askvity

What is meant by spiral galaxy?

Published in Galaxies 2 mins read

A spiral galaxy is a type of galaxy characterized by a rotating disc with spiral arms that extend outward from a dense central region.

Understanding Spiral Galaxies

Spiral galaxies are a visually captivating class of galaxies, distinguished by their unique structure and dynamics.

Key Features

  • Rotating Disc: A fundamental characteristic of spiral galaxies is their rotating, flattened disc. This disc is where most of the galaxy's stars, gas, and dust reside.
  • Spiral Arms: These arms are prominent features that curve out from the galaxy's center. They are regions of intense star formation, making them appear brighter than other parts of the galaxy.
  • Dense Central Region: Spiral galaxies usually have a concentrated region in the center, known as the bulge, which is composed of older stars.
  • Examples: Our own galaxy, the Milky Way, is a classic example of a spiral galaxy.

Classification of Galaxies

Spiral galaxies fall under one of the four main categories of galaxies:

Category Description
Spiral Characterized by a rotating disc with spiral arms extending from a central bulge.
Barred Spiral A type of spiral galaxy where the spiral arms originate from a bar-shaped structure in the center.
Elliptical Smooth, oval-shaped galaxies with little to no star formation.
Irregular Galaxies that do not fit into the other categories due to their lack of defined shapes and structures.

Visual Characteristics

  • The spiral arms are not static; they are density waves moving through the galaxy's disc, triggering star formation.
  • Younger, hotter, and bluer stars reside in the spiral arms, while older, redder stars are primarily in the bulge and halo.
  • The central bulge is often considered a mini galaxy within the larger spiral galaxy, having a different population of stars.

Summary

In essence, a spiral galaxy is a galaxy with a central bulge surrounded by a rotating disc featuring prominent spiral arms, like our own Milky Way. These arms are regions of active star formation, making spiral galaxies dynamic and visually striking astronomical objects.

Related Articles