Just in case you’ve forgotten how brain-destroyingly big Saturn is:
[Click to encronosenate.]
This shot of the ringed wonder was taken by the Cassini spacecraft when it was well over 2 million kilometers from the planet. The spacecraft was south of the rings, looking "up" toward the north. The Sun is shining down on the rings from this perspective, so they look darker than you might expect, and the use of a near-infrared filter accentuates storms in the southern hemisphere cloudtops.
So why does this picture grind my mind to dust? Look at the the very top, near the center. Can you see that dot of light? You might need to click the picture to get the hi-res version to see it better; that’s how small it is.
Except it isn’t. That dot of light is Mimas, a moon of Saturn, and it’s 400 km – 250 miles – across! That’s roughly the size of the state of Missouri, and compared to Saturn it’s reduced to a mere pixel of light. And even then, Saturn’s rings are still too big to fit in this picture!
The scale of the solar system crushes me. And yet there we are, poking around and sticking our noses into it. We humans are pretty awesome.
Image credit: NASA/JPL-Caltech/Space Science Institute
In late 2010, amateur astronomers discovered a white spot on Saturn – a gigantic storm forming in its northern hemisphere. The storm grew rapidly, and within weeks had embiggened to an almost unbelievable size, much larger than our entire planet. The winds in Saturn’s atmosphere sheared the storm, pulling it apart while it still raged, and after three months the storm had wrapped completely around the planet, stretched to the ridiculous length of 300,000 km (180,000 miles) – 3/4 of the distance from the Earth to the Moon!
By mid-2011 the storm had nearly subsided – its remnants could still be seen in images taken by the Cassini spacecraft orbiting the ringed world – but the teeth had been taken out of it. Still, there was one surprise left in it.
Observations taken in the infrared by Cassini as well as from Earth show that the storm was not just big and violent, it also formed a vortex (a storm within a storm, if you like) that got hot – well, hot for frigid Saturn, that is. In the heart of the system, the temperature rose by an incredible 80° Celsius – a difference in temperature that’s like starting in the depths of winter in Anchorage, Alaska and then going to the height of summer in the Sahara!
The image here [click to encronosenate] is from the Very Large Telescope in Chile, and was taken in the infrared, where the heat in the vortex is fairly obvious. Mind you, it’s not like it was a firestorm: the maximum temperature was still a chilly -150° Celsius, but compared to Saturn’s usual -220 or so degrees, that’s pretty dang hot.
The rise in temperature was unexpected. A 20° rise is about the usual fare for these things, but then, this wasn’t a usual storm. Apparently, this hot spot started as two separate vortices, spawned by the storm seen in visible light, and moving around the planet at slightly different speeds. They eventually merged, forming this one ginormous vortex, which at its biggest was over 62,000 km (38,000 miles) across. Interestingly, it grew to this size around the time the visible storm had faded away.
Here’s a video from NASA’s Goddard Space Flight Center featuring planetary scientist Brigette Hesman describing the event:
Like any planet with an active atmosphere, storms on Saturn are common, but one this big had never been seen before. I’d say it was fortunate that we had a spacecraft like Cassini orbiting the planet when the storm erupted, but luck had very little to do with it: it was hard work and dedication that gave us that view. Cassini is such a well-crafted machine that it has operated nearly flawlessly for over eight years orbiting the distant planet. Its design and launch took decades to complete, and it took another seven years just to get to Saturn in the first place.
My point? Luck favors those who are prepared and have planned for rare circumstance. A storm like this one may not happen very often, but we were ready for it by having Cassini there in the first place, and by having a fleet of Earth-based telescopes with their eyes on the sky to support it.
… and having said that, I’ll note an irony: although it was right there, Cassini didn’t discover the storm in the first place. Why not? Because there’s just too damn much to see in the Saturn system! The storm erupted rapidly, and Cassini was busy looking at the rings and moons, so it missed the storm’s genesis. This is not a failure on the part of Cassini or its designers and users: instead, it should be seen as a clarion call for more spacecraft, more explorers in our solar system observing all the myriad worlds.
When I see images and science like this, I am filled with awe and joy, but I’m also struck with an implacable thought: what else are we missing?
Image credit: Leigh N. Fletcher, University of Oxford, UK, and ESO; NASA/JPL-Caltech/SSI
Pretty much every picture of Saturn sent back home from the Cassini spacecraft is devastatingly gorgeous, but it’s confession time: I prefer the greyscale ones to the pictures in color.
Why? Because this:
Holy ringed gas giant awesomeness! [Click to encronosenate.]
This shot was taken earlier this year, in June, when Cassini was about 3 million kilometers from the planet. Saturn has a thick haze above its cloud tops, obscuring much of the details of the clouds below (one of the main reasons it doesn’t sport the same spectacular cloud bands as its big brother Jupiter), but this image was taken using a near-infrared filter – just outside the normal range of human vision (centered at 752 nanometers, for those who want details) – that can see some light that gets through the haze. The white spots and elongated features are the tops of clouds of ammonia, some of which are thousands and even tens of thousands of kilometers long.
I love the angle on this picture. Cassini was south of Saturn’s equator, looking north. The northern hemisphere of the planet is edging toward summer right now, so the Sun is shining down on the rings, projecting their shadow on the southern hemisphere. We see the rings here from the unlit side, so they look a bit darker than you might be used to. However, since they’re made almost entirely of water ice, they’re transparent and scatter sunlight, so you can see them even from their shadowed side.
As a bonus, you can also see the tiny moon Enceladus on the lower left. Of course, when I say "tiny", I mean the size of my home state of Colorado.
This picture is jaw-droppingly beautiful, and I think a big part of that is that it’s greyscale (what some people call "black and white", which isn’t accurate since we see lots of shades of grey). While color images can be stunning, there is something about the contrast and chocolaty smoothness of greyscale that makes pictures like this more magnificent, more dramatic, and more brooding. I don’t know what it is – it’s the same phenomenon that happens with old movies, too – but for me it’s certainly a powerful effect.
As if Saturn needs any help.
Image credit: NASA/JPL-Caltech/Space Science Institute
There is a whole lot of awesome in a picture of Saturn and its rings just released from the Cassini spacecraft. Check this out:
Cassini was about 2 million kilometers (1.2 million miles) from Saturn when it took this picture, so we’re seeing a decently wide-angle view. At the time, the spacecraft was below the plane of the rings, looking north (up, if you like). The Sun is off mostly to the left and up a bit.
The first cool thing is obviously the shadow of the planet itself cast on the rings. It cuts across like a black scythe! As I looked at the picture my eyes and brain kept trying to fill in the missing arc of rings, which was amplified by a slight afterimage as my eyes moved around. It’s a difficult illusion to ignore.
Second, I love how you can see all the different rings in the picture, including the thin, lumpy F-ring outside the main band. The big gap is called the Cassini Division; it’s not really an empty space since there are many faint thin rings inside it. They’re just hard to see here. The Cassini Division is fairly easy to spot even through a small telescope, looking from Earth like someone took a knife to the rings and sliced them.
Third, you can see the tiny moons Janus (below the rings on the left) and Epimetheus (above the rings on the left) as well. I wonder how hard it is to get a picture like this without seeing any moons in it? Saturn has quite the fleet of them.
Fourth, look to the left, just where the inner arc of the rings cuts across Saturn. You can see the planet right through the rings! The rings aren’t solid; they’re composed of gazillions of particles of nearly pure water ice. There are spaces between the particles, so we can partially see through them, like looking through a screened window.
Fifth, and perhaps most cool of all: the part of Saturn we’re seeing here is the night side, entirely unlit by the Sun. The bottom (southern) part of Saturn is only noticeable by its absence! But what’s that glow in the north?
That, my friends, is ringshine! Although this part of Saturn is in nighttime, the Sun is still shining on the rings (wherever you don’t see Saturn’s shadow across them). The ring particles are very bright and shiny. They reflect the sunlight, which then illuminates the northern hemisphere of Saturn. The southern half is still dark because the ice particles tend to reflect light back up, like a mirror. Since the Sun is coming from the north, that’s the way the light gets reflected. I’ll note that most of the light gets reflected away from Saturn, to the upper right in this picture, but enough is reflected back to make the cloud tops glow softly.
This happens on Earth too, when sunlight reflects off the Earth and illuminates the dark part of the Moon. This is called Earthshine, also poetically called "the old Moon in the new Moon’s arms." It’s quite lovely.
And it’s science! Which is lovely, too.
Image credit: NASA/JPL-Caltech/Space Science Institute
[BAFacts are short, tweetable astronomy/space facts that I post every day. On some occasions, they wind up needing a bit of a mathematical explanation. The math is pretty easy, and it adds a lot of coolness, which I’m passing on to you! You’re welcome.]
Today’s BAFact: Jupiter is so big you could fit every other planet in the solar system inside it with room to spare.
Volume is a tricky thing. Our brains are pretty good at judging relative linear sizes of things: this thing is twice as long as that thing, for example. But volume increases far more rapidly than linear size. Take a cube where each side is one centimeter. It has a volume of one cubic centimeter (cc). Now double the length of each side to 2 cm. It looks twice as big, but its volume goes up to 8 cc! The volume of a cube is a the length x width x height, so there you go.
Spheres are the same way: the volume increases with the cube of the radius. Specifically, volume = 4/3 x π x (radius)3. So one sphere might look slightly larger than another, but in fact have a lot more volume.
Such is the way of Jupiter. I see pictures of it compared to the other planets, and honestly Saturn looks only slightly smaller – Saturn’s radius is about 60,000 km compared to Jupiter’s 71,000. But that turns out to make a huge difference in volume!
Here’s a table I created to compare the planets. The first number column is the planet’s equatorial radius in kilometers (the biggest planets aren’t perfect spheres, but as you’ll see this doesn’t matter). The second number column is the volume in cubic km based on that radius. The third is the volume of the planet divided by the volume of Jupiter (so that ratio = 1 for Jupiter itself). The last column is the same, but rounded to two decimal places to make it easier to read.
The big conclusion here is pretty obvious when you look at that last column. Even though Saturn is only a little smaller than Jupiter, it only has 60% of the big guy’s volume! Uranus and Neptune together are only another 9%. If you combine all the planets in our solar system, they add up to only about 70% of Jupiter’s volume. That leaves a lot of room left over for all the moons and asteroids in the solar system, too!
So Jupiter really is a monster. There’s a half-joke astronomers say: The solar system consists of the Sun, Jupiter, and assorted rubble. As you can see, that’s really not that far off from the truth!
Image credit: NASA
– BAFact math: Give him an inch and he’ll take a light year
– BAFact math: how big does the Sun look from Pluto?
– BAFact math: How bright is the Sun from Pluto?
– Announcing BAFacts: a daily dose of sciencey fun
What the heck is in the air this past week? First we see a simulated image of the sky from Mars go massively viral because people thought it actually showed Earth in the Martian sky, then a clearly Photoshopped pic of two "Suns" setting on Mars gets passed around.
And now a new slice of oddness enters the field: a picture of a planetary alignment over the Giza Pyramids, saying this only happens once every 2737 years. Because planetary alignments and the pyramids play such a large role in New Age/astrological beliefs, there is clearly some sort of spiritual message implied here.
Well, I hate to be a thricely-bursting-bubble person, but here we go again, again. Let me be clear: while there will be an event more-or-less like this in December, and it should be pretty and quite cool to see, the claims being made are somewhat exaggerated. The picture itself isn’t real, and the planets won’t really look like that from Giza. Also, alignments like this happen fairly often, though to be fair getting them spaced out to fit over the pyramids in this way probably is relatively rare.
Busting your Cheops
Here’s the picture making the rounds:
It clearly shows the three pyramids in Giza, Egypt, with three planets above them. There are various versions of this picture I’ve seen; most are like this with almost no explanation. Some say the planets are Mercury, Venus, and Saturn, and some mention this is what it will look like on December 3rd, 2012, just before sunrise.
First, this obviously cannot be an actual photo if the event hasn’t happened yet! This must be a Photoshop job. That’s fine if it’s only to show what things are supposed to look like, and no one is claiming this is an actual photo.
However, it hardly matters. There are lots of other problems with this planetary alignment claim.
What’s your angle?
The first thing I did when I saw this was ask: is there really going to be a close conjunction of three planets on December 3rd?
The answer is yes! Mercury, Venus, and Saturn will all be within a relatively small distance of each other in the sky on that date. This isn’t a particularly tight configuration like Venus and Jupiter were earlier this year – in this case, they’ll be 14 degrees apart, nearly 30 times the width of the full Moon on the sky – but it’s still pretty nifty.
The second thing I did, though, was ask myself: will they really look like that in the sky as seen from Giza?
The answer this time is no. I used the software planetarium program SkySafari to show what the three planets would look like in the sky before sunrise on December 3rd as seen from the location of the pyramids, and got this:
In this picture, the yellow line is the ecliptic, the path of the Sun in the sky through the year. The green horizontal line is the horizon, and the three planets are labeled.
Note the angle of the planets: in the picture going viral, the planets are much closer to horizontal, but in reality the line connecting the planets is at a much steeper angle. It’s nearly vertical, in fact. This may not seem like a big deal, but having the planets closer to horizontal like in the viral picture is more spectacular than what will really happen, exaggerating the claim.
Not only that, but in the pyramid picture the planets are almost exactly on a line, like beads on a string. But as you can see in the picture above, they’re not nearly that colinear. Again it’s looking like the pyramid picture is exaggerating the situation.
I noticed something else funny as well.
Here’s a satellite view of the three pyramids, courtesy Google maps:
In 2010, a storm erupted in Saturn’s northern hemisphere. It grew, and grew, and GREW, until it physically wrapped around the planet. At its peak it was 300,000 kilometers (180,000 miles) in length: 3/4 of the distance from the Earth to the Moon!
As you might expect, a storm like that might generate lightning… and even from a distance of 3.3 million km (2 million miles), the lightning flashes were bright enough that they were visible to the Cassini spacecraft:
Holy. Haleakala. [Click to encronosenate, and you want to.]
The lightning flash can be seen in the image on the left, indicated by the arrow. It happened while Cassini happened to be using a blue filter, which is why it appears to be that color. The white and tan milky clouds are from the storm itself.
The lightning has several analogies to storms here on Earth; the brightness was comparable to the brightest of terrestrial lightning strokes, and was produced in an atmospheric layer where water droplets freeze, like here as well.
But bear in mind the scale here. The head of that storm you can see in the image here is roughly the same size as our entire planet Earth. Storms like this must happen every so often on Saturn, given the odds of us happening to see one just as we also happen to have a spacecraft there that can take a really good look at it.
Always remember: when we gaze out at the objects in our solar system, and even beyond, these aren’t just static painting of long ago events, unchanging and forever frozen. They are actual worlds, dynamic and ever-shifting. And as alien as they are, there is always something analogous to Earth about them, something that will always remind us of, and teach us more about, our home.
Image credit: NASA/JPL-Caltech/Space Science Institute
The mighty planet Saturn is circled by a fleet of moons, each as different from the other as individual people. And as weird and alien as it seems, this Saturnian system of planet and moons have some similarities to our own Earth and Moon. For example, as they orbit Saturn, the moons can be eclipsed by it when they pass behind the planet and into its shadow.
The Cassini spacecraft caught exactly this event as the icy moon Enceladus slipped into Saturn’s shadow last October… and there’s more here than might initially meet the eye:
That’s amazing [click to penumbrenate]. But it may not be obvious what you’re seeing at first! Enceladus is the moon to the upper left. It’s about 500 kilometers (330 miles) across, and its surface is almost entirely water ice. At the time this shot was taken, it was about 26,000 km (16,000 miles) from Cassini.
If the moon were just sitting out there, half of it would be lit by the Sun, and half would be in darkness. Cassini was off to the side a bit when this was taken, so we see the hemisphere that is almost entirely lit by the Sun. The day/night line – called the terminator – runs from the upper left to lower right of the moon on its left side as seen here.
But because Enceladus was partially into Saturn’s shadow, the sunlit side of the moon that would normally be painfully bright is dusky and dark. The shadow is deepest toward the bottom of the moon. The geometry of this scene depends on so many angles! The terminator line, the position of Cassini relative to the moon and Sun, the position of Saturn, and even the curve of the planet itself as its shadow envelops the moon.
And we’re not done. Photobombing the scene at the lower right is the monster moon Titan, which is 10 times bigger in diameter than Enceladus! But it was over a million kilometers away from Cassini when this picture was taken, so it actually looks smaller than its very much smaller sibling. It appears dark, even compared to the shadowed Enceladus, because Titan only reflects about 1/5th of the light that hits it, while shinier Enceladus reflects almost all the light that impinges on its icy surface.
Funny, too: the edge of Titan looks fuzzy, because it has a thick atmosphere. Enceladus has no atmosphere, but still looks a bit fuzzy as well due to Saturn’s shadow: the planet does have an atmosphere, so the shadow itself isn’t sharp.
The complexities of understanding even a seemingly simple picture are ridiculous when that picture comes from Saturn. But that’s so often true: things do appear easy at first glance, but far more complicated when you peer more deeply. The Universe, as are human affairs, is rarely so black-and-white.
Image credit: NASA/JPL-Caltech/Space Science Institute
The Cassini spacecraft has been orbiting Saturn since late 2004, and has spent most of that time more or less in the same plane as the rings and moons. That allows it to pass close to these interesting places and see them in high resolution.
But scientists and engineers recently changed that, flinging the probe into a more inclined orbit so that it can see things from a different vantage point, literally getting a new perspective on them. For example, from this tipped path, it was able to clearly see the south pole of Titan, Saturn’s ginormous moon – the biggest in the soar system, bigger than the planet Mercury! And what it saw surprised everyone, and for good reason:
Isn’t that weird looking? Like some kind of bacterium, or a cell. In fact, it is a cell, but not the biological kind. It’s an air cell, a vortex, a spinning around the pole. Titan has a thick atmosphere (thicker than Earth’s in fact) and it moves. This cell of air rotates once every 9 hours or so, far faster than Titan’s own 16 day spin. Cassini took enough images to make this animation of the vortex’s motion:
Things like this are seen at the poles of other words; Saturn itself has one, as does Venus. Titan also has a "hood" a haze layer over its north pole. That may be a seasonal feature, and right now winter is coming for Titan’s southern hemisphere*. Perhaps this vortex plays a part in forming the polar hood, and we’ll see one over the south pole soon.
That’s not clear yet, but it may become so as Cassini continues to investigate this incredible system. It’s been there for almost 8 years, and we’ve barely scratched the surface of what’s going on. There’s a whole lot of real estate in the Saturn system, and it changes all the time. We could use 50 Cassinis stationed there, and it still wouldn’t be enough to gather up all the beauty and amazing slices of nature to be seen.
Credits: Video: NASA/JPL-Caltech/Space Science Institute; Music: “Passing Action” by Kevin MacLeod
If you showed me this picture with no preamble, I’d know it was from Cassini, and showed a moon of Saturn, but I’d be baffled as to which one it is:
[Click to ensithenate.]
If you told me it was Mimas, I’d be surprised… and I was when I saw it! But it’s true. Mimas is a 400 km ball of mostly ice (and some rock) orbiting Saturn about 180,000 km out. From this angle, Cassini was looking down at the north pole from a steep angle, and that’s not how we usually see it.
This is how we usually see it! The giant crater Herschel dominates the face of the moon, giving it as definite Vaderesque feel. But in the big image the crater isn’t visible, so the landscape looks markedly different.
This image was processed by Ian Regan, who notes that the blue band you can see around the edge of the moon is real. It’s a bluer region that wraps around the equatorial regions of Mimas, the origin of which is still something of a mystery. However, it does match the very odd thermal pattern seen by cameras on board Cassini, a pattern that makes Mimas look like a giant PacMan in the sky.
Cassini takes so many pictures it’s ironically not surprising that some will be surprising. Still, when it comes to astronomy, surprises are fun. They’re also a chance to learn something — as I did since I didn’t know about the blue band. And I also learned that even a familiar place can look very different if you get a different angle on it.