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Radial Velocity Method To Detect Exoplanets iPhone case by Science Photo Library. Protect your iPhone with an impact-resistant, slim-profile, hard-shell case. The image is printed directly onto the case and wrapped around the edges for a beautiful presentation. Simply snap the case onto your iPhone for instant protection and direct access to all of the phone's features!
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Illustration showing how the radial velocity method (also known as Doppler spectroscopy) can be used to detect extrasolar planets (exoplanets). The... more
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Protect your with an impact-resistant, slim-profile, hard-shell case. The image is printed directly onto the case and wrapped around the edges for a beautiful presentation. Simply snap the case onto your for instant protection and direct access to all of the phone's features!
Illustration showing how the radial velocity method (also known as Doppler spectroscopy) can be used to detect extrasolar planets (exoplanets). The radial velocity method relies on the fact that a star does not remain stationary when it is orbited by a planet, but responds to the gravitational pull of the planet. When viewed from a distance, these slight movements affect the star's normal light spectrum (shown at bottom). If the star is moving towards the observer, then the spectrum would appear slightly shifted towards the blue; if it is moving away, it will be shifted towards the red. Using highly sensitive spectrographs, a star's spectrum can be tracked over time. Regular, periodic shifts towards the red, blue, and back again indicate the presence of a body orbiting the star. Transit methods for detecting exoplanets can provide an estimate of a planet's size, but not the mass. Using both methods, combining mass and size, the planet's density can be calculated which is an important
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