Definition
Stars of a given mass are smallest in size when in their main-sequence stage and are hence called dwarfs; this use of the term should not be confused with white dwarfs, the end stage (death) of low-mass stars. Stars similar to the Sun spend most of their luminous careers burning hydrogen in their cores. It is during this main-sequence or dwarf-star phase that the energy output can be stable over periods of time long enough to support the evolution of life as we know it. Dwarf stars are prime targets for searches for transiting planets as small as the Earth. Recent attention has focused on the coolest dwarf stars of spectral type M, because they range from one half to one tenth the diameter of the Sun. Planetary transits around such stars are thus much deeper and easier to detect; in addition, for a given planetary mass, the wobble of the star will be larger, making radial velocity and astrometry measurements easier. The habitable zonewhere water could be liquid is also...
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© 2014 Springer-Verlag Berlin Heidelberg
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Latham, D.W. (2014). Dwarf Star. In: Amils, R., et al. Encyclopedia of Astrobiology. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-27833-4_466-4
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DOI: https://doi.org/10.1007/978-3-642-27833-4_466-4
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Publisher Name: Springer, Berlin, Heidelberg
Online ISBN: 978-3-642-27833-4
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Latest
Dwarf Star- Published:
- 15 October 2022
DOI: https://doi.org/10.1007/978-3-642-27833-4_466-5
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Dwarf Star- Published:
- 23 April 2015
DOI: https://doi.org/10.1007/978-3-642-27833-4_466-4