Chapter 13: Other Planetary Systems Flashcards

1
Q

What are the three methods for detecting extra solar planets?

A

The astrometric, doppler, and transit method.

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2
Q

What is the astrometric method?

A

This method uses very precise measurments to detect motion in stars.

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3
Q

What is the doppler method?

A

This method looks for doppler shifts to detect steller movement.

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4
Q

What is the transit method?

A

This method searches for transits and eclipses by monitoring a stars brightness over a period of time.

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5
Q

Why can the transit method only detect a fraction of extrasolar planets?

A

The transit method requires the planet’s orbit to be lined up such that the planet passes between earth and its star.

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6
Q

What are the key advantages to the astrometric method?

A

Detects planets in all orbit orientations except edge-on.

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7
Q

What are the key advantages to the doppler method?

A

Possible from ground based telescopes

Detects planets in all orbit orientations except face on

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8
Q

What are the key advantages to the transit method?

A

Allows many stars to be oberved at once

Can detect very small planets

Feasible with small telescopes

Can probide some atmospheric data in cases of measurable eclipses

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9
Q

What are the major limitations with the astrometric method?

A

Generally possible only for relatively nearby stars

Biased towards finding massive planets that orbit far from their stars

May require years of obervation to detect these planets

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10
Q

What are the major limitations with the doppler method?

A

Biased toward finding massive planet with close in orbits

Underestimates star’s true motion exept when system viewed edge-on

Requires stellar spectra which means large telescopes and long observation times

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11
Q

What are the major limitations with the transit method?

A

Possible only for planets with edge-on orbits as viewed from earth

For small planets, requires sensitivity possible only from space observatory

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12
Q

What is a “hot jupiter”?

A

A extrasolar gas giant that orbits close to the sun.

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13
Q

What method(s) can be used to determine planetary distance? How are they used?

A

The astrometric, doppler, and transit method can all be used to determine the orbital distance of a planet. This is done using the orbital period and Newton’s version of Kepler’s third law.

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14
Q

What method(s) can be used to determine planetary eccentricity? How are they used?

A

The doppler and the astrometric method can be used. This is done by creating velocity curves and by using astrometric star positions.

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15
Q

What method(s) can be used to determine planetary inclination? How are they used?

A

The transit method and the astrometric method can be used. This is because astrometric methods measure any inclination angle, and transits can only be used on edge on orbits.

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16
Q

What method(s) can be used to determine planetary mass? How are they used?

A

The astrometric, and doppler method can be used. This is done by the amount of stellar motion caused by the planet’s gravitational tug.

17
Q

What method(s) can be used to determine planetary size? How are they used?

A

The transit method can be used. The size is calculated by the amount of a dip in the star’s brightness during a transit.

18
Q

What method(s) can be used to determine planetary density? How are they used?

A

The doppler and the transit method can be used. This is done by dividing the mass by the volume.

19
Q

What method(s) can be used to determine planetary atromospheric compostion and temperature? How are they used?

A

The transit and direct detection can be used. Transits and eclipses provide data on atmostpehric composition and temperature.

20
Q

What method(s) can be used to determine planetary atromospheric compostion and temperature? How are they used?

A

The transit and direct detection can be used. Transits and eclipses provide data on atmostpehric composition and temperature.

21
Q

What is the accepted explination for “hot jupiters”

A

It is likely caused by a planetary migration in which the solar nebula forces gas giants to migrate towards their star.