2.4 Exoplanets Flashcards

1
Q

What is an exoplanet

A

A planet orbiting s star other than our own - outside the solar system

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2
Q

Why are exoplanets difficult to find

A

They are so far away we need very advanced technology to see them or find them

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3
Q

Why are the 3 main techniques for finding an exoplanet indirect

A

They rely on observing the effect on their host star

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4
Q

What is astrometry

A

As massive exoplanets orbit their parent star their gravitational pull can cause the star to wobble/ change position

These wobbles can be detected - we measure the precise position of the star relative to eachother to see if they move over time

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5
Q

What limits the accuracy of astrometry

A

The turbulence of our atmosphere

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6
Q

What’s the transit method

A

If an exoplanet moves across its star in their orbit they cause a typically 1% drop in brightness
- by measuring amount of light received by a star over a period of time

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7
Q

What’s the problem with the transit method

A

It has to be On the same plane as we are in order to see it moving across

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8
Q

What’s radial velocity (using Doppler shifts) method

A

The wobbling of a star did to exoplanets gravity can also cause wavelengths to be slightly red-shifted and blue-shifted on a regular time scale as a star moved away from us and towards us

Spectroscopy is able to reveal small shifts in wavelength and has been proved the most successful

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9
Q

Why does the atmosphere have a negative affect on discovering exoplanets

A

Small rocky exoplanets like earth can’t be discover due to atmospheric turbulence

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10
Q

Why can we find earth like planets

A

They need to be:

Not to big - likely a gas giant

Medium- earth like relatively small mass so little effect on host star

Too small - not enough gravity to hold onto atmosphere

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11
Q

What are the 2 essential chemical ingredients for life

A

Carbon - element had ability to make compass and form basis of more complex molecules (chemical building blocks of life)

Liquid water - excellent solvent and transport mechanism for nutrients
Need for photosynthesis and to break down large molecules (hydrolysis)

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12
Q

What are the 2 principal origins of water on earth

A

Our gassing of hydrogen and oxygen from volcanoes to produce steam and condense to water

Deposited by comets containing ice striking earth

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13
Q

Where must a planet be to sustain life

A

Habitable Zone
Or
Goldilocks zone

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14
Q

What’s the habitable / Goldilocks zone

A

A narrow range of distances from the star which the temperature allows liquid water to exist - neither to hold or cold

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15
Q

What did frank drake do in 1961

A

Made the Drake equation

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16
Q

What is the Drake equation

A

Combine estimated probabilities of a number of factors That as a result estimate number of civilisations in our galaxy that could communicate with us

17
Q

Where in our solar system could life exist

A

Jupiters moon Europa

Mars

18
Q

How do we use space probes to search for signs of life

A

Test for microbes or bi-products

19
Q

How does spectral analysis of planetary atmospheres test for life

A

Search for gases such as oxygen and methane that are produced by living organisms

20
Q

How does the analysis of radio waves help search for life

A

Try to detect signals that could have originated from extra terrestrial intelligent forms of life in Galaxy

21
Q

What are the ethical problems of finding life

A

Would it be wiser to transfer organisms from one environment into a totally different one where they could become extinct or adapt too well and flourish

Could life on Earth be threatened we don’t know their capabilities

Do we really want to discover that we aren’t alone?

22
Q

Name some factors of the Drake equation

A

L= length of time signals released into space

Fp= fraction of those stars that have planets

R*= average rate of star formation per year in our galaxy

Fi= fraction of that life that goes on to develop intelligence