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Summary of Galaxies and Milky Way

Science

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Galaxies and Milky Way

Goals

1. Understand what galaxies are and identify their key characteristics.

2. Learn about the Milky Way and distinguish it from other galaxies.

3. Introduce the different types of galaxies: spiral, elliptical, and irregular.

Contextualization

Galaxies are enormous assemblies of stars, planets, dust, and gas, all held together by gravity. Our very own galaxy, the Milky Way, is just one of the countless galaxies in the universe. By exploring the structure and diversity of galaxies, we can gain insight into our position in the cosmos and how the universe has evolved. For example, studying the Milky Way can provide valuable information about star formation and the distribution of dark matter. Moreover, knowledge about galaxies is essential for advancing technologies in astronomy and space exploration, including developing more sophisticated telescopes and upcoming space missions.

Subject Relevance

To Remember!

Definition of Galaxies

Galaxies are vast clusters of stars, planets, dust, and gas, bound together by gravity. They come in various sizes, shapes, and compositions. It's estimated that billions of galaxies exist, each housing billions of stars.

  • Galaxies fall into three main categories: spiral, elliptical, and irregular.

  • Each galaxy features a supermassive black hole at its core.

  • The Milky Way is the galaxy that contains our Solar System.

Types of Galaxies

Galaxies are generally categorized into three types: spiral, elliptical, and irregular. Each type has unique characteristics that affect its shape, composition, and how it evolves.

  • Spiral Galaxies: Feature spiral arms that radiate from a central core, with the Milky Way and Andromeda as prime examples.

  • Elliptical Galaxies: Have an oval shape and mainly consist of older stars. They typically contain little gas and dust, resulting in minimal new star formation.

  • Irregular Galaxies: Don't have a defined shape, often due to gravitational interactions with nearby galaxies.

Characteristics of the Milky Way

The Milky Way is a barred spiral galaxy that spans about 100,000 light-years in diameter. It is estimated to contain between 100 and 400 billion stars and has a supermassive black hole at its centre, known as Sagittarius A*.

  • The Milky Way features a spiral structure with at least four prominent arms.

  • Our Solar System resides in the Orion Arm, roughly 27,000 light-years from the galactic center.

  • This galaxy is composed of several regions, including the central bulge, the galactic disk, and the halo.

Practical Applications

  • Space Telescopes: The exploration of galaxies has led to space telescopes like Hubble, which provide intricate images and data about the structure and composition of galaxies.

  • Space Missions: Organizations such as NASA and ESA leverage knowledge about galaxies to plan ambitious space exploration missions and investigate phenomena like black holes and dark matter.

  • Observation Technology: Insights into galaxies guide the development of new technologies for astronomical observation, including high-resolution sensors and software for analyzing astronomical data.

Key Terms

  • Galaxy: A large cluster of stars, planets, dust, and gas held together by gravity.

  • Milky Way: The barred spiral galaxy that contains our Solar System.

  • Spiral Galaxy: A galaxy characterized by spiral arms that extend from a central core.

  • Elliptical Galaxy: A galaxy shaped like an ellipse, primarily composed of older stars.

  • Irregular Galaxy: A galaxy that doesn't have a well-defined shape and often arises from gravitational interactions.

  • Supermassive Black Hole: An object of extremely massive density found at the center of galaxies, including our Milky Way.

Questions for Reflections

  • How may our understanding of galaxies impact the development of new technologies and scientific discoveries?

  • In what ways can knowledge of the Milky Way enhance our understanding of the universe's formation and evolution?

  • What are the key distinctions between the various types of galaxies, and how might these differences shape our understanding of the universe?

Create a Galaxy Model

Construct a model representing one of the galaxy types studied (spiral, elliptical, or irregular) using readily available materials.

Instructions

  • Form groups of 3 to 4 students.

  • Select a galaxy type (spiral, elliptical, or irregular) to model.

  • Research visuals and information related to the chosen galaxy type for reference.

  • Use paper, glue, paint, glitter, scissors, and brushes to create the model.

  • Draw and colour the base of the galaxy on paper, using suitable colours and shapes.

  • Incorporate glitter to symbolize stars and other luminous components.

  • Present the completed model to the class, explaining the features of the galaxy represented.

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