Stars, Galaxies, and the Universe Section 3 Section3: Star Groups Preview Objectives Constellations Multiple-Star Systems Star Clusters Galaxies Contents.

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Presentation transcript:

Stars, Galaxies, and the Universe Section 3 Section3: Star Groups Preview Objectives Constellations Multiple-Star Systems Star Clusters Galaxies Contents of Galaxies The Milky way Quasars

Stars, Galaxies, and the Universe Section 3 Objectives Describe the characteristics that identify a constellation. Describe the three main types of galaxies. Explain how a quasar differs from a typical galaxy.

Stars, Galaxies, and the Universe Section 3 Constellations Dividing Up the Sky constellation one of 88 regions into which the sky has been divided in order to describe the locations of celestial objects; a group of stars organized in a recognizable pattern In 1930, astronomers around the world agreed upon a standard set of 88 constellations. You can use a map of the constellations to locate a particular star.

Stars, Galaxies, and the Universe Section 3 Constellations, continued Naming Constellations Many of the modern names we use for the constellations come from Latin. Some constellations are named for real or imaginary animals, such as Ursa Major (the great bear) or ancient gods or legendary heroes, such as Hercules or Orion.

Stars, Galaxies, and the Universe Section 3 Constellations, continued The Constellation Orion

Stars, Galaxies, and the Universe Section 3 Multiple-Star Systems Over half of all observed stars form multiple-star systems. Binary stars are pairs of stars that revolve around each other and are held together by gravity. The center of mass, or barycenter, is somewhere between the two stars. In star systems that have more than two stars, two stars may revolve rapidly around a common barycenter, while a third star revolves more slowly at a greater distance from the pair.

Stars, Galaxies, and the Universe Section 3 Multiple-Star Systems, continued Reading Check What percentage of stars are in multiple-star systems? More than 50% of all stars are in multiple-star systems.

Stars, Galaxies, and the Universe Section 3 Star Clusters Sometimes, nebulas collapse to form groups of hundreds or thousands of stars called clusters. Globular clusters have a spherical shape and can contain up to 100,000 stars. An open cluster is loosely shaped and rarely contains more than a few hundred stars.

Stars, Galaxies, and the Universe Section 3 Galaxies galaxy a collection of stars, dust, and gas bound together by gravity Galaxies are the major building blocks of the universe. Astronomers estimate that the universe contains hundreds of billions of galaxies. A typical galaxy, such as the Milky Way, has a diameter of about 100,000 light-years and may contain more than 200 billion stars.

Stars, Galaxies, and the Universe Section 3 Galaxies, continued Distances to Galaxies Giant stars called Cepheid variables brighten and fade in a regular pattern. Most Cepheids have regular cycles. The longer the cycle, the brighter the star’s absolute magnitude. Scientists compare the Cepheid’s absolute magnitude and the Cepheid’s apparent magnitude to calculate the distance to the Cepheid variable. This distance tells scientists the distance to the galaxy in which the Cepheid is located.

Stars, Galaxies, and the Universe Section 3 Galaxies, continued Types of Galaxies Galaxies are classified by shape into three main types. A spiral galaxy has a nucleus of bright stars and flattened arms that spiral around the nucleus. Elliptical galaxies have various shapes and are extremely bright in the center and do not have spiral arms. An irregular galaxy has no particular shape, and is fairly rich in dust and gas.

Stars, Galaxies, and the Universe Section 3 Contents of Galaxies

Stars, Galaxies, and the Universe Section 3 The Milky Way The galaxy in which we live, the Milky Way, is a spiral galaxy in which the sun is one of hundreds of billions of stars. Two irregular galaxies, the Large Magellanic Cloud and Small Magellanic Cloud, are our closest neighbors. These three galaxies are called the Local Group.

Stars, Galaxies, and the Universe Section 3 Quasars quasar quasi-stellar radio source; a very luminous object that produces energy at a high rate. Quasars appear as points of light, similar to stars. Quasars are located in the centers of galaxies that are distant from Earth. Quasars are among the most distant objects that have been observed from Earth.