APOD: A Laser Strike at the Galactic Center (2010 Sep 06)

Comments and questions about the APOD on the main view screen.
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APOD: A Laser Strike at the Galactic Center (2010 Sep 06)

Post by APOD Robot » Mon Sep 06, 2010 4:01 am

Image A Laser Strike at the Galactic Center

Explanation: Why are these people shooting a powerful laser into the center of our Galaxy? Fortunately, this is not meant to be the first step in a Galactic war. Rather, astronomers at the Very Large Telescope (VLT) site in Chile are trying to measure the distortions of Earth's ever changing atmosphere. Constant imaging of high-altitude atoms excited by the laser -- which appear like an artificial star -- allow astronomers to instantly measure atmospheric blurring. This information is fed back to a VLT telescope mirror which is then slightly deformed to minimize this blurring. In this case, a VLT was observing our Galaxy's center, and so Earth's atmospheric blurring in that direction was needed. As for inter-galaxy warfare, when viewed from our Galaxy's center, no casualties are expected. In fact, the light from this powerful laser would combine with light from our Sun to together appear only as bright as a faint and distant star.

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Re: APOD: A Laser Strike at the Galactic Center (2010 Sep 06

Post by alter-ego » Mon Sep 06, 2010 5:25 am

This is only the beginning..
Achieving diffraction limited imaging at both a larger aperture and wider FOV is driving this technology harder:
Development of Multi-Laser Guide Star Adaptive Optics Techniques for Extremely Large Telescopes
Development of Multi-Laser Guide Star Adaptive Optics<br />Techniques for Extremely Large Telescopes
Development of Multi-Laser Guide Star Adaptive Optics
Techniques for Extremely Large Telescopes
<<Abstract: We outline ongoing work at the MMT telescope to develop altitude-conjugated adaptive
optics using a constellation of laser guide stars. We describe how the new techniques will be
applied to the planned Giant Magellan Telescope.
OCIS codes: (010.1080) Adaptive optics; (110.6770) Telescopes
1. Need for multiple laser guide stars on extremely large telescopes
The unique advance to be made with an extremely large telescope (ELT), but also the greatest challenge, will be to
obtain very high resolution, diffraction limited images for any scientific target. Tomography with multiple sodium
laser guide stars is required, even for small fields, because of focal anisoplanatism (the cone effect). The same
beacons will yield reconstructions of the wavefront aberration near the ground, allowing for correction of low-level
turbulence over a wide field of view, and also of dynamic aberrations in the telescope optics. These are likely to be
induced by wind in ELTs, with their enormous wind loading.
ELT requirements for adaptive optics to the diffraction limit are daunting, if we are to go beyond correction of
the isoplanatic patch around bright stars. The field in this case is small, since the integrated wavefront distortion
depends sensitively on the direction of view. For telescopes in the 8 m class, the need for a bright star can be
avoided, though not the narrow field of correction, by use of a single sodium laser beacon created by resonance
scattering in the atmospheric sodium layer, 90 km high. In this way, much of the sky should be accessible in near
infrared bands. The requirement for tuning a high power laser precisely to the 589 nm resonance line has proven a
major technical challenge for nearly 20 years, though there is now hope that CW lasers with adequate power will be
forthcoming. The Air Force group at the Starfire Optical Range, Kirtland Air Force Base, have recently
demonstrated 50 W of projected power from a CW summed-frequency YAG laser.
But for ELTs, the task is more complex. The single laser solution breaks down because of focus anisoplanatism.
To correct even a narrow field of view, several powerful lasers beacons will be required, and the aberration for a
distant star must be derived by tomography from the wavefronts measured for each beacon. A further complication
is the defocus of the sodium beacon because the 10 km sodium layer thickness, acceptable for 8 m aperture with
axial projection, is outside the depth of focus for an ELT
. Methods to overcome this efficiently are possible [1-3],
but they rely on use of a pulsed laser and tracking sequential pulses through the layer. While studies of pulsed
sodium lasers are underway for the Gemini Observatory, we would seem to be still years away from fielding
multiple pulsed tuned lasers of adequate power and at an affordable cost.>>

Laser Development for Sodium Laser Guide Stars at ESO
Laser Development for Sodium Laser Guide Stars at ESO<br />Simplified schematic - Second Harmonic Generation of 1178nm Fiber Laser
Laser Development for Sodium Laser Guide Stars at ESO
Simplified schematic - Second Harmonic Generation of 1178nm Fiber Laser
ESO Laser Specifications
ESO Laser Specifications
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Re: APOD: A Laser Strike at the Galactic Center (2010 Sep 06

Post by Microbots » Mon Sep 06, 2010 6:08 am

Is all the NASA pics CGI or actually REAL?? Cos the sky in the pic looks put in by an artist or computer...

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Re: APOD: A Laser Strike at the Galactic Center (2010 Sep 06

Post by Ann » Mon Sep 06, 2010 7:09 am

I don't know about the rest of you, but to me today's APOD looks mildly indecent. Wonder what will spawn from this penetration of the galactic center by a human laser beam?

Image

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Re: APOD: A Laser Strike at the Galactic Center (2010 Sep 06

Post by Czerno » Mon Sep 06, 2010 7:43 am

APOD Robot wrote:In fact, the light from this powerful laser would combine with light from our Sun to together appear only as bright as a faint and distant star.
After atmosperic absorption and scattering, interactions with interstellar material, coherency loss and angular dispersion, and even assuming the absence of large intercepting objects in the line of "sight", what proportion of the photonic contents of this miserable beam coud be expected to reach Galaxy center (if not practically zero) ? How often would they get albeit "one" photon from the laser ?
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Re: APOD: A Laser Strike at the Galactic Center (2010 Sep 06

Post by owlice » Mon Sep 06, 2010 9:05 am

This image first appeared on Asterisk on the Recent Submissions: 2010 September 1-3 thread. How DO Drs. Nemiroff and Bonnell select just one image/day from among so many...? I think I'd explode!
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Re: APOD: A Laser Strike at the Galactic Center (2010 Sep 06

Post by neufer » Mon Sep 06, 2010 10:17 am

Microbots wrote:Is all the NASA pics CGI or actually REAL?? Cos the sky in the pic looks put in by an artist or computer...
It does seem a bit weird, doesn't it.

Think about it as train tracks pointing towards some distant "vanishing point."
To Native Americans who first saw them they probably looked a bit weird too:
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Re: APOD: A Laser Strike at the Galactic Center (2010 Sep 06

Post by logmark » Mon Sep 06, 2010 12:14 pm

What's with the return to earth-centric thinking? Just because WE couldn't resolve a laser from a background star's output doesn't mean THEY couldn't. On the one hand we are constantly developing new techniques and technologies to improve our ability to resolve images - have indeed resolved stars with their own planetary systems - while on the other hand we are forgetting that THEY may have solved these things long ago...and even if they haven't yet they've got quite a few years to do so before this beam reaches them. I'm just saying... :-)

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Re: APOD: A Laser Strike at the Galactic Center (2010 Sep 06

Post by celestemekent » Mon Sep 06, 2010 12:21 pm

are you sure that some alien scientist is not right now painfully yelling about some stupid people on this distant plant burning his eyes with a laser.

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Re: APOD: A Laser Strike at the Galactic Center (2010 Sep 06

Post by León » Mon Sep 06, 2010 12:52 pm

Perhaps the light passing through a cluster of galaxies such as Abell, suffer the same distortion. More in http://segunpasanlossiglos.blogspot.com/

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Re: APOD: A Laser Strike at the Galactic Center (2010 Sep 06

Post by Henning Makholm » Mon Sep 06, 2010 1:03 pm

celestemekent wrote:are you sure that some alien scientist is not right now painfully yelling about some stupid people on this distant plant burning his eyes with a laser.
Quite sure. The laser outputs 17 W at 589 nm. Even ignoring the atmosphere, the beam will not stay exactly parallel to the stars, but will diffract at the laser's aperture and spread out slightly. Let's say at least 0.1 arcsecond (which would require the aperture to be on the order of a meter). So for people in the beam, the laser will be about as bright as an isotropic source that emits 17 W * 4pi / 0.1 arcsec² = about 10^15 W. The Sun outputs about 10^26 W, so the laser is about as bright as the light from a star 27 magnitudes dimmer than the sun itself!
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Re: APOD: A Laser Strike at the Galactic Center (2010 Sep 06

Post by orin stepanek » Mon Sep 06, 2010 1:12 pm

http://www.youtube.com/watch?v=e1nUn6vT1yc
I'm a Sci Fi fan; I used to watch this movie! I did like Battlestar Galactica better though. 8-)
I don't thint lasers will make effictive weapons al long range though. I can see where they may do some damage. Though a laser beam can go a long way; http://www.metacafe.com/watch/833126/hu ... eam_range/ it wouldn't be dangerous to other planetary sociaties when fired from Earth. 8-)
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Re: APOD: A Laser Strike at the Galactic Center (2010 Sep 06

Post by AndyG » Mon Sep 06, 2010 1:55 pm

Henning Makholm wrote:The Sun outputs about 10^26 W, so the laser is about as bright as the light from a star 27 magnitudes dimmer than the sun itself!
27 magnitudes is vast. So I thought I'd try and be clever and recommend our alien uses a filter centred on 589nm to reduce this huge disparity, but obviously the laser's wavelength, well inside the visible light spectrum, is not far off the Sun's peak power output = not much saving there.

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Re: APOD: A Laser Strike at the Galactic Center (2010 Sep 06

Post by neufer » Mon Sep 06, 2010 2:53 pm

AndyG wrote:
Henning Makholm wrote:The Sun outputs about 10^26 W, so the laser is about as bright as the light from a star 27 magnitudes dimmer than the sun itself!
27 magnitudes is vast. So I thought I'd try and be clever and recommend our alien uses a filter centred on 589nm to reduce this huge disparity, but obviously the laser's wavelength, well inside the visible light spectrum, is not far off the Sun's peak power output = not much saving there.
http://en.wikipedia.org/wiki/SETI wrote:
<<Search for Extra-Terrestrial Intelligence (SETI) is the collective name for a number of activities people undertake to search for intelligent extraterrestrial life. While most SETI sky searches have studied the radio spectrum, some SETI researchers have considered the possibility that alien civilizations might be using powerful lasers for interstellar communications at optical wavelengths. The idea was first suggested by R. N. Schwartz and Charles Hard Townes in a 1961 paper published in the journal Nature titled "Interstellar and Interplanetary Communication by Optical Masers". In 1983, Townes, one of the inventors of the laser, published a detailed study of the idea in the US journal Proceedings of the National Academy of Sciences. Most SETI researchers agreed with the idea.

The 1971 Cyclops study discounted the possibility of optical SETI, reasoning that construction of a laser system that could outshine the bright central star of a remote star system would be too difficult. Some SETI advocates, such as Frank Drake, have suggested that such a judgment was too conservative; early 21st century humans have no means of knowing how a superior technology is communicating or would communicate, and negative results may simply mean humans are making the wrong searches.

There are two problems with optical SETI. The first problem is that lasers are highly "monochromatic", that is, they emit light only on one frequency, making it troublesome to figure out what frequency to look for. However, according to the uncertainty principle, emitting light in narrow pulses results in a broad spectrum of emission; the spread in frequency becomes higher as the pulse width becomes narrower, making it easier to detect an emission.

The other problem is that while radio transmissions can be broadcast in all directions, lasers are highly directional. This means that a laser beam could be easily blocked by clouds of interstellar dust, and Earth would have to cross its direct line of fire by chance to receive it.

Optical SETI supporters have conducted paper studies of the effectiveness of using contemporary high-energy lasers and a ten-meter focus mirror as an interstellar beacon. The analysis shows that an infrared pulse from a laser, focused into a narrow beam by such a mirror, would appear thousands of times brighter than the Sun to a distant civilization in the beam's line of fire. The Cyclops study proved incorrect in suggesting a laser beam would be inherently hard to see.

Such a system could be made to automatically steer itself through a target list, sending a pulse to each target at a constant rate. This would allow targeting of all Sun-like stars within a distance of 100 light-years. The studies have also described an automatic laser pulse detector system with a low-cost, two-meter mirror made of carbon composite materials, focusing on an array of light detectors. This automatic detector system could perform sky surveys to detect laser flashes from civilizations attempting contact.

In the 1980s, two Soviet researchers conducted a short optical SETI search, but turned up nothing. During much of the 1990s, the optical SETI cause was kept alive through searches by Stuart Kingsley, a dedicated British amateur living in the US state of Ohio.

Several optical SETI experiments are now in progress. A Harvard-Smithsonian group that includes Paul Horowitz designed a laser detector and mounted it on Harvard's 155 centimeter (61 inch) optical telescope. This telescope is currently being used for a more conventional star survey, and the optical SETI survey is "piggybacking" on that effort. Between October 1998 and November 1999, the survey inspected about 2,500 stars. Nothing that resembled an intentional laser signal was detected, but efforts continue. The Harvard-Smithsonian group is now working with Princeton University to mount a similar detector system on Princeton's 91-centimeter (36-inch) telescope. The Harvard and Princeton telescopes will be "ganged" to track the same targets at the same time, with the intent being to detect the same signal in both locations as a means of reducing errors from detector noise.

The Harvard-Smithsonian group is now building a dedicated all-sky optical survey system along the lines of that described above, featuring a 1.8-meter (72-inch) telescope. The new optical SETI survey telescope is being set up at the Oak Ridge Observatory in Harvard, Massachusetts. The University of California, Berkeley, home of SERENDIP and SETI@home, is also conducting optical SETI searches. One is being directed by Geoffrey Marcy, an extrasolar planet hunter, and involves examination of records of spectra taken during extrasolar planet hunts for a continuous, rather than pulsed, laser signal. The other Berkeley optical SETI effort is more like that being pursued by the Harvard-Smithsonian group.>>
http://www.theaustralian.com.au/news/health-science/watch-this-space/story-e6frg8gf-1225710664198 wrote:
The Australian: May 09, 2009 12:00AM
Greg Callaghan

<<AFTER you've spent more than 20 years hunting for an alien signal, you think you'd be celebrating if you noticed a mysterious pulse suddenly rising up on your computer readouts. A regular pulse, amid the random clatter of the cosmos, suggests that someone very smart at the other end is sending a message.

But when Ragbir Bhathal, an astrophysicist at the University of Western Sydney, who teaches the only university-based course on SETI (search for extraterrestrial intelligence) in Australia, detected the suspicious signal on a clear night last December, he knew better than to crack open the special bottle of champagne he has tucked away for the history-making occasion. Instead, he's spent the past few months meticulously investigating whether the unrecognised signature was caused by a glitch in his instrumentation, a rogue astrophysical phenomenon, or some unknown random noise. Even if he picks up the signal again - he's been scouring the same co-ordinates of the night sky on an almost daily basis since - the scientific rule book dictates he'll need to get it peer-reviewed before he can take his announcement to the world. "And that is a lot of ifs," he concedes.

The hunt for extraterrestrial life has been boosted recently by the discovery last month of a rocky world not unlike our own, about 20 light years away, which its Swiss discoverers have dubbed Gliese 581e, the latest in a long line of planet discoveries during the past decade (350 and counting). Although Gliese 581e is too close to its host sun to support life, it's the first planet believed to be rocky like our own, a kind of super-hot Earth quite unlike the long line of gas and ice giants discovered to date.

With the launch of NASA's Kepler space telescope in March, specifically designed to detect smaller Earth-like planets, astronomers are confident that the discovery of a blue planet, orbiting in the so-called Goldilocks zone, where liquid water can support life, is edging closer by the day. But it will still be up to ground-based telescopes to confirm the mass of the planet, as space-based telescopes such as the Kepler can only yield its approximate diameter.

The quest of SETI astronomers, however, is not just for the discovery of an Earth-like planet but for life intelligent enough to transmit meaningful signals across vast stretches of space. For more than 40 years, they have been doggedly searching for alien transmissions via radio telescope, tracking tens of millions of radio signals across different sections of the night sky, but so far the results have been, by any scientific standard, dismal. There has been a handful of false alarms - the detection of short, intense bursts of electromagnetic energy that might be transmitted by an advanced civilisation - but these have been later shown to be caused by other cosmic phenomena, such as quasars.

The belief that an alien civilisation might also be listening to our television and radio signals has also been dashed by the recent discovery that the signals don't, as once thought, reach into deep space: they eventually become so weak that they disappear in the roar of the electromagnetic noise. That is partly why the OZ OSETI (o for optical) project and a handful of its US counterparts have turned to laser pulse technology in what is the most ambitious effort yet to detect a signal from an alien species. "For an advanced civilisation, radio wave technology would be old hat," Bhathal says. "My strong feeling is that if there are (extraterrestrial intelligence) civilisations out there, they will send the signal by laser pulses or laser flashes."

In 2000, science fiction writer Arthur C. Clarke, a former patron of the Australian SETI project, advised Bhathal to "let the better spectrum, light" drive his search for ET. Bhathal's OZ OSETI project is the only dedicated project for searching for ET in the optical spectrum in the southern hemisphere. "NASA is already using lasers for space communication and it's not unrealistic to imagine that an extraterrestrial intelligence might be using them as well," Bhathal says. "In terms of Earth technology today, we have achieved a maximum of 1015 watts of laser power for a brief period, butan advanced civilisation could have lasers with powers of 1025." He admits, however, that our failure to pick up any interstellar signals so far could mean that advanced civilisations are using a communications technique still not discovered on Earth. "It is risky to judge everything by our own technology," he says.

The search field of the OZ OSETI project is 100 light years from Earth: a short walk around the block in galactic terms, but an area large enough to contain at least 1000 stars and possibly 20 times as many planets. While the discovery of worlds outside our solar system has given weight to the idea that the universe may be teeming with life - albeit sprinkled across an incomprehensibly wide area - it's the key cosmic numbers that have astronomers in disagreement. For example, how often do the magic ingredients for life - a rocky planet, located at just the right distance from its sun at justthe right moment in the sun's life - come together? If the answer is very often, there ought to be lots of planets like our own, and life may be more the rule than a miraculous accident. In 1960, Frank Drake, now a professor of astronomy at the University of Southern California, estimated that there could be up to a million technological civilisations in the Milky Way galaxy alone. But Bhathal believes "we are nowhere near being able to put a sensible figure on how common life may be".

What we do know is that our sun is a perfectly ordinary star in a rotating island of 100 billion stars, the Milky Way galaxy, which in turn is just one of 100 billion or so galaxies in the observable universe. The laws of mathematics weigh heavily in favour of the idea that we are not alone. Moreover, the discovery of more than 300 planets suggests that solar systems such as ours may not be all that unusual. It's very likely that smaller and rockier worlds are more common than the gas giants, which are easier to find because of the greater wriggle they exert in a star's path.

"The low-mass planets are much harder to find because they have a smaller Doppler amplitude," says Chris Tinney of the department of astrophysics at the University of NSW. "It might also mean we are not looking in the right way. But we're now certain that low-mass planets are more common. The Kepler space telescope will no doubt help usfind them." Tinney explains that while the basic techniques for detecting planets have been around for some time, what's revolutionised the field has been the dramatic technological improvements in spectrographs and telescopic power. "Planet searching has now become a sexy field and private donors in the US are putting money into it," Tinney says.

Other satellite projects such as the Allen telescope array, named after Paul Allen, the Microsoft co-founder who donated $US13million towards its creation, are also coming online. The array uses an incredible 350 satellite dishes to scan the sky for the faint whisper of radio signals from celestial objects such as quasars. There's also the hardware already in space if ET happens to be passing through our neighbourhood. The Pioneer 10 spacecraft, launched in 1972, included an aluminium plate with human figures, a drawing of the planets and an outline of the spacecraft's course. The last, extremely weak signal from this surprisingly robust spacecraft was received in 2006. If it's still around, Pioneer 10 would now be hurtling somewhere in the interstellar void outside our solar system.

With the discovery of more planets, the relatively new science of exobiology, dedicated to the study of extraterrestrial life, has gained the gleam of scientific respectability. But the field is still trying to overcome the UFO stigma, laments Ain de Horta, a project scientist with the Australian SETI Institute. "There are still those in the scientific community who look down their noses at us, but that's increasingly unusual these days. There's a growing recognition that this is important science, with the potential to answer one of the most fundamental questions facing humanity. Those who lump us in with the UFO nuts tend not to be scientists," says de Horta. "We're counting on the physics being the same elsewhere in the universe."

De Horta's institute is, in collaboration with CSIRO's Parkes telescope, scouring radio waves in its search for ET. "If an alien civilisation has developed technology it's likely to be based on most ofthe same principles as our own. Like us, forexample, they would have discovered radio waves." Even so, de Horta concedes, life elsewhere in the universe might resemble nothing we know on Earth. It could be moulded by different chemistries, different gravity and different climatic environments.

In any case, it's highly unlikely we'll ever have a face-to-face meeting, as space travel even at Star Trek's warp drive wouldn't get us there in less than thousands of years. A two-way conversation would take decades. And even for that to happen, says de Horta, we would need intelligent life to be reaching its technological prime at the same time as ours and transmitting radio waves at a wavelength that we can detect. "The whole argument about communication hinges on the longevity of a species and their use of a technology that is recognisable to us," he says.

What all the planet hunters and SETI have in common is a white-hot passion for discovering alien worlds. Bhathal knows that the odds of finding anything are long and the area he is scanning, as big as it is, may still not be extensive enough to yield anything, but he's determined to keep his eyes on the sky. "There (have) to be other Earth-like worlds. Otherwise what do we have? A whole lot of wasted space.">>
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Re: APOD: A Laser Strike at the Galactic Center (2010 Sep 06

Post by bystander » Mon Sep 06, 2010 4:04 pm

A Laser Beam Towards the Milky Way's Centre
ESO Picture of the Week | potw1036a | 06 Sept 2010
In mid-August 2010 ESO Photo Ambassador Yuri Beletsky snapped this amazing photo at ESO’s Paranal Observatory. A group of astronomers were observing the centre of the Milky Way using the laser guide star facility at Yepun, one of the four Unit Telescopes of the Very Large Telescope (VLT).

Yepun’s laser beam crosses the majestic southern sky and creates an artificial star at an altitude of 90 km high in the Earth's mesosphere. The Laser Guide Star (LGS) is part of the VLT’s adaptive optics system and is used as a reference to correct the blurring effect of the atmosphere on images. The colour of the laser is precisely tuned to energise a layer of sodium atoms found in one of the upper layers of the atmosphere — one can recognise the familiar colour of sodium street lamps in the colour of the laser. This layer of sodium atoms is thought to be a leftover from meteorites entering the Earth’s atmosphere. When excited by the light from the laser, the atoms start glowing, forming a small bright spot that can be used as an artificial reference star for the adaptive optics. Using this technique, astronomers can obtain sharper observations. For example, when looking towards the centre of our Milky Way, researchers can better monitor the galactic core, where a central supermassive black hole, surrounded by closely orbiting stars, is swallowing gas and dust.

The photo, which was chosen as Astronomy Picture of the Day for 6 September 2010, was taken with a wide-angle lens and covers about 180 degrees of the sky.
Astronomers are putting stars in their skies
New Scientist | Short Sharp Science | 06 Sept 2010

For more on adaptive optics, see:
http://asterisk.apod.com/vie ... 31&t=20534
http://asterisk.apod.com/vie ... 31&t=19870
http://asterisk.apod.com/vie ... 31&t=19168

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Re: APOD: A Laser Strike at the Galactic Center (2010 Sep 06

Post by Henning Makholm » Mon Sep 06, 2010 9:17 pm

neufer wrote:
Optical SETI supporters have conducted paper studies of the effectiveness of using contemporary high-energy lasers and a ten-meter focus mirror as an interstellar beacon. The analysis shows that an infrared pulse from a laser, focused into a narrow beam by such a mirror, would appear thousands of times brighter than the Sun to a distant civilization in the beam's line of fire. The Cyclops study proved incorrect in suggesting a laser beam would be inherently hard to see.
If my calculations above are correct (somebody please check them!), this seems to assume a diffraction-limited beam from a megawatt-or-more laser. That would be a weapons-grade system of a kind that has not really been demonstrated in practice. Which doesn't mean that it is impossible, of course, but it is a far cry from what is happening at Paranal.

... hmm, it says "infrared". Using far infrared instead of visible light will make it harder to collimate the beam, but that is made up for by the fact that the Sun is less bright in infrared. Whether it's actually an advantage depends on how well the receiving aliens are able to filter out the relevant wavelengths at different parts of the EM spectrum.
Henning Makholm

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Re: APOD: A Laser Strike at the Galactic Center (2010 Sep 06

Post by Guest » Mon Sep 06, 2010 11:24 pm

celestemekent wrote:are you sure that some alien scientist is not right now painfully yelling about some stupid people on this distant plant burning his eyes with a laser.
Yep heshould start yelling in about 26,000 ± 1,400 years!

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Re: APOD: A Laser Strike at the Galactic Center (2010 Sep 06

Post by neufer » Tue Sep 07, 2010 2:28 am

Henning Makholm wrote:
http://en.wikipedia.org/wiki/SETI wrote:Optical SETI supporters have conducted paper studies of the effectiveness of using contemporary high-energy lasers and a ten-meter focus mirror as an interstellar beacon. The analysis shows that an infrared pulse from a laser, focused into a narrow beam by such a mirror, would appear thousands of times brighter than the Sun to a distant civilization in the beam's line of fire. The Cyclops study proved incorrect in suggesting a laser beam would be inherently hard to see.
If my calculations above are correct (somebody please check them!), this seems to assume a diffraction-limited beam from a megawatt-or-more laser. That would be a weapons-grade system of a kind that has not really been demonstrated in practice. Which doesn't mean that it is impossible, of course, but it is a far cry from what is happening at Paranal.

... hmm, it says "infrared". Using far infrared instead of visible light will make it harder to collimate the beam, but that is made up for by the fact that the Sun is less bright in infrared. Whether it's actually an advantage depends on how well the receiving aliens are able to filter out the relevant wavelengths at different parts of the EM spectrum.
Image
That would be a near-infrared weapons-grade system
of a kind that really has been demonstrated in practice.


It is certainly a far cry from what is happening at Paranal
but if one really wanted to send a (far cry) message....
http://en.wikipedia.org/wiki/Chemical_oxygen_iodine_laser wrote:
<<Chemical oxygen iodine laser, or COIL, is an infrared chemical laser. As the beam is infrared, it cannot be seen with the naked eye. It is capable of output power scaling up to megawatts in continuous mode. Its output wavelength is 1.315 µm, the wavelength of transition of atomic iodine. COIL is the main weapon laser for the military airborne laser and advanced tactical laser programs. On February 11 2010, this weapon was successfully deployed to shoot down a missile off the central California coast in a test conducted with a laser aboard a Boeing jumbo jet launched from the Point Mugu Naval Warfare Center.>>
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Re: APOD: A Laser Strike at the Galactic Center (2010 Sep 06

Post by dprice » Tue Sep 07, 2010 12:25 pm

So how come you can see the beam on a clear night like that? I thought lasers of any color are invisible unless there is dust to reflect the color.
dp

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Re: APOD: A Laser Strike at the Galactic Center (2010 Sep 06

Post by Chris Peterson » Tue Sep 07, 2010 2:08 pm

dprice wrote:So how come you can see the beam on a clear night like that? I thought lasers of any color are invisible unless there is dust to reflect the color.
There is dust everywhere. And the laser scatters from air molecules, as well. Only a tiny fraction of the laser's full output is being scattered, but the exposure is obviously long- 30 seconds or more- and you can compare the apparent brightness of the laser to the apparent brightness of objects in the sky to get a sense of how dim it would appear visually.
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Re: APOD: A Laser Strike at the Galactic Center (2010 Sep 06

Post by swainy (tc) » Tue Sep 07, 2010 8:32 pm

Chris Peterson wrote:There is dust everywhere.
Yes, Its hard to see, but when the suns rays come through the window, it easy to see.


Nice one Chris. :wink:
tc

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alter-ego
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Re: APOD: A Laser Strike at the Galactic Center (2010 Sep 06

Post by alter-ego » Wed Sep 08, 2010 5:47 am

Henning Makholm wrote:
neufer wrote:
Optical SETI supporters have conducted paper studies of the effectiveness of using contemporary high-energy lasers and a ten-meter focus mirror as an interstellar beacon. The analysis shows that an infrared pulse from a laser, focused into a narrow beam by such a mirror, would appear thousands of times brighter than the Sun to a distant civilization in the beam's line of fire. The Cyclops study proved incorrect in suggesting a laser beam would be inherently hard to see.
If my calculations above are correct (somebody please check them!), this seems to assume a diffraction-limited beam from a megawatt-or-more laser. That would be a weapons-grade system of a kind that has not really been demonstrated in practice. Which doesn't mean that it is impossible, of course, but it is a far cry from what is happening at Paranal.
Henning,
I used the following equation to find the Laser-to-Solar Irradiance Ratio that ET would see arbitrarily far away.
Irradiance Ratio Calculation
Irradiance Ratio Calculation
I was a bit confused what solar wavelength range you were integrating over, so I did a more general calculation which includes wavelength detection resolution (binning). If the brightness ratio = 1, then averaged over a given bin, the laser has the same brightness as the sun (so the sum is 2x the solar black body intensity). The equation assumes a 1xDL (diffraction limited) beam, and includes diffraction but no losses.
A 10 meter dia mirror is used for the following results:
For the 589nm CW laser, about 20W is required for ~10x laser irradiance enhancement within a 100 femtometer wavelength bin (the laser has a 5.8fm bandwidth) Searching for a 100fm line seems like a needle in a haystack to me.
For the 1.315um COIL CW laser, 1MW also yields ~10x brightness enhancement, but within a spacious 5nm bin. Still small, but seems manageable by today's technology. You can see the advantage of the NIR laser by virtue of its power capability. I don't know the BW of the COIL, but it is most likely <1nm.

For comparison (but not really a useful one), you would need ~25MW of COIL power to equal the power within the visible 300nm bin (nominally 400nm to 700nm).

I think I did this right. AndyG's point about using a filter is exactly what the above calculations address.
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Re: APOD: A Laser Strike at the Galactic Center (2010 Sep 06

Post by neufer » Wed Sep 08, 2010 11:58 am

swainy (tc) wrote:
Chris Peterson wrote:There is dust everywhere.
Yes, Its hard to see, but when the suns rays come through the window, it easy to see.
http://asterisk.apod.com/vie ... 77#p131624
Art Neuendorffer

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Henning Makholm
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Re: APOD: A Laser Strike at the Galactic Center (2010 Sep 06

Post by Henning Makholm » Wed Sep 08, 2010 12:02 pm

alter-ego wrote:
Henning Makholm wrote:If my calculations above are correct (somebody please check them!),
I was a bit confused what solar wavelength range you were integrating over,
Oh, the entire spectrum. That's a bit lazy (it's what it was quickest to find a figure for), but I figured that whatever filter the hypothetical alien astronomer (who would be blinded by the laser) would be looking through could not possibly make a dent in the 27 magnitudes of difference I'd found.

I didn't actually calculate anything for my later claim about "megawatt-or-more" COIL rating. I simply guesstimated a filter bandwidth that would contain at least 1e-6 or thereabouts of the solar power output, since I don't really know how easy filtering is at different parts of the spectrum.
Henning Makholm

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Re: APOD: A Laser Strike at the Galactic Center (2010 Sep 06

Post by ntlgnce@yahoo.com » Tue Sep 14, 2010 11:45 pm

I have a question That pertains to " A Laser Strike at the Galactic Center (2010 Sep 06) " If we were to zoom in on the galatic center with the hubble at the same time that we are shining the laser at it, we should in theory be able to see the end of the laser beam moving through space twards the galatic center. Thats if the theory that light only travles at a certin speed. How long would it take for the laser to reach the center?

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