Abstract
While we can imagine numerous scenarios in which diverse types of planets could support life in exotic conditions, for pragmatic reasons the most attention still goes to an Earth-like situation where a surface or near-subsurface biome is made possible by the presence of liquid water. With few exceptions, by far the most important source of energy determining the planet’s surface conditions is instellation from the host star. This is not a constant quantity over the star’s life. If long-term stability is necessary to support detectable life, then the stellar evolution must be taken into account when determining habitability. Stellar composition in turn has a fundamental effect on stellar evolution. The range of variation in individual elements observed in nearby stars is much larger than what is considered in most stellar modeling and can result in gigayear-scale changes in the evolution of sun-like stars. Measurements of stellar composition can also provide insight into the nature of the planets themselves.
References
Airapetian VS, Glocer A, Khazanov GV et al (2017) How hospitable are space weather affected habitable zones? The role of ion escape. ApJ 836:L3
Aleksandrov IV, Goncharov AF, Stishov SM, Yakovenko EV (1989) High-pressure research: application to earth and planetary sciences. J Exp Theor Phys 50:127
Allegre CJ, Poirier JP, Humler E, Hofmann AW (1995) The chemical composition of the Earth. Earth Planet Sci Lett 134:515
Ammann MW, Brodholt JP, Dobson DP (2011) Ferrous iron diffusion in ferro-periclase across the spin transition. E&PSL 302:393
Anbar AD, Duan Y, Lyons TW, et al (2007) A whiff of oxygen before the great oxidation event?. Science 317:1903
Arnett D (1996) Supernovae and nucleosynthesis, Princeton University Press: New Jersey
Asplund M, Grevesse N, Sauval AJ, Scott P (2009) The chemical composition of the Sun. Annu Rev Astron Astrophys 47:481–522
Barnes R, Mullins K, Goldblatt C, Meadows VS, Kasting JF, Heller R (2013) Tidal Venuses: triggering a climate catastrophe via tidal heating. Astrobiology 13:225–250
Barnes R, Meadows VS, Evans N (2015) Comparative habitability of transiting exoplanets. ApJ 814:91
Batalha NM et al (2013) A survey for very short-period planets in the Kepler data. ApJ Supplement 204:24
Bond JC et al (2006) Abundance distribution of stars with planets. MNRAS 370:163
Bond JC et al (2008) Beyond the iron peak: r- and s-process elemental abundances in stars with planets. ApJ 682:1234
Bond JC, OBrien DP, Lauretta DS (2010) The compositional diversity of extrasolar terrestrial planets. I. In situ simulations. ApJ 715:1050
Borucki WJ et al (2010) Kepler planet-detection mission: introduction and first results. Science 327
Caffau E, Ludwig HG, Malherbe JM, Bonifacio P, Steffen M, Monaco L (2013) The photospheric solar oxygen project: III. Investigation of the centre-to-limb variation of the 630 nm [O I]-Ni I blend. A&A 554:126
Caldeira K, Kasting JF (1992) Susceptibility of the early Earth to irreversible glaciation. Nature 359:226
Carter-Bond JC, OBrien DP, Raymond SN (2012) The Compositional Diversity Of Extrasolar Terrestrial Planets. II. Migration simulations. Astrophys J 760:44
Catanzarite J, Shao M (2011) The occurrence rate of Earth analog planets orbiting Sun-like stars. ApJ 738:151
Chandrasekhar S (1939) An introduction to the study of stellar structure. The University of Chicago Press, Chicago
de Bruijne JHJ, Rygl KLJ, Antoja T (2014) EAS Publications Ser. 67, The Milky Way Unravelled by Gaia: GREAT Science from the Gaia Data Releases ed N. Walton et al (Barcelona: EAS Publications Series) 23
de Koker N, Karki BB, Stixrude L (2013) Thermodynamics of the MgO-SiO2 liquid system in. Earth's lower mantle from first principles. E&PSL 361:58
De Silva GM et al (2006) Chemical homogeneity in the hyades. ApJ 151:455
Delgado Mena E, Israelian G, Gonza’lez Herna’ndez JI, Bond JC, Santos NC, Udry S, Mayor M (2010) Chemical clues on the formation of planetary systems: C/O versus Mg/Si for HARPS GTO sample. ApJ 725:2349
Driscoll PE, Barnes R (2015) Tidal heating of Earth-like exoplanets around M stars. Astrobiology 15:739
Fabbian D, Asplund M, Barklem PS, Carlsson M, Kiselman D (2009) Neutral oxygen spectral line formation revisited with new collisional data: large departures from LTE at low metallicity. A&A 500:1221
Gaidos E (2013) Candidate planets in the habitable zones of Kepler stars. ApJ 770:90
González Hernández JI, Israelian G, Santos NC, Sousa S, Delgado-Mena E, Neves V, Udry S (2010) Searching for the signatures of terrestrial planets in solar analogs. ApJ 720:1592
Grocholski B, Shim SH, Prakapenka VB (2013) Stability, metastability, and elastic properties of a dense silica polymorph, seifertite. J Geophys Res (unpublished data)
Hinkel NR, Young PA, Timmes FX, et al (2014) Stellar abundances in the solar neighborhood: the Hypatia catalog. ApJ 148:54
Hinkel NR, Mamajek EE, Turnbull MC, et al (2017) A Catalog of Stellar Unified Properties (CATSUP) for 951 FGK-stars within 30 pc. ApJ 848:34
Hirose K, Takafuji N, Sata N, Ohishi Y (2005) Determination of post-perovskite phase transition boundary in MgSiO3 using Au and MgO pressure standards. Earth Planet Sci Lett 237:239251
Iglesias CA, Rogers FJ (1996) Updated Opal Opacities. ApJ 464:943
Isobe T, Feigelson ED, Akritas MG, Babu GJ (1990) Linear regression in astronomy. ApJ 364:104
Kane SR (2014) Habitable zone dependence on stellar parameter uncertainties. ApJ 782:111
Kasting JF, Whitmire DP, Reynolds RT (1993) Habitable zones around main sequence stars. Icarus 101:108
Kopparapu RK, Ramirez RM, SchottelKotte J, et al (2014) ApJL 787:L29
Kopparapu RK, Wolf ET, Haqq-Misra J, et al (2016) The inner edge of the habitable zone for synchronously rotating planets around low-mass stars using general circulation models. ApJ 819:84
Lammer H, Kasting JF, Chassefie’re E, et al (2008) Atmospheric escape and evolution of terrestrial planets and satellites. Space Sci Rev 139:399
Leconte J, Forget F, Charnay B, et al (2013) 3D climate modeling of close-in land planets: Circulation patterns, climate moist bistability, and habitability. A&A 554:A69
Madhusudhan N, Lee KKM, Mousis O (2012) A possible carbon-rich interior in super-Earth 55 Cancri e. Astrophys J Lett 759:L40
McDonough WF, Sun SS (1995) The composition of the Earth. Chem Geol 120:223
Meynet G, Maeder A (2000) Stellar evolution with rotation. V. Changes in all the outputs of massive star models. A&A 361:101
Mishenina TV, Soubiran C, Bienaymé O, Korotin SA, Belik SI, Usenko IA, Kovtyukh VV (2008) Spectroscopic investigation of stars on the lower main sequence. A&A 489:923
Neves V, Santos NC, Sousa SG, Correia ACM, Israelian G (2009) Chemical abundances of 451 stars from the HARPS GTO planet search program. A&A 497:563
Nissen PE (2013) The carbon-to-oxygen ratio in stars with planets. A&A 552:73
Oishi M, Kamaya H (2016) A simple evolutional model of the UV habitable zone and the possibility of persistent life existence: the effects of mass and metallicity. Astrophys Space Sci 361(2):1–6
Pagano MD, Young PA, Challa P (2017) The elemental abundances of 518 FGK stars and planetary implications. ApJ in review
Petigura EA, Howard AW, Marcy GW (2013) Prevalence of Earth-size planets orbiting Sun-like stars. PNAS 110
Ramírez I, Allende Prieto C, Lambert DL (2007) Oxygen abundances in nearby stars. A&A 465:271
Reiners A (2012) Observations of cool-star magnetic fields. Living Rev Sol Phys 9:1
Ricolleau A, Fiquet G, Addad A, Menguy N, Vanni C, Perrillat JP, Daniel I, Cardon H, Guignot N (2008) Analytical transmission microscopy study of a natural MORB sample assemblage transformed at high pressure and high temperature. Am Mineral 93:144153
Ringwood AE (1966) Advances in Earth science. MIT Press, Boston, pp 287–356
Rogers FJ, Swenson FJ, Iglesias CA (1996) OPAL equation-of-state tables for astrophysical applications. ApJ 456:902
Seager S, Kuchner M, Hier-Majumder CA, Militzer B (2007) Mass-radius relationships for solid exoplanets. ApJ 699:1297
Sen S Widgeon SJ Navrotsky A Mera G, Tavakoli A, Ionescu E, Riedelc R (2013) Carbon substitution for oxygen in silicates in planetary interiors. Proc Natl Acad Sci 110(40):15904
Shields AL, Bitz CM, Meadows VS, Joshi MM, Robinson TD (2014) Differences IN water vapor radiative transfer among 1D models can significantly affect the inner edge of the habitable zone. ApJ 785:L9
Shkolnik EL, Llama J (2017) Signatures of star-planet interactions. arXiv:1712.02814
Stishov SM, Popova SV (1961) Geokhimiya 10:837839
Stuart A, Ord K (2009) Kendall’s advanced theory of statistics, volume 1: distribution theory. Wiley, New Jersey
Takeda Y (2007) Fundamental parameters and elemental abundances of 160 F–G–K stars based on OAO spectrum database. PASJ 59:335
Truitt A, Young PA (2017) Expanding the catalog: considering the importance of carbon, magnesium, and neon in the evolution of stars and habitable zones. ApJ 835:87
Truitt A, Young PA, Spacek A, et al (2015) A catalog of stellar evolution profiles and the effects of variable composition on habitable systems. ApJ 804:145
Unterborn CT, Kabbes JE, Pigott J, Reaman D, Panero WR (2013) The role of carbon in extrasolar planetary geodynamics and habitability (N.B. correct reference ApJ 793, 194). ApJ arXiv:1311.0024v3
Valle G, Dell’Omodarme M, Prada Moroni PG, et al (2014) Uncertainties in grid-based estimates of stellar mass and radius. SCEPtER: Stellar CharactEristics Pisa Estimation gRid. A&A 567:A133
Wolf ET, Shields AL, Kopparapu RK, Haqq-Misra J, Toon OB (2017) Constraints on climate and habitability for Earth-like exoplanets determined from a general circulation model. ApJ 837:107
Yoshida M, Onodera A, Ueno M, Takemura K, Shimomura O (1993) Pressure-induced phase transition in SiC. Phys Rev B 48:1058710590
Young PA, Liebst K, Pagano M (2012) THE impact of stellar abundance variations on stellar habitable zone evolution. ApJ 755:31
Young PA, Desch SJ, Anbar AD et al (2014) Astrobiological stoichiometry. Astrobiology 14:603
Zahnle KJ, Catling DC (2017) The cosmic shoreline: the evidence that escape determines which planets have atmospheres, and what this may mean for Proxima Centauri B. ApJ 843:122
Acknowledgments
Some of the results reported herein benefitted from collaborations and/or information exchange within NASA’s Nexus for Exoplanet System Science (NExSS) research coordination network sponsored by NASA’s Science Mission Directorate.
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Young, P.A. (2018). Stellar Composition, Structure and Evolution: Impact on Habitability. In: Deeg, H., Belmonte, J. (eds) Handbook of Exoplanets . Springer, Cham. https://doi.org/10.1007/978-3-319-30648-3_60-1
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DOI: https://doi.org/10.1007/978-3-319-30648-3_60-1
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