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When the Earth photobombs the Sun

The Solar Dynamics Observatory is a NASA satellite that observes the Sun 24 hours a day. It orbits the Earth, placed carefully so that it takes 24 hours to circle the Earth once — what we call a geosynchronous orbit. This maximizes its output, and allows scientists to squeeze as much data from it as possible.

But, twice a year, the geometry of SDO’s orbit aligns in such a way that the Earth itself gets between the observatory and the Sun. When that happens, you get an eclipse! We’re in one of those "eclipse seasons" now, and around midnight last night UTC one such eclipse occurred. The folks at SDO created a nifty video from the images collected during that time:

That’s cool. You can see the Earth barreling through the image, blocking SDO’s view. SDO has several different cameras which look at the Sun at different wavelengths of ultraviolet and optical light. The first view, colored red, is actually in ultraviolet (at 304 Angstroms, if you’re keeping track). The next view, colored gold, is even further in the UV (193 Angstroms). Then they cycle through a bunch of different wavelengths, giving a psychedelic journey through ...


East of the Blue Marble

Last week, I posted an exceptional image of our home world as seen by the Suomi NPP Earth-observing satellite. The image was so popular that NASA released a second one, this time of the Eastern hemisphere, showing once again why it’s called the Blue Marble:

[Click to engaiaenate, or grab the terrestrialicious 11,500 x 11,500 pixel shot].

Like the other one, this is a mosaic, created over six different orbits — the bright north/south swaths are actually the reflection of the Sun in the ocean as the satellite passed over that area multiple times.

Although the satellite is in low Earth orbit, just a few hundred kilometers off the surface, the images have been mosaicked together to represent the view as if you were about 13,000 km (8000 miles) away. You’re seeing most of but not quite all of the entire hemisphere here. The inset image shows why; the farther you are from Earth the more of it you see.

If you’re having a hard time picturing that, imagine taking a camera and holding it a couple of centimeters from your ...


Amazing moonset video taken from space!

Thanks to astronaut Ron Garan on Google+, I was alerted to some amazing footage of the Moon setting as seen by astronauts on board the International Space Station. I uploaded it to YouTube and added some comments to show you something really cool…

[Set it to high-def and make it full screen!]

Astonishing, isn’t it? As the Moon sets, you’re seeing it through thicker and thicker air. The air acts like a lens, bending the light upward. The part of the Moon nearer the Earth’s limb gets bent up more, so the Moon looks like it’s getting flattened. Watch it again; the top of the Moon doesn’t appear to be affected much. It looks more like the bottom slows down and the top pushes into it. You can read about this effect in more detail in an earlier blog post.

Weirdly, as I watched the video, it looked very much like the whole Moon was shrinking as it set, as if it were receding rapidly. When I saw that I knew intuitively that couldn’t be real; the ISS is only moving a few thousand kilometers ...


Mosaic of home

Just before Halloween last year, NASA launched into orbit the improbably named National Polar-orbiting Operational Environmental Satellite System Preparatory Project, which they thankfully shortened to NPP. In its low 800 km (500 mile) orbit it looks down at the Earth to investigate our environment. It only sees a portion of the Earth at any one time, but if you take observations taken during a single day — say, on January 4, 2012 — and stitch them all together, you get this magnificent shot:

[Click to engaiaenate, or download the Big McLarge Huge 8000 x 8000 pixel version.]

Man, the resolution is so high is like you’re actually there.

Oh wait.

In fact, the biggest version is 8000 pixels across, and the Earth is about 8000 miles wide, so the resolution is about a mile per pixel. We’re not seeing the entire hemisphere here, but the view is roughly 8000 km across (judging from the size of the US compared to the view). The big image is 8000 pixels wide, so the resolution of that mosaic is about 1 km/pixel. The Earth is big.

NPP was recently renamed Suomi NPP in honor of Verner Suomi, a pioneer in using satellites in meteorology. I like that we tend to name satellites and space probes after people whose work made those very missions possible, or for people we honor and respect (my favorite is still Sojourner, the Mars rover named after Sojourner Truth… with the bonus of the name being a pun).

Apropos of nothing, I’ll note the images making up this seamless mosaic were taken around the same time the Earth was at perihelion, when it was closest to the Sun in its orbit. There is nothing particularly important about that fact, but still… when I see pictures like this I think about how amazing our planet is, and how wonderfully well-adapted we are to it. Evolution is a stochastic process, a semi-random series of bumps and false starts that literally made us who were are today. But that doesn’t change the feeling of comfort I get when I see a picture of Earth, floating in space, sitting in the brightest and warmest sunlight of the year.

It’s home, and I’m glad we’re taking such a close look at it.


Related posts:

- New satellite gets INSANELY hi-res view of Earth
- Rosetta takes some home pictures
- Earth from Rosetta
- What does a lunar eclipse look like from the Moon?


Wait just a (leap) second

Clock at midnightThis summer will be a little bit longer than usual. A tiny little bit: one second, to be precise. The world’s official time keepers are adding a single second to the clocks at the end of June. This "leap second" is needed to keep various time scales in synch. It’s a bit of a pain and won’t really affect people much, but if it weren’t done things would get messy eventually.

This gets a bit detailed — which is where the fun is! — but in short it goes like this. We have two systems to measure time: our everyday one which is based on the rotation of the Earth, and a fancy-schmancy scientific and precise one based on vibrations of atoms. The two systems aren’t quite in synch, though, since the Earth counts a day as a tiny bit longer than the atomic clocks say it is. So every now and again, to get them back together, we add a leap second on to the atomic clocks. That holds them back for one second, and then things are lined up once again.

There. Nice and simple. But that’s spackling over all the really cool details! If you want a little more info, you can read the US Naval Observatory’s press release on this (PDF).

If you want the gory details, then sit back, and let me borrow a second of your time.


Time after time

There are lots of ways of keeping time. The basic unit day is based on the physical rotation of the Earth, and year is how long it takes to go around the Sun. But we need finer units than those! So we decided long ago to divide the day into 24 hours, and those into 60 minutes each, and those into 60 seconds each. In that case, there are 86,400 seconds in a day. OK, easy enough.

For most of us, that is enough. But scientists are picky (or "anal" if you want to be technical) and like to be more precise than that. And the thing is, the Earth is a bit of a sloppy time keeper. Tidal effects from the Sun and Moon, for example, slow it a bit. Other effects come in as well, changing the rate of the Earth’s rotation.

To account for this, in 1956 the International Committee for Weights and Measures made a decision: we’ll base the length of the second on the year, not the day. In fact, we’ll take the year as it was in the year 1900 (a nice round number, so why not) and say that the length of the second is exactly 1/31,556,925.9747 of the year as measured at the beginning of January 1900*.

OK, fine. Now scientists have their anal precise definition, normal people have calendars, and we’re all happy, right?

Right?


Sunrise, sunset

Yeah. Not so much. Defining the second as a fraction of a year is fine and all, but it kind of leaves the unit of "day" out in the cold. To define that, we use what’s called a mean solar day, which is essentially the time it takes for the center of the Sun’s disk to pass a point in the sky twice. So basically look at the Sun, mark its position and note the time, and wait for it to pass that point in the sky again. That’s a solar day.

But this doesn’t depend on the second or the year! And remember, the length of the day is slowly increasing. You can ask yourself – and you should – hey, when were there exactly 86,400 seconds (as we now define them based on the year 1900) in one solar day? Because if the day is getting longer, there are more seconds in a day now than there were a hundred years ago.

The answer, it turns out is in the year 1820. More or less, but close enough. Back then, a solar day had 86,400 of these new-fangled seconds in it. But that’s not true any more. The Earth has been slowing, the day getting longer, and now, almost two centuries later, there are about 86,400.002 seconds in a day.

Yup. The day has 2 extra milliseconds in it. That may not sound like much, but it adds up. Over the course of a single year we have an extra 365 of those 2 millisecond slices of time. That adds up to about 0.73 seconds every year. After a year, the calendar is off by about 3/4 of a second because the Earth’s rotation is slow. In two years that’s 1.46 seconds, and after ten years it’s over 7 seconds!

We can’t have that, obviously. But what can you do?


The Atomic Age

In 1972 a new timekeeping system was adopted: Coordinated Universal Time, or UTC, based on an atomic clock. The idea is that atoms are pretty good timekeepers, and in particular a cesium atom makes an excellent clock (I describe why here). In a sense using an atomic clock makes it unnecessary to use the Earth as a clock… but we humans have this pesky desire to use clocks in our everyday lives, and to base them on things like sunrise and sunset — in other words the Earth’s rotation (the aforementioned system, which is called Universal Time 1 or UT1).

And we know the Earth’s rotation is a bit slower than it was, and every year we have these dangling 0.73 seconds. That means that the Earth time is lagging behind the atomic time by that much every year.

The fix for that is to add leap seconds when needed. The International Earth Rotation and Reference Systems Service (IERS) are the folks who keep track of these things, and they decided that when the lag between UT1 and UTC gets to be more than 0.9 seconds, they add a leap second to the end of a convenient month, and the two get back to being much closer in synch.

That’s why we were adding one at the end of June.

And we’re done. Right?

Right?


Stop the Earth, I wanna get off!

Nope. I want to clear up a misconception (used by creationists sometimes) first… and then I have to add one more thing.

Some people think that because we have to add leap seconds every year or so, the Earth must be slowing by a tremendous rate. But that’s not the case: the reason we add leap seconds is because the two time systems have clocks that tick at different rates, essentially. It’s not much, but over time it adds up. I’ve written about this before:

Imagine you have two clocks. One thinks there are 86,400 seconds in a day, the other thinks that there are 86,401, so the second clock runs a tad bit slower than the first. Every day, it’s one second behind, clicking over to midnight one second after the first clock does. Mind you, it keeps accurate time according to its own gears: every day has 86,401 seconds, so it’s not slowing down.

However, to keep it synchronized with the other clock, we’d either have to subtract a second from the second clock (yikes, terminology is a bit confusing there!) or add one to the first clock every day. So we’d need a leap second every day, but not because the clock is slowing. It’s only because it runs at a different (but constant) rate.

So it’s not that the Earth is slowing down so much. If the Earth were to maintain its current spin rate from now on, we’d still have to add leap seconds every now and again, because it’s running slow. In that case, we could simply insert leap seconds at regular intervals and everyone’s happy.

But there’s still one more thing. Of course there is.


Staggering seconds

The final issue is that the Earth isn’t slowing at a constant rate. There are a lot of factors that change the Earth’s spin — weather, damming rivers, earthquakes, and so on — that add up over time. So it’s not just that the Earth is slow compared to an atomic clock, but also that the amount it’s slow changes! We can’t just add a leap second every 15 months or whatever; we have to watch the Earth’s spin carefully and add them in as needed. Since 1972 when all this started, there have been 24 leap seconds added to atomic clocks. Sometimes the interval between them has been less than a year, and sometimes it’s been quite a bit more. The last one was added on December 31, 2008.


Cutting the cord

After all this, you might be wondering why we bother. Why not just decouple the two clocks, and let them go their separate ways?

A lot of scientists do in fact feel this way. But it turns out to be really, really complicated to do that. A lot of computer systems (including satellite navigation systems) have software written a while ago, and changing that would be difficult and have unforeseen consequences. Fiddling with that may be dangerous.

At a recent meeting of the American Astronautical Society, there was a session on this topic. A paper was written (PDF) giving an overview of it. It gets a little technical, but it might make for interesting reading for any chronological geeks out there.

I think I lean toward the present system of keeping the systems in tune by using leap seconds. It’s a small price to pay for having our own internal clocks based on the spinning planet.

… but I wonder. There will come a day when we leave this planet for others. The Moon, Mars, and beyond. When we do, we’ll have to worry about timekeeping there as well. We do have one for Mars, but it will have the same inherent problems we do now.

It’s actually kind of neat: there may — there will — be a time when we do need a truly Universal time system. What will we do then?

Images courtesy of zoutedrop’s Flickr stream; NASA; Ozymandias.


* There are different ways of measuring the year, too so they went with a tropical year, which was a pretty decent choice.


Related posts:

- Take a flying leap second
- Followup: leap seconds
- Another orbit? Why, you don’t look a rotation older than 4.56 billion years!
- Why we have leap days (one of my favorite posts of all time)


Another Kepler milestone: Astronomers find two Earth-sized planets orbiting the same star!

Astronomers have achieved a big milestone in the search for another Earth: the two smallest confirmed planets ever found orbiting another star… and they’re both about the size of Earth!


Artist’s illustration of the Kepler-20 planets with Earth and Venus for size comparison.

The planets are called Kepler-20e and Kepler-20f, and as you can see by the illustration above they are very close to the same size as our home world: 20e is about 11,100 km (6900 miles) in diameter, and 20f about 13,200 km (8200 miles) across. For comparison, Earth has a diameter of 12,760 km (7930 miles). This makes them the smallest confirmed exoplanets seen orbiting another star! The previous record holder was Kepler-10b, which has a diameter about 40% bigger than Earth’s.

To be clear: while these planets are the size of Earth, they are nowhere near Earth-like. The star, Kepler-20, is very much like the Sun, though a bit smaller and cooler (and 950 light years away). However, both planets orbit the star much closer than Earth does; 7.6 million km (4.7 million miles) and 16.6 million km (10.3 million miles), respectively. This is so much closer that both planets must have surface temperatures far hotter than ours, 760°C and 430°C (1400°F and 800°F). Even on the "cooler" planet Kepler-20f, it’s hot enough to melt tin and zinc.

So don’t start packing your bags to visit, even if you could spare a few million years to get there via rocket (950 light years is a bit of a hike). I’ll note that we don’t know the masses of these planets either. I’ll explain that in a moment, but given their sizes it’s expected they’ll have masses similar to Earth’s.

So this is very exciting! For one thing, it shows that Kepler can indeed find planets the size of Earth orbiting distant stars. That right away is fantastic; that’s the main goal of Kepler in the first place.

For another, it shows that our solar system is not entirely unique. We do know of several other stars hosting solar systems of their own, but those planets tend to be very massive; they’re easier for us to find. Since Kepler-20e and f are so close to Earth-sized, this is a big achievement.

And we’re still not done: there are three other planets in the Kepler-20 system! The others are much larger than the Earth: named Kepler-20b, c, and d, they have diameters of 24,000, 40,000, and 35,000 km (15,000, 24,600, and 22,000 miles); smaller than Uranus and Neptune, but still pretty hefty. We do have the masses for them: 8.7, 16.1, and about 20 times the mass of the Earth. Call them "super-Earths" if you like.

All these planets huddle pretty closely to their star; the orbit of Kepler-20f, the farthest from the star, would still fit comfortably inside the orbit of Mercury! Oddly, the configuration is very different than our own solar system. While ours has the lower-mass planets close in and the bigger ones farther out, in the Kepler-20 system they alternate, going big-little-big-little-big.

So how do we know all this? The Kepler observatory is in space, staring at one patch of sky all the time. There are 100,000 stars in its field of view, including Kepler-20. If there are planets orbiting a star, and we see the orbit of that planet edge-on, then once per orbit the planet directly passes between us and the star, blocking its light a little bit. This is called a transit, and the bigger the planet, the more light it blocks. That’s how the sizes of the five planets were found.

As these planets orbit their star their gravity tugs on it, and that can be measured by carefully observing the star’s light. As a planet pulls it one way and then another, there is a very small Doppler shift in the starlight, and the amount of that shift tells us how hard the planet is tugging on the star, and that in turn depends on the mass of the planet. Only the three bigger planets in the Kepler-20 system pull hard enough for us to measure, which is why we don’t have the masses of 20e and 20f; they’re too small to measure.

Also, to be clear, we don’t have direct images of these planets (those pictures above are drawings). They were found indirectly by how they affected their star. But these methods are now tried-and-true, and the existence of these five planets has been confirmed. They’re real.

This is a fantastic discovery for so many reasons: the smallest planets found orbiting another star, the first Earth-sized planets seen by Kepler, both in the same solar system, and in such an oddly-configured and compact system at that. This means we need to think more about how such planets can form, of course, since it’s so weird… but no matter what, it means we’re that much closer to finding the ultimate goal: an Earth-sized planet orbiting a Sun-like star in that star’s habitable zone, where liquid water can exist.

Every time I hear news like this, I wonder how much longer we’ll be waiting to hear that news… and I strongly suspect it won’t be too much longer.

Image credit: NASA/Ames/JPL-Caltech


Related posts:

- Kepler confirms first planet found in the habitable zone of a Sun-like star!
- A boiling superEarth joins the exoplanet roster
- Big news: first “solid” exoplanet found!
- Two exoplanets discovered by "citizen scientists"


Top 14 Solar System Pictures of 2011

Click here to view gallery


Mesmerizing visualization of a geomagnetic storm

When the Sun belches out an eructation of subatomic particles, they can travel across the solar system and interact with the Earth’s magnetic field. This can make our field ring like a bell, shaking the particles trapped within, and generating electromagnetic noise and signals across the radio spectrum. The CARISMA radio array can detect these emissions and learn about how the Sun’s and Earth’s fields interact.

That’s the science. But there’s art here, too: the Lighthouse agency commissioned artists to create digital artwork based on science, and one group, Semiconductor, used the CARISMA data to do so. Based on the data, they translated the radio waves (which are like the light we see, but less energetic) and converted them to sound. This has been done many times before, but what’s cool is that they then created an animation based on the converted sounds, an astonishing and odd and mesmerizing animation. Watch:

How wild is that? It reminds me of the movie "Forbidden Planet". The vibrating patterns are wonderful, and while I’m not sure how much scientific insight can be gained from them, the aesthetics are riveting. And I can hope the underlying purpose of this will be seen: to show that science is beauty, science is art, and that if this gets someone who might not otherwise be interested to poke a little further into it, then mission accomplished.


Related posts:

- Cosmically creepy chords
- Listen in on the Perseid meteor shower
- Saturn, the forbidden planet
- Phoenix sings


New satellite gets INSANELY hi-res view of Earth

On October 28th, the National Polar-orbiting Operational Environmental Satellite System Preparatory Project (NPP) satellite launched into low-Earth orbit from Vandenberg Air Force base in California. Designed to observe Earth’s environment and climate, it’s in an 800 km (500 mile) orbit, and on November 21 it took its first images of the planet below.

And what a picture! Check. This. Out.

[Click to engaiaenate.]

What’s that, I hear you ask? It doesn’t look like that big a deal? That’s because I had to shrink the flippin’ huge 6000×6000 original image to fit the blog! The whole swath shows the planet from Canada to South America, but here’s a closer-up version:

This zooms in a bit to show Florida, Cuba, and part of Hispaniola. You can really see an amazing amount of detail, even in this compressed version.

But wait! We can zoom in even more!

Yegads. Florida dominates the upper left, with stippled clouds and Lake Okeechobee visible. You can also see the jade-green Atlantic waters, and the islands of the Bahamas, Nassau, and Freeport. And even that isn’t full-res! Download the big picture to scan over it yourself. It’s stunningly beautiful.

The image was taken with the Visible Infrared Imager Radiometer Suite, or VIIRS, which, as its names states, takes visible and IR images of the Earth. It can be used to observe hurricanes, fires, ocean surface temperatures, aerosols in the air, volcanoes, and more. It continues the incredibly valuable work done by the MODIS instruments on Terra and Aqua, two NASA Earth-observing satellites. All of these data are extremely important, in that they provide a continuous observational database of the Earth — a dynamic system that changes on very short timescales. VIIRS can deliver this data rapidly, making it that much more an asset in NASA’s toolbox.

Even as NASA’s budget gets cut, and even as climate change denial continues, the science rolls on. We must study our planet if we are to understand it, and we must study it if we are to continue to survive on it. NPP and VIIRS will help scientists — all of us — in that task.

Credit: NASA/NPP team


Related posts:

- Oh. So that’s why they call it that.
- Hurricane Irene from start to finish
- Irene sidles up to the east coast
- Ice island heading south off Labrador
- A long, thin, volcanic plume from space


An astronaut’s away-from-home movie: Fragile Oasis

Astronaut Ron Garan’s photography is a common feature here at BA Central, and although his still photos are incredible, he hadn’t tried time-lapse photography until his last trip up to the space station.

He took a series of images and he himself created a video from them, called "Time Lapse From Space – Literally. The Journey Home". It’s similar to the time lapse I posted recently of the Earth from space, but has some new stuff in it:

Breathtaking, isn’t it?

This is part of a project Ron is working on called Fragile Oasis, an effort to get everyone to see the Earth as a single home for humanity, and to inspire people to make a difference, change things for the better. About his feelings as he gazed down on the Earth from space, Ron writes:

It was very moving to see the beauty of the planet we’ve been given. But as I looked down at this indescribably beautiful fragile oasis, this island that has been given to us and has protected all life from the harshness of space, I couldn’t help thinking of the inequity that exists.

I couldn’t help but think of the people who don’t have clean water to drink, enough food to eat, of the social injustice, conflict, and poverty that exist.

The stark contrast between the beauty of our planet and the unfortunate realities of life for many of its inhabitants reaffirmed the belief I share with so many. Each and every one of us on this planet has the responsibility to leave it a little better than we found it.

I can’t argue with that. In fact, I strongly support this effort, and hope everyone out there spreads the word.


Related posts:

- JAW DROPPING Space Station time lapse!
- The twice reflected Moon light
- A new day, from space
- Expedition 28 from the ISS lands safely in Kazakhstan