Toggle navigation
Pre-K
Kindergarten
1st Grade
2nd Grade
3rd Grade
4th Grade
5th Grade
Middle School
High School
Phonics
Fun Games
Math
Math Games
Math Worksheets
Algebra
Language Arts
Science
Social Studies
Literature
Languages
Themes
Quizzes
Timelines
Login
Home
>
Quizzes
>
Physics Quizzes
> Astronomy : Lives of Stars (I) Quiz
Astronomy : Lives of Stars (I) Quiz
Quiz
*Theme/Title:
Lives of Stars (I)
* Description/Instructions
Clouds of hydrogen gas, dust, ice and molecules exist in space. Over time, the cloud becomes dense by attracting neighboring particles. This increases the mass and gravity of the cloud. This is called a protostar. Density of the protostar increases as more gas, dust and ice are attracted to the cloud and matter begins to compress until the pressure and temperature rises. When the central temperature of the protostar reaches ten million Kelvin, the hydrogen nuclei begin to fuse to produce helium. This is a thermonuclear reaction and a star is born. The star is unstable until the internal pressure equals the outer pressure.
Larger stars burn faster than smaller stars and are very bright. When hydrogen fusion in the star’s center ceases, then helium nuclei begin to fuse. The temperature increases and the star swells in size and becomes a red giant. When helium fusion stops and the internal and external pressures are no longer equal, the outer layers of the red giant are cast off to form a planetary nebula, such as the Crab Nebula in the constellation Taurus. The shrunken remnant is called a white dwarf. Slowly, the white dwarf cools to become a black dwarf. This is the life cycle of stars that are the same size as or smaller than our sun.
This quiz covers the life cycle of stars. Use the above information to assist in answering the questions. Read the description and identify the best answer from the choices.
Group:
Physics
Physics Quizzes
Topic:
Astronomy
Share
All Quizzes
To link to this page, copy the following code to your site:
Lives of Stars (I)