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A Search for Habitable Planets Transit Tracks: Finding Extrasolar Planets a science & math activity.

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Presentation on theme: "A Search for Habitable Planets Transit Tracks: Finding Extrasolar Planets a science & math activity."— Presentation transcript:

1 A Search for Habitable Planets Transit Tracks: Finding Extrasolar Planets a science & math activity

2 A Search for Habitable Planets “transit”

3 A Search for Habitable Planets “transit”

4 A Search for Habitable Planets “transit”

5 A Search for Habitable Planets What’s this?

6 A Search for Habitable Planets A transit of Venus across the Sun takes place when the planet Venus passes directly between the Sun and Earth, so that Venus blocks a small spot of the Sun’s disk. Since the Sun is over 100 times larger in diameter than Venus, the spot is very small indeed.

7 A Search for Habitable Planets Account of Jeremiah Horrock’s observations of the transit of Venus

8 A Search for Habitable Planets TIME BRIGHTNESS 0 0 Imagine you have a light sensor aimed at the star. What would the transit of a book look like if you made a graph of light intensity vs time?

9 A Search for Habitable Planets Like this? TIME 0 0 BRIGHTNESS

10 A Search for Habitable Planets What would the transit of a planet look like if you made a graph of light intensity vs time? TIME 0 0 BRIGHTNESS

11 A Search for Habitable Planets TIME 0 0 Perhaps like this? Such graphs are called “light curves.” How would a planet’s size and orbit period affect the transit—light curve? BRIGHTNESS

12 A Search for Habitable Planets The light curve can lead to finding the SIZE of the planet and its DISTANCE from the star. Why would those characteristics be important?

13 A Search for Habitable Planets

14 Is there a relationship between the planet’s period (time for one orbit) and how its distance from the star?

15 A Search for Habitable Planets Kepler’s 3 rd Law

16 A Search for Habitable Planets

17 A 3 = p 2

18 A Search for Habitable Planets

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20 Kepler 4-b

21 A Search for Habitable Planets

22 Planet’s Size: Deducing the Planet’s Radius from Transit Data A p /A s = Z Converting to a percentage 100 ( A p /A s ) = Z% 100 (π r p 2 / π r s 2 ) = Z% 100 ( r p 2 / r s 2 ) = Z% r p 2 / r s 2 = Z%/100 r p 2 = r s 2 (Z%/100) r p = r s /10 √ Z% area of a circle = π r 2 The Sun is about 100 times the radius of the Earth. r sun = 100 r earth Substituting: r p = 100 r earth /10 ( √ Z% ) r p = 10 r earth ( √ Z% )

23 A Search for Habitable Planets

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26 A guy who’s thought a lot about planets ( By permission Sternwarte Kremsmünster)


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