Planetary orbits that are face-on to our line of sight produce no Doppler shift in the stellar spectrum.
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Q16: A planet's density can be measured by
Q17: The reason that most extrasolar planets are
Q18: The Doppler technique only provides a measure
Q19: The astrometric technique of planet detection works
Q20: A planet is detected via the Doppler
Q22: The Kepler mission has been able to
Q23: If every star had an Earth-like planet
Q24: Most of the planets discovered around other
Q25: The Doppler technique for planet detection has
Q26: Astronomers have discovered more planets around other
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