"There is always a heavy demand for fresh mediocrity. In every generation the least cultivated taste has the largest appetite." -Paul Gauguin
From our vantage point within the Milky Way, it sure does appear impressive. Hundreds of billions of stars shine in our own cosmic backyard, with our galaxy spanning a whopping 100,000 light years from end-to-end. Yet not only is that small compared to our nearest large neighbor, Andromeda, but it’s not even 20% as large as the largest spiral galaxies we find.
While tidal disruption might create the largest spiral galaxies, we have giant ellipticals that are many times larger than a spiral will ever achieve. Some of the biggest ones of all are found at the centers of massive galaxy clusters, but in the scheme of the entire observable Universe, only one galaxy can truly be the largest.
Which is it, and how do we know? Find out on this edition of Mostly Mute Monday!
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I make the volume of IC1011 on the order of 10^20 ly^3 (assuming triaxial ellipsoid with axes in the proportion 1:0.75:0.6, which seems about right for the more common shapes of elliptical galaxies). The Milky Way's volume is on the order of 10^13 ly^3. But there are only about 1000 times more stars in IC1011... what gives, are these giant ellipticals especially sparse? My numbers suggest a star density of only 1/10000th the milky way's--for every 10,000 stars in our night sky, extinguish all but one of them. Is this really what we'd expect to find in IC1011? (I know this is an oversimplification, because density is greater near the middle of a galaxy, but maybe the orders of magnitude aren't too far off?)
Hi Ethan. Quick question. The Standard Model doesn't seem to prohibit a Universe of age 1 Trillion years (72 of ours stacked together). At a quintillion maybe proton decay might have an effect ... but so what. Is the 13.8 GY age of the Universe simply stochastic?
thanks -- doug watts.