It was meant as a joke (do I really have to point that out?) and we were specifically talking about ducks. 

It was meant as a joke (do I really have to point that out?) and we were specifically talking about ducks.![]()
1 trillion Watts = 10^12 W
100 billion billion Watts = 10^20 W
The energy output of a star = 7.16x10-7 r^2 T^4 W where r is the radius of the star in metres and T is its surface temperature in Kelvin. For the Sun and HD 164595 (which has a slightly lower mass and temperature than the Sun), the energy output is about 4x10^26 W -- greater by 100 trillion times than 1 trillion Watts and 10,000 than 100 billion billion Watts. So only a small proportion of the star's energy would have to be captured and used to generate the signal in either scenario.
http://www.schoolphysics.co.uk/age16-19/Astrophysics/text/Power_output_of_a_star/index.html
Still would be quite a trick to pull it off. If it is an actual signal, props to them on making it happen.![]()
Maybe it's not just a signal, it's a test firing of their new mega-ray!
Yeah, maybe it's Standard Galactic for, "This one's ripe!" The dinner bell.Maybe they're craving some BBQ humans?!?![]()
That's no moon, it's a space station...Maybe it's not just a signal, it's a test firing of their new mega-ray!
That's how they killed Hitler.That's no moon, it's a space station...
They recorded it at about 11 Ghz, which puts it firmly in the microwave spectrum. That would be a good band for a long-range, point-to-point communications attempt, which is probably the main reason they asked SETI to investigate. OTOH, it would be very difficult to generate a signal of that intensity using known materials; that kind of output would probably vaporize the transmitter in the process (or that could be the whole point if the transmitter is something like a bomb-pumped maser).1 trillion Watts = 10^12 W
100 billion billion Watts = 10^20 W
The energy output of a star = 7.16x10-7 r^2 T^4 W where r is the radius of the star in metres and T is its surface temperature in Kelvin. For the Sun and HD 164595 (which has a slightly lower mass and temperature than the Sun), the energy output is about 4x10^26 W -- greater by 100 trillion times than 1 trillion Watts and 10,000 than 100 billion billion Watts. So only a small proportion of the star's energy would have to be captured and used to generate the signal in either scenario.
http://www.schoolphysics.co.uk/age16-19/Astrophysics/text/Power_output_of_a_star/index.html
The peak power in the largest solar flares is about 10^20 W lasting from between a few minutes up to about an hour typically (at peak output, that's the equivalent of the total explosive yield of 25,000 1-megaton H bombs per second). I'd have to investigate how much of that is in the GHz region (presumably generated by magnetobremsstrahlung) but it's not inconceivable that there might be sufficient power available. However, the time series profile of a flare (in the microwave region, a rapid rise followed by a prolonged decay perhaps with additional superimposed rapid rises) doesn't look like what was reported (although that might be an artefact of how the signal was detected -- perhaps it swept through the lobe of the antenna sensitivity -- I'm not familiar with the observatory).
Perhaps there is a civilization there that isn't so advanced that they've "harnessed 100% of the output of the host star" or whatever - but IS advanced enough to use a naturally occurring flare of their star* to send a powerful signal toward a planet they think is a likely candidate for life like theirs?So we're getting all worked up for some stupid solar flares?
if there're any people in the vicinity they must be getting one hell of a tan!I suspect there isn't enough power available in the microwave region to explain the signal (most of the power emitted is probably in high-energy X ray photons) but it might also depend on whether the EM radiation can be constrained to be emitted in a preferred direction because of the magnetic field configuration along which the electrons are gyrating.
The flux density of solar radiation at 10 GHz received at the Earth = 1.24 x 10^-20 Wm^-2Hz^-1 = 1.24 x 10^6 Jy (Janskys)But solar flares or CMEs producing microwaves at that frequency... is there actual precedent for that?
The flux density of solar radiation at 10 GHz received at the Earth = 1.24 x 10^-20 Wm^-2Hz^-1 = 1.24 x 10^6 Jy (Janskys)
http://www.cv.nrao.edu/course/astr534/Brightness.html
The peak flux density at 17 GHz from the great flare of July 7, 1966 measured at Earth = 10^-18 Wm^-2Hz^-1 = 10^8 Jy
http://adsabs.harvard.edu/full/1969SoPh....8..119H
Not quite the same frequency but it seems tenable that a flare can outshine a star by a factor of about 100 at a microwave frequency of 10-20 GHz.
That's just a distance of 1 AU though. There are 63241 AU in a light year so at one light year distant, the flux density from the flare would drop to 1/(63241^2) of the value or 2.5 x 10^-10 * 10^8 Jy = 2.5 x 10^-2 Jy.
At the distance of HD164595 (95 ly), the flux density would drop by a further 1/(95^2) or 1.1 x 10^-4 to 2.75 x 10^-6 Jy. Anyone know what was the strength of the signal received by the RATAN-600 radio telescope? The graph I've seen doesn't show the units on the Y axis.
http://www.centauri-dreams.org/wp-content/images/ratan_3.jpeg
Who is this addressed to? It seems you are having an one-sided conversation.The flux density of solar radiation at 10 GHz received at the Earth = 1.24 x 10^-20 Wm^-2Hz^-1 = 1.24 x 10^6 Jy (Janskys)
http://www.cv.nrao.edu/course/astr534/Brightness.html
The peak flux density at 17 GHz from the great flare of July 7, 1966 measured at Earth = 10^-18 Wm^-2Hz^-1 = 10^8 Jy
http://adsabs.harvard.edu/full/1969SoPh....8..119H
Not quite the same frequency but it seems tenable that a flare can outshine a star by a factor of about 100 at a microwave frequency of 10-20 GHz.
That's just a distance of 1 AU though. There are 63241 AU in a light year so at one light year distant, the flux density from the flare would drop to 1/(63241^2) of the value or 2.5 x 10^-10 * 10^8 Jy = 2.5 x 10^-2 Jy.
At the distance of HD164595 (95 ly), the flux density would drop by a further 1/(95^2) or 1.1 x 10^-4 to 2.75 x 10^-6 Jy. Anyone know what was the strength of the signal and the channel width as received by the RATAN-600 radio telescope? The graph I've seen doesn't show the units on the Y axis.
http://www.centauri-dreams.org/wp-content/images/ratan_3.jpeg
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