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Thread: Question about optical resolution of spy satelites

  1. #1
    Hello everyone, I'm a major lurker on this board...just never had much to say I guess. [img]/phpBB/images/smiles/icon_smile.gif[/img]

    I'm wondering if there is a theoretical maximum on resolution capabilities of a "spy" satelite, or if it's just a matter of magnification? For instance would it ever be possible for a satelite in orbit to read a newspaper on the ground, or is there a fundamental limit based on the wavelength of light or other fancy-sounding terms?

    Thanks everyone...this board is an endless source of entertainment. I should have my language translation software for decoding the HUb'-bot's code available soon...I'll let you all know.

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    This issue concerns the Rayleigh criterion for resolution. The Rayleigh criterion states that the best possible angular resolution of a lens is given by:

    1.22 lambda/d

    where lambda is the wavelength of light, d is the diameter of the lens, and the angle is given in radians.

    To read a newspaper, let us say the satelite is in near earth orbit, ~250 miles up=~400,000m. You would need an angular resolution of .001m/400,000m (assuming you need a 1mm resolution to read the paper) or 2.5e-9 radians. In order to resolve this you would need a lens of
    d=1.22*5e-7m/2.5e-9
    or d=~2.4e2 m or 240m wide lens!
    So not likely.

    <font size=-1>[ This Message was edited by: Zathras on 2002-10-30 17:20 ]</font>

  3. #3
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    I can't say much about what is possible now but I can tell you what was possible in 1974.

    I was in Viet Nam and periodicly got intellegence photos for my missions that show the target area. One time we got a photo that showed a man sitting in a captured jeep. He was looking up at the sky and you could see the rank insignia on his collar. When we got to the target we could recognize him among the captives.

    I would assume it has gotten better since then.

  4. #4
    Thanks for the equations. I thought there was something to do with the wavelength of light. I ran the math for the 1m resolution photos that are released to the public and it results in .244m lens. What a huge difference. Any idea on what the maximum resolution of current satellites might be? Or perhaps the maximum sized lens that could be put in orbit? Are there other factors that might affect resolution besides lens diameter (computers, digital imaging, etc).

    I really have no idea why I'm on this topic today. I have a very intelligent roommate that leans towards conspiracy theories and hearing him say "Well everyone knows the govt. has spy satellites that can read your newspaper" is just begging for a rebuttal. [img]/phpBB/images/smiles/icon_smile.gif[/img]

    I originally found this board after seeing an apollo hoax site and finding it pretty convincing. I went looking for the other side and it took about 5 minutes of research before I realized how incredibly stupid it was. Since then I've developed an immense amount of pleasure watching pseudo-science get utterly demolished. Keep up the good fight guys.

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    On 2002-10-30 15:37, Russ wrote:
    I can't say much about what is possible now but I can tell you what was possible in 1974.

    ...

    I would assume it has gotten better since then.
    I know you say you know what you saw, but would bet is isn't from a satellite. It perhaps COULD have been an airphoto.

    The satellite would have to be HUGE to have the equipment necessary to get that kind of resolution from space. Just the lens or mirror would have to be hundreds of meters in diameter.

    CJSF
    "In the nightgown of the sullen moon, How the windows lean into the room, In the nightgown of the sullen moon."
    -They Might Be Giants

  6. #6
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    So they can't tell my blood type by looking at a mosquito bite on my arm?


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    Only if you scratch it and spread the blood around a little... [img]/phpBB/images/smiles/icon_smile.gif[/img]

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    What if you get the mosquito before she can fly away?

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    The Guy was probably looking up at the FAC taking the photo. [img]/phpBB/images/smiles/icon_smile.gif[/img] -Colt

    Edit: FAC= Forward Air Controller, small airplanes used to orient ground forces and for recon.[img]/phpBB/images/smiles/icon_biggrin.gif[/img]
    _________________
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    <font size=-1>[ This Message was edited by: Colt on 2002-10-31 15:39 ]</font>

  10. #10

    Sort of a Johnny come lately but...

    I was researching stuff on the web and came across this post. The Rayleigh Criterion, is quite well done, however as the devil's advocate, a smaller lens could be used if you considered UV "light" say in the region of 10nm, then you're calculation works out to a more managable 4.88 metres.

    Now don't ask me if or how you can convert UV into a visible image (I don't work in area 51 ) but thought I'd toss this out as an idea to consider.

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    The biggest problem with that is that the atmosphere isn't especially transparent to UV, especially when compared to visible light (which is lucky for us, or we'd all have terrible sunburns 24/7)

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    Hubbles 2.4 meter mirror achieves a resolution of about 0.04 arcseconds. That's equivalent to 58 mm at a distance of 300 km. The spy satellites are roughly the same size as Hubble, but they're looking down through a turbulent atmosphere.

    KH-11 has a 2.3 meter primary.
    According to an estimate by the private Federation of American Scientists (FAS), three satellites operated by the U.S. National Reconnaissance Office (NRO) have resolutions as sharp as 10 centimeters (3.93 inches) -- in other words, the satellites can discern a softball-sized object from several hundred miles away.
    Spy Satellites: Still a Few Steps Ahead

  13. #13
    The similarity there between the size of the Hubble mirror and the KH-11 mirror is not coincidental

    Doug

  14. #14
    Sounds like someone unloaded a cruddy mirror left over from a spy satellite program on NASA.

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    Quote Originally Posted by Ronald Brak View Post
    Sounds like someone unloaded a cruddy mirror left over from a spy satellite program on NASA.
    No, they were making so many of them that they got sloppy

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    It is possible that the new "negative refractive index" materials will allow imaging beyond the diffraction limit in astronomy. If so, the size of the lens or mirror required will be dramatically smaller than is the case now.
    These "superlenses" have beat the diffraction limit in microscopy where the lens can be put very close to the imaged objects in experiments. But it is not proven they can be used in astronomy where the lens will be far from the imaged object.

    New superlens opens door to nanoscale optical imaging and high-density optoelectronic devices.
    By Sarah Yang, Media Relations | 21 April 2005
    "BERKELEY – A group of scientists at the University of California, Berkeley, is giving new relevance to the term "sharper image" by creating a superlens that can overcome a limitation in physics that has historically constrained the resolution of optical images."
    ...
    "In the long run, this line of research could lead to even higher resolution imaging for distant objects, the researchers said. This includes more detailed views of other planets as well as of human movement through surveillance satellites."
    http://www.berkeley.edu/news/media/r...uperlens.shtml



    Bob Clark

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    Quote Originally Posted by herocomplex View Post
    ...is a theoretical maximum on resolution capabilities of a "spy" satellite...would it ever be possible for a satellite in orbit to read a newspaper on the ground, or is there a fundamental limit based on the wavelength of light or other fancy-sounding terms?...
    Yes there's a fundamental limit, based on currently-understood optical physics.

    Under perfect conditions and assuming lowest possible perigee, current optical spy satellites might resolve about 1.5 to 2 inches. This assumes perfect adaptive optics to cancel atmospheric distortion.

    The typical resolution is probably worse than this because the perigee isn't normally that low, the atmosphere isn't perfectly clear and adaptive optics don't work perfectly. They definitely can't read a newspaper or license plate, but under ideal conditions might crudely identify a person by body shape.

    Unlike the movies, optical spy satellites don't hover overhead in geostationary positions. They typically operate in very low orbits, thus are only overhead a couple of times per day for maybe 20 minutes per pass. That plus cloud cover is the real limitation.

    Details: KH-11/12 optical spy satellites are somewhat larger and heavier than the Hubble Space Telescope. They are about 4.5 meters in diameter, 15 meters long, and weigh about 18 tons (36,000 pounds, or 16,300 kg). About 14,000 pounds of this is maneuvering propellant.

    The optics are thought to be about 2.5 meters in diameter, roughly the size of Hubble's primary mirror. They likely have adaptive optics of some type.

    The orbit perigee is variously reported as 95 miles (153 km) or 170 miles (274 km). Given the fuel capacity, it's likely they can maneuver substantially.

    http://www.fas.org/spp/military/program/imint/kh-12.htm
    http://www.astronautix.com/craft/impystal.htm

    From this we can calculate the theoretical linear resolution. Angular resolution at 500 nanometers is:

    resolution = 250000 * wavelength / diameter, or 0.05 arc seconds

    Linear resolution at distances of 153 and 274 km is given by:

    res = tan (angle) * distance, or 3.7 cm (1.4 in) at 153 km and 6.6 cm (2.6 in) at 274 km.

    The Lacrosse/Onyx radar-based recon sats use synthetic aperture radar to image though clouds. Their resolution might be about 1 meter:

    http://www.fas.org/spp/military/prog.../xlacrosse.htm

    Practical use of negative refractive index optics to exceed diffraction-limited resolution is a new development. Current use is for microscopes. Whether it's applicable to telescopes is being researched. Discussion: http://www.bautforum.com/showthread.php?t=54814

  18. #18
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    Quote Originally Posted by joema View Post
    Yes there's a fundamental limit, based on currently-understood optical physics.
    Great post, but I couldn't resist the opening for this...

    [Sarcastic puppet mode]
    Then why not move the Hubble to the ISS?
    You say:
    "They typically operate in very low orbits."
    So its clear that Hubble can too!
    "spy satellites are somewhat larger and heavier than the Hubble Space Telescope." AND "About 14,000 pounds of this is maneuvering propellant." AND Given the fuel capacity, it's likely they can maneuver substantially."
    So if that can be done with these telescopes, then there is no issue that can't be easily resolved with HST.
    [/Sarcastic puppet mode]
    Oh by the way...I saved you from bolding and colors.

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    Quote Originally Posted by hhEb09'1 View Post
    No, they were making so many of them that they got sloppy
    But sloppy in a very precise way, right?

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    Quote Originally Posted by Squink View Post
    The spy satellites are roughly the same size as Hubble, but they're looking down through a turbulent atmosphere.
    Pardon the naive question but surely adaptive optics can work both ways? If it is possible for ground equipment it must be feasible for space-based even if it has to be much hardier and probably less fancy, I am sure some basic AO can be used?
    The impossible often has a kind of integrity the merely improbable lacks. -Douglas Adams


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    Quote Originally Posted by mantiss View Post
    Pardon the naive question but surely adaptive optics can work both ways? If it is possible for ground equipment it must be feasible for space-based even if it has to be much hardier and probably less fancy, I am sure some basic AO can be used?
    Situational, I guess. If you think about it, the bulk of your adaptive optics scopes are situated as high up as possible to minimize the atmosphere between them and space. With spysats, you don't have the luxury. If what you're looking at is 50 feet below sea level in the Netherlands (as an example), you've got all the atmosphere an astronomer could never want between you and it, and that's going to play hell on your resolution capability.

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    Quote Originally Posted by joema View Post
    Unlike the movies, optical spy satellites don't hover overhead in geostationary positions. They typically operate in very low orbits, thus are only overhead a couple of times per day for maybe 20 minutes per pass. That plus cloud cover is the real limitation.

    Details: KH-11/12 optical spy satellites are somewhat larger and heavier than the Hubble Space Telescope.
    That's not really true. The KH satellites typically are in Molniya orbits, which can "hover". See The BA's article about it.

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    Quote Originally Posted by Doodler View Post
    Situational, I guess. If you think about it, the bulk of your adaptive optics scopes are situated as high up as possible to minimize the atmosphere between them and space. With spysats, you don't have the luxury.
    Unless, of course, your intention is to spy on the astronomers .

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    Quote Originally Posted by pghnative View Post
    Unless, of course, your intention is to spy on the astronomers .
    Oh, I imagine that gets fun, a stargazer and a spook playing peekaboo tag through their respective 'scopes.

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    Quote Originally Posted by Doodler View Post
    Oh, I imagine that gets fun, a stargazer and a spook playing peekaboo tag through their respective 'scopes.
    Each trying to blind the other, one with an artificial star, and the other with an artificial astronomer.

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    Quote Originally Posted by hhEb09'1 View Post
    That's not really true. The KH satellites typically are in Molniya orbits, which can "hover". See The BA's article about it.
    I don't think that's correct. A Molniya orbit is a specific type of highly elliptical orbit. A Molniya orbit has:
    (1) an orbital inclination of 63.4 degrees
    (2) an orbital period of 12 hours
    (3) No perigee precession (orbital mechanics ensure perigee stays at the same place)

    If the orbit doesn't have those exact characteristics, by definition it's not a Molniya orbit: http://en.wikipedia.org/wiki/Molniya_orbit

    Molniya orbits typically have apogee in the northern hemisphere and an apogee altitude of about 40,000 km (24,850 miles).

    Molniya orbits do have long "apogee dwell". This is useful for communications satellites and missile warning satellites, since they can work from high altitude. It would tremendously handicap an optical spy satellite by vastly reducing the resolution.

    A KH-12 satellite's max theoretical resolution at apogee in a Molniya orbit would be reduced to 31 feet (vs about 2 inches in a low orbit). So while a Molniya orbit allows a certain amount of "hovering", it's at a very high altitude that would make an optical spy satellite almost useless.

    Satellites (inc'l optical spy satellites) can be visually tracked by amateurs and the orbital elements computed. From this we know KH optical spy satellites have an orbital inclination of about 97-98 degrees (vs 63.4 degrees for a Molniya orbit), an orbital period of roughly 90 minutes (vs 12 hr for a Molniya orbit): http://www.fas.org/spp/military/prog...t/andronov.htm

    It's true the KH spy satellites have somewhat elliptical orbits, but this is very mild relative to the 40,000 km apogee of a Molniya orbit.

    A key purpose of a Molniya orbit is there's no perigee precession, so no manuvering fuel is required to maintain it. By contrast the KH satellites have a huge amount of manuvering fuel and likely change orbital elements quite a bit.

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    Quote Originally Posted by joema View Post
    I don't think that's correct. A Molniya orbit is a specific type of highly elliptical orbit.
    Maybe not precisely, but here is another source, that says "[KH] satellites are in egg-shaped elliptical orbits ranging from a low of 175 miles to a high of 625 miles above Earth. Each passes over its assigned observation target on the ground twice a day."

    I'm not sure what they mean by "egg-shaped"
    Quote Originally Posted by joema View Post
    A KH-12 satellite's max theoretical resolution at apogee in a Molniya orbit would be reduced to 31 feet (vs about 2 inches in a low orbit).
    What values were you using for that calculation?

  28. #28
    Quote Originally Posted by Zathras View Post
    This issue concerns the Rayleigh criterion for resolution. The Rayleigh criterion states that the best possible angular resolution of a lens is given by:

    1.22 lambda/d

    where lambda is the wavelength of light, d is the diameter of the lens, and the angle is given in radians.

    To read a newspaper, let us say the satelite is in near earth orbit, ~250 miles up=~400,000m. You would need an angular resolution of .001m/400,000m (assuming you need a 1mm resolution to read the paper) or 2.5e-9 radians. In order to resolve this you would need a lens of
    d=1.22*5e-7m/2.5e-9
    or d=~2.4e2 m or 240m wide lens!
    So not likely.

    <font size=-1>[ This Message was edited by: Zathras on 2002-10-30 17:20 ]</font>

    You could, in principle, use smaller lenses that were separated by that (or greater) distance. It doesn't have to be a single lens, but at optical wavelengths I imagine you have a host of technical difficulties in making that work.

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    Quote Originally Posted by Doodler View Post
    you've got all the atmosphere an astronomer could never want between you and it, and that's going to play hell on your resolution capability.
    Is it though? Looking down through the atmosphere is a different game than looking up.

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    Quote Originally Posted by hhEb09'1 View Post
    What values were you using for that calculation?
    It appears he was using 40,000 km, which is the value for apogee of a Molniya orbit, according to the 2nd link in the BA's article. I get 34 ft, not 31, but clearly close enough. This assumes we all agree that to either:

    - hover (theoretical true geosynchronous)
    - essentially hover (real-life geosynchronous where some wobble is allowed)
    - psuedo-hover (Molniya orbit, which is nearly geosynchronous at apogee)

    that you must be ~ 40,000 km above the earths surface, AND we all agree that joema's posted calculation for theortical resolution of visible light is correct.

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