A Survey of Exoplanetary Detection Techniques
arXiv:1805.02771
Abstract
Exoplanets, or planets outside our own solar system, have long been of interest to astronomers; however, only in the past two decades have scientists had the technology to characterize and study planets so far away from us. With advanced telescopes and spectrometers, astronomers are discovering more exoplanets every year. The two most prolific methods for detecting exoplanets, radial velocity, which measures the wobble of an exoplanet's parent star, and transit, which detects the passage of a planet in front of its star, are responsible for the discovery of the vast majority of exoplanets we know about so far. Other methods such as direct imaging, timing, and gravitational microlensing are less applicable but can sometimes yield accurate data to confirm planets found by radial velocity or transit photometry. Astronomers will continue to find large numbers of new exoplanets in the near future, but it will become increasingly harder to do so after all the planets close to our solar system are discovered.
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