Chapter 13 home work 9 Other Planetary Systems Flashcards
Which of the following properties can be inferred from the star’s orbital period?
the planet’s orbital radius the planet’s mass both the planet’s orbital radius and its mass neither the planet’s orbital radius nor its mass
the planet’s orbital radius
Is it possible to determine the planet’s mass from the star’s velocity curve?
yes, by measuring the star's orbital period only yes, by measuring only the change in the star's orbital velocity over the orbit yes, by measuring both the star's orbital period and its change in velocity over the orbit no, because the star's spectrum cannot tell us about the planet
yes, by measuring both the star’s orbital period and its change in velocity over the orbit
Consider the planet that causes the stellar motion shown in Plot 2 (be sure you have clicked the “Plot 2” button in the lower window of the animation). What can be said about a different planet orbiting the same star with an orbital period of 500 days?
The planet must be farther from the star. The planet must be more massive. The planet must be less massive. The planet must be closer to the star.
The planet must be closer to the star.
The ______ was used to find a jupiter sized planet through careful measurements of the changing position of a star
Astrometric technique
Discovering planets through the _________ requires obtaining and studying many spectra of the same star.
Doppler technique
The _____ is currently searching for planet transits around some 100,000 stars.
Kepler mission
The ________ is used to find extrasolar planets by carefully monitoring chnages in a star’s brightness with time.
transit technique
The _________ is being designed to measure very small changes in stellar positions, which should allow it to discover many extrasolar planets.
GAIA Astrometry Mission
Proposed plans for the _______ would someday provide us with the first actual images and spectra of terrestrial worlds orbiting other stars.
Terrestrial Planet Finder mission
Each item describes a characteristic that applies to one of the three planet-detection methods shown following. Match the items to the correct planet-finding method. Doppler Method:
Used for most of the first 200 extrasolar planets detections
Current best-suited to find Jupiter sized extrasolar planets orbiting close to their stars
Planet detection strategy of Nasa’s Kepler Mission
Allows for the extrasolar planets radius to be determined
Can potentially detect planets in only a few percent of all planetary systems
Looks for very slight, periodic dimming of a star
This method was first to identify Earth-sized extrasolar planets.
Measures precise changes in a star’s position in the sky, fractions of acrseconds.
Used for most of the first 200 extrasolar planets detections
Current best-suited to find Jupiter sized extrasolar planets orbiting close to their stars
Each item describes a characteristic that applies to one of the three planet-detection methods shown following. Match the items to the correct planet-finding method. Transit Method:
Used for most of the first 200 extrasolar planets detections
Current best-suited to find Jupiter sized extrasolar planets orbiting close to their stars
Planet detection strategy of Nasa’s Kepler Mission
Allows for the extrasolar planets radius to be determined
Can potentially detect planets in only a few percent of all planetary systems
Looks for very slight, periodic dimming of a star
This method was first to identify Earth-sized extrasolar planets.
Measures precise changes in a star’s position in the sky, fractions of acrseconds.
Planet detection strategy of Nasa’s Kepler Mission
Allows for the extrasolar planets radius to be determined
Can potentially detect planets in only a few percent of all planetary systems
Looks for very slight, periodic dimming of a star
This method was first to identify Earth-sized extrasolar planets.
Each item describes a characteristic that applies to one of the three planet-detection methods shown following. Match the items to the correct planet-finding method. Astrometric Method:
Used for most of the first 200 extrasolar planets detections
Current best-suited to find Jupiter sized extrasolar planets orbiting close to their stars
Planet detection strategy of Nasa’s Kepler Mission
Allows for the extrasolar planets radius to be determined
Can potentially detect planets in only a few percent of all planetary systems
Looks for very slight, periodic dimming of a star
This method was first to identify Earth-sized extrasolar planets.
Measures precise changes in a star’s position in the sky, fractions of acrseconds.
Measures precise changes in a star’s position in the sky, fractions of acrseconds.
The graph above shows how a star’s orbital speed varies with time due to the gravitational tug of an orbiting planet. These data were obtained by measuring __________.
the precise wavelengths of spectral lines in the spectrum of the orbiting planet the precise brightness of the star divided by the precise brightness of the planet the precise wavelengths of spectral lines in the spectrum of the star the orbital period of the planet that is orbiting the star
the precise wavelengths of spectral lines in the spectrum of the star
The graph above shows how a star’s orbital speed varies with time due to the gravitational tug of an orbiting planet. Based on these data, the planet’s orbital period is about:
2 days. 4 days. 6 days. 50 days.
4 days.
This diagram shows the orbital path of the Sun around the center of mass of our solar system as it would appear from a distance of 30 light-years for the period 1960-2025. If aliens had constructed this graph at their home star system, they could learn all of the following except:
the fact that large, icy objects orbit the Sun in the Kuiper belt. the fact that the Sun has more than two planets. the mass and orbital period of Jupiter. the orbital distance of Saturn.
the fact that large, icy objects orbit the Sun in the Kuiper belt.