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DPS 2015: Pluto's small moons Styx, Nix, Kerberos, and Hydra [UPDATED]

Posted by Emily Lakdawalla

10-11-2015 14:18 CST

Topics: New Horizons, explaining science, Pluto's small moons, conference report

EDIT Nov 13: The sizes I reported for Styx and Kerberos were not the most up-to-date ones. I have updated them with information from Hal Weaver. --ESL

How to make sense of a day and a half of packed scientific sessions and hallway conversation on Pluto? Based on past experience, it's best to cut a big problem into smaller pieces and take them on one at a time. So for my first post on results from the Division for Planetary Sciences meeting, I'm going to tell you about Pluto's small moons: Styx, Nix, Kerberos, and Hydra. Here is a visual guide to the four:

Family portrait of Pluto's moons

NASA / JHUAPL / SwRI

Family portrait of Pluto's moons
This composite image shows a sliver of Pluto's large moon, Charon, and all four of Pluto's small moons, as resolved by the Long Range Reconnaissance Imager (LORRI) on New Horizons. All the moons are displayed with a common intensity stretch and spatial scale (see scale bar). Charon is by far the largest of Pluto's moons, with a diameter of 1,212 kilometers. Nix and Hydra have comparable sizes, approximately 40 kilometers across in their longest dimension above. Kerberos and Styx are much smaller and have comparable sizes, roughly 10-12 kilometers across in their longest dimension. All four small moons have highly elongated shapes, a characteristic thought to be typical of small bodies in the Kuiper Belt.

And a graphic that shows their positions with respect to New Horizons at the moment of closest approach. New Horizons crossed the equatorial plane of Pluto at a distance near Charon's orbit some time before closest approach, so it is "behind" everything else in the diagram here.

Positions of the moons of Pluto during the New Horizons flyby

Courtesy Hal Weaver

Positions of the moons of Pluto during the New Horizons flyby
At the time of closest approach to Pluto, Nix was on the same side of Pluto as New Horizons; all the other moons were farther away. Consequently, New Horizons' best images of smaller moons are of Nix. Note that the moment of closest approach is not the same as the moment of the moon-plane crossing. When New Horizons crossed the plane containing the moons' orbits, it was at a distance from Pluto near Charon's orbit.

Here's a summary of the physical and orbital characteristics of these worlds as reported at the conference.

BodyMagnitudeSemimajor axis (km)Orbital periodSpin period (days)Spin period (per orbit)Dimensions (km)
Styx 27 42,656 ± 78 20.162 3.239 6.22 10 x 5.3
Nix 23.5 48,694 ± 3 24.855 1.829 13.6 54 x 41 x 36
Kerberos 26.5 57,783 ± 19 32.168 5.33 6.04 12 x 7.5
Hydra 23.0 64,738 ± 3 38.202 0.4295 88.9 43 x 33

Sources: semimajor axes: Showalter and Hamilton 2015; orbit data: Mark Showalter; sizes: Bill McKinnon & Hal Weaver.

The most surprising results are the rotation states of the moons. To explain why they're surprising, consider the regular satellites in the solar system. Very nearly all of the moons that formed around the planets -- the so-called regular moons -- are locked in synchronous rotation, where their rotational axes are perpendicular to the planets' equatorial planes, and where they rotate once for each orbit around the planet, keeping the same face of the moon pointed at the planet at all times. Charon and Pluto are mutually tidally locked. But Styx, Nix, Kerberos, and Hydra, although lying in the Pluto-Charon equatorial plane in circular orbits, have wacky rotation states, with axes pointed every which way, and non-synchronous rotation. Hydra, in particular, rotates once in 10 hours!

NASA / JHUAPL / SwRI / M. Showalter

Pluto's "pandemonium" moons
Most inner moons in the solar system keep one face pointed toward their central planet; this animation shows that certainly isn’t the case with the small moons of Pluto, which behave like spinning tops. Pluto is shown at center with, in order from closest to farthest orbit, its moons Charon, Styx, Nix, Kerberos and Hydra.

The pole orientations are weird, too. Styx's pole is sideways (with an inclination of 82 degrees), and Nix's pole is oriented 132 degrees from Pluto's equatorial plane, meaning that it rotates "backwards". Not only that, but its rotation rate has increased by 10% since its discovery. At the press briefing, I asked Mark Showalter if Pluto's small moons were more like the outer, irregular satellites of giant planets than they were like the "ringmoons". He said no, because they are presumed to have formed within the Pluto system, but yes, in that Pluto appears to have no influence whatsoever on their rotation. "They should be paying more attention to their parent than they are," he said. But they are paying some attention: he pointed out that it's the outermost, Hydra, that's spinning fastest. Its spin is actually similar to lots of other Kuiper belt objects; it's fairly easy, he said, to make Kuiper belt objects spin at that rate from collisions. As you go inward from Hydra, the moons spin more slowly, perhaps having been slowed to their present rates by Pluto. The system is chaotic, but the fast spin rates actually stabilize the rotation states, meaning that it takes longer for them to change orientation and speed than it would if they were slow rotators.

Hal Weaver presented data on their brightness and color. All have quite bright surfaces, with albedo of "at least 60%", which is unusual in the Kuiper belt. They are neutral in color, intermediate in brightness and color between Pluto and Charon. Nix is slightly redder than Hydra. Their color is consistent with water ice composition. At least Nix and Hydra and possibly all of them appear to have formed as mergers of two or more smaller bodies, meaning Pluto had more moons originally. All this means they're likely collisional fragments, evidence for the collision that likely created the Pluto-Charon system in the first place. Unfortunately, it makes them poor proxies for small, primordial Kuiper belt objects, so it's a good thing New Horizons has found another small, likely primitive body to target (more on that later). The New Horizons team doesn't currently have a good explanation for how these little things maintained their bright color for the age of the solar system, or for why their axes are so tilted.

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.

Both Nix and Hydra show several small craters. They have no visible boulders or layering, though there are color differences across their surfaces from those impact craters. The images of Kerberos and Styx are too low-resolution for craters to be visible. What the Kerberos images do show is that Kerberos is much, much smaller (and hence brighter) than the Showalter and Hamilton Hubble study predicted. Showalter told me that the cause of that incorrect prediction was an incorrect mass determination for Kerberos -- "so what we're learning is that it's tough to determine the masses of the moons." Robert Jacobson reported that Styx and Kerberos' masses are so low that the error bars are still bigger than the mass estimates for both.

New Horizons searched diligently for more moons, but the possibility of further small moons interior to Hydra has pretty much been ruled out now, as John Spencer showed in his presentation. It appears that the region of space from Styx to Hydra is "dynamically full" -- there's just no stable orbit for further small bodies -- and intense searches yielded no sign of anything bigger than about 2 kilometers across in the space between Pluto and Charon. If there are any undiscovered moons in the Pluto system, they are quite small. But even that is unlikely, as New Horizons' searches for rings around Pluto have also turned up nothing. Spencer held out some hope, saying the "ring story might change" as we get the rest of the data down from the spacecraft.

And yes, quite a lot more data still lie on the spacecraft. Our highest-resolution images of the small moons are on the ground, but there remains a higher-phase Nix image on the spacecraft, which will be good for topography. And a lot more color, composition, and ring search data remains to be downlinked.

Thanks to Matt Francis for sharing some of his notes from the afternoon Pluto session so that I could go see Ceres talks!


 
See other posts from November 2015

 

Or read more blog entries about: New Horizons, explaining science, Pluto's small moons, conference report

Comments:

Josh: 11/10/2015 05:06 CST

Any news on whether the red material was excavated from or delivered to Nix?

Kenny A. Chaffin: 11/10/2015 09:01 CST

Thanks for this, wonderful to see this great data continue to come in from New Horizons!

Dan Bloch: 11/10/2015 11:47 CST

Note that even though the highest resolution images of Nix are on the ground, we haven't seen them yet. The 8:07 images are about 0.8 km/pixel. The best ones will be from two hours later, at .3 km/pixel.

stfletch: 11/11/2015 07:12 CST

Actually we have one image from the .3 km/pixel LORRI set and that is the one shown in the composite image at the top of the page. We should get another 15 images that from this set which were taken at the same time. We should also get a MVIC pan at 0.44 km/pixel which I assume is the higher phase image Emily refers too.

Dan Bloch: 11/13/2015 12:24 CST

Interesting. You're half-right. The image on this page is .8 km/pixel. But this one is .3 km/pixel: https://twitter.com/NewHorizonsIMG/status/661665065515487232

Darin Ragozzine: 11/13/2015 04:55 CST

Also fun to note that Danielle Hastings and I have found that the outer satellite of Haumea, Hi'iaka, is also a regular satellite with an unexpectedly fast 10 hour spin period. We're not sure yet if there's a direct connection, but probably tidal despinning doesn't work the way we think it should. Using impacts to spin things up does not work... work by another student (Luke Burkhart) shows that you can't spin up a satellite, not destroy it, and maintain a near zero eccentricity and inclination. Look for Danielle's paper coming out soon! :)

Dan Bloch: 11/27/2015 12:03 CST

Never mind, stfletch was right. The one I found was the same image with more processing.

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