What keeps most galactic stars from falling into the centeral black hole?

  • #1
KurtLudwig
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I believe that it is mainly conservation of angular momentum that keeps galactic stars apart and from rapidly falling into a central black hole.
We know from Kepler's Second Law, that a line from a planet to the Sun sweeps an equal area in equal time. The planet's velocity increases when it orbits closer to the Sun. The area swept is a triangle 1/2 r v sin (theta) = constant, asserted by Kepler, based on observations by Tycho Brahe. (From a college physics text book by Ohanian.)

Similarly, stars in the Milky Way galaxy orbit the Andromeda black hole. Conservation of angular momentum keeps most stars from falling in. Also, Newtonian gravity rapidly decreases with distance form the central black hole.

What keeps the stars in a star cluster apart? I believe that the relative motions of the stars and their relative angular momenta keep the stars apart.

How is Modified Newtonian Dynamics involved in keeping stars together and from wandering off into space?
 
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  • #2
I agree. But it is important to realize that the significance of a black hole is not so much tremendous gravitational effects as it is having all that mass compressed into a tiny space. A black hole has no greater gravitational effect then the same amount of mass spread out would have. There can be small black holes that do not have significant gravitational effects unless you get very close. In fact, many black holes at the center of galaxies are a small percentage of the total mass of their galaxy.
 
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  • #3
KurtLudwig said:
Similarly, stars in the Milky Way galaxy orbit the Andromeda black hole.
Uh, Sagittarius A is going to be sorry to hear about this change.
 
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  • #4
phinds said:
Uh, Sagittarius A is going to be sorry to hear about this change.
Technically Sagittarius A* if we are talking the Milky Way black hole.
(Sagittarius A is a larger grouping)
 
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  • #5
Orodruin said:
Technically Sagittarius A* if we are talking the Milky Way black hole.
(Sagittarius A is a larger grouping)
Huh. I didn't realize that. I've always heard it called Sag-A-Star but thought I'd use the formal name (incorrectly it seems). Thanks for the correction.
 
  • #6
It's called Sagittarius A Star because it's not a star. Go figure.
 
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Since we're in all-out quibble mode - stars in galaxies don't follow Kepler's Law. That applies to the situation where the central mass is all there is, and an elliptical orbit among stars that make up a distributed mass is not that.

We've quibbled about the Andromeda black hole. There might (or might not) be two. M31 has an odd double-nucleus structure, which may indicate two central black holes today, two central black holes in the past, or something else. I think "something else" is today's leading candidate explanation, but consensus has shifted in the past and might continue to do so. It's behavior changes on human timescales, so we may get some new evidence that clarifies things some time.
 
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1. Why don’t all the stars in a galaxy fall into the central black hole?

Stars do not typically fall into the central black hole because they are in orbit around the black hole, much like planets orbiting the Sun. The stars have enough tangential velocity and are at a sufficient distance to maintain stable orbits, preventing them from being pulled directly into the black hole.

2. What role does angular momentum play in keeping stars from falling into the black hole?

Angular momentum is crucial in preventing stars from falling into the black hole. It is a physical quantity that represents the amount of rotation an object has in its motion around another object. Stars with sufficient angular momentum will continue orbiting the black hole instead of spiraling into it, as the conservation of angular momentum maintains their stable orbits.

3. How does the mass of the black hole affect the stability of a galaxy’s stars?

The mass of the central black hole can influence the orbits of nearby stars. More massive black holes exert a stronger gravitational pull, potentially affecting the orbits of stars and drawing them closer. However, even with a massive black hole, most stars remain stable in their orbits due to their velocity and distance from the black hole.

4. Can stars ever escape the gravitational pull of a black hole?

Yes, stars can escape the gravitational pull of a black hole under certain conditions. If a star gains additional energy, for example, from interactions with other stars or from dynamic events within the galaxy, it can achieve escape velocity and move out of the black hole’s gravitational influence.

5. What happens to a star if it gets too close to a black hole?

If a star gets too close to a black hole, it can undergo a process known as tidal disruption. The gravitational forces of the black hole can stretch and pull the star apart, often leading to a significant portion of the star’s material being accreted onto the black hole. This process can also emit intense radiation and lead to observable flares.

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