11 Moons You Should Get to Know

You may have heard already that a fifth moon was discovered orbiting Pluto. (If not, Hubble spotted a fifth moon orbiting Pluto.) We know just enough about P5 to know that it's tiny, and it's a moon. Here are some other wild and wonderful worlds that orbit other worlds:

1. Phobos

The larger and innermost moon of Mars, Phobos is probably a captured asteroid. It's covered in craters, including the gigantic Stickney Crater created by an impact that was nearly severe enough to destroy the moon altogether. It orbits very close to Mars, so close that a person on the surface might see Phobos rise twice a day, and eclipses are common. It's so low, in fact, that when meteorites strike Mars, Phobos plows through the debris. Because it's tidally locked, one side always faces forwards, and passing through impact debris has left long grooves radiating away from the leading point. Tidal interactions are slowly dragging Phobos lower and lower. Once it drops low enough, it will shatter from the strain, forming a rocky ring around the planet for a while before it all falls out of orbit and rains down on Mars. Given how many crater chains and crazy-big craters there are on Mars, this has probably happened before.

Phobos, taken by Mars Reconnaissance Orbiter; Stickney Crater is at lower right

2. Io

Io is the innermost of the four moons that Galileo spotted around Jupiter in 1610. When Voyager 1 made the first close flyby of Io, astronomer Linda Morabito spotted something shocking in the image data: it was the dome-shaped plume of a gigantic volcano, one of more than 400 that dot the moon. Io is unusual for an outer-solar system moon, being made mostly of rock rather than ice, but it is constantly pulled and stressed by Jupiter and its orbital resonance with Ganymede and Europa. Huge mountains on Io have been lifted up as chunks of sulfurous crust tip on their sides from the strain, floating above an ocean of magma. It is far more geologically active than any other body in the solar system, including Earth, and its surface changes substantially in short periods of time as volcanoes spew lava for hundreds of kilometers. They also spew charged dust hundreds of kilometers into space where it is captured into Jupiter's radiation belts, creating a band called the Io torus, driving auroras on Jupiter, and powering a natural maser that can be picked up by ham radio gear on Earth.

Above: First view of an Ioan volcano by Voyager 1; the "dome" at top left is the plume of the volcano Pele

Io, taken by Galileo Orbiter; the bright red ring at lower left is material deposited by the volcano Pele, in the middle of the ring. The dark patch at the upper right edge of the ring is Pillan Patera, and did not exist on Galileo's previous pass by Io

3. Ganymede

The largest moon in our solar system and the third of Jupiter's Galilean satellites, Ganymede is a rocky iceball -- or an icy rockball, depending on your perspective. Bigger than Mercury (though less massive) and more like a planet than a moon, Ganymede has a proper magnetosphere, probably generated within a liquid iron core, and it is believed to also have a subsurface saltwater ocean. It is no longer being heated by the tidal resonance with Io and Europa, and so its surface is older, alternating young-ish areas of light, grooved terrain and dark, ancient surfaces covered in impact craters. It has many crater chains, probably caused by broken-up comets captured by Jupiter, just like Comet Shoemaker-Levy 9, which impacted Jupiter in 1994.

Ganymede in color, by Galileo, and a close-up of Enki Catena, one of the clearest crater chains

4. Titan

The second-largest moon in the solar system, Saturn's Titan is the only moon with a substantial atmosphere, which is much deeper than Earth's. It's so thick and the gravity so weak, in fact, that you could strap wings on your arms and flap them like a bird to fly. The air is mostly nitrogen, but the rest is mostly hydrocarbons, giving Titan's atmosphere a thick orange smoggy haze that is opaque to visible light. Cassini studies Titan in infrared light (which can penetrate the haze) and with radar -- and in 2004, via the Huygens Probe, an atmosphere probe became the first spacecraft to transmit from the surface of a moon other than our own. Titan is remarkably earthlike, apart from being so cold that water is as hard as rock; in addition to the atmosphere, it is the only place other than Earth known to have bodies of liquid on the surface -- lakes as large as the Great Lakes, except that it's not water: it's probably methane or ethane. The climate is probably similar to some of our deserts, with gigantic monsoons perhaps once a decade or more, and long droughts between. NASA scientists are working on a mission called Titan Mare Explorer (TiME) specifically to study the lakes of Titan.

Titan with Saturn, by Cassini

Radar image of lakes and rivers on Titan, and Huygens' last image of the surface of Titan; notice the rounded shapes of the pebbles, as if worn by liquid, and erosion patterns below them just like under river rocks on Earth.

5. Enceladus

This moon of Saturn is the shiniest thing in the solar system, as bright as freshly fallen snow. Its density suggests it is made almost entirely of water ice, and the widespread smooth, young terrain on its southern hemisphere is a sign of active volcanism. When Cassini arrived, it proved scientists right: not only did Enceladus have cryovolcanism, but it still does. Water is being spewed thousands of kilometers out into space from cracks around the southern pole of Enceladus, feeding Saturn's diffuse E ring, and proving directly for the first time that at least one place in the solar system has a subsurface ocean. The Cassini spacecraft has actually flown through these plumes and sampled the material directly, the only time material from another moon has been directly studied. Because Enceladus is geologically active and definitely possesses water, some scientists think it could support life, but of course there is no way to tell right now. The idea was bolstered, however, when Cassini detected hydrocarbons in the material spewed out from the interior, showing that the materials needed for life do exist there.

6. Hyperion

Hyperion is a porous, jumbled mass of ice and a bit of rock tumbling chaotically as it goes around Saturn. It's one of the oddest looking moons in the solar system; it looks very much like a sea sponge. It is covered with sharp craters on top of craters, with dark hydrocarbons filling their bottoms and making them look like deep holes. Though it's hard to see amid all the other craters, there is one staggeringly larger crater nearly as wide as the moon itself; it's amazing it didn't break the moon apart. Its density is very low, suggesting it is probably a rubble pile. All the other moons, like our Moon, always show the same face, but Hyperion doesn't; it's constantly tugged and yanked by the gravity of other moons, making it totally impossible to predict how long a day will last, or where the sun will rise tomorrow.

Hyperion, enhanced color, by Cassini

7. Iapetus

Hyperion's not the only weird thing orbiting Saturn; the third largest moon of Saturn is a mysterious world called Iapetus. When Giovanni Cassini discovered the moon in 1671, he realized he could only see it on one side and deduced that its leading side must be black and its trailing side must be white. Voyager finally proved him right in 1980, but the dark leading side, called Cassini Regio, remained mysterious until its namesake spacecraft arrived in 2004. The Cassini probe revealed that it's overlaid with a thin layer of dark material, possibly blasted off of Phoebe and very similar to the dark material in Hyperion's craters, but found even bigger mysteries that nobody had imagined. Iapetus is severely cratered, with an ancient surface that shouldn't be as bright as it is, and some extremely large craters and a huge equatorial ridge, thirteen kilometers high, which nearly encircles the moon. It looks a bit like the Death Star.

Iapetus light side (false color) and dark side (grayscale) by Cassini; note the huge ridge and many enormous craters

8. Prometheus

Bigger than Phobos but much farther away, Saturn's Prometheus was the ninth moon discovered in Voyager 1 data. It's a lumpy, irregular chunk of cratered ice, unremarkable except for what it does to Saturn's narrow F ring. The F ring is a very thin band with peculiar features, and scientists had struggled to explain why ever since Pioneer 11 had first spotted it. The answer is that it is "shepherded" gravitationally by two tiny moons: Prometheus, which orbits inside the ring, and Pandora, which orbits just outside. The two moons push material in towards the ring, and when they get close, carve grooves and channels in it and and steal material out of it. Although the moon is certainly not geologically active, the craters are not sharp and distinct as on many other bodies; it appears to be covered in a thick layer of dust. The singer Enya was inspired by the dance of Prometheus and Pandora, and wrote a song called "Shepherd Moons" about them.

Prometheus, dragging material off of the F-ring and creating a wave in its wake

9. Miranda

Uranus is a very strange planet in its own right, with its axis tilted on its side producing wild seasonal shifts, and a magnetic axis that is so off-center it doesn't even pass through the planet's core. But most of its moons seem fairly ordinary -- except for Miranda. It's made mostly of ice, but it looks very much as if a giant smashed it apart and then put it back together blindfolded, leaving its surface a radical mishmash of dissimilar terrain. This may be an illusion; it's possible all of this was caused by volcanism as Miranda wandered in and out of orbital resonances with other moons of Uranus, but the more intriguing notion is that it really was smashed apart, with the different terrains resulting as the chunks recoalesced. Until another spacecraft visits Uranus, we will never know.

Miranda, by Voyager 2

10. Triton

Triton is the only large moon of Neptune, and probably doesn't belong there: although it has a nearly perfect orbit and rotates synchronously, it cannot possibly have formed there because its orbit is retrograde -- it goes around Neptune in the opposite direction to the planet's rotation. This causes tidal interactions that lower Triton's orbit; like Phobos, this moon is ultimately doomed. In about 3.6 billion years, it will be within Neptune's Roche limit and shatter into a billion pieces, creating a shining ring system like Saturn's. Triton has a lot in common with Kuiper belt objects such as Pluto, and since Neptune is in an orbital resonance with Pluto, Triton may be somehow related to Pluto; some scientists suspect that Triton had a large moon similar to Charon, and that interactions with Neptune caused that moon to be ejected and Triton to be captured, becoming a moon itself and probably ejecting any large moons that Neptune already had. Triton is mostly made of rock and water ice, with a smattering of other ices. It's also geologically active, and was the second place after Earth where volcanism was seen -- cryovolcanoes have massively resurfaced large areas, and Voyager 2 photographed towering geysers of nitrogen gas and dust spewing up to 8 kilometers into space.

Above: From Voyager 2, this is Triton's strange, "cantaloupe" textured surface; the dark smudges in the white region are geyser plumes

11. Charon

Charon is the largest satellite of Pluto, so big that Pluto and Charon are sometimes called a double planet -- their center of gravity is out in open space, and Pluto and Charon really orbit one another! (They're also joined by four smaller moons: Nix, Hydra, and the yet-unnamed P4 and P5.) Pluto and Charon are also unusual for being mutually synchronous -- not only does Charon face the same side towards Pluto, but Pluto also faces the same side towards Charon. So if you stood on Pluto, underneath Charon, and looked up, you would see Charon fixed immobile in the sky while the stars wheeled endlessly by in the background. (The brightest of those would be the Sun, too dim at this distance to wash out all the other stars in the sky.) To date, this moon has never been visited, and our best pictures are vague images from the Hubble space telescope. But that will change in July 2015, when the New Horizons probe will make its brief visit to this distant system on its way out of our solar system.

Above: The Pluto system, taken by the Hubble Space Telescope. The biggest thing is Pluto, the second biggest is Charon, and the two other objects are Nix and Hydra; P4 and P5 are not visible in this image

The Pluto system, featuring all 5 of Pluto's satellites

Look Up! Residents of Maine and Michigan Might Catch a Glimpse of the Northern Lights Tonight

The aurora borealis, a celestial show usually reserved for spectators near the arctic circle, could potentially appear over parts of the continental U.S. on the night of February 15. As Newsweek reports, a solar storm is on track to illuminate the skies above Maine and Michigan.

The Northern Lights (and the Southern Lights) are caused by electrons from the sun colliding with gases in the Earth’s atmosphere. The solar particles transfer some of their energy to oxygen and nitrogen molecules on contact, and as these excited molecules settle back to their normal states they release light particles. The results are glowing waves of blue, green, purple, and pink light creating a spectacle for viewers on Earth.

The more solar particles pelt the atmosphere, the more vivid these lights become. Following a moderate solar flare that burst from the sun on Monday, the NOAA Space Weather Prediction Center forecast a solar light show for tonight. While the Northern Lights are most visible from higher latitudes where the planet’s magnetic field is strongest, northern states are occasionally treated to a view. This is because the magnetic North Pole is closer to the U.S. than the geographic North Pole.

This Thursday night into Friday morning is expected to be one of those occasions. To catch a glimpse of the phenomena from your backyard, wait for the sun to go down and look toward the sky. People living in places with little cloud cover and light pollution will have the best chance of spotting it.

[h/t Newsweek]

Kevin Gill, Flickr // CC BY-2.0
10 Facts About the Dwarf Planet Haumea
Kevin Gill, Flickr // CC BY-2.0
Kevin Gill, Flickr // CC BY-2.0

In terms of sheer weirdness, few objects in the solar system can compete with the dwarf planet Haumea. It has a strange shape, unusual brightness, two moons, and a wild rotation. Its unique features, however, can tell astronomers a lot about the formation of the solar system and the chaotic early years that characterized it. Here are a few things you need to know about Haumea, the tiny world beyond Neptune.


Haumea is a trans-Neptunian object; its orbit, in other words, is beyond that of the farthest ice giant in the solar system. Its discovery was reported to the International Astronomical Union in 2005, and its status as a dwarf planet—the fifth, after Ceres, Eris, Makemake, and Pluto—was made official three years later. Dwarf planets have the mass of a planet and have achieved hydrostatic equilibrium (i.e., they're round), but have not "cleared their neighborhoods" (meaning their gravity is not dominant in their orbit). Haumea is notable for the large amount of water ice on its surface, and for its size: Only Pluto and Eris are larger in the trans-Neptunian region, and Pluto only slightly, with a 1475-mile diameter versus Haumea's 1442-mile diameter. That means three Haumeas could fit sit by side in Earth—and yet it only has 1/1400th of the mass of our planet.


There is some disagreement over who discovered Haumea. A team of astronomers at the Sierra Nevada Observatory in Spain first reported its discovery to the Minor Planet Center of the International Astronomical Union on July 27, 2005. A team led by Mike Brown from the Palomar Observatory in California had discovered the object earlier, but had not reported their results, waiting to develop the science and present it at a conference. They later discovered that their files had been accessed by the Spanish team the night before the announcement was made. The Spanish team says that, yes, they did run across those files, having found them in a Google search before making their report to the Minor Planet Center, but that it was happenstance—the result of due diligence to make sure the object had never been reported. In the end, the IAU gave credit for the discovery to the Spanish team—but used the name proposed by the Caltech team.


In Hawaiian mythology, Haumea is the goddess of fertility and childbirth. The name was proposed by the astronomers at Caltech to honor the place where Haumea's moon was discovered: the Keck Observatory on Mauna Kea, Hawaii. Its moons—Hi'iaka and Namaka—are named for two of Haumea's children.


Haumea is the farthest known object in the solar system to possess a ring system. This discovery was recently published in the journal Nature. But why does it have rings? And how? "It is not entirely clear to us yet," says lead author Jose-Luis Ortiz, a researcher at the Institute of Astrophysics of Andalusia and leader of the Spanish team of astronomers who discovered Haumea.


In addition to being extremely fast, oddly shaped, and ringed, Haumea is very bright. This brightness is a result of the dwarf planet's composition. On the inside, it's rocky. On the outside, it is covered by a thin film of crystalline water ice [PDF]—the same kind of ice that's in your freezer. That gives Haumea a high albedo, or reflectiveness. It's about as bright as a snow-covered frozen lake on a sunny day.


If you lived to be a year old on Haumea, you would be 284 years old back on Earth. And if you think a Haumean year is unusual, that's nothing next to the length of a Haumean day. It takes 3.9 hours for Haumea to make a full rotation, which means it has by far the fastest spin, and thus shortest day, of any object in the solar system larger than 62 miles.


haumea rotation gif
Stephanie Hoover, Wikipedia // Public Domain

As a result of this tornadic rotation, Haumea has an odd shape; its speed compresses it so much that rather than taking a spherical, soccer ball shape, it is flattened and elongated into looking something like a rugby ball.


Ortiz says there are several mechanisms that can have led to rings around the dwarf planet: "One of our favorite scenarios has to do with collisions on Haumea, which can release material from the surface and send it to orbit." Part of the material that remains closer to Haumea can form a ring, and material further away can help form moons. "Because Haumea spins so quickly," Ortiz adds, "it is also possible that material is shed from the surface due to the centrifugal force, or maybe small collisions can trigger ejections of mass. This can also give rise to a ring and moons."


Ortiz says that while the rings haven't transformed scientists' understanding of Haumea, they have clarified the orbit of its largest moon, Hi'iaka—it is equatorial, meaning it circles around Haumea's equator. Hi'iaka is notable for the crystalline water ice on its surface, similar to that on its parent body.


It's not easy to study Haumea. The dwarf planet, and other objects at that distance from the Sun, are indiscernible to all but the largest telescopes. One technique used by astronomers to study such objects is called "stellar occultation," in which the object is observed as it crosses in front of a star, causing the star to temporarily dim. (This is how exoplanets—those planets orbiting other stars—are also often located and studied.) This technique doesn't always work for objects beyond the orbit of Neptune, however; astronomers must know the objects' orbits and the position of the would-be eclipsed stars to astounding levels of accuracy, which is not always the case. Moreover, Ortiz says, their sizes are oftentimes very small, "comparable to the size of a small coin viewed at a distance of a couple hundred kilometers."


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