Transcript Exoplanets: PowerPoint presentation
Exoplanets
Big Science: Big Telescopes
Jodrell Bank Discovery Centre
Contents
Part 1: Big Telescopes
– Why do we need so many telescopes?
– Why build big telescopes?
Part 2: Big Science
– Hunting for exoplanets – Are We Alone in the Universe?
Part 1: Big Telescopes Why do we need so many telescopes?
Light is an electromagnetic wave that travels through space...
...but light is not the only EM wave travelling through space
Part 1: Big Telescopes Why do we need so many telescopes?
An object can give off any of these EM waves...
Radio waves
km to metres
Microwaves
centimetres
Infrared
micrometres
Visible light
tenths of a micrometre
Ultraviolet
nanometres
X-rays
tenths of nanometres
Gamma rays
hundredths of nanometres Astronomers observe the universe in all of these waves
Part 1: Big Telescopes Why do we need so many telescopes?
Part 1: Big Telescopes
The Lovell Telescope
Why build big telescopes?
Telescopes collect EM waves and bring them to a focus
Part 1: Big Telescopes Why build big telescopes?
• Larger telescopes collect more waves • Fainter objects can be seen • Like a pupil dilating in dim light!
Why build big telescopes?
Larger telescopes can also create sharper images
Part 1: Big Telescopes
The Square Kilometre Array
Why build big telescopes?
• • • Planned for 2020, it will be the most powerful radio telescope ever It will be so sensitive it could detect an airport radar 50 light years away It will collect enough data every day to fill 15 million 64 GB iPods
1. How do you think it would it affect your vision, if your eyes were half the size?
2. If your eyes could see radio waves, what do you think a mobile phone mast would look like?
1. How do you think it would it affect your vision, if your eyes were half the size?
Your eyes couldn’t collect as much light, so things would be darker . Also, things would be more blurry.
2. If your eyes could see radio waves, what do you think a mobile phone mast would look like?
It would look bright, like a streetlamp!
Part 2: Big Science
The hunt for exoplanets
The hunt for exoplanets
Part 2: Big Science The hunt for exoplanets
Before we continue…
1. Multiply your time by 100 days
(e.g. 2 seconds becomes 200 days)
This is to make your results more realistic!
2. How many Earth years does it take for your planet to orbit its star?
Part 2: Big Science The hunt for exoplanets
Analysing your results: How far out is your planet?
Kepler’s third law
For planets orbiting the Sun…
Orbit in Earth years
2
Distance from Sun in A.U.
3
1 A.U. (or ‘Astronomical Unit’) is just the distance between the Earth and the Sun
T
2
D
3
How far away would your planet be from its star?
The hunt for exoplanets Part 2: Big Science
Analysing your results: How far out is your planet?
T
2
D
3 3
T
2
D
Compare your planet to our Solar System.
Distance from Sun to… Mercury =
0.4
Venus =
0.7
AU AU Earth =
1
Mars =
1.5
AU AU Jupiter = Saturn =
5 9.5
Uranus =
19
AU Neptune =
30
AU AU AU
Part 2: Big Science The hunt for exoplanets
Analysing your results: How big is your planet?
You have already calculated the percentage starlight blocked by your planet (B)
Area of planet
B
Area of star Area of a circle?
r
2
B
R
2 Radius of Sun =
700,000 km What’s the radius of your planet?
Part 2: Big Science The hunt for exoplanets
Analysing your results: How big is your planet?
r
2
B
R
2
r
BR
2
Compare your planet to our Solar System.
Radius of Earth =
6,400 km
Radius of Jupiter =
70,000 km
Part 2: Big Science Are we alone?
Are we alone in the universe?
August 2013: Scientists have detected a total of 929 exoplanets
Part 2: Big Science Are we alone?
620 light years away Star Kepler-22
Part 2: Big Science
In 2011, astronomers found planet ‘Kepler-22B’ around this star…
• • Kepler-22B is… Approximately Earth sized.
About the same distance away from its star as the Earth is from the Sun.
AND, its star is very similar to the Sun!
Are we alone?
Are we alone?
What do you think?
Part 2: Big Science Extension activity
What type of exoplanets do you think are the easiest to find?
Why?
1. Larger exoplanets 2. Exoplanets that are closer to their stars Both of these cause a larger dip in the star’s light, making them easier to detect.
So far, most of the exoplanets found have been “hot Jupiters”.
These are large gas planets, but very close to their star.
Part 2: Big Science Extension activity What assumptions did we make when calculating the distance and size of your exoplanet?
• That your star is like the Sun In actual fact, the star may be a different mass. This will change how quickly a planet orbits around it, which will affect the distance calculation.
Also, the star may be a different size. This will affect the planet size calculation.
In real life, astronomers take measurements of a star’s light to see if it is like the Sun or not.
• That your planet passes next to your star In actual fact the planet will likely be hundreds of millions of km closer to us than the star, which will make it look slightly bigger. This will also affect the planet size calculation.
In real life, astronomers estimate the distances to stars and planets, so they can take this into account.
Part 2: Big Science Extension activity
Consider the following questions...
1. Can you think of any situations where the method we have used to detect exoplanets would not work? (hint: look at the animation below for one way) 2. We assumed that your stars were identical to the Sun. What effect would it have on the size of your planet if the star were actually… a) Larger than the Sun b) Smaller than the Sun 3. What effect would it have on your planet’s distance from the star if your star was… a) More massive than the Sun (more gravity) b) Less massive than the Sun (less gravity) 4. If your star is like the Sun, do you think there is any chance of there being life on your planet? Why?
5. Would there be more or less chance of life if your star was… a) Hotter than the Sun b) Colder than the Sun
Part 2: Big Science Extension activity
Answers…
1. This method only works if, from our point of view, the planet passes in front of the star. If the planet orbits the star on a different plane, we will not see a dip in the light.
2. We calculated the size of your planet by comparing it to the size of your star, which we said was the same as the Sun. If your star was… a) Larger than the Sun; the planet would be larger than calculated.
b) Smaller than the Sun; the planet would be smaller than calculated 3. We calculated the distance of your planet from its star by looking at how fast your planet was orbiting its star. We assumed the relationship was the same as the planets of the Solar System going around the Sun. If your star was… a) More massive than the Sun (more gravity), then the planet would orbit quicker than expected. Therefore, the planet may be further out than calculated.
b) Less massive than the Sun (less gravity), then the planet would orbit slower than expected. Therefore, the planet may be closer to its star than calculated.
Questions 4 and 5 depend on your results.