zanket
03-07-03, 06:59 AM
I’m trying to better understand the dark matter issue and have a question.
I don’t understand this picture from this site (http://www.owlnet.rice.edu/~spac250/elio/spac.html):
http://www.owlnet.rice.edu/~spac250/elio/expected
Doesn’t the chart assume there’s negligible mass beyond the central bulge? If the mass beyond the bulge instead dropped off percentage-wise as the radius increased, wouldn’t the chart flatline as in the following actual rotation curve (from here ( http://astron.berkeley.edu/~mwhite/darkmatter/rotcurve.html)) at R = 10?:
http://astron.berkeley.edu/~mwhite/darkmatter/rotation.gif
In a spreadsheet I forced the mass to fit each point in the actual rotation curve above. A plot of the mass showed nothing unusual. It was nearly linear with respect to the radius, meaning that it drops off percentage-wise as the radius increases. So why invoke dark matter to explain the actual rotation curve above, when we can just invoke a slightly different mass distribution than we visually see?
(One of the best sites about dark matter I’ve found is this one ( http://www.astro.queensu.ca/~dursi/dm-tutorial/dm0.html), which has some excellent educational applets like here ( http://www.astro.queensu.ca/~dursi/dm-tutorial/rot-vel.html) about rotation velocity.)
I don’t understand this picture from this site (http://www.owlnet.rice.edu/~spac250/elio/spac.html):
http://www.owlnet.rice.edu/~spac250/elio/expected
Doesn’t the chart assume there’s negligible mass beyond the central bulge? If the mass beyond the bulge instead dropped off percentage-wise as the radius increased, wouldn’t the chart flatline as in the following actual rotation curve (from here ( http://astron.berkeley.edu/~mwhite/darkmatter/rotcurve.html)) at R = 10?:
http://astron.berkeley.edu/~mwhite/darkmatter/rotation.gif
In a spreadsheet I forced the mass to fit each point in the actual rotation curve above. A plot of the mass showed nothing unusual. It was nearly linear with respect to the radius, meaning that it drops off percentage-wise as the radius increases. So why invoke dark matter to explain the actual rotation curve above, when we can just invoke a slightly different mass distribution than we visually see?
(One of the best sites about dark matter I’ve found is this one ( http://www.astro.queensu.ca/~dursi/dm-tutorial/dm0.html), which has some excellent educational applets like here ( http://www.astro.queensu.ca/~dursi/dm-tutorial/rot-vel.html) about rotation velocity.)