<p><BR/>Replying to:<BR/><DIV CLASS='Discussion_PostQuote'>The evidence would seem to bear that out. IMO the missing mass/dark matter is contained in the physical infrastructure of each and every solar system.</DIV></p><p>This statement is not inaccurate. However, it is not entirely complete. These findings are not concerned about scales at the level of stellar systems. They are not even realy concerned with the galactic scale. This is more about the overdense regions referred to as galactic clusters and the intracluster medium and the associated dark matter with these overdense regions. </p><p>Have you actually read the papers, or are you just throwing out your uninformed opinion. </p><p> Replying to:<BR/><DIV CLASS='Discussion_PostQuote'>I think that's a bad "assumption". The intergalacitic material does seem to "interact" during these collisoins, but the vast majority of mass seems to "pass on through" the collision process.</DIV></p><p>Exactly!!! How can it be a bad assumption when you just repeated,<strong><em> precisely</em></strong>, what is going on in these collisions? </p><p>Replying to:<BR/><DIV CLASS='Discussion_PostQuote'>By *assuming* that most baryonic matter is in the plsamas between the stars, you may be setting yourself up here.</DIV></p><p>It's not <em><strong>my</strong></em> assumption. Not to mention that you don't understand what the 'assumption' is. It has little to nothing to do with the interstellar medium. </p><p>Replying to:<BR/><DIV CLASS='Discussion_PostQuote'>Some of the matter surely does reside in the interstellar medium, but it's not clear to me that "most" baryonic matter reside in that medium.</DIV></p><p>Again, it's not about the interstellar medium. I doubt, during these collisions, that galaxies are even colliding... much less the interstellar medium. This is about the INTRACLUSTER MEDIUM. </p><p>Replying to:<BR/><DIV CLASS='Discussion_PostQuote'>IMO you are *assuming* something that doesn't seem to be the case based on the obsservations.</DIV></p><p>Educate yourself on what they are actualy observing and get back to me on this statement. </p><p>Replying to:<BR/><DIV CLASS='Discussion_PostQuote'>You seem to "assume" that the majority of baryonic matter is in the plasma between the stars, whereas these observations would suggest otherwise IMO.</DIV></p><p>Educate yourself on what they are actualy observing and get back to me on this statement. </p><p>Replying to:<BR/><DIV CLASS='Discussion_PostQuote'>Most of the mass seems to "pass on through" these colllision events.</DIV></p><p>Agreed. </p><p>Replying to:<BR/><DIV CLASS='Discussion_PostQuote'>That makes sense if "most" of the baryonic matter is contained in the solar system infrastructures of each galaxy.</DIV></p><p>I understand what you are alluding to. However, this has nothing to do with what they are observing. Familiarize yourself with it an you might understand. First, it is highly unlikely that the galaxies within the cluster are actually colliding. Again, this is about the intracluster medium. What they are observing is a large portion of the visible matter is being left behind as these clusters pass throug each other. Through lensing data, they measure that these two cluster have retained their mass despite leaving behind most of their visible matter. In other words, the visible matter of each cluster is really insignificant when measuring their overall mass. </p><p>Replying to:<BR/><DIV CLASS='Discussion_PostQuote'>These items would tend to "hold together" and pass on through a collision process, whereas the plasma threads between stars would tend to interact with the plasmas in the other galaxy.</DIV></p><p>Nothing to do with what is going on between stars. </p><p>Replying to:<BR/><DIV CLASS='Discussion_PostQuote'>If you don't *assume* that most of the baryonic matter resides in the interstellar medium, then it's likely that most of the mass of each galaxy would be relatively uneffected by the collision.</DIV></p><p>Nothing to do with what is going on between starts. </p><p>Replying to:<BR/><DIV CLASS='Discussion_PostQuote'>IMO these studies do suggest that we "missed something", and we underestimate the mass of galaxies.</DIV></p><p>This has nothing to do with individual galaxies, so you should say "IM uniformed O". </p><p>Replying to:<BR/><DIV CLASS='Discussion_PostQuote'>That "something" we missed IMO is the fact that most of the matter in all galaxies resides in the solar system infrastructure, not in the plasmas between the stars.</DIV></p><p>Another uninformed opinion. </p><p>Replying to:<BR/><DIV CLASS='Discussion_PostQuote'>IMO that's the key here to understanding these observations, not the introduction of new forms of non bayonic matter. <br /> Posted by michaelmozina</DIV></p><p>Folks have tried. MOND and TeVeS have put forth a yeoman-like effort to explain this. However, they have come up short. They still have their foot in the door and may still have something to contribute, but it's not looking good. The difference between the MOND folks and you is that the MOND folks actually understand what it is they are trying compete with.</p><p>Nothing wrong with thinking outside the box. However, it is highly recommended to understand what is going on *inside* first. </p> <div class="Discussion_UserSignature"> <div> </div><br /><div><span style="color:#0000ff" class="Apple-style-span">"If something's hard to do, then it's not worth doing." - Homer Simpson</span></div> </div>