Wednesday, September 2, 2015

Laser weapons that could blast asteroids away from Earth and make interstellar travel a reality: HUBBLE PHOTOS

 

 

 

 

Laser weapons that could blast asteroids away from Earth and make interstellar travel a reality

 

 
  • Massive array of laser beams could intercept and deflect asteroids
  • 'laser drive' could also propel spacecraft close to speed of light
  • Lab experiment shows theory of laser arrays is correct

 

Researchers have unveiled the ultimate sci-fi laser weapon.

DE-STAR, or Directed Energy System for Targeting of Asteroids and exploRation, uses a massive array of laser beams to intercept and deflect asteroids - and could also be used as a photon drive for insterstellar travel.

Researchers have revealed the system working in the lab - albeit on a smaller scale.

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To simulate a laser's ability to deflect an asteroid, researchers directed a laser onto the target until it glowed white hot, producing a 'rocket engine' using the asteroid itself as the propellant.

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To simulate a laser's ability to deflect an asteroid, researchers directed a laser onto the target until it glowed white hot, producing a 'rocket engine' using the asteroid itself as the propellant.

PHOTON PROPULSION

The students also explored photon propulsion, which is key to the group's latest project, DEEP-IN, or Directed Energy Propulsion for Interstellar exploratioN.

The DEEP-IN concept relies on photon propulsion, whereby thrust from photons emitted from the laser array could be used to propel a spacecraft.

This allows for the possibility of relativistic flight - speeds approaching the speed of light - for the small spacecraft required for future interstellar missions.

The group has been awarded one of 15 proof-of-concept grants from NASA Innovative Advanced Concepts.

The NASA program aims to turn what sounds like science fiction into science fact through the development of pioneering technologies.

It is the brainchild of UC Santa Barbara physicist Philip Lubin and Gary B. Hughes, a researcher and professor at California Polytechnic State University, San Luis Obispo.

To simulate a laser's ability to deflect an asteroid, Travis Brashears led a group of students in tests that simulate space conditions.

Using basalt, the composition of which is similar to known asteroids, they directed a laser onto the basalt target until it glowed white hot, a process called laser ablation, which erodes material from the sample.

This changes the object's mass and produces a 'rocket engine' using the asteroid itself as the propellant.

In space, this would be powerful enough to alter its course.

'What happens is a process called sublimation or vaporization, which turns a solid or liquid into a gas,' explained Brashears, now a freshman at UC Berkeley who started working in the lab during high school as part of UCSB's Research Mentorship Program.

'That gas causes a plume cloud — mass ejection — which generates an opposite and equal reaction or thrust — and that's what we measure.'

Then the team simulated a spinning asteroid using basalt to determine whether they could slow, stop and change its rotation direction.

They used magnets to spin the basalt and then directed the laser in the opposite direction to slow the rotation.

'Our video shows the basalt sample slowing down, stopping and changing direction and then spinning up again,' said Brashears.

'That's how much force we're getting.

'It's a nice way to show this process and to demonstrate that de-spinning an asteroid is actually possible as predicted in our papers.'

According to Lubin, a professor of physics at UCSB, manipulating the speed of a spinning asteroid offers another important possibility in space: the ability to explore, capture and mine asteroids.

This is something NASA aims to do with its Asteroid Redirect Mission.

The mission — which remains theoretical — is intended to visit a large near-Earth asteroid, collect and return a boulder from its surface and possibly redirect the asteroid into a stable orbit around the moon.

HOW LASERS COULD LEAD TO INSTERSTELLAR TRAVEL

A laser-powered wafer-thin spacecraft capable of reaching Alpha Centauri in 20 years may sound like the stuff of science fiction, but it's not.

And while such a launch isn't imminent, the possibility of one in the future does exist, according to UC Santa Barbara physics professor Philip Lubin.

To further explore that possibility, Lubin and his team in UCSB's Experimental Cosmology Group will study photo-driven propulsion — the use of lasers as a means to power a spacecraft.

The group has been awarded one of 15 proof-of-concept grants from NASA Innovative Advanced Concepts.

The NASA program aims to turn what sounds like science fiction into science fact through the development of pioneering technologies.

'One of humanity's grand challenges is to explore other solar systems by sending probes — and eventually life,' said Lubin.

'We propose a system that will allow us to take the first step toward interstellar exploration using directed energy propulsion combined with miniature probes.

'Along with recent work on wafer-scale photonics, we can now envision combining these technologies to enable a realistic approach to sending probes far outside our solar system.'

The UCSB group's ultimate goal is to send small probes to supplement the current long-range remote sensing done by orbital and ground-based telescopes. 

The DEEP-IN design keeps the main propulsion driver back in Earth's orbit (or nearby) yet still capable of propelling highly integrated spacecraft to speeds vastly higher than anything scientists can currently achieve.

The laser photon driver would use photon pressure in the form of streamed energy to power the spacecraft as it travels away from Earth. With no intrinsic speed limit, this technology allows for the relativistic speeds necessary for interstellar flight.

The same systems can be used for many other purposes, according to Lubin, including travel inside our solar system — such as rapid transit to Mars with much larger probes — and planetary defense.

'While not suitable for every spacecraft design, this approach opens up radically new possibilities,' Lubin said.

'The project is a step toward the first interstellar mission, but more importantly we are studying and designing the relevant technological base.

'This will give us the ability to build a single photon driver capable of sending out literally millions of low-mass probes.

'All asteroids rotate; it's just a question of relative to whom and how fast,' explained Lubin.

'To mine an asteroid, it needs to be moving slowly enough so you can capture it.

'Our lab experiments show very graphically a practical way to de-spin or redirect an asteroid. It's a vivid demonstration that the technique works very well.'

The DE-STAR system could be leveraged for many other uses, such as stopping the rotation of a spinning asteroid and achieving relativistic propulsion, the team say.

Using basalt, the composition of which is similar to known asteroids, they directed a laser onto the basalt target until it glowed white hot, a process called laser ablation, which erodes material from the sample.

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Using basalt, the composition of which is similar to known asteroids, they directed a laser onto the basalt target until it glowed white hot, a process called laser ablation, which erodes material from the sample.

HOW WARP SPEED IS PART OF EINSTEIN'S THEORY OF RELATIVITY

The theory of special relativity, revealed by Albert Einstein in 1905, says that no object can reach the speed of light.

In the next couple of years, Einstein presented his theory of general relativity, which is made up of various field equations that could be solved in different ways.

As part of his theory, he found that a number of the solutions for the Einstein field equations allow physicists to move space itself faster than light.

This means, in theory, we could warp space, bending the space in front of a spacecraft while stretching out the space behind it.

In addition, the students explored photon propulsion, which is key to the group's latest project, DEEP-IN, or Directed Energy Propulsion for Interstellar exploratioN.

The DEEP-IN concept relies on photon propulsion, whereby thrust from photons emitted from the laser array could be used to propel a spacecraft.

This allows for the possibility of relativistic flight — speeds approaching the speed of light — for the small spacecraft required for future interstellar missions.

The team also tested a photon recycler, a device that reuses photons from the laser by shining them on a reflector cavity.

'We have a second mirror at some distance away that bounces the photons back and forth like a ping-pong ball onto the spacecraft reflector.' Brashears said.

The basalt is mounted on a torsion balance to hold it steady for the laser.<br /><br />Asteroid Deflection: Science Fiction or Reality

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The basalt is mounted on a torsion balance to hold it steady for the laser. Asteroid Deflection: Science Fiction or Reality

'In effect, we're recycling these photons to achieve a force multiplication that allows the vehicle to go even faster.

'So far, with a simple implementation, we have achieved an amplification factor of five. Much more is possible with refinement.

'This works as predicted, though implementing it into the full flight system will be complex.'

NASA'S IMPOSSIBLE FUEL-FREE THRUSTERS DO WORK, CLAIM SCIENTISTS

While not quite a warp drive, researchers have recently found a EMDrive propulsion system could work, and it would permit travel at speeds until now only seen in science fiction.

When the concept was first proposed it was considered impossible because it went against the laws of physics. But subsequent tests last reveal it could be a possibility.

The new drive could carry passengers and their equipment to the moon in as little as four hours.

A trip to Alpha Centauri, which would take tens of thousands of years to reach right now, could be reached in just 100 years.

The system is based on electromagnetic drive, or EMDrive, which converts electrical energy into thrust without the need for rocket fuel.

According to classical physics, the EMDrive should be impossible because it seems to violate the law of conservation of momentum.

The law states that the momentum of a system is constant if there are no external forces acting on the system – which is why propellant is required in traditional rockets.

When London-based Roger Sawyer came up with concept in 2000, the only team that took him seriously was a group of Chinese scientists.

In 2009, the team allegedly produced 720 millinewton (or 72g) of thrust, enough to build a satellite thruster. But still, nobody believed they had achieved this.

Researchers from the US, UK and China have demonstrated EMDrives over the past few decades, but their results have been controversial as no one has been exactly sure how it works.

But earlier this year, Nasa built an EMDrive that works in conditions like those in space, according to users on forum NasaSpaceFlight.com.

Martin Tajmar, professor and chair for Space Systems at the Dresden University of Technology, last month presented his work at the American Institute for Aeronautics and Astronautics' Propulsion and Energy Forum in Orlando last month.

'Our measurements reveal thrusts as expected from previous claims after carefully studying thermal and electromagnetic interferences,' wrote Tajmar in the paper.

 

 

 

 

570 megapixel image of a COMET: Stunning shot of Lovejoy shocks scientists

  • Comet sprung up in a photo snapped taken by the Dark Energy Camera as it scanned the southern sky
  • At the time this image was taken, the comet was passing about 51 million miles (82 million km) from Earth
  • The camera is sensitive to light up to eight billion light years away, and so was able to capture it in detail
  • The Dark Energy Survey (DES) is designed to find out why the expansion of the universe is speeding up

Comet Lovejoy has made a surprise appearance in an image taken by the world's most powerful digital camera.

The comet sprung up in a photo snapped taken by the 570-megapixel Dark Energy Camera as it was scanning the southern sky.

At the time this image was taken, the comet was passing about 51 million miles (82 million km) from Earth. It appeared as a burst of green light against sky full of stars.

The comet sprung up in a photo snapped taken by the 570-megapixel Dark Energy Camera in December as it was scanning the southern sky. At the time this image was taken, the comet was passing about 51 million miles (82 million km) from Earth. It appeared as a burst of green light against sky full of stars. Each of the rectangles represents one of the 62 individual fields of the camera

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The comet sprung up in a photo snapped taken by the 570-megapixel Dark Energy Camera in December as it was scanning the southern sky. At the time this image was taken, the comet was passing about 51 million miles (82 million km) from Earth. It appeared as a burst of green light against sky full of stars. Each of the rectangles represents one of the 62 individual fields of the camera

'It reminds us that before we can look out beyond our galaxy to the far reaches of the universe, we need to watch out for celestial objects that are much closer to home,' wrote the team on the Dark Energy Detectives blog.

The Dark Energy Camera is sensitive to light up to eight billion light years away, and so was able to capture the view in incredible detail.

The Dark Energy Survey (DES) is designed to find out why the expansion of the universe is speeding up, instead of slowing down due to gravity.

It is currently looking into the mystery of dark energy, the force believed to be causing that acceleration.

he comet's centre is a ball of ice roughly three miles (5 km) across, and the visible head of the comet is a cloud of gas and dust about 400,000 miles (640,000 km) in diameter. Pictured is a shot taken by an amateur astronomer earlier this year

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he comet's centre is a ball of ice roughly three miles (5 km) across, and the visible head of the comet is a cloud of gas and dust about 400,000 miles (640,000 km) in diameter. Pictured is a shot taken by an amateur astronomer earlier this year

COMET LOVEJOY: KEY FACTS

Comet Lovejoy was first spotted by Australian Terry Lovejoy on August 17 and in recent weeks has been dramatically captured on camera by amateur astronomers around the world.

The comet’s centre is a ball of ice roughly three miles (5 km) across, and the visible head of the comet is a cloud of gas and dust about 400,000 miles (640,000 km) in diameter.

The comet's distinctive green glow comes from molecules of diatomic carbon - two carbon atoms joined together - and cyanogen fluorescing in the ultraviolet light from the sun.

Its tail takes on a blue tinge due to the carbon monoxide it contains. 

Comet Lovejoy was first spotted by Australian Terry Lovejoy, who has a prolific record among amateur astronomers, and he named the comet.

To date, Mr Lovejoy, from Queensland, has discovered five comets, all using relatively simple equipment compared to what's found at a professional observatory.

It was first spotted on August 17 and in recent weeks has been dramatically captured on camera by amateur astronomers around the world.

The comet's centre is a ball of ice roughly three miles (5 km) across, and the visible head of the comet is a cloud of gas and dust about 400,000 miles (640,000 km) in diameter.

The comet's distinctive green glow comes from molecules of diatomic carbon - two carbon atoms joined together - and cyanogen fluorescing in the ultraviolet light from the sun.

Its tail takes on a blue tinge due to the carbon monoxide it contains.

Comets are essentially piles of rock, gravel, and dust held together by various kinds of ice - essentially water and carbon dioxide ice.

As the comet nears the sun, its icy tail turns into a gas and blows away - due to pressure from the solar wind and sunlight.

They also release dust and gravel which tend to follow the comet around the sun - and if the Earth's orbit intersects this material it results in annual meteor showers

 

The comet's distinctive green glow comes from molecules of diatomic carbon - two carbon atoms joined together - and cyanogen fluorescing in the ultraviolet light from the sun.Its tail takes on a blue tinge due to the carbon monoxide it contains The comet's distinctive green glow comes from molecules of diatomic carbon - two carbon atoms joined together - and cyanogen fluorescing in the ultraviolet light from the sun.Its tail takes on a blue tinge due to the carbon monoxide it contains

The comet's distinctive green glow comes from molecules of diatomic carbon - two carbon atoms joined together - and cyanogen fluorescing in the ultraviolet light from the sun.Its tail takes on a blue tinge due to the carbon monoxide it contains

More than any other telescope in orbit, Hubble has expanded the frontiers of human knowledge.

For 25 years, astronomers have used it to peer deep into distant galaxies with unrivalled clarity, revealing the breathtaking beauty of our universe.

In the April issue of National Geographic, some of the most stunning images beamed back for the telescope have been revealed.  

The Horsehead Nebula is a cold, dark cloud of gas and dust, silhouetted against the bright nebula IC 434. The bright area at the top left edge is a young star still embedded in its nursery of gas and dust. The nebula is relatively close at 1,500 light years from Earth

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The Horsehead Nebula is a cold, dark cloud of gas and dust, silhouetted against the bright nebula IC 434. The bright area at the top left edge is a young star still embedded in its nursery of gas and dust. The nebula is relatively close at 1,500 light years from Earth

Hubble has helped scientists understand how planets and galaxies form, detected black holes and changed our theories surrounding dark energy, a mysterious force that causes the universe to expand faster and faster as time goes on.

The hundreds of thousands of images beamed back from Hubble have helped scientists unravel cosmic mysteries as well as estimate the age of the universe to about 14 billion years old.

Among them is the Horsehead Nebula - a cold, dark cloud of gas and dust, silhouetted against the bright nebula IC 434 1,500 light years from Earth.

Another remarkable image shows a display of starlight, glowing gas, and silhouetted dark clouds of interstellar dust that forms the spiral galaxy NGC 130. This is one of Hubble's largest images ever made of a complete galaxy.

Some of the most striking scenes are created during the death throes of intermediate-mass stars, when great clouds of superheated gas are expelled into space. 

Hubble's panoramic view of the Andromeda Galaxy (related)

 

In 2002, a dull star in an obscure constellation suddenly became 600,000 times more luminous than our sun, temporarily making it the brightest star in the Milky Way. The mysterious star, called V838 Monocerotis, has since faded back to obscurity. But observations by the Hubble Space Telescope of a phenomenon called a "light echo" around the star have uncovered remarkable new features

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In 2002, a dull star in an obscure constellation suddenly became 600,000 times more luminous than our sun, temporarily making it the brightest star in the Milky Way. The mysterious star, called V838 Monocerotis, has since faded back to obscurity. But observations by the Hubble Space Telescope of a phenomenon called a 'light echo' around the star have uncovered remarkable new features

This huge, young stellar grouping, called R136, is only a few million years old and resides in the 30 Doradus Nebula, a turbulent star-birth region in the Large Magellanic Cloud, a satellite galaxy of the Milky Way

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This huge, young stellar grouping, called R136, is only a few million years old and resides in the 30 Doradus Nebula, a turbulent star-birth region in the Large Magellanic Cloud, a satellite galaxy of the Milky Way

The telescope captured a display of starlight, glowing gas, and silhouetted dark clouds of interstellar dust in this 4-foot-by-8-foot image of the barred spiral galaxy NGC 130. This is one of Hubble's largest images ever made of a complete galaxy

 

The telescope captured a display of starlight, glowing gas, and silhouetted dark clouds of interstellar dust in this 4-foot-by-8-foot image of the barred spiral galaxy NGC 130. This is one of Hubble's largest images ever made of a complete galaxy

'Launched into orbit aboard the space shuttle Discovery on April 24, 1990, amid flurries of hope and hype, the Hubble Space Telescope promptly faltered,' explained Timothy Ferris writing in April's issue of National Geographic

An iconic image from Hubble captures the dying breaths from planetary nebula NGC 6302. Known perhaps more appropriately as the Bug or Butterfly Nebula, this complex nebula lies roughly 3800 light-years away from us within the Milky Way.

But at first, astronomers didn't expect Hubble to amount to much.

'Launched into orbit aboard the space shuttle Discovery on April 24, 1990, amid flurries of hope and hype, the Hubble Space Telescope promptly faltered,' explained Timothy Ferris writing in April's issue of National Geographic.

'Rather than remaining locked on its celestial targets, it trembled and shook, quaking like a photophobic vampire whenever sunlight struck its solar panels.

'Opening its protective front door to let starlight in perturbed the telescope so badly that it fell into an electronic coma.

'Worst of all, Hubble turned out to be myopic. Its primary light-gathering mirror, eight feet in diameter and said to be the smoothest large object ever fashioned by humans, had been figured perfectly wrong.'

The telescope's design had been a compromise. While astronomers had wanted a bigger telescope in a higher orbit, they could only get 350 miles (550km) high so that astronauts in space could reach it for repairs.

Next month, the telescope - which is the length of a large school bus and weighs as much as two adult elephants - will celebrate its 25th anniversary.

To celebrate Hubble astronomers recently revisited one of its most stunning photos to date, known as 'the pillars of creation.'

Taken in 1995, the team revealed never-before-seen details of three giant columns of cold gas bathed in the scorching ultraviolet light from a cluster of young, massive stars in a small region of the Eagle Nebula, or M16.

The new Hubble photo is sharper than the original, and also has a  wider field of view. It also reveals the base of the cold, gassy columns for the first time.

And in January the sharpest and largest image ever taken of the Andromeda Galaxy - the nearest spiral galaxy to our Milky Way.

The Hubble image shows more than 100 million stars and thousands of star clusters embedded in a section of the galaxy’s pancake-shaped disc stretching across over 40,000 light-years.

The sweeping view, which reveals one third of our galactic neighbour, also suggests that the galaxy may have been battered by a collision with another galaxy two billion years ago.

The panoramic image has 1.5 billion pixels — meaning you would need more than 600 HD television screens to display the whole image.

It traces the galaxy from its central galactic bulge on the left, where stars are densely packed together, across lanes of stars and dust to the sparser outskirts of its outer disc on the right.

'That human beings find them to be as beautiful and evocative as photos of earthly sunsets and mountain peaks affirms anew that nature is all of a piece, and that we're part of it,' said Ferris.

Some of the most striking scenes are created during the death throes of intermediate-mass stars, when great clouds of superheated gas are expelled into space. This image from Hubble captures the dying breaths from planetary nebula NGC 6302. Known perhaps more appropriately as the Bug or Butterfly Nebula, this complex nebula lies roughly 3800 light-years away from us within the Milky Way

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Some of the most striking scenes are created during the death throes of intermediate-mass stars, when great clouds of superheated gas are expelled into space. This image from Hubble captures the dying breaths from planetary nebula NGC 6302. Known perhaps more appropriately as the Bug or Butterfly Nebula, this complex nebula lies roughly 3800 light-years away from us within the Milky Way

Click on the image to zoom in

The new Hubble photo of the pillars of creation is sharper than the original, and also has a wider field of view. It also reveals the base of the cold, gassy columns for the first time

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The new Hubble photo of the pillars of creation is sharper than the original, and also has a wider field of view. It also reveals the base of the cold, gassy columns for the first time

 

 

 

 

   

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