Spiral Galaxies: 3 Distinguishing Characteristics

  • Context: High School 
  • Thread starter Thread starter zcapa14
  • Start date Start date
  • Tags Tags
    Spiral
Click For Summary

Discussion Overview

The discussion centers on identifying three distinguishing characteristics that can differ among spiral galaxies. Participants explore various aspects related to their structure, classification, and observable properties.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested

Main Points Raised

  • Some participants suggest that the arms of spiral galaxies are a distinguishing feature.
  • Others propose that the disklike structure, central bulge, and arms are key characteristics.
  • One participant describes the Hubble classification scheme, noting the distinction between regular and barred spirals and the importance of arm tightness.
  • Another participant lists several characteristics that differentiate spiral galaxies from elliptical ones, including organized rotation, presence of gas and dust, active star formation, and the existence of spiral arms.
  • Variations among spiral galaxies include the size of the bulge, presence of bars, number of spiral arms, continuity of the arms, wrapping angle, and overall color indicating star formation levels.
  • Measurement of rotation curves and ellipticities is mentioned as a method for further classification.

Areas of Agreement / Disagreement

Participants express multiple competing views on the distinguishing characteristics of spiral galaxies, and the discussion remains unresolved regarding which specific characteristics are most significant.

Contextual Notes

Some claims depend on specific classification systems, and there are unresolved aspects regarding the criteria used for distinguishing features among spiral galaxies.

zcapa14
Messages
4
Reaction score
0
What are three distinguishing characteristics that can differ among spiral galaxies?
 
Astronomy news on Phys.org
the arms? i think is one.
 
i would guess that its disklike structure, with the buldge at the center, and arms .
 
The best know classification scheme is the Hubble system. It establishes two basic types - regular and barred - and three subclasses of each type based on how tightly the arms are wrapped. The de Vaucouleurs classification system is a more detailed version of the Hubble scheme which profiles spirals 3 dimensionally. The DDO, or van den Bergh scheme factors luminosity into the mix and the Yerkes, or Morgan system factors in the integrated spectrum. For an overview see:
http://www.astro.ufl.edu/~vicki/Lecture2.pdf .
Of course there are other systems at well, but these are the most widely used.
 
Last edited by a moderator:
Welcome to Physics Forums zcapa14!

Just a friendly word of advice - please read the guidelines (and note that duplicate posts are not welcome here).
 
zcapa14 said:
What are three distinguishing characteristics that can differ among spiral galaxies?

If you mean things that distinguish them from ellipticals, then there are a lot:

1. They have disks with organized rotation.
2. They have a lot of gas and dust.
3. They have active star formation.
4. They're bluer (consequence of #3).
5. They can have spiral arms (density waves).
6. They're more common outside of clusters.
7. They sometimes have bulges.
8. They sometimes have bars.

From one spiral to another, the following things are known to vary and can be used to classify them:

1. The size of the bulge.
2. Whether or not there's a bar.
3. The number of spiral arms.
4. The continuity of the spiral arms.
5. The angle about which the arms wrap.
6. How blue they are (rough measure of amount of star formation)
7. Amount of gas and dust.

There are other things, but those can all be visually apparent. You can also measure rotation curves, ellipticities, etc.
 

Similar threads

  • · Replies 2 ·
Replies
2
Views
6K
  • · Replies 4 ·
Replies
4
Views
2K
  • · Replies 17 ·
Replies
17
Views
2K
Replies
3
Views
2K
Replies
3
Views
2K
  • · Replies 2 ·
Replies
2
Views
2K
  • · Replies 10 ·
Replies
10
Views
5K
  • · Replies 25 ·
Replies
25
Views
4K
  • · Replies 1 ·
Replies
1
Views
2K
  • · Replies 5 ·
Replies
5
Views
2K