![]() |
|
|
Thread Tools | Display Modes |
#21
|
|||
|
|||
![]()
Astronomers tell us the stars in our galaxy are in lock step. They turn
like the spokes in a wheel. That is true of stars inside the hub. Because of the great gravity of that huge BH they have to revolve around the blackhole so very fast that the gravitation that keeps our sun in lock step with the rest of the galaxy has no effect on stars making up the hub. Not in the books but that is the way I see it. Bert |
#22
|
|||
|
|||
![]()
My post says inside the hub. It should read outside the hub,and inside
the hub ithe stars are not in lock step Bert |
#23
|
|||
|
|||
![]()
"G=EMC^2 Glazier" wrote in message
... My post says inside the hub. It should read outside the hub,and inside the hub ithe stars are not in lock step Bert It's kind of hart to tell what you mean when you use terms like "in lock step", but it sounds like you had it right (sort of) the first time. The bulge exhibits characteristics of solid-body rotation, the disk exhibits characteristics of differential rotation. |
#24
|
|||
|
|||
![]()
Zinni to Bert:
It's kind of hart to tell what you mean when you use terms like "in lock step", but it sounds like you had it right (sort of) the first time. Got a question for the gurus on non-Keplerian rotation of galaxies- In our solar system, well over 99% of the mass of the system is contained in the nucleus (the sun). And the rest of the system naturally obeys the Keplerian laws of orbital mechanics, orbiting about the massive nucleus. But in contrast to a solar system, a galaxy's nucleus (presumably a BH) does not contain the overwhelming mass of the system; rather it contains a miniscule percentage of the total mass. So the question is Why should a galaxy be expected to display Keplerian rotation? Would not a more unitary (or 'frisbee-like') rotation be expected, just as is observed? Or, is the mass of the nucleus sufficiently high that Keplerian rotation *should* be expected? oc |
#25
|
|||
|
|||
![]()
"Bill Sheppard" wrote in message
... Why should a galaxy be expected to display Keplerian rotation? Would not a more unitary (or 'frisbee-like') rotation be expected, just as is observed? Hey Bill In fact, Keplerian rotation is not expected IN THE DISK. Let me back-track for a second. There is a well known result attributable to Newton that says ... - Given a spherical shell of uniform density, its net gravitational effect on a test particle outside of the spherical shell will be exactly the same as if all of its mass were concentrated in a single point at its centre. and ... - Given a spherical shell of uniform density, its net gravitational effect on a test particle (anywhere) inside of the spherical shell will be exactly ZERO. This result also holds true for rings of uniform density and a test particle in the plane of the ring either inside or outside of it. So, if we view the galaxy as approximating a series of rings of uniform density (a good approximation for most of the disk) only the mass internal to the orbit of a test particle need be considered. As we move out from the centre of the galaxy there is more and more mass internal to the orbit to be considered. The rotation curve IN THE DISK is part way between solid-body and Keplerian. It is only once we get to the outer reaches of the galaxy, were the visible matter thins to such an extent that we would expect no appreciable change in the mass internal to the orbit of our test particle as we move out, that we expect a Keplerian rotation curve to kick in. We do not however get what we expect, the orbital velocities do not start to drop according to Kepler, thus leading to the theory of Dark Matter. |
#26
|
|||
|
|||
![]()
Hi oc The sun has 99% of all the mass of the solar system. and gravity
is a mutual attraction. Still it is hard for me to see Neptune and Pluton so far away from the sun,and staying in orbit. Then we have Mercury so close to the sun. It has to be revolving very fast as not to fall into the sun. The planets are not in lock step nor is the solar system like a solid frisbee. With the huge area of the Milky Way,and gravity getting weaker the inverse square of distance. There is no way the blackhole at the center of the hub even with a mass of2.6 million suns can keep our sun that is 26million LY away in orbit,and all the other millions,and millions of stars from leaving the galaxy and escaping into space. That is why when they add up the mass of the Milky Way astronomers tell us 95% of the mass(gravity) is missing. This holds true for all spiral galaxies(I don't know about elliptical) The term in lock step means the stars are not gaining on each other. To me it means the Big,and Little dippers will keep their shape. I hope that stays true for they are the only constellations I can find Well oc even if they find a lot of dark matter I can see a problem,for it would have to be spread out between the stars very evenly,and with the right force of gravity to accomplish what we observe. Bert |
#27
|
|||
|
|||
![]()
"G=EMC^2 Glazier" wrote in message...
... Hi Painius Just had this interesting thought. the stars that make up the hub and have a 2.6 million solar mass blackhole at their center must be revolving around it very fast. How fast is very fast? Lots of stars must be falling through the event horizon every day. Stars of great mass could be colliding(gut feeling thats true) To much stuff and angular motion in a small area can cause choas. Bert I don't think anyone really knows how fast, Bert. I *do* know that most people have some idea that stars are "thick as thieves" at the galaxy hub, but once you get there, it's like the asteroid belt. The stars are far enough apart to mean that collisions are very few and far between. I could be wrong, but i don't think the black hole grows very fast. Here's a neat article... http://www.nature.com/nsu/020107/020107-9.html ....raises LOTS of questions, doesn't it. happy days and... starry starry nights! -- Your heart up hanging on the wall Just dripping tears so painfully, You ne'er felt love so true as mine, I want your heart inside me. Protected from all manner, form And shape of harm it will e'er be, If you say no, I fade and die, I need your heart inside me. Paine Ellsworth |
#28
|
|||
|
|||
![]()
Hi Painius Thanks for that site. Seems the Milky Way hub is a very
dynamic place I like our spot in right field a lot better. Bert |
#29
|
|||
|
|||
![]()
"G=EMC^2 Glazier" wrote in message...
... Hi Painius Thanks for that site. Seems the Milky Way hub is a very dynamic place I like our spot in right field a lot better. Bert Welcome! Yes, it appears that for our form of life, i.e. carbon-based, we're all better off being the hicks of the Milky Way! Other possible bases for life might be... silicon germanium tin lead ununquadium This is just a reflection that i perceive from the periodic table of the elements. Carbon-based is probably the toughest form of life. If a carbon-based lifeform cannot live at the hub of the Galaxy, nobody can. I *could* be wrong about this. Ununquadium-based life would be a manufactured form. We're not ready for this, are we. happy days and... starry starry nights! -- a Secret of the Universe... so please don't breathe a word of this-- the Moon above will smile perverse whene'er it sees two lovers kiss; (breathe not a single word of this!) Paine Ellsworth |
#30
|
|||
|
|||
![]()
Hi Painius I have a picture(framed) taken by the Hubble of the
Cartwheel galaxy It has a bright oval shaped hub. I can see arms coming out of the hub and going to the great big ring around it. The ring seems very bright,and must have billions of stars making up its structure. It is good this Cartwheel galaxy was not seen edge on,because than it would look like a spiral galaxy. I wonder how common this shape galaxy are? Almost looks like a huge explosion could have caused the ring. Bert |
Thread Tools | |
Display Modes | |
|
|
![]() |
||||
Thread | Thread Starter | Forum | Replies | Last Post |
Glimpse at Early Universe Reveals Surprisingly Mature Galaxies (Forwarded) | Andrew Yee | Astronomy Misc | 0 | July 28th 04 01:45 AM |
Faintest Spectra Ever Raise Glaring Question: Why do Galaxies inthe Young Universe Appear so Mature? (Forwarded) | Andrew Yee | Astronomy Misc | 0 | January 5th 04 07:39 PM |
Astrophysicists Discover Massive Forming Galaxies in Young GalaxyClusters (Forwarded) | Andrew Yee | Astronomy Misc | 0 | October 26th 03 07:57 PM |
New Insight into the Cosmic Renaissance Epoch (Forwarded) | Andrew Yee | Astronomy Misc | 0 | August 21st 03 02:10 PM |
Astronomers reveal the first detailed maps of galaxy distributionin the early universe (Forwarded) | Andrew Yee | Astronomy Misc | 0 | July 18th 03 12:23 AM |