Is the Milky Way a Resonance-Ring Galaxy?

In summary: Morgan and his collaborators showed that our Galaxy has two major spiral arms, rather symmetrically arranged, and a number of shorter, fainter arms." (Source...)So while there is a considerable amount of evidence to support the theory that the Milky Way is a spiral galaxy, it is ultimately just a theory based on observations and our understanding of galactic structures. It is possible that our understanding may change or be refined in the future as we gather more data and make new observations.
  • #1
vincentm
323
3
I hope this is the right section. But, can anyone here tell me how is it that we know the our galaxy is a spiral one, i don't doubt what I've read, but i need an explanation. I read something about density waves and how they power the rotation of our galaxy andor other galaxies. But how do we know for sure ours is a spiral body?
 
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  • #2
if I am not misstagen spiral is the most common form of a galaxy. so by that we can tell its more likly it is. but then we can't be sure. so if we take a look at stars where they are how far it is and place them in a computer we would be able to see that they form a spiral and can by that draw the conclution that the galaxy is a spiral.
 
  • #3
Initially, our knowledge about galactic structure came primarily from observing other galaxies, since dust obscured all but a small fraction of our own. From such observations, we determined that there were two basic types of large galaxies: spirals and ellipticals. Since these two types were qualitatively very different, it was a rather simple matter to infer that our galaxy was a spiral. Evidence included:

- A disk. Just look at the sky on any clear night and you'll see a band of stars stretching across the sky. This is the Milky Way disk. Ellipticals don't have a large stellar disk like that.
- Young stars. We observe young, blue stars in the Milky Way, just as we do in many spirals. Ellipticals, on the other hand, tend to have old, red populations.
- Gas. Ellipticals generally have very little gas, while we have been observing neutral and ionized gas in the Milky Way for many years now.

Those are just the obvious qualities. Since then, a much more detailed analysis has been done and we've found spiral arms, a bar, and a multi-disk structure.


I read something about density waves and how they power the rotation of our galaxy andor other galaxies.

The rotation of the galaxy doesn't need power because there is very little dissipation. It just comes from the initial angular momentum of the matter that collapsed to form the galaxy. The spiral arms are just, as you say, density waves that form as a result of instabilities in the disk. They have been known to initiate star formation, so perhaps that's what you're thinking of.
 
  • #4
Zelos said:
if I am not misstagen spiral is the most common form of a galaxy.

The most numerous type of galaxy is most likely the dwarf spheroidal galaxy (not much bigger than a globular cluster), but it's hard to tell because we can't see them beyond the local group. Of the large galaxies, spirals are more numerous overall, but it depends on where you're looking. Outside of galaxy clusters, spirals are more common, but inside them you will find many more ellipticals.
 
  • #5
vincentm said:
But, can anyone here tell me how is it that we know the our galaxy is a spiral one?
As well as the optical evidence as to the nature of our galaxy that SpaceTiger has described the most direct evidence is the mapping by radio astronomy of HI regions at 21cm wavelength, and now IR astronomy, both of which can 'see through' the dust in the galactic disc. The map clearly showed spiral arms, but quite close together. We now know the Milky Way is a Barred Spiral with a small bar across the centre from which a close formation of arms spiral out. A SBa type of galaxy, quite 'special'!

Garth
 
  • #6
Garth said:
We now know the Milky Way is a Barred Spiral with a small bar across the centre from which a close formation of arms spiral out. A SBa type of galaxy, quite 'special'!
See http://www.sciam.com/article.cfm?chanID=sa003&articleID=000EC3D4-5193-1302-919383414B7F0000.
Garth
 
  • #7
I did a little research on my own and found quite a few Milky Way bars at the local supermarket.
 
  • #8
Garth said:
See http://www.sciam.com/article.cfm?chanID=sa003&articleID=000EC3D4-5193-1302-919383414B7F0000.
Garth
and here.

Garth
 
  • #10
  • #11
Garth said:
That WAS my link! (big version) :biggrin:
Garth
Right you are. I was thinking about deleting my post, but I decided it's good to have a link to the apod page with the brief explanation written by a professional astronomer. :wink:
 
  • #12
jimmysnyder said:
Right you are. I was thinking about deleting my post, but I decided it's good to have a link to the apod page with the brief explanation written by a professional astronomer. :wink:
And quite right too!
Garth
 
  • #13
vincentm said:
I hope this is the right section. But, can anyone here tell me how is it that we know the our galaxy is a spiral one, i don't doubt what I've read, but i need an explanation. I read something about density waves and how they power the rotation of our galaxy andor other galaxies. But how do we know for sure ours is a spiral body?



It was William Parsons (3rd Earl of Rosse) that first observed spiral structure in some "nebulae".

Many people over the ensuing years speculated that the Milky Way had spiral arms too.

However, it was not until 1951 that the first scientific evidence was presented. In the 1940s Walter Baade recognized that in (other) spiral galaxies, the older, redder, stars tended to reside in the central regions (of the galaxy) while younger (blue-white) stars are to be found in the spiral arms, along with HII regions.

In 1951 at Yerkes Observatory, William Morgan, along with Donald Osterbrock and Stewart Sharpless, determined the distances to many (dozens) of blue giants and HII regions "close" to our solar system. This enabled them to map segments of a few of MW spiral arms for the first time.


"Morgan announced these findings at a 1951 meeting of the AAS, presenting a model of the spiral arms that used cotton balls to depict the positions of the luminous nebuluae. The results were greeted with a rare, emotional ovation that included clapping of hands and stomping of feet"
(page 434 of "Archives of the Universe", by Bartusiak)

The results were published in the article:

"Some features of Galactic Structure in the Neighborhood of the Sun"
The Astrophysical Journal, Volume 57 (1952). By Morgan, Sharpless, & Osterbrock.

Radio observations soon advanced our knowledge of the MW spiral structure (particularly the early ones by Oort, Muller, and van de Hulst).
 
  • #14
I was reading in http://www.solstation.com/x-objects/gal-ring.htm that some barred galaxies have outer rings which might be a result of a resonance with the dynamics of the bar. These galaxies have an own name "resonace-ring galaxies". It seams that the Milky Way contains such a structure (see link above), so may be the Milky Way should be classified as a resonace-ring galaxy?
 

1. What is the structure of the Milky Way?

The Milky Way is a spiral galaxy, meaning it has a distinct spiral shape with arms that radiate out from the center.

2. How do we know that the Milky Way is a spiral galaxy?

Scientists have used telescopes and other instruments to observe the shape and structure of the Milky Way. They have also studied the movement and distribution of stars and gas within the galaxy to confirm its spiral structure.

3. How many arms does the Milky Way have?

The exact number of arms in the Milky Way is a matter of debate among scientists. Some believe there are two major arms, while others suggest there may be four or more arms.

4. How does the spiral shape of the Milky Way form?

The spiral shape of the Milky Way is formed by the rotation of the galaxy. As the stars and gas within the galaxy rotate, they are pulled outwards by centrifugal force, creating the spiral arms.

5. What is the significance of the Milky Way being a spiral galaxy?

The spiral shape of the Milky Way allows for the formation and stability of stars and planets. The spiral arms also serve as regions of high gas and dust density, where new stars can form. Additionally, the spiral structure allows for efficient mixing of gas and other materials throughout the galaxy, aiding in the evolution of the Milky Way.

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