Download Stefan-Boltzmann Law

Survey
yes no Was this document useful for you?
   Thank you for your participation!

* Your assessment is very important for improving the workof artificial intelligence, which forms the content of this project

Document related concepts

Ursa Minor wikipedia , lookup

Timeline of astronomy wikipedia , lookup

Star formation wikipedia , lookup

Stellar evolution wikipedia , lookup

IK Pegasi wikipedia , lookup

Astronomical spectroscopy wikipedia , lookup

Hayashi track wikipedia , lookup

Transcript
Tutorial: Stefan-Boltzmann Law
(Adapted from Lecture-Tutorials for Introductory Astronomy, ©CAPER Team, Preliminary Edition, 2002)
Part I: Size, Temperature, and Luminosity
Beginning astronomy students often think that they must come up with totally new and different explanations for things
that go on in other places of the Universe besides Earth. This is not the case! If you are not venturing near a black hole
nor attempting to go nearly as fast as the speed of light, the physics we know here on Earth applies to the rest of the
solar system, the Galaxy, and the Universe. In this tutorial you will be led through the steps to understanding the
Stefan-Boltzmann Law:
The amount of energy put out per second (the number of watts) is proportional to the surface area of the sphere (4 pi
times the radius squared) and the temperature raised to the 4 th power.
L  4r 2T 4
You are comparing the ability of a grouping of electric hot plates (shown below as burners on a “stove top”) of different
sizes and temperatures to bring identical pot of water to a boil. The pots are all as large as the largest hot plate. The
temperatures of the hot plates are coded: the lighter the shade of gray, the higher the temperature.
1. For each pair of hot plates (read horizontally), circle the one that will boil the water more quickly. Is there a set of
burners for which there is no way to tell? If so, which ones?
2. If you use two hot plates of the same size, can you assume that the one that boils water first is at the higher
temperature? (This is meant to be obvious.) Which lettered example(s) above supports your answer?
4. If you use two hot plates of different sizes, can you assume that the one that boils water first is at a higher
temperature? Which lettered example(s) above supports your answer?
5. Two students are discussing their answers to question 4:
First student: In 1d, the hot plate on the left boils water quicker than the one on the right, even though it is
smaller. The hot plate’s higher temperature is what makes it boil water more quickly.
Second student: But, the size of the hot plate also plays a part in making it feel hot. If the hot plate on the left
were the size of a pinhead, the water would take a long time to boil! I bet that if the size difference were great
enough, the one at the lower temperature could boil the water first.
You are called in to mediate this argument. What do you say? Whom do you agree with and why?
5/14/2017
841018305
tu 103
The time it takes for the water to come to a boil is determined by the rate at which the element transfers energy to the
pot. This rate is related to both the size and the temperature of the hot plate. For stars, the rate at which energy is
emitted is called luminosity, and it is an intrinsic characteristic (part of its true nature) of the star. Similar to the above
example, a star’s luminosity can be increased by:
o increasing its temperature; or
o increasing its surface area (increasing its radius or size).
This relationship between size, surface temperature, and luminosity is usually referred to as the Stefan-Boltzmann law.
Our knowledge of this law allows us to compare the sizes and temperatures of stars. For example, let’s say we know a
star’s luminosity and its temperature. What can we determine? What if we have some estimate of the star’s radius and
its temperature, what can we calculate?
6. If two hot plates are at the same temperature and one boils water more quickly, what can you conclude about the
sizes of the hot plates?
7. Likewise, if two stars have the same surface temperature and one is more luminous, what can you conclude about the
sizes of the stars?
Part II: Application to the H-R Diagram
8. Compare the following pairs of stars which
may have similar temperatures or luminosities
or radii. If the quantities are very close, then
consider them identical for purposes of this
comparison.
Pair
Arcturus & tau Ceti
Sun & alpha Centauri A
Barnard’s Star & Aldebaran
white dwarf & Barnard’s Star
Spica and Canopus
Spica & Sirius
More luminous
Hotter
9. Which pairs of stars were the hardest to figure out? Why do you think this was so?
tu 104
Larger