 1 and 15. The images have been resized to account for the changing distance between New Horizons and the Pluto system during that time, which ranged from 50 to 35 million kilometers.

I'm very pleased with how it came out! Now, what else can I do with these pictures, as we watch New Horizons get closer and closer to Pluto and Charon?

 

 
See other posts from June 2015

 

Or read more blog entries about: trans-neptunian objects, New Horizons, pretty pictures, Pluto, amateur image processing, Charon, dwarf planets beyond Neptune, many worlds, animation

Comments:

Mike J.: 06/16/2015 09:13 CDT

I am interested in following the New Horizons encounter of Pluto. I am prepared to take a day off from work to see images or whatever data comes back. My question is what day should I plan on remaining home to see the most? Shall I take off July 14 or 15.? Or will images be much slower to arrive? I am in the Eastern Time Zone.

Chris: 06/17/2015 12:39 CDT

Mike, thankfully Emily is prescient as always and already has a very thorough post written about the days around encounter. http://www.planetary.org/blogs/emily-lakdawalla/2015/03101637-pluto-image-expectations.html The short answer is, there will be some images returned before the flyby, and some shortly after. Not a huge amount- they will come down eventually. Not much will happen on earth on the 14th besides receiving a beacon from NH as the spacecraft will be very busy. I'm looking forward to it too!

Mewo: 06/17/2015 02:04 CDT

I see that some of the latest LORRI images are rotated 90 degrees with respect to each other. The New Horizon team must be looking for rings and more little moons.

Astrostu: 06/17/2015 10:58 CDT

Mewo— Yes, rings, moons, and potential hazards.

RRLittle: 06/17/2015 02:10 CDT

Great work there. Certainly evident now that these two are tidally locked!

physicsfun: 06/18/2015 12:49 CDT

Love to see these images aligned on the center of mass of the system.

Michael Richmond: 06/18/2015 12:01 CDT

Great work, Emily! I peeled apart your GIF and measured the positions of Pluto and Charon in each image, then computed the position of Charon relative to Pluto, and finally made a graph showing the apparent orbital motion. I can provide details upon request. See the graph at http://stupendous.rit.edu/richmond/temp/charon_orbit.png

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