How Can We Move the Earth?

How Can We Move the Earth?

Sooner or later we’re going to want to move the Earth further away from the Sun. It turns out, there are a few techniques that might actually make this possible. Not easy, but possible.

You live here. I live here. Everybody lives here. For now.

In 500 million years the gradual heating of the Sun will burn away all life on Earth. Then we might have to move. Even if we get past the 500 million year deadline, the Sun will die as a red giant in about 5 billion years.

Let’s review our options? We could die… orrrr we could move the Earth. Just like any other mad science scheme, there’s a hundred ways to skin this cat. We could launch powerful rockets off the Earth, which would push the Earth a little bit in the opposite direction.

We could build a giant teleporter and disassemble the Earth atom by atom into a new location. We could repeatedly smash things into the Earth. Eventually knocking it off orbit, possibly also changing its axis and or rotation.

We could paint half the Earth silver, stop it rotating and let the Sun push it away. We could dig a giant hole down to the core and repeatedly detonate warheads inside the Earth forcing molten material to fly off into space, propelling us forwards like a deflating balloon.

Sure, maybe that does all sound a little crazy. We could build a gravity tug, and slowly pull the Earth away from the Sun. What’s a gravity tug? I’m so glad you asked.

You could build a solar sail with a huge mass connected to it. This gigantic weight would want to fall towards the Earth, and the Earth slowly drifts towards the weight. The solar sail is being pushed away by the Sun dragging both the weight and as a result the Earth along with it. This would take a very, very, very long time.

The Solar Sail demonstration mission.  Credit: NASA
The Solar Sail demonstration mission. Credit: NASA

Here’s the best idea scientists have come up with so far. Gravity assists: Attach rockets to an asteroid, comet or Kuiper belt object and have it fall on a trajectory that takes it close to the Earth. Earth and this space rock would exchange a little momentum.

The rock slows down a bit and goes into a new orbit, and the Earth speeds up a little. That additional momentum pushes our orbit up a tiny little bit, and now we’re further away from the Sun. You’d need to do this tens of thousands or even a million times.

You might think, “Hey, that’s crazy. Where would you get all this stuff to hurl past the Earth?”. Don’t worry, the Oort cloud alone has billions of objects with a total of 30 times the mass of the Earth.

To prepare for Roastpocalypse, If we started now, we should cause a close pass with a large object every few thousand years. We bring them within 10,000 km of the surface of the Earth, which would have the likely side effect of causing severe tides and storms.

The layout of the solar system, including the Oort Cloud, on a logarithmic scale. Credit: NASA
The layout of the solar system, including the Oort Cloud, on a logarithmic scale. Credit: NASA

Oh, and get the math wrong and you’ll smash an asteroid into the Earth. Just so you know, these would be way bigger than the object that killed the dinosaurs. One hit from a 100km diameter object would sterilize the biosphere.

If we pushed the Earth out to about 1.5 times its current orbit, which might get a little too cozy with Mars for comfort, we’d give the Earth another 5 billion years of habitability,

Then the Sun turns into a red giant, and then dies as a white dwarf. And nothing can help us then… except perhaps some kind of planet sized star gate.

What do you think? What’s the best suggestion you’ve got to move the Earth out to a safe distance? Tell us in the comments below.

Why is Everything Spherical?

Why is Everything Spherical?

Have you ever noticed that everything in space is a sphere? The Sun, the Earth, the Moon and the other planets and their moons… all spheres. Except for the stuff which isn’t spheres. What’s going on?

Have you noticed that a good portion of things in space are shaped like a sphere? Stars, planets, and moons are all spherical.

Why? It all comes down to gravity. All the atoms in an object pull towards a common center of gravity, and they’re resisted outwards by whatever force is holding them apart. The final result could be a sphere… but not always, as we’re about to learn.

Consider a glass of water. If you could see the individual molecules jostling around, you’d see them trying to fit in as snugly as they can, tension making the top of the water smooth and even.

Imagine a planet made entirely of water. If there were no winds, it would be perfectly smooth. The water molecules on the north pole are pulling towards the molecules on the south pole. The ones on the left are pulling towards the right. With all points pulling towards the center of the mass you would get a perfect sphere.

Gravity and surface tension pull it in, and molecular forces are pushing it outward. If you could hold this massive water droplet in an environment where it would remain undisturbed, eventually the water would reach a perfect balance. This is known as “hydrostatic equilibrium”.

Stars, planets and moons can be made of gas, ice or rock. Get enough mass in one area, and it’s going to pull all that stuff into a roughly spherical shape. Less massive objects, such as asteroids, comets, and smaller moons have less gravity, so they may not pull into perfect spheres.

UT Jupiter Oval BA Chris Go
Jupiter Credit: Christopher Go

As you know, most of the celestial bodies we’ve mentioned rotate on an axis, and guess what, those ones aren’t actually spheres either. The rapid rotation flattens out the middle, and makes them wider across the equator than from pole to pole. Earth is perfect example of this, and we call its shape an oblate spheroid.

Jupiter is even more flattened because it spins more rapidly. A day on Jupiter is a short 9.9 hours long. Which leaves it a distorted imperfect sphere at 71,500 km across the equator and just 66,900 from pole to pole.

Stars are similar. Our Sun rotates slowly, so it’s almost a perfect sphere, but there are stars out there that spin very, very quickly. VFTS 102, a giant star in the Tarantula nebula is spinning 100 times faster than the Sun. Any faster and it would tear itself apart from centripetal forces.

This oblate spheroid shape helps indicate why there are lots of flattened disks out there. This rapid spinning, where centripetal forces overcome gravitational attraction that creates this shape. You can see it in black hole accretion disks, solar systems, and galaxies.

Objects tend to form into spheres. If they’re massive enough, they’ll overcome the forces preventing it. But… if they’re spinning rapidly enough, they’ll flatten out all the way into disks.

Watch the Rise and Fall of a Towering Inferno on the Sun

A solar prominence imaged on May 27, 2014. Earth and Moon are shown to scale at the bottom. (NASA/SDO)

Caught on camera by NASA’s Solar Dynamics Observatory, a prominence blazes hundreds of thousands of miles out from the Sun’s surface (i.e., photosphere) on May 27, 2014. The image above, seen in extreme ultraviolet wavelengths, shows a brief snapshot of the event with the column of solar plasma stretching nearly as far as the distance between Earth and the Moon.

Watch a video of the event below:

The video covers a span of about two hours.

Although it might look fiery in these images, a prominence isn’t flame — it’s powered by rising magnetic fields trapping and carrying the Sun’s superheated material up into the corona. And while this may not have been a unique or unusual event — or even particularly long-lived — it’s still an impressive reminder of the immense scale and energy of our home star!

Credit: NASA/SDO

The Sun Fires Off a Third X-Class Flare

A "triple X" on June 10-11, 2014 with three flares from AR2087 (NASA/SDO/GSFC)

Remember yesterday when we mentioned two X-class flares erupting from the Sun within the space of about an hour? We probably should have waited a bit and gone for the trifecta: this morning the same active region flared yet again, making it three high-powered flares within a single 24-hour period.

(And to think this active region has only just come around the corner!)
On June 10, 2014, AR2087 announced its arrival around the southwestern limb of the Sun with an X2.2 flare at 11:41 UT (7:41 a.m. EDT). Then, just over an hour later, another eruption: an X1.5 flare at 12:55 UT. This got pretty much everyone’s attention… here comes 2087!

Perhaps figuring third time’s a charm, the active region blazed with a third flare this morning at 9:05 UT (5:05 a.m. EDT). “Only” an X1-class, it was the weakest of the three but AR2087 still has plenty of time for more as it makes its way around the Sun’s face — all the while aiming more and more our way, too.

Here’s a video of SDO observations showing the two June 10 flares:

X-class flares are the strongest in the letter-classification of solar flares, which send blasts of electromagnetic energy out into the Solar System. While these most recent three are low on the X-scale, they may result in increased auroral activity — especially since it appears that the first two were followed by a pair of CMEs that “cannibalized” each other on their way out. The resulting merged cloud of charged particles is expected to nick Earth’s magnetic field on Friday, June 13. (Source: Spaceweather.com)

No CME has been observed from the June 11 flare, but again: AR2087 hasn’t left the stage yet. Stay tuned!

Source: NASA. Learn more about how solar flares impact us on Earth here.

Curiosity Captures Mercury from Mars

Image of the Sun as seen from Mars by Curiosity. Mercury is the circled dark spot.

NASA’s Curiosity rover may be busy exploring the rugged and rocky interior of Gale Crater, but it does get a chance to skygaze on occasion. And while looking at the Sun on June 3, 2014 (mission Sol 649) the rover’s Mastcam spotted another member of our Solar System: tiny Mercury, flitting across the Sun’s face.

Silhouetted against the bright disk of the Sun, Mercury barely appears as a hazy blur in the filtered Mastcam images. But it was moving relatively quickly during the transit, passing the darker smudges of two Earth-sized sunspots over the course of several hours.

It’s the first time Mercury has ever been imaged from Mars, and also the first time we’ve observed a planet transiting our Sun from another world besides our own.

Watch an animation of the transit below:

Animated blink comparison showing Mercury's movement across the Sun
Animated 1-hour interval blink comparison showing Mercury’s movement across the Sun

Because the sunspots move along with the rotation of the Sun (and the Sun rotates once avery 25 days around its equator) Mercury makes a fast pass as it travels along on one of its 88-day-long years.

Watch an HD version of the event here.

In reality this was no chance spotting, but rather a carefully calculated observation using the Mastcam’s right 100mm telephoto lens and neutral density filter, which is used to routinely image the Sun in order to measure the dustiness of the Martian atmosphere.

“This is a nod to the relevance of planetary transits to the history of astronomy on Earth. Observations of Venus transits were used to measure the size of the solar system, and Mercury transits were used to measure the size of the sun.”

– Mark Lemmon, Texas A&M University, member of the Mastcan science team

Read more: Amazing Transit of Venus Images from Around the World

The next chance for Curiosity to spot Mercury will come in April 2015 and, if the rover is still operating by then — perhaps with some upgrades by future human visitors? — it may capture Earth similarly passing across the Sun in November of 2084.

Source: NASA/JPL

Image/animation credit: NASA/JPL-Caltech/MSSS/Texas A&M

The Sun Pops Off Two X-Class Solar Flares in One Day

A solar flare bursts off the left limb of the sun in this image captured by NASA's Solar Dynamics Observatory on June 10, 2014, at 7:41 a.m. EDT. This is classified as an X2.2 flare, shown in a blend of two wavelengths of light: 171 and 131 angstroms, colorized in gold and red, respectively. Image Credit: NASA/SDO/Goddard/Wiessinger.

In only a little over an hour, the Sun released two X-class solar flares today. The first occurred at 11:42 UTC (7:42 a.m. EDT) and the second blasted out at 12:52 UTC (8:52 a.m. EDT) on June 10, 2014. According to SpaceWeather.com, forecasters were expecting an X-class flare today, but not two…and certainly not from region of the Sun where the flares originated. Solar scientists have been keeping an eye on sunspot regions AR2080 and AR2085, especially since they are now directly facing Earth, and those two sunspots have ‘delta-class’ magnetic fields that harbor energy for X-flares.

But the active region on the Sun that actually produced the flares was AR2087, which just appeared “around the corner” on the southeastern limb of the Sun. The first flare was a X2.2-flare and the second was an X1.5-flare.

See the image of #2 below from the Solar Dynamics Observatory:

The second X-class flare of June 10, 2014, appears as a bright flash on the left side of this image from NASA’s Solar Dynamics Observatory. This image shows light in the 193-angstrom wavelength, which is typically colorized in yellow. It was captured at 8:55 a.m EDT, just after the flare peaked. Image Credit: NASA/SDO.
The second X-class flare of June 10, 2014, appears as a bright flash on the left side of this image from NASA’s Solar Dynamics Observatory. This image shows light in the 193-angstrom wavelength, which is typically colorized in yellow. It was captured at 8:55 a.m EDT, just after the flare peaked. Image Credit: NASA/SDO.

Solar flares are explosions on the Sun that release energy, light and high speed particles into space, and the biggest flares are known as X-class.

Here are some recent astrophotos of the Sun taken by members of Universe Today’s Flickr group:

The Sun in white light on June 10, 2014. Taken with a William Optics 70mm refractor fitted with a Thousand Oaks solar filter, 2 x Barlow and Canon 1100D. Credit and copyright: Mary Spicer.
The Sun in white light on June 10, 2014. Taken with a William Optics 70mm refractor fitted with a Thousand Oaks solar filter, 2 x Barlow and Canon 1100D. Credit and copyright: Mary Spicer.
The full solar disk in hydrogen alpha on June 10, 2014. Credit and copyright: John Brady.
The full solar disk in hydrogen alpha on June 10, 2014. Credit and copyright: John Brady.
A look at the Sun from the UK on June 9, 2014. Prime focus single shot in whitelight, Canon 600D attached to Maksutov 127mm telescope fitted with homemade Baader Solarfilm filter. Credit and copyright: Sarah and Simon Fisher.
A look at the Sun from the UK on June 9, 2014. Prime focus single shot in whitelight, Canon 600D attached to Maksutov 127mm telescope fitted with homemade Baader Solarfilm filter. Credit and copyright: Sarah and Simon Fisher.

Solar flares are classified on a system that divides solar flares according to their strength. The smallest ones are A-class (near background levels), followed by B, C, M and X. Similar to the Richter scale for earthquakes, each letter represents a 10-fold increase in energy output. So an X is ten times an M and 100 times a C. Within each letter class there is a finer scale from 1 to 9.

Here’s NASA’s video guide to X-Class flares:

NASA says these flares are often associated with solar magnetic storms known as coronal mass ejections (CMEs). The number of solar flares increases approximately every 11 years. Watch this video below about why solar scientists think the solar maximum is happening now:

Read more on today’s flares from NASA.

Jaw-Dropping Sunset Timelapse from Sweden

The setting Sun as it passed over the church of a small village called Ås. You can clearly see two sunspots visible on the Sun (#2079 and #2077), both about the size of one Earth diameter. Credit and copyright: Göran Strand.

This is not your basic sunset timelapse! It combines a close-up view of the Sun with a solar telescope along with the landscape in the foreground. Astrophotographer Göran Strand from Sweden has been planning this photoshoot for a year, and it turned out spectacularly.

“Yesterday I went out to shoot a sunset I’ve planed since last summer,” Göran said via email. “This time of the year, the Sun passes right behind a big radar tower if you stand at the Swedish National Biathlon Arena in Östersund. The radar tower is located about 8 km away from the arena in a small village called Ås. I shoot the movie using my solar telescope to capture the structures on the Sun. The timing was perfect and the Sun looked really nice since it was full of sunspots and big filaments.”

Note the size of the Earth inserted for reference.

Below is a beautiful image taken a few days earlier by Göran of the setting Sun:

See more of Göran’s work at his website, Facebook, or Twitter.

Astrophotos: The Wispy Edge of the Sun

Sun in H-alpha, prominences May 17, 2014. Credit and copyright: Mary Spicer.

It’s like a total solar eclipse — without the Moon! Using a special hydrogen-alpha filter that completely blocks the Sun’s photosphere (visible surface) these images show just the Sun’s corona and the dancing solar prominences. The filter blocks all light from the Sun except for the red light emitted by excited hydrogen atoms, which are responsible for the distinctive color of prominences and the chromosphere, the wispy, hot layer of gas that overlies the photosphere.

Of course, never look directly at the Sun with the naked eye or through a telescope without a special solar filter.

The image above by Mary Spicer was taken with a Coronado PST, 2 x Barlow plus Canon 1100D. ISO-3200 1/400 second exposure, processed in Lightroom and Focus Magic.

See more below:

Solar prominences on April 21, 2014. Credit and copyright: Roger Hutchinson.
Solar prominences on April 21, 2014. Credit and copyright: Roger Hutchinson.

These images by Roger Hutchinson were taken with a Lunt LS60 Ha, Skyris 618C, and 2.5x Powermate.

Solar prominences on May 18, 2014 in H-alpha. Credit and copyright: Roger Hutchinson.
Solar prominences on May 18, 2014 in H-alpha. Credit and copyright: Roger Hutchinson.

Want to get your astrophoto featured on Universe Today? Join our Flickr group or send us your images by email (this means you’re giving us permission to post them). Please explain what’s in the picture, when you took it, the equipment you used, etc.

If Pigs Could Fly – A Quick Guide to Solar Halos and Other Curiosities

A circumscribed halo encloses the more common 22-degree halo around the sun Saturday morning (May 17. Credit: Bob King

Call it a porcine occultation. It took nearly a year but I finally got help from the ornamental pig in my wife’s flower garden. This weekend it became the preferred method for blocking the sun to better see and photograph a beautiful pair of solar halos. We often associate solar and lunar halos with winter because they require ice crystals for their formation, but they happen during all seasons. 

Nature keeps it simple. Light refracting through or reflecting from six-sided plate and column (pencil-shaped) ice crystals in high clouds is responsible for almost all halos and their variations.
Nature keeps it simple. Light refracting through or reflecting from six-sided plate and column (pencil-shaped) ice crystals in high clouds is responsible for almost all halos and their variations.

Lower clouds, like the puffy cumulus dotting the sky on a summer day, are composed of water droplets. A typical cumulus spans about a kilometer and contains 1.1 million pounds of water. Cirrostratus clouds are much higher (18,000 feet and up) and colder and formed instead of ice crystals. They’re often the first clouds to betray an incoming frontal system.

Cirrostratus are thin and fibrous and give the blue sky a milky look.  Most halos and related phenomena originate in countless millions of hexagonal plate and pencil-shaped ice crystals wafting about like diamond dust in these often featureless clouds.

This is the top end of a hexagonal column-shaped ice crystal. Light refracting (bending) through billions of these crystals spreads out to form a typical solar halo. Credit: Donalbein
This is the top end of a hexagonal column-shaped ice crystal. Light refracting (bending) through the 60-degree angled faces of millions of these crystals is concentrated into a ring of light 22 degrees from the sun. As light leaves the crystal, the shorter blue and purple wavelengths are refracted slightly more than red, tinting the outer edge of the halo blue and inner edge red. Credit: Donalbein with additions by the author

In winter, the sun is generally low in the sky, making it hard to miss a halo. Come summer, when the sun is much higher up, halo spotters have to be more deliberate and make a point to look up more often. The 22-degree halo is the most common; it’s the inner of the two halos in the photo above. With a radius of 22 degrees, an outstretched hand at arm’s length will comfortably fit between sun and circle.

Light refracted or bent through millions of randomly oriented pencil-shaped crystals exits at angles from 22 degrees up to 50 degrees, however most of the light is concentrated around 22 degrees, resulting in the familiar 22-degree radius halo. No light gets bent and concentrated at angles fewer than 22 degrees, which is why the sky looks darker inside the halo than outside. Finally, a small fraction of the light exits the crystals between 22 and 50 degrees creating a soft outer edge to the circle as well as a large, more diffuse disk of light as far as 50 degrees from the sun.

The sun on Dec. 6, 2013 with a 22-degree halo and two luminous canine companions or sundogs. Credit: Bob King
The sun on Dec. 6, 2013 with a 22-degree halo and two luminous canine companions or sundogs. Similar halos and ‘moondogs’ can be seen around a bright moon. Credit: Bob King

Sundogs, also called mock suns or parhelia, are brilliant and often colorful patches of light that accompany the sun on either side of a halo. Not as frequent as halos, they’re still common enough to spot half a dozen times or more a year. Depending on how extensive the cloud cover is, you might see only one sundog instead of the more typical pair. Sundogs form when light refracts through hexagonal plate-shaped ice crystals with their flat sides parallel to the ground. They appear when the sun is near the horizon and on the same horizontal plane as the ice crystals. As in halos, red light is refracted less than blue, coloring the dog’s ‘head’ red and its hind quarters blue. Mock sun is an apt term as occasionally a sundog will shine with the intensity of a second sun. They’re responsible for some of the daytime ‘UFO’ sightings. Check this one one out on YouTube.

An especially colorful sundog with a 'tail' from 2008. Credit: Bob King
An especially colorful sundog with a ‘tail’. Red light is bent less than blue as it emerges from the ice crystal, tinting the sundog’s inner edge. Blue is bent more and colors the outer half. If you look closely, all colors of the rainbow are seen. Credit: Bob King

Wobbly crystals make for taller sundogs. Like real dogs, ice crystal sundogs can grow tails. These are part of the much larger parhelic circle, a rarely-seen narrow band of light encircling the entire sky at the sun’s altitude formed when millions of both plate and column crystals reflect light from their vertical faces. Short tails extend from each mock sun in the photo above.

A couple hours after the flying pig image, the sun was beyond 50 degrees altitude. The circumscribed halo had vanished! Credit: Bob King
About 2 hours after the flying pig image, the sun climbed beyond 50 degrees altitude. The circumscribed halo vanished! Credit: Bob King

There’s almost no end to atmospheric ice antics. Many are rare like the giant 46-degree halo or the 9 and 18-degree halos formed from pyramidal ice crystals. Oftentimes halos are accompanied by arcs or modified arcs as in the flying pig image.  When the sun is low, you’ll occasionally see an arc shaped like a bird in flight tangent to the top of the halo and rarely, to its bottom. When the sun reaches an altitude of 29 degrees, these tangent arcs – both upper and lower – change shape and merge into a circumscribed halo wrapped around and overlapping the top and bottom of the main halo. At 50 degrees altitude and beyond, the circumscribed halo disappears … for a time. If the clouds persist, you can watch it return when the sun dips below 29 degrees and the two arcs separate again.

Maybe you’re not a halo watcher, but anyone who keeps an eye on the weather and studies the daytime sky in preparation for a night of skywatching can enjoy these icy appetizers.

Astrophoto: Space Station Creates a Zipper on the Sun

A mosaic of 46 images showing the transit of the ISS across the sun visible from southwest London on May 16, 2014 at 06:23 UT. Credit and copyright: Roger Hutchinson.

“I’ve been wanting to get one of these for ages!” said astrophotographer Roger Hutchinson from London, England. This awesome image of the International Space Station transiting across the Sun earlier today — which creates a “zipper”-like effect on the Sun’s surface – is a composite of 46 images, taken from Southwest SW London on May 16, 2014 at 06:23 UT. Roger used a Lunt LS60 Ha telescope and a Skyris 274C camera.

Amazing.

Want to get your astrophoto featured on Universe Today? Join our Flickr group or send us your images by email (this means you’re giving us permission to post them). Please explain what’s in the picture, when you took it, the equipment you used, etc.