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Exoplanetary Discovery

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Red Dwarfs

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Abstract

To state the obvious, this chapter represents a moving target. Although one can, for example, blithely state that of the end of December 2017, a total of 3605 planets had been confirmed, of which 1414 were Neptune-like; by the time this book goes to press that figure will, most likely, be out of date. Therefore, consider this chapter as an incomplete portrait that has many of its key features presented but not all of the hues and textures indicative of a complete work.

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Notes

  1. 1.

    The mass of the planet is determined through: Mp = (Vstar∗Mstar)/Vpl, where Vstar can be found from the Doppler velocity, K. In turn, K = Vstar∗sinθ, where θ is the inclination of the planet’s orbit to the line that is perpendicular to the line-of-sight.

  2. 2.

    Popular Science writer Mary Roach would say BEER is an example of “PLEASE”—Pretty Lame Excuse for an Acronym, Scientists and Experimenters. One concurs…

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    David S. Stevenson

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Stevenson, D.S. (2019). Exoplanetary Discovery. In: Red Dwarfs. Springer, Cham. https://doi.org/10.1007/978-3-030-25550-3_2

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