Stories
Slash Boxes
Comments

SoylentNews is people

SoylentNews is powered by your submissions, so send in your scoop. Only 16 submissions in the queue.
posted by martyb on Monday September 02, @01:18PM   Printer-friendly

Even Earth's mightiest telescopes aren't up to the task of imaging Apollo lunar landing sites. A lack of resolution is the biggest reason why:

Back in the early 2000s, when I was butting heads seemingly every week with people who believed the Apollo moon landings were faked, such individuals would pull out an argument they thought was their ace in the hole: If NASA's Hubble Space Telescope is powerful enough to see the intricate details of distant galaxies, why can't it see the Apollo astronaut boot prints on our own moon?

Like most conspiratorial thinking, this argument seems persuasive on its surface but falls apart under the slightest scrutiny. Those taken in by it have a misunderstanding of two things: how telescopes work and just how big space is.

Many people think a telescope's purpose is to magnify images. Certainly manufacturers of inexpensive (read: cheap) telescopes love to market them as such: "150x power!" they print in huge lettering on the box (along with highly misleading photographs from much bigger telescopes). While magnification is important, a telescope's real strength is in its resolution, however. The difference is subtle but critical.

Magnification is just how much you can zoom in on an object, making it look bigger. That's important because while astronomical objects are physically big, they're very far away, so they appear small in the sky. Magnifying them makes them easier to see.

Resolution, on the other hand, is the ability to distinguish two objects that are very close together. For example, you might perceive two stars orbiting each other—a binary star—as a single star because they're too closely spaced for your eye to separate. You can't resolve them. Looking through a telescope with higher resolution, however, you might be able to discern the separation between them, revealing that they are two individual stars.

But isn't that just magnification, then? No—because magnification only makes things bigger! This is easy to demonstrate with a photograph: you can zoom in on the photograph as much as you'd like, but past a certain limit, you're just magnifying the pixels, and you can't get any more information out of it. To break through that wall, you have to gain resolution rather than magnification.

[...] At its best, Hubble's resolution is about 0.05 arcsecond—a very tiny angle! But how much detail it can see in real terms depends on the target's distance and physical size. For example, 0.05 arcsecond is equivalent to the apparent size of a dime seen from about 140 kilometers away.

That brings us back to the conspiracy theorists and their gripe about spotting boot prints on the moon. Galaxies are typically tens of millions or even billions of light-years from Earth. At those distances, Hubble can resolve objects a few light-years across—tens of trillions of kilometers—at best. So while it looks like we're seeing galaxies in great detail in those spectacular Hubble images, the smallest thing we can see is still tremendously huge.

Meanwhile the moon is only about 380,000 km from us—and from Hubble. At that distance, Hubble's resolution surprisingly limits it to resolving objects no smaller than about 90 meters across. So not only can we not see the astronauts' boot prints in Hubble images but we also can't even see the Apollo lunar landers, which were only about four meters across!


Original Submission

 
This discussion was created by martyb (76) for logged-in users only. Log in and try again!
Display Options Threshold/Breakthrough Mark All as Read Mark All as Unread
The Fine Print: The following comments are owned by whoever posted them. We are not responsible for them in any way.
  • (Score: 4, Interesting) by VLM on Monday September 02, @03:09PM

    by VLM (445) on Monday September 02, @03:09PM (#1370921)

    Here's a pretty good EE analogy:

    optic diameter, size, sets the signal to noise ratio.

    The shape of the optic (magnification) sets the gain.

    From playing with amplifiers we "all know" that if you have a small weak noisy signal then turning up the gain (amplification, magnification) all you get is a loud noise, not a clear noise.

    People who've never used a scope (people buying a scope for a kid, perhaps) think all the money in a scope is in the magnification or gain, but actually, all the money in a scope is in the diameter or SNR or resolution.

    Now what would be interesting is "how close do you have to be?" Its generally accepted that a NSA satellite from the 80s deployed from the Space Shuttle bay could under absolutely ideal conditions with a lot of good luck probably get a license plate correct or at least not too wrong. Also its unclear what they mean by image the plate; there's a single pixel indicating there is or is not a plate installed on the car, or are they imaging the screws so they can tell if I have a standard or Philips screw holding the plate to the car? So, a somewhat smaller scope in orbit around the moon should easily be able to image the landing sites, probably.

    Another novelty is indirect proof. It would be beyond trivial to take a zillion photos around sunrise and sunset of very long shadows from very short lunar things in the region of the landing, and do an annoying amount of image processing to generate a 3-d model of the landing site based upon zillions of different shadow images, although it only exists in the equations there's no single photographic shot showing more than some strangely shaped shadow blotches. At the instant of sunrise, a "short" flag has an infinitely long shadow, if the surface of the moon were perfectly flat (which it is not). Like a MRI or CAT scan but using shadows.

    A final novelty would be some kind of scintillation study. In theory, the shiny bits should be ... shiny, even if you can't resolve the image. Imagine a pile of dominos laying in my backyard, even if you can't image them, sometimes the sunlight will be very bright when the angles are "just right" and you could generate an elaborate model of the pile of shiny dominos based on the number, timing, and angle of reflections, even if you couldn't resolve the image of the dominos. I know there's laser retroreflectors on the moon and I know if you blast the F out of the site from earth you can get "some" photons back to the earth and they've been doing that since the landings. However, I wonder how things are in 2024... just how small of a scope would you need to detect the standard deviation of light intensity from a single pixel where the landing is supposed to be is just slightly off from all the nearby pixels? I'm not talking about directly imaging, or even 3-D modeling, just and anomaly in the light intensity showing there's obviously a mirror or gold foil thermal insulation or something down there.

    Starting Score:    1  point
    Moderation   +2  
       Interesting=2, Total=2
    Extra 'Interesting' Modifier   0  
    Karma-Bonus Modifier   +1  

    Total Score:   4