Introduction to Astronomy
Astronomy
Introduction to Astronomy
Astronomy
Literacy / Driving Question Board Connections
Nonfiction Science Literacy Resources
Graphic Organizers / Thinking Maps
Driving Question Boards
Multilingual Learner Language Expectations
An Introduction to Astronomy
We invite you to come along on a series of voyages to explore the universe as astronomers understand it today. Beyond Earth are vast and magnificent realms full of objects that have no counterpart on our home planet. Nevertheless, we hope to show you that the evolution of the universe has been directly responsible for your presence on Earth today.
Astronomy is defined as the study of the objects that lie beyond our planet Earth and the processes by which these objects interact with one another. We will see, though, that it is much more. It is also humanity’s attempt to organize what we learn into a clear history of the universe, from the instant of its birth in the Big Bang to the present moment. Throughout this book, we emphasize that science is a progress report—one that changes constantly as new techniques and instruments allow us to probe the universe more deeply.
Suggested Course Sequence
Chapter 1 Science and the Universe • [optional: Selected sections of Chapter 4: Earth, Moon, and Sky and perhaps parts of Chapter 3, Orbits and Gravity]
Chapter 5 Radiation and Spectra (perhaps shortening the readings on spectra to match what you do in class)
Chapter 6 Astronomical Instruments
Unit Standards
What is the NGSS & 3 Dimensional Science Learning and Why is it Important?
Science Practices - Disciplinary Core Ideas - Crosscutting Concepts
Clarification Statement: Emphasis is on the energy transfer mechanisms that allow energy from nuclear fusion in the sun’s core to reach Earth. Examples of evidence for the model include observations of the masses and lifetimes of other stars, as well as the ways that the sun’s radiation varies due to sudden solar flares (“space weather”), the 11-year sunspot cycle, and non-cyclic variations over centuries.
Boundary Statement: Assessment does not include details of the atomic and sub-atomic processes involved with the sun’s nuclear fusion.
Clarification Statement: Emphasis is on the astronomical evidence of the red shift of light from galaxies as an indication that the universe is currently expanding, the cosmic microwave background as the remnant radiation from the Big Bang, and the observed composition of ordinary matter of the universe, primarily found in stars and interstellar gases (from the spectra of electromagnetic radiation from stars), which matches that predicted by the Big Bang theory (3/4 hydrogen and 1/4 helium).
Boundary Statement: none
Clarification Statement: Emphasis is on the way nucleosynthesis, and therefore the different elements created, varies as a function of the mass of a star and the stage of its lifetime.
Boundary Statement: Details of the many different nucleosynthesis pathways for stars of differing masses are not assessed.
Clarification Statement: Emphasis is on Newtonian gravitational laws governing orbital motions, which apply to human-made satellites as well as planets and moons.
Boundary Statement: Mathematical representations for the gravitational attraction of bodies and Kepler’s Laws of orbital motions should not deal with more than two bodies, nor involve calculus.
Learning Objectives / Career Connections
By the end of this chapter, students should be able to:
Chapter 1
Define the main features of the celestial sphere
Explain the system astronomers use to describe the sky
Describe how motions of the stars appear to us on Earth
Describe how motions of the Sun, Moon, and planets appear to us on Earth
Understand the modern meaning of the term constellation
Chapter 5
Explain the evidence for Maxwell’s electromagnetic model of light
Describe the relationship between wavelength, frequency, and speed of light
Discuss the particle model of light and the definition of photon
Explain how and why the amount of light we see from an object depends upon its distance
Chapter 6
Describe the three basic components of a modern system for measuring astronomical sources
Describe the main functions of a telescope
Describe the two basic types of visible-light telescopes and how they form images
Using ChatGPT to find local Colorado Phenomena
Use the following prompt, adjust accordingly. "I am a high school science teacher looking for a local Colorado phenomena to address NGSS standard (enter standard you are looking for... example HS-LS1-6)"
Career Connections
Connecting what students are learning to careers not only deepens their engagement in school but also helps them make more informed choices about their future. Browse the following related career profiles to discover what scientists really do on the job and what it takes to prepare for these careers. For additional profiles visit your Year at a Glance Page.
Hands On, Minds On Connections
Hands-On Labs / Lab Safety
St Vrain Science Center
Simulations
GIZMOS
Nearpod Lessons / Activities / Videos
LabXchange Lessons / Activities / Videos