Cataloging the Universe - An Audio Course from Tumble Media!
Tumble Media
8 episodes
9 months ago
This seven-lesson audio course will take you on a journey, starting at the turn of the 20th century, as we learn how scientists came to understand how massive the universe, and how it contains many more galaxies than we ever imagined before. You'll also get to learn how to classify galaxies, and do some sky watching of your own. These seven lessons align with NGSS standard 5-ESS1-1: Stellar Brightness and Distance.
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This seven-lesson audio course will take you on a journey, starting at the turn of the 20th century, as we learn how scientists came to understand how massive the universe, and how it contains many more galaxies than we ever imagined before. You'll also get to learn how to classify galaxies, and do some sky watching of your own. These seven lessons align with NGSS standard 5-ESS1-1: Stellar Brightness and Distance.
Cataloging the Universe - An Audio Course from Tumble Media!
7 minutes
2 years ago
Lesson 3 - Observing Mystery Objects
It’s time-traveling time again! This time, we’ll be going to France in the 1700s to talk to French astronomer Charles Messier. Messier is observing the sky and making a list of what he finds. Come along with Marshall as he finds out why Messier’s list will prove to be important for centuries of astronomers to come.
Resources included with this lesson:
Listening Questions
Discussion Questions
Download the free resources for this course on the “Cataloging the Universe” website:
https://www.sciencepodcastforkids.com/universe
Cataloging the Universe - An Audio Course from Tumble Media!
This seven-lesson audio course will take you on a journey, starting at the turn of the 20th century, as we learn how scientists came to understand how massive the universe, and how it contains many more galaxies than we ever imagined before. You'll also get to learn how to classify galaxies, and do some sky watching of your own. These seven lessons align with NGSS standard 5-ESS1-1: Stellar Brightness and Distance.
