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7 Astounding Facts About Jupiter

Jupiter is the largest planet in the solar system. It's so large that all of the other planets in the solar system could fit inside it. If we really paid attention to the sky, we'd do nothing but freak out that there's a giant, terrifying, stormy orb of pressure and gas up there. Mental Floss spoke about Jupiter with an expert: Barry Mauk, the lead investigator of the JEDI instrument on the Juno spacecraft, which entered Jupiter's orbit on July 4, 2016 to conduct the most in-depth scientific analysis of the planet ever. Mauk is a principal staff physicist at the Johns Hopkins University Applied Physics Laboratory, which built JEDI. Here's what you need to know about Jupiter.

1. JUPITER IS REALLY, REALLY BIG.

Thirteen hundred Earths could fit inside of Jupiter, like a big celestial gumball machine. It's big, OK? And its powerful magnetosphere is even bigger—bigger, in fact, than the Sun, a fact made even more astounding when you consider that the Sun could hold a thousand Jupiters.

The amount of time it takes Jupiter to rotate on its axis is known as a Jovian day (Jove is another name for Jupiter in Roman mythology). It only takes about 9.9 hours, but a Jovian year is 4333 Earth days long.

Jupiter is about 5.2 astronomical units from the Sun, compared with Earth's 1 AU. As such, it takes sunlight about 43 minutes to reach Jupiter. The planet has a lot of moons, too: 69 of them, and that number is still growing. (Two of those moons were discovered just this summer.) Those moons are good news for the future of the planet's exploration, as they might provide a landing surface. Jupiter isn't an option because it is a giant ball of gas with no surface that we know of—or at least, no surface that is accessible.

2. YES, IT'S A GAS GIANT. NO, YOU CAN'T JUST FLY YOUR SPACESHIP THROUGH IT.

Despite being a giant ball of gas, you can't fly through it like a cloud. Its furious storms, ammonia atmosphere, and atmospheric pressure would all annihilate you. How great is the pressure at the center of Jupiter? Nobody knows, exactly, because its center is such a confounding mystery. But pressure at sea level here on Earth is about 14.7 pounds per square inch. That's pretty comfortable. Pressure at the bottom of the Mariana Trench in the Pacific Ocean is much less pleasant at about 16,000 psi. Still, with the right equipment, it's manageable, as submarines like the Deepsea Challenger have proven.

Jupiter's pressure is not manageable. At something like 650,000,000 psi, the "bottom" of Jupiter would compress the Deepsea Challenger to… nobody knows! Because once you start reaching those pressures and heats, the very properties of matter itself become unknowable. (If, in fact, its center consists of liquid metallic hydrogen, you know right away that something weird is going on down there, because we're describing hydrogen as liquid metal. Down is up, up is down—nothing matters at the center of Jupiter.)

3. JUPITER'S GORGEOUS AURORA? IT'S A SIGN THAT JUPITER IS TRYING TO SPIN UP SPACE ITSELF.

One of the things that most excites Mauk about Jupiter, he tells Mental Floss, is that it is a stepping stone from our solar system to the rest of the universe. "Jupiter is the place to go to if you want to understand how processes that operate within our solar system might apply to more distant astrophysical objects out in the universe," he says. Jupiter, for example, can help scientists unlock some mysteries of stellar nurseries and regions like the Crab Nebula, where powerful magnetic fields play essential roles.

Consider Jupiter's stunning auroras. "Earth's aurora is powered by the solar wind blowing over the magnetic field of Earth. Jupiter's aurora is powered by rotation. And Jupiter's very bright aurora—it's the most intense aurora in the solar system—is a signature of Jupiter's attempt to spin up its space environment. Jupiter is trying to keep the space environment around it rotating at the same rate that Jupiter is."

Why is this important? Because astrophysical objects use magnetic fields to shed angular momentum. "An example of that is solar system formation," he says, where molecular clouds that would normally collapse to form stellar or solar systems spin so fast they can't collapse. "Magnetic fields are thought to be one of the mechanisms by which angular momentum gets shed by a central object." Auroras are evidence of this phenomenon.

4. ITS GIANT RED SPOT IS ACTUALLY A GIANT RED CATEGORY 12 HURRICANE.

The Great Red Spot is a massive storm that has been raging on Jupiter for centuries. Though its size varies, at its largest you could fit Earth, Venus, and Mars in there (and probably squeeze Mercury in there too if you really tried); at its smallest it could "only" hold the planet Earth. With wind speeds peaking at 400 miles per hour, it doesn't even fit on the Saffir-Simpson Hurricane Scale used to measure such giant storms on Earth, though you could extrapolate its speed to being about a Category 12—more powerful, even, than "Humpty's revenge." (It would be an F7 tornado on the Fujita scale—an F7 tornado the size of the terrestrial planets of the solar system. The most powerful tornado ever recorded on Earth was an F5, in Oklahoma.)

Scientists recently discovered that the red storm is raging at 2400°F, heating the planet's upper atmosphere. Still, the chemistry of the spot and its exact nature are still in question. Answers may come on July 11, 2017, when the Juno spacecraft makes a direct pass over the Great Red Spot, marking the most intensive exploration of it ever attempted.

5. THE MOST PRESSING QUESTION FOR SCIENTISTS: HOW DID JUPITER FORM?

Despite having been studied intently since 1609, when Galileo Galilei perfected his telescope, Jupiter remains a stormy mystery in space. The most pressing question is how the planet formed. Answering it will reveal to scientists the story of the early solar system and unlock the secrets of the formation of other worlds. As the most dominant object orbiting the Sun, and likely the oldest planet, in a very real way, the story of Jupiter is the story of the solar system itself.

Essential to the story of Jupiter's birth is whether or not it has a core. The best guess is that pressures at Jupiter's center have compressed hydrogen to a liquid metal state. (Hydrogen is by far the dominant constituent of Jupiter.)

One of the prime objectives of the Juno mission is to find out if a rocky core exists at the planet's center. The traditional theory is that Jupiter has a rocky core that's about 10 times the mass of Earth, and that core collects gases and other materials around it. Behold: the Jupiter you know and love. But recently, some scientists have proposed that Jupiter may have no core at all, and may have formed from the gas and dust particles that "lumped together" just after the formation of the Sun and compressed rapidly, allowing a planet to form without need of a rocky base.

Current data from the Juno mission suggests that perhaps neither model is accurate, and that Jupiter's core is "fuzzy"—without a clear line separating layers—and that it is much larger than anyone expected. Such unexpected results are consistent with Juno's tendency thus far to return textbook-shredding revelations. Already, data returned from the mission have invalidated vast swaths of conventional thinking concerning the Jovian interior.

6. WE'RE KEEPING A CLOSE EYE ON IT.

The Juno spacecraft isn't our first attempt to get a grip on the cosmic behemoth that is Jupiter, and won't be our last. The spacecraft is currently zipping along just 3000 miles above Jupiter's cloud, at top speeds of 130,000 mph. It is rotating on a hugely oblong orbit that takes it close to the planet and then zinging off 5 million miles away. This orbit lasts 53 days. The mission has completed five orbits so far, four of which collected science data, and the mission is budgeted through 2018, at which time NASA officials will have to decide whether to extend its mission and learn more, or just shrug and say, "Ehn, we know enough. Destroy the spacecraft."

Once Juno ends, the next mission slated to launch to the Jovian system is the European Space Agency's JUICE mission in 2022. NASA's Europa Clipper will launch in that same timeframe, and upon its arrival in the system, will study the ocean moon Europa from Jupiter's orbit (where it is largely protected from the punishing radiation environment caused by the planet's magnetosphere).

7. YOU DON'T NEED TO TAKE NASA'S WORD ON JUPITER. YOU CAN SEE IT YOURSELF.

With just about any telescope and a little bit of work, you can see Jupiter in surprising detail. Your view won't be as crisp as the one from Galileo (the spacecraft), but it'll be at least as good as it was for Galileo (the scientist). You can see its stripes from Earth, and with enough telescope power, even the Great Red Spot. Point a pair of binoculars at Jupiter, and you can see the four Galilean moons—Io, Europa, Callisto, and Ganymede—the same ones found by Galileo, who by spotting the moons ended the idea of a geocentric model of the solar system. Jupiter will next be at opposition (that is, as close to Earth and as bright as it'll get) on May 9, 2018.

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10 Astonishing Things You Should Know About the Milky Way
Anne Dirkse, Flickr // CC BY-SA 2.0
Anne Dirkse, Flickr // CC BY-SA 2.0

Our little star and the tiny planets that circle it are part of a galaxy called the Milky Way. Its name comes from the Greek galaxias kyklos ("milky circle") and Latin via lactea ("milky road"). Find a remote area in a national park, miles from the nearest street light, and you'll see exactly why the name makes sense and what all the fuss is about. Above is not a sky of black, but a luminous sea of whites, blues, greens, and tans. Here are a few things you might not know about our spiraling home in the universe.

1. THE MILKY WAY IS GIGANTIC.

The Milky Way galaxy is about 1,000,000,000,000,000,000 kilometers (about 621,371,000,000,000,000 miles) across. Even traveling at the speed of light, it would still take you well over 100,000 years to go from one end of the galaxy to the other. So it's big. Not quite as big as space itself, which is "vastly, hugely, mind-bogglingly big," as Douglas Adams wrote, but respectably large. And that's just one galaxy. Consider how many galaxies there are in the universe: One recent estimate says 2 trillion.

2. IT'S JAM-PACKED WITH CELESTIAL STUFF.

artist's illustration of the milky way galaxy and its center
An artist's concept of the Milky Way and the supermassive black hole Sagittarius A* at its core.
ESA–C. Carreau

The Milky Way is a barred spiral galaxy composed of an estimated 300 billion stars, along with dust, gas, and celestial phenomena such as nebulae, all of which orbits around a hub of sorts called the Galactic Center, with a supermassive black hole called Sagittarius A* (pronounced "A-star") at its core. The bar refers to the characteristic arrangement of stars at the interior of the galaxy, with interstellar gas essentially being channeled inward to feed an interstellar nursery. There are four spiral arms of the galaxy, with the Sun residing on the inner part of a minor arm called Orion. We're located in the boondocks of the Milky Way, but that is OK. There is definitely life here, but everywhere else is a question mark. For all we know, this might be the galactic Paris.

3. FOR A SPIRAL GALAXY, IT'S PRETTY TYPICAL …

If you looked at all the spiral galaxies in the local volume of the universe, the Milky Way wouldn't stand out as being much different than any other. "As galaxies go, the Milky Way is pretty ordinary for its type," Steve Majewski, a professor of astronomy at the University of Virginia and the principal investigator on the Apache Point Observatory Galactic Evolution Experiment (APOGEE), tells Mental Floss. "It's got a pretty regular form. It's got its usual complement of star clusters around it. It's got a supermassive black hole in the center, which most galaxies seem to indicate they have. From that point of view, the Milky Way is a pretty run-of-the-mill spiral galaxy."

4. …AND YET IT STANDS OUT AMONG ALL GALAXIES.

On the other hand, he tells Mental Floss, spiral galaxies in general tend to be larger than most other types of galaxies. "If you did a census of all the galaxies in the universe, the Milky Way would seem rather unusual because it is very big, our type being one of the biggest kinds of galaxies that there are in the universe." From a human perspective, the most important thing about the Milky Way is that it definitely managed to produce life. If they exist, the creatures in Andromeda, the galaxy next door (see #9), probably feel the same way about their own.

5. FIGURING OUT ITS STRUCTURE FROM THE INSIDE IS A CHALLENGE.


John McSporran, Flickr // CC BY 2.0

We have a very close-up view of the phenomena and forces at work in the Milky Way because we live inside of it, but that internal perspective places astronomers at a disadvantage when it comes to determining a galactic pattern. "We have a nice view of the Andromeda galaxy because we can see the whole thing laid out in front of us," Majewski says. "We don't have that opportunity in the Milky Way."

To figure out its structure, astronomers have to think like band members during a football halftime show. Though spectators in the stands can easily see the letters and shapes being made on the field by the marchers, the band can't see the shapes they are making. Rather, they can only work together in some coordinated way, moving to make these patterns and motions on the field. So it is with telescopes and stars.

6. INTERSTELLAR DUST BLOCKS OUR VIEW OF SOME PARTS OF THE GALAXY.

Interstellar dust further stymies astronomers. "That dust blocks our light, our view of the more distant parts of the Milky Way," Majewski says. "There are areas of the galaxy that are relatively obscured from view because they are behind huge columns of dust that we can't see through in the optical wavelengths that our eyes work in." To ameliorate this problem, astronomers sometimes work in longer wavelengths such as radio or infrared, which lessen the effects of the dust.

7. THE MILKY WAY SPINS, BUT ITS SPEED DOESN'T ADD UP …

Astronomers can make pretty reasonable estimates of the mass of the galaxy by the amount of light they can see. They can count the galaxy's stars and calculate how much those stars should weigh. They can account for all the dust in the galaxy and all of the gas. And when they tally the mass of everything they can see, they find that it is far short of what is needed to account for the gravity that causes the Milky Way to spin.

In short, our Sun is about two-thirds of the way from the center of the galaxy, and astronomers know that it goes around the galaxy at about 144 miles per second. "If you calculate it based on the amount of matter interior to the orbit of the Sun, how fast we should be going around, the number you should get is around 150 or 160 kilometers [93–99 miles] per second," Majewski says. "Further out, the stars are rotating even faster than they should if you just account for what we call luminous matter. Clearly there is some other substance in the Milky Way exerting a gravitational effect. We call it dark matter."

8. … AND WE BLAME DARK MATTER FOR THAT.

Dark matter is a big problem in galactic studies. "In the Milky Way, we study it by looking at the orbits of stars and star clusters and satellite galaxies, and then trying to figure out how much mass do we need interior to the orbit of that thing to get it moving at the speed that we can measure," Majewski says. "And so by doing this kind of analysis for objects at different radii across the galaxy, we actually have a fairly good idea of the distribution of the dark matter in the Milky Way—and yet we still have no idea what the dark matter is."

9. THE MILKY WAY IS ON A COLLISION COURSE WITH ANDROMEDA. BUT DON'T PANIC.

andromeda galaxy
The Andromeda galaxy
ESA/Hubble & NASA

Sometime in the next 4 or 5 billion years, the Milky Way and Andromeda galaxies will smash into each other. The two galaxies are about the same size and have about the same number of stars, but there is no cause for alarm. "Even though there are 300 billion stars in our galaxy and a comparable number, or maybe more, in Andromeda, when they collide together, not a single star is expected to hit another star. The space between stars is that vast," Majewski says.

10. WE'RE THROWING EVERYTHING WE HAVE AT STUDYING IT.

There are countless spacecraft and telescopes studying the Milky Way. Most famous is the Hubble Space Telescope, while other space telescopes such as Chandra, Spitzer, and Kepler are also returning data to help astronomers unlock the mysteries of our swirling patch of stars. The next landmark telescope in development is NASA's James Webb Space Telescope. It should finally launch in 2019. Meanwhile, such ambitious projects as APOGEE are working out the structure and evolution of our spiral home by doing "galactic archaeology." APOGEE is a survey of the Milky Way using spectroscopy, measuring the chemical compositions of hundreds of thousands of stars across the galaxy in great detail. The properties of stars around us are fossil evidence of their formation, which, when combined with their ages, helps astronomers understand the timeline and evolution of the galaxy we call home. 

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Mysterious 'Hypatia Stone' Is Like Nothing Else in Our Solar System
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In 1996, Egyptian geologist Aly Barakat discovered a tiny, one-ounce stone in the eastern Sahara. Ever since, scientists have been trying to figure out where exactly the mysterious pebble originated. As Popular Mechanics reports, it probably wasn't anywhere near Earth. A new study in Geochimica et Cosmochimica Acta finds that the micro-compounds in the rock don't match anything we've ever found in our solar system.

Scientists have known for several years that the fragment, known as the Hypatia stone, was extraterrestrial in origin. But this new study finds that it's even weirder than we thought. Led by University of Johannesburg geologists, the research team performed mineral analyses on the microdiamond-studded rock that showed that it is made of matter that predates the existence of our Sun or any of the planets in the solar system. And, its chemical composition doesn't resemble anything we've found on Earth or in comets or meteorites we have studied.

Lead researcher Jan Kramers told Popular Mechanics that the rock was likely created in the early solar nebula, a giant cloud of homogenous interstellar dust from which the Sun and its planets formed. While some of the basic materials in the pebble are found on Earth—carbon, aluminum, iron, silicon—they exist in wildly different ratios than materials we've seen before. Researchers believe the rock's microscopic diamonds were created by the shock of the impact with Earth's atmosphere or crust.

"When Hypatia was first found to be extraterrestrial, it was a sensation, but these latest results are opening up even bigger questions about its origins," as study co-author Marco Andreoli said in a press release.

The study suggests the early solar nebula may not have been as homogenous as we thought. "If Hypatia itself is not presolar, [some of its chemical] features indicate that the solar nebula wasn't the same kind of dust everywhere—which starts tugging at the generally accepted view of the formation of our solar system," Kramer said.

The researchers plan to further probe the rock's origins, hopefully solving some of the puzzles this study has presented.

[h/t Popular Mechanics]

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