The value of the Hubble constant plays a crucial role in cosmology in calculating the age of the universe. The most direct way to obtain it is to measure the distances to stars and galaxies and galaxy clusters and map them against their speeds. The Hubble-Lemaitre law of cosmic expansion predicts that the resulting data should lie on a straight line and from the slope of that line one gets the value of the constant. But while obtaining the speeds of each stellar object is relatively easy using the red shift of light, measuring distances is a very tedious and painstaking business in which one has to use a ‘ladder method’ involving different techniques, starting with finding the distances to the objects closest to you and using those results to find the distances to the next distance set, often using a different method, and so on. This technique is highly prone to systematic errors because any error at any stage gets magnified as you go to more distant elements. The people who do this kind of work have to pay extremely close attention to detail and I salute them for their diligence.
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