Unit Nine: Stars
Daily Star Dates *(varies depending on class)
In Class - Epsilon Auriga
In Class - Parallax Lab
In Class - Stellar Properties Observations
In Class - Sun Structure and Features
In Class - Secrets of the Sun Video
In Class - HR Diagram Lab
In Class - Life-cycle of Stars worksheet
Use this link to listen to the 2 minute podcast. Keep a journal record of the topics discussed.
Our "@Home" Planetarium - we can not always be in the planetarium, especially when we're at home. This is a web-based version of the planetarium - or, at least, as close as you can get. You just have to set it up on your computer.
When the earth travels around the sun, nearby stars appear to shift their position with the background stars. This shift in position is called PARALLAX.
Just as looking at a gas gauge in the car from the passenger seat, or not looking directly down on a measuring stick. The angle of viewing can change the resulting measurements. Ancient Greeks used "parallax" to determine the distance of far off ships before they landed.
Objective: Observe how the parallax angle changes with distance to the observers.
In the Planetarium, we will use about 20 of the brightest stars to gather information about the stars brightness, distance, color, and temperature. Using this info, determine the relationship between brightness and distance of the stars. Also, we will determine the relationship between a star's color and its temperature.
If you miss the planetarium, research the information for the following stars:
Sol, Rigel, Betelgeuse, Pollux, Castor, Sirius, Procyon, Polaris, Thuban, Mizar, Dubhe, Aldebaran, Capella, Arcturus, Regulus, and Spica.
We will look at our SUN! *Warning: Never look directly at the sun!!!
Step1: Using the Sunspotter, Eclipse Glasses, and Solar Filters you task is to trace an image of the sun on your paper.
Step 2: Follow the demonstration in class with water and a hot plate. Relate your observations to the demonstration to how the interior of the sun operates.
Take a look at this link, which will show you the anatomy of the sun. The following layers will be reviewed as well as their properties:
Core
Radiation Zone
Convection Zone
Photosphere
Chromosphere
Corona
Watch Secrets of the Sun and answer questions on the attached worksheet.
You are about to create the "Single Most Important Graph In All of Astronomy"! Use the HR Diagram Data and the graph paper, plot the stars ABSOLUTE magnitude and Spectral Type (aka: its temperature).
Whiteboard your results and groups stars together into 3 sections on your graph.
Part 1: Human Evolution
Rank each of the following pictures by age, going from youngest to oldest. Put a 1 in the blank by the picture you think is the youngest person, a 2 in the blank by the second youngest, and so on. If you wish, try to guess the age of each person.
Part 2: Stellar Evolution LOW Mass Stars
The images below show six NASA images of the formation sequence of LOW mass stars. Your FIRST task is to figure out and record the correct sequence of pictures from birth formation to stellar death. SECOND task is to write a detailed description so clear that any student would be able to use it to come up with the exact same sequence.
Part 3: Stellar Evolution HIGH Mass Stars
The images below show seven NASA images of the formation sequence of HIGH mass stars. Your FIRST task is to figure out and record the correct sequence of pictures from birth (Hint: These stars are born the same way) formation to stellar death (Hint: There are 2 possible outcomes for the end of this stars life). SECOND task is to write a detailed description so clear that any student would be able to use it to come up with the exact same sequence.
Links:
StarForge - Nebula to Protostar formation
Stellar Evolution Review - need Firefox to run.