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mikeemmert
Guest
Here's an interesting paper on using Olber's paradox to determine the total mass of objects in the Kuiper belt:<br /><br />http://tinyurl.com/an9px<br /><br />It's kind of technical. Basically, Olber's paradox states that if the universe is infinite, then there would be an infinite number of stars, therefore the entire surface of the sky would be solid starlight and the Earth's surface would quickly rise to the temperature of the average star (~4000 - 5000 degrees K.).<br /><br />This idea was around for centuries until Edwin Hubble determined that distant stars were receding from us, thus redshifting average starlight to the microwave background (1.9 mm wavelength, 2.725 degrees K).<br /><br />Scott Kenyon and Rogier Windhorst concieved of the idea of photographing a patch of the Kuiper belt and measuring the light and heat coming from the <font color="yellow">entire frame <font color="white">to determine the amount of radiation coming from the small objects in the Kuiper belt.<br /><br />Particles smaller than 1 micron have been blown away by the solar wind and the pressure of sunlight. The Poynting-Robertson effect has removed particle up to 100 microns in size by the opposite effect - the particle plows into solar radiation and spirals into the sun. So what they were trying to do was to measure the total radiation from all objects from 100 microns on up to the largest objects.<br /><br />Because of the square-cube law, the total surface area of xillions (x-illion = a large, poorly defined number) of small particles is much larger than the surface area of a single large object, even if their total mass is much smaller. If it so happened that a large object was in the frame, it would only take up a few pixels, whereas each pixel in the entire frame would have the sum of the light of xillions of particles.<br /><br />This and similar papers have been used for the estimate of the total mass of the Kuiper belt. However, I have</font></font>