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keermalec
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Hi, I really am not knowledgeable on the matter but one big criticism of BB which one often hears and is talked about on this thread is the question of Dark Matter.<br /><br />Now it seems to me DM could be simply accounted for by the following three groups of cosmic bodies:<br /><br />1. Dead stars<br />2. Bodies insufficiently massive to become stars<br />3. Stars insufficiently bright to be visible at such long distances<br /><br /><br />1. "Dead" stars<br />--------------------<br />Doesn't the BB theory imply that 10 billion years ago therer was a massive production of first-generation "giant" stars? We know that giant stars die quickly, and form black holes. Can't this massive population of black holes form a significant portion of the Dark Matter which we can't observe but who's gravitational effect is established?<br /><br /><br />2. Low-mass objects<br />--------------------------<br />If stars form the same way planetoids accrete in a protostellar disk (as i believe has been modelled), then the mass of small objects outweighs the mass of large objects. Therefore there should be more "dark" matter than "bright" matter.<br /><br /><br />3. Dim stars<br />---------------<br />I can't help but notice in common star charts, that the further away from Earth one goes, the less one finds dim stars. Isn't this simply because we can't see them?<br /> <br /><br />Have these three populations been quantified at all?<br /><br />My impression is there is no need to "invent" a "Dark Matter" with special physical characteristics to explain why visible stars do not account for gravitational effects observed. I do realise this is only a part of the discussion above but I believe it is an important point. <div class="Discussion_UserSignature"> <p><em>“An error does not become a mistake until you refuse to correct it.” John F. Kennedy</em></p> </div>