Astronomy

Essential Knowledge and Skills Related SOL
Students should be able to:  
Recognize that the Big Bang Theory states that the universe began as a dense sphere that expanded and eventually condensed into galaxies.

ES.14 e
ES.1e

Recognize that the solar nebular theory explains that the planets formed through condensing of the solar nebula.

ES.14 e
ES.2 a, b, c, d

Discuss the evidence for the origin of the universe and origin of the solar system respectively.

ES.14 a
ES.2 a, b, c, d

Understand that

  • stars have a finite lifetime and evolve over time;
  • the mass of a star controls its evolution, length of its lifetime, and ultimate fate, as shown by the Hertsprung-Russell diagram;
  • stars form by condensation of interstellar gas;
  • galaxies are collections of large numbers (billions) of stars.

ES.14 b, c

Identify the basic types of galaxies as spiral, elliptical, and irregular.

ES.14 d

Identify the basic types of galaxies as spiral, elliptical, and irregular.

ES.14 b

Define a light year as the distance light travels in one year. It is the most commonly used measurement for distance in astronomy

ES.14 d

Identify and classify the following celestial bodies in the Milky Way Galaxy (sun, planets and their moons, comets, meteors, and asteroids).

ES.14 a, b, c, d, e
ES.4 a, c

Describe the sun as a star that consists largely of hydrogen gas. Its energy comes from nuclear fusion of hydrogen to helium.

ES.14 b, c

Recognize that

  • the Earth is the third planet from the sun;
  • the four inner (terrestrial) planets consist mostly of solid rock;
  • four of the outer planets are gas giants, consisting of thick outer layers of gaseous materials, perhaps with a small rocky core;
  • the fifth outer planet, Pluto, has an unknown composition, and appears solid.


ES.14 a
ES.4 c

Draw a diagram of the solar system and label the planets.

ES.4 c, d

Name the characteristics of celestial bodies:

  • Moons are natural satellites of planets that vary widely in composition.
  • Comets orbit the sun and consist mostly of frozen gases.
  • Asteroids are rocky or metallic iron objects ranging in size from millimeters to kilometers. They are the source of most meteorites.

ES.4 c, d

Recognize the following ways the Earth’s atmosphere has changed due to human, biologic, or geological activity:

  • Human activities have increased the carbon dioxide content of the atmosphere.
  • Man-made chemicals have decreased the ozone concentration in the upper atmosphere.
  • Volcanic activity and meteorite impacts can inject large quantities of dust and gases into the atmosphere.

ES.12 d, e

Compare the Earth’s atmosphere to that of

  • the atmosphere of Venus, which is mostly carbon dioxide and very dense;
  • the atmosphere of Mars, which is very thin and mostly carbon dioxide.

ES.4 c

Relate that much of our knowledge about the solar system is a result of space exploration efforts. These efforts continue to improve our understanding of the solar system.

ES.4 d

Summarize important space research information, including

  • much of our information about our galaxy and the universe comes from ground-based observations as well as information derived from utilizing the electromagnetic spectrum;
  • the Hubble Space telescope has greatly improved our understanding of the universe;
  • Apollo 11 was the first manned landing on the moon.

ES.4 d


Sample Classroom Assessment Methods

  • Lab practical on interpreting Hertzsprung-Russell Diagram
  • Student generated scale models on planetary size and distance
  • Quizzes
  • Unit tests

Sample Resources

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