Lecture 17: Exoplanets II Flashcards

(4 cards)

1
Q

what is spectroscopy for exoplanets and what can it be used for?

A

technique that analyses the light from a star after it passes through or reflects off an exoplanets atmosphere

can be used to learn about planets size, density etc

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2
Q

3 methods of spectroscopy

A

transit spectroscopy

direct imaging

doppler spectroscopy

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3
Q

what are primary and secondary eclipse, and what type of spectra can we take from them?

A

primary eclipse: a transmission spectrum when the planet transits in front of the host star- absorption

secondary eclipse: an emission spectrum as the planet passes behind the host star

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4
Q

explain the existence of hot jupiters and eccentricities

A

hot jupiters are planets that have masses and radii similar to jupiter, but periods of only 4 days

they likely come form further out and migrate inward

large range of eccentricities likely due to dynamical interactions in multiple planet systems

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