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2012 Annual Report - Jesus College - University of Cambridge

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18 ASTROPHYSICS I <strong>Jesus</strong> <strong>College</strong> <strong>Annual</strong> <strong>Report</strong> <strong>2012</strong><br />

This high-resolution image <strong>of</strong> the Hubble Ultra-Deep Field includes galaxies <strong>of</strong> various ages, sizes, shapes and colours. The smallest,<br />

reddest galaxies, <strong>of</strong> which there are approximately 10,000, are some <strong>of</strong> the most distant galaxies to have been imaged by an optical<br />

telescope, probably existing shortly after the Big Bang<br />

We cannot follow the exact orbits <strong>of</strong> many individual galaxies very well. But we can modify<br />

the statistical description to try to answer a range <strong>of</strong> questions important for our<br />

understanding.<br />

For example, we can ask if the presence <strong>of</strong> a galaxy in any particular volume <strong>of</strong> space<br />

increases the probability that there is another galaxy nearby. Since galaxies attract one<br />

another by gravity, the answer, unsurprisingly, is ‘yes’. What was unexpected is the detailed<br />

spatial dependence <strong>of</strong> this increased probability. It was observed only about forty years<br />

ago. So far, it has been calculated just for the case where the increased probability for<br />

gravity bringing two galaxies close to each other is relatively small. But we know that<br />

clusters form which are very dense, and the corresponding increase in the probability <strong>of</strong>

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