Help Shape the Future of Space Exploration

Join The Planetary Society Now  arrow.png

Join our eNewsletter for updates & action alerts

    Please leave this field empty
Blogs
Facebook Twitter Email RSS AddThis

Headshot of Emily Lakdawalla

Roundup of the September 11, 2015 New Horizons raw image release

Posted By Emily Lakdawalla

15-09-2015 16:47 CDT

Topics: trans-neptunian objects, New Horizons, pretty pictures, Pluto, amateur image processing, Charon, Pluto's small moons

Last Friday the Internet received its first post-encounter pile of goodies from the New Horizons flyby of the Pluto system. The mission gave a preview of some of the good stuff the day before, but there was a lot more to be excited about in the first of what will be many fun Friday raw image releases on the mission's raw image website. Last Friday's haul of new pictures included:

A very important difference between the latest haul of images and the ones we were getting in July is that New Horizons is now transmitting all its data to Earth with lossless compression. This is a major change in plan. Principal Investigator Alan Stern explained in a Hangout on Friday. The science team found that while performing JPEG compression on the images before transmitting them from the spacecraft made the data come down more quickly, the cost in terms of the quality of the data was too high; too many science investigations were being too negatively impacted by the inability to tell the difference between small features and compression artifacts. So they have decided not to do any compression and just go straight to lossless data transmission. The images that are getting shared to the raw images website are converted to JPEG format before being shared, which does introduce compression artifacts in the images being shown to the public. In my experience of the data so far, those artifacts are minimal; these new images are far more detailed and crisp than what we were seeing in July.

To give you a sense of what we've received and how much we have left to receive, here is a visual summary of all the Pluto images released from the period spanning 48 hours before closest approach. I chose this period because I have a detailed list of observations that New Horizons planned to make during this time, so I can get a sense of what hasn't come down yet. If you look down the right side of the image, you'll see a column of text, some of which is blue and some of which is gray. If it's gray, there are no released images from that observation yet. If it's blue, some images have been released. They're in time order, so you can interpolate to get a sense of what size and resolution of Pluto images we're still waiting for. We have a lot of goodies already, but there even more yet to come. What's particularly striking is that we have nothing on the ground yet from the moment of closest approach up to about 4 hours after the flyby. One of the things they did during that time is that they shot a high-resolution mosaic in a single strip across Pluto. I'm especially looking forward to seeing the first images from that observation!

New Horizons LORRI data from 48 hours around closest approach (as of 2015-09-09)

NASA / JHUAPL / SwRI / Emily Lakdawalla

New Horizons LORRI data from 48 hours around closest approach (as of 2015-09-09)

(I plan to make summaries like this for Charon, Nix, and Hydra as well, in the future.)

What can we do with all the new data? I'm most excited about the new global views of Pluto, Nix, and Hydra. Here's that enormous Pluto global mosaic:

High-resolution global mosaic of Pluto

NASA / JHUAPL / SwRI / Emily Lakdawalla

High-resolution global mosaic of Pluto
This global view of Pluto is a mosaic of 15 individual LORRI frames captured from a distance of about 170,000 kilometers around 08:45 on July 14, 2015. It has a resolution of about 850 meters per pixel.

I could spend hours staring at this mosaic alone. I am particularly intrigued by the upper left quadrant. The ices up there are doing interesting things, and there are hints of differences in types of surfaces from place to place. It helps to play with the contrast to emphasize those differences. Play with the slider in the image below and watch how different terrain types pop out at you.

Before & After: New Horizons global view of Pluto with contrast adjustment
Before & After: New Horizons global view of Pluto with contrast adjustment
 

NASA / JHUAPL / SwRI / Emily Lakdawalla

Before & After: New Horizons global view of Pluto with contrast adjustment
A high-resolution global mosaic of Pluto looks very different with different contrast settings. In particular, darkening the image reveals very subtle brightness variations in the upper left portion of the globe.

Here is our new best view of Nix:

Nix from New Horizons

NASA / JHUAPL / SwRI / Emily Lakdawalla

Nix from New Horizons
This image is a combination of four taken on July 14 at about 8:07 UTC as New Horizons passed through the Pluto system. It has been enlarged by a factor of three from its original resolution.

It just so happens that this photo was taken at very nearly the same time as New Horizons' color camera, Ralph MVIC, took a color picture. Taking the color from that observation and combining it with the new LORRI image, you discover that Nix has a weird red crater. I don't believe I've ever seen a red crater before; impact craters are usually bluer than the stuff they sit on, because space weathering makes things red and impact craters usually dig up fresher, grayer material (which looks blue when contrasted with the redder, older surface). Maybe this crater is red because we're seeing material from the impactor. Maybe it's red because Nix really is red on the inside. Maybe it's not an impact crater.

Nix from New Horizons

NASA / JHUAPL / SwRI / Emily Lakdawalla

Nix from New Horizons
This image is a combination of four taken on July 14 at about 8:07 UTC as New Horizons passed through the Pluto system. The grayscale LORRI image has been enlarged by a factor of three and overlaid with color information from an image taken by Ralph MVIC at about the same time. Nix has an unusual red crater feature on its surface -- and no other obvious craters.

The new images of Hydra are very similar to ones we already had, but because they were returned losslessly, there is more detail visible. In particular, there are at least two small craters present:

Hydra from New Horizons

NASA / JHUAPL / SwRI / Emily Lakdawalla

Hydra from New Horizons
A stack of three images taken at about 07:42 on July 14, 2015 from a distance of 230,000 kilometers. Hydra appears to have at least two small craters on it.

Unfortunately we don't yet have MVIC color data to overlay on the LORRI image of Hydra, but one thing you can do is to compare the apparent sizes of Hydra and Nix. I say "apparent" because these things are small and lumpy and will appear to be different sizes depending upon our point of view on them:

Nix and Hydra, to scale

NASA / JHUAPL / SwRI / Emily Lakdawalla

Nix and Hydra, to scale
New Horizons took these photos of Nix and Hydra as it approached for its flyby; they have been resized to the same scale of about 380 meters per pixel. The two moons appear to be very close to the same size; in this image, Nix (left) measures 30 by 48 km, and Hydra measures 36 by 52 km. We may be seeing neither moon's longest or shortest dimensions, so these dimensions are consistent with the minimum and maximum dimensions measured from Hubble (26 by 56 km for Nix and 34 by 58 km for Hydra).

That lovely global view wasn't the only Nix data in the pile. There were also 16 images that initially looked blank. When I took a second look, though, I found something really lovely: A crescent Nix. It appears to have a bite taken out of it -- is this the rim of the red crater? Or some other feature?

Crescent Nix

NASA / JHUAPL / SwRI / Emily Lakdawalla

Crescent Nix
This is a stack of 16 images taken by New Horizons about 3 hours after closest approach. Nix's outline is very faint but clear. The resolution of this image, which has been enlarged by a factor of 3 from the original, is 310 meters per pixel, and the phase angle is 158 degrees.

I played with these Nix images for a long time yesterday evening, but they are very gnarly because of the very low light levels -- this is the one set of images for which the JPEG compression before posting has caused me problems. I wrote about the processing steps of my work on Twitter. As I was looking at images, I noticed that there were very bright pixels here in there that kept to consistent patterns from image to image, and realized that a crescent Nix is such a very faint object -- even when New Horizons is quite close to it -- that lots of faint background stars are visible in the images, and they're actually brighter than Nix appears. So I tried aligning the images on the background stars, and produced this. Not the most beautiful picture I've ever made, but it really brings home how faint the light from Nix is.

Nix crosses Orion's head

NASA / JHUAPL / SwRI / Emily Lakdawalla

Nix crosses Orion's head
New Horizons took 16 photos of Nix about 3 hours after the flyby over a period spanning about four minutes, in four sets of four rapid-fire images. Here, the images have been aligned on background stars and then stacked. With the stars fixed, a crescent Nix appears as a set of four smeared blurs. Astrometry.net successfully located the star field in Orion's head.

Let's see, what else? The additional approach images of Pluto begin to lend themselves to an approach rotation animation. I played with that for some time yesterday but am not yet satisfied with the results. Here's a version I posted on Twitter; I'll wait for more frames to come down to improve my work on it and put it in the image library.

The one body in the Pluto system for which Friday didn't provide much additional material was Charon. There were a couple more approach images downloaded, but nothing substantially different from what we've seen before. Hopefully this coming Friday's haul will include more from Charon. I don't know about you, but I can't wait for Friday -- and I think that's going to be true for the next year!

 

 
See other posts from September 2015

 

Read more blog entries about: trans-neptunian objects, New Horizons, pretty pictures, Pluto, amateur image processing, Charon, Pluto's small moons

Comments:

Mewo: 09/15/2015 11:28 CDT

Oooooooo! Nice. The data just gets better and better. Those terrain boundaries are fascinating. Are there going to be images of Styx and Kerberos as well? Would be cool to see why Kerberos is so black compared to the other moons. And finding similarities and differences between Pluto's little moons and the similarly sized PT1 will tell us so much.

stfletch: 09/16/2015 02:40 CDT

According to the JPL New Horizons flyby timeline, only a few images where taken of Kerberos and Styx and none from particualrly close range. The best images of Styx where taken from about 600,000km away at a resolution of 3km / pixel - hence we will only get an image around 2-3 pixels across. Things are a little better for Kerberos, with 2 images take from around 360,000km away at a resolution of 1.8km / pixel. Assuming a diameter for Kerberos of around 25km this would give an image 14-15 pixels across.

jumpjack: 09/16/2015 03:32 CDT

How can I project the disk into a flat (mercator or cylindrical) projection?

Joshaeus: 09/17/2015 06:55 CDT

My observations on these pics: 1 - As already noted, Tombaugh regio has few or no craters and the dark regions have a lot. 2 - Something NOT previously noted is that the other regions have intermediate numbers of small craters, not dissimilar in number to those on Charon's surface. Since a thick volatile crust of N2, CO, etc would be expected to destroy craters within tens of millions of years - an age far younger than the (already considerably smaller than expected) number of craters implies - Pluto probably doesn't have a thick volatile layer in most areas on its surface, and some other resurfacing method must have removed much of the missing craters. 3 - Curiously enough, the craters outside of the dark regions - even large ones - rarely seem to have central peaks in these pics...maybe the crust in those areas is built in such a way that prohibits peak formation or in a way that ensures that any peaks that do form quickly collapse... 4 - Large craters outside of the dark regions appear to be very flat...leads one to wonder if Pluto is warm enough - perhaps due to the strongly implied ongoing geologic activity - for viscous relaxation to occur, as it does for icy bodies in the saturnian and Jovian systems.

Leave a Comment:

You must be logged in to submit a comment. Log in now.

Space in Images

Pretty pictures and
awe-inspiring science.

See More

Join the New Millennium Committee

Let’s invent the future together!

Become a Member

Connect With Us

Facebook, Twitter, YouTube and more…
Continue the conversation with our online community!