The ______ method of planet-hunting relies on a periodic dimming of the star being orbited.

Get ready for the Dual Enrollment Earth Science Test. Study strategically with multiple choice questions that include hints and detailed explanations.

Multiple Choice

The ______ method of planet-hunting relies on a periodic dimming of the star being orbited.

Explanation:
The transit method detects periodic dimming of a star’s light when a planet passes in front of it from our viewpoint, blocking a small portion of the light. This regular, repeating drop in brightness tells us a planet is orbiting the star and provides two key pieces of information: the planet’s size from how deep the dip is, and its orbital period from how often the dips occur. The method works best when the planet’s orbit is edge-on enough for the planet to cross the star as seen from Earth, and it requires continuous monitoring to catch multiple transits and confirm the signal. Other planet-hunting methods work differently: the Doppler (or radial velocity) method looks for shifts in the star’s spectral lines caused by the star wobbling due to the planet’s gravity; direct imaging tries to capture actual light from the planet; microlensing relies on gravitational lensing when a foreground star-planet system passes in front of a background star, briefly magnifying its light.

The transit method detects periodic dimming of a star’s light when a planet passes in front of it from our viewpoint, blocking a small portion of the light. This regular, repeating drop in brightness tells us a planet is orbiting the star and provides two key pieces of information: the planet’s size from how deep the dip is, and its orbital period from how often the dips occur. The method works best when the planet’s orbit is edge-on enough for the planet to cross the star as seen from Earth, and it requires continuous monitoring to catch multiple transits and confirm the signal.

Other planet-hunting methods work differently: the Doppler (or radial velocity) method looks for shifts in the star’s spectral lines caused by the star wobbling due to the planet’s gravity; direct imaging tries to capture actual light from the planet; microlensing relies on gravitational lensing when a foreground star-planet system passes in front of a background star, briefly magnifying its light.

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