Abstract
Atmosphere escape is observed in the solar system for a variety of objects, including the sun all the way down to Pluto. It should, therefore, come as no surprise that planets orbiting other stars may exhibit similar phenomena, providing an opportunity to explore the effects of atmosphere escape across a range of conditions not encountered in the solar system. Improvements in understanding the upper atmospheres of exoplanets and the time evolution of stellar X-ray to ultraviolet fluxes for a range of stellar masses have, together, enabled careful models of planet evolution that include the impact of atmospheric escape. A clear picture is emerging where some planets are left relatively unscathed, while others may experience substantial planetary evaporation that completely determines their bulk properties and ultimate fate. This chapter introduces some of the basic concepts for understanding the role of atmospheric escape and large-scale planetary evaporation in the long-term evolution of Jupiter-mass down to super-Earth-mass exoplanets.
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References
Baraffe I, Chabrier G, Allard F, Hauschildt PH (2002) Evolutionary models for low-mass stars and brown dwarfs: uncertainties and limits at very young ages. A&A 382:563–572. doi:10.1051/0004-6361:20011638, astro-ph/0111385
Baraffe I, Chabrier G, Barman TS, Allard F, Hauschildt PH (2003) Evolutionary models for cool brown dwarfs and extrasolar giant planets. The case of HD 209458. A&A 402:701–712. doi:10.1051/0004-6361:20030252, astro-ph/0302293
Baraffe I, Selsis F, Chabrier G et al (2004) The effect of evaporation on the evolution of close-in giant planets. A&A 419:L13–L16. doi:10.1051/0004-6361:20040129, astro-ph/0404101
Baraffe I, Chabrier G, Barman TS et al (2005) Hot-Jupiters and hot-Neptunes: a common origin? A&A 436:L47–L51. doi:10.1051/0004-6361:200500123, astro-ph/0505054
Baraffe I, Alibert Y, Chabrier G, Benz W (2006) Birth and fate of hot-Neptune planets. A&A 450:1221–1229. doi:10.1051/0004-6361:20054040, astro-ph/0512091
Barman TS, Hauschildt PH, Allard F (2005) Phase-dependent properties of extrasolar planet atmospheres. ApJ 632:1132–1139. doi:10.1086/444349, astro-ph/0507136
Burrows A, Marley M, Hubbard WB et al (1997) A nongray theory of extrasolar giant planets and brown dwarfs. ApJ 491:856–875. doi:10.1086/305002, astro-ph/9705201
Burrows A, Sudarsky D, Hubbard WB (2003) A theory for the radius of the transiting giant planet HD 209458b. ApJ 594:545–551. doi:10.1086/376897, astro-ph/0305277
Chabrier G, Baraffe I (1997) Structure and evolution of low-mass stars. A&A 327:1039–1053, astro-ph/9704118
Chen H, Rogers LA (2016) Evolutionary analysis of gaseous sub-Neptune-mass planets with MESA. ApJ 831:180. doi:10.3847/0004-637X/831/2/180, 1603.06596
Ehrenreich D, Bourrier V, Wheatley PJ et al (2015) A giant comet-like cloud of hydrogen escaping the warm Neptune-mass exoplanet GJ 436b. Nature 522:459–461. doi:10.1038/nature14501, 1506.07541
Erkaev NV, Kulikov YN, Lammer H et al (2007) Roche lobe effects on the atmospheric loss from “Hot Jupiters”. A&A 472:329–334. doi:10.1051/0004-6361:20066929, astro-ph/0612729
Findeisen K, Hillenbrand L (2010) Ultraviolet-selected field and pre-main-sequence stars toward taurus and upper scorpius. AJ 139:1338–1359. doi:10.1088/0004-6256/139/4/1338, 1001.3684
Forget F, Leconte J (2014) Possible climates on terrestrial exoplanets. Philos Trans R Soc Lond A 372:20130,084–20130,084. doi:10.1098/rsta.2013.0084, 1311.3101
Fortney JJ, Nettelmann N (2010) The interior structure, composition, and evolution of giant planets. Space Sci Rev 152:423–447. doi:10.1007/s11214-009-9582-x, 0912.0533
France K, Froning CS, Linsky JL et al (2013) The ultraviolet radiation environment around M dwarf exoplanet host stars. ApJ 763:149. doi:10.1088/0004-637X/763/2/149, 1212.4833
Gondoin P (2012) Dynamo regime transition among Sun-like stars in M 34. A time evolution model of X-ray activity on the main sequence. A&A 546:A117. doi:10.1051/0004-6361/201219823
Gondoin P, Gandolfi D, Fridlund M et al (2012) From CoRoT 102899501 to the Sun. A time evolution model of chromospheric activity on the main sequence. A&A 548:A15. doi:10.1051/0004-6361/201219101, 1210.3221
Güdel M (2004) X-ray astronomy of stellar coronae. A&A Rev 12:71–237. doi:10.1007/s00159-004-0023-2, astro-ph/0406661
Guillot T, Burrows A, Hubbard WB, Lunine JI, Saumon D (1996) Giant planets at small orbital distances. ApJ 459:L35. doi:10.1086/309935, astro-ph/9511109
Hansen BMS, Barman T (2007) Two classes of hot Jupiters. ApJ 671:861–871. doi:10.1086/523038, 0706.3052
Howe AR, Burrows A (2015) Evolutionary models of super-earths and mini-Neptunes incorporating cooling and mass loss. ApJ 808:150. doi:10.1088/0004-637X/808/2/150, 1505.02784
Hubbard WB, Burrows A, Lunine JI (2002) Theory of giant planets. ARA&A 40:103–136. doi:10.1146/annurev.astro.40.060401.093917
Hubbard WB, Hattori MF, Burrows A, Hubeny I (2007a) A mass function constraint on extrasolar giant planet evaporation rates. ApJ 658:L59–L62. doi:10.1086/513422, astro-ph/0702276
Hubbard WB, Hattori MF, Burrows A, Hubeny I, Sudarsky D (2007b) Effects of mass loss for highly-irradiated giant planets. Icarus 187:358–364. doi:10.1016/j.icarus.2006.10.019
Hunten DM (1982) Thermal and nonthermal escape mechanisms for terrestrial bodies. Planet Space Sci 30:773–783. doi:10.1016/0032-0633(82)90110-6
Inamdar NK, Schlichting HE (2016) Stealing the gas: giant impacts and the large diversity in exoplanet densities. ApJ 817:L13. doi:10.3847/2041-8205/817/2/L13, 1510.02090
Jin S, Mordasini C, Parmentier V et al (2014) Planetary population synthesis coupled with atmospheric escape: a statistical view of evaporation. ApJ 795:65. doi:10.1088/0004-637X/795/1/65, 1409.2879
Koskinen TT, Harris MJ, Yelle RV, Lavvas P (2013a) The escape of heavy atoms from the ionosphere of HD209458b. I. A photochemical-dynamical model of the thermosphere. Icarus 226:1678–1694. doi:10.1016/j.icarus.2012.09.027, 1210.1536
Koskinen TT, Yelle RV, Harris MJ, Lavvas P (2013b) The escape of heavy atoms from the ionosphere of HD209458b. II. Interpretation of the observations. Icarus 226:1695–1708. doi:10.1016/j.icarus.2012.09.026, 1210.1543
Koskinen TT, Lavvas P, Harris MJ, Yelle RV (2014a) Thermal escape from extrasolar giant planets. Philos Trans R Soc Lond A 372:20130,089–20130,089. doi:10.1098/rsta.2013.0089, 1312.1947
Koskinen TT, Yelle RV, Lavvas P, Y-K Cho J (2014b) Electrodynamics on extrasolar giant planets. ApJ 796:16. doi:10.1088/0004-637X/796/1/16, 1409.7027
Kulow JR, France K, Linsky J, Loyd ROP (2014) Lyα Transit spectroscopy and the neutral hydrogen tail of the hot Neptune GJ 436b. ApJ 786:132. doi:10.1088/0004-637X/786/2/132, 1403.6834
Lammer H, Selsis F, Ribas I et al (2003) Atmospheric loss of exoplanets resulting from stellar X-ray and extreme-ultraviolet heating. ApJ 598:L121–L124. doi:10.1086/380815
Lammer H, Erkaev NV, Fossati L et al (2016) Identifying the ‘true’ radius of the hot sub-Neptune CoRoT-24b by mass-loss modelling. MNRAS 461:L62–L66. doi:10.1093/mnrasl/slw095, 1605.03595
Lecavelier Des Etangs A (2007) A diagram to determine the evaporation status of extrasolar planets. A&A 461:1185–1193. doi:10.1051/0004-6361:20065014, astro-ph/0609744
Lecavelier des Etangs A, Vidal-Madjar A, McConnell JC, Hébrard G (2004) Atmospheric escape from hot Jupiters. A&A 418:L1–L4. doi:10.1051/0004-6361:20040106, astro-ph/0403369
Linsky JL, France K, Ayres T (2013) Computing intrinsic LYα fluxes of F5 V to M5 V stars. ApJ 766:69. doi:10.1088/0004-637X/766/2/69, 1301.5711
Linsky JL, Fontenla J, France K (2014) The intrinsic extreme ultraviolet fluxes of F5 V TO M5 V stars. ApJ 780:61. doi:10.1088/0004-637X/780/1/61, 1310.1360
Lissauer JJ, Jontof-Hutter D, Rowe JF et al (2013) All six planets known to orbit kepler-11 have low densities. ApJ 770:131. doi:10.1088/0004-637X/770/2/131, 1303.0227
Lopez ED (2016) Born dry in the photo-evaporation desert: Kepler’s ultra-short-period planets formed water-poor. ArXiv e-prints 1610.01170
Lopez ED, Fortney JJ (2013) The role of core mass in controlling evaporation: the Kepler radius distribution and the Kepler-36 density dichotomy. ApJ 776:2. doi:10.1088/0004-637X/776/1/2, 1305.0269
Lopez ED, Fortney JJ (2014) Understanding the mass-radius relation for sub-Neptunes: radius as a proxy for composition. ApJ 792:1. doi:10.1088/0004-637X/792/1/1, 1311.0329
Lopez ED, Fortney JJ, Miller N (2012) How thermal evolution and mass-loss sculpt populations of super-earths and sub-Neptunes: application to the Kepler-11 system and beyond. ApJ 761:59. doi:10.1088/0004-637X/761/1/59, 1205.0010
Murray-Clay RA, Chiang EI, Murray N (2009) Atmospheric escape from hot Jupiters. ApJ 693:23–42. doi:10.1088/0004-637X/693/1/23, 0811.0006
Noyes RW, Hartmann LW, Baliunas SL, Duncan DK, Vaughan AH (1984) Rotation, convection, and magnetic activity in lower main-sequence stars. ApJ 279:763–777. doi:10.1086/161945
Núñez A, Agüeros MA (2016) The X-ray luminosity function of M37 and the evolution of coronal activity in low-mass stars. ApJ 830:44. doi:10.3847/0004-637X/830/1/44, 1607.05789
Owen JE, Jackson AP (2012) Planetary evaporation by UV – X-ray radiation: basic hydrodynamics. MNRAS 425:2931–2947. doi:10.1111/j.1365-2966.2012.21481.x, 1206.2367
Parke Loyd RO, Koskinen TT, France K, Schneider C, Redfield S (2017) Ultraviolet C II and Si III transit spectroscopy and modeling of the evaporating atmosphere of GJ436b. ApJ 834:L17. doi:10.3847/2041-8213/834/2/L17, 1612.08962
Poppenhaeger K, Czesla S, Schröter S et al (2012) The high-energy environment in the super-earth system CoRoT-7. A&A 541:A26. doi:10.1051/0004-6361/201118507, 1203.4080
Reiners A, Mohanty S (2012) Radius-dependent angular momentum evolution in low-mass stars. I. ApJ 746:43. doi:10.1088/0004-637X/746/1/43, 1111.7071
Ribas I, Guinan EF, Güdel M, Audard M (2005) Evolution of the solar activity over time and effects on planetary atmospheres. I. High-energy irradiances (1–1700 Å). ApJ 622:680–694. doi:10.1086/427977, astro-ph/0412253
Ribas I, Porto de Mello GF, Ferreira LD et al (2010) Evolution of the solar activity over time and effects on planetary atmospheres. II. κ 1 Ceti, an analog of the sun when life arose on earth. ApJ 714:384-395. doi:10.1088/0004-637X/714/1/384, 1003.3561
Seiff A, Kirk DB, Knight TCD et al (1998) Thermal structure of Jupiter’s atmosphere near the edge of a 5-μm hot spot in the north equatorial belt. J Geophys Res 103:22,857–22,890. doi:10.1029/98JE01766
Shkolnik EL, Barman TS (2014) HAZMAT. I. The evolution of far-UV and near-UV emission from early M stars. AJ 148:64. doi:10.1088/0004-6256/148/4/64, 1407.1344
Shkolnik EL, Rolph KA, Peacock S, Barman TS (2014) Predicting Lyα and Mg II fluxes from K and M dwarfs using galaxy evolution explorer ultraviolet photometry. ApJ 796:L20. doi:10.1088/2041-8205/796/1/L20, 1410.4263
Stelzer B, Marino A, Micela G, López-Santiago J, Liefke C (2013) The UV and X-ray activity of the M dwarfs within 10 pc of the Sun. MNRAS 431:2063–2079. doi:10.1093/mnras/stt225, 1302.1061
Tian F (2015) Atmospheric escape from solar system terrestrial planets and exoplanets. Annu Rev Earth Planet Sci 43:459–476. doi:10.1146/annurev-earth-060313-054834
Tian F, Ida S (2015) Water contents of Earth-mass planets around M dwarfs. Nat Geosci 8:177–180. doi:10.1038/ngeo2372
Tian F, Toon OB, Pavlov AA, De Sterck H (2005) Transonic hydrodynamic escape of hydrogen from extrasolar planetary atmospheres. ApJ 621:1049–1060. doi:10.1086/427204
Tian F, Chassefière E, Leblanc F, Brain D (2013) Atmospheric escape and climate evolution of terrestrial planets, pp 567–581. doi:10.2458/azu_uapress_9780816530595-ch23
Valencia D, O’Connell RJ, Sasselov D (2006) Internal structure of massive terrestrial planets. Icarus 181:545–554. doi:10.1016/j.icarus.2005.11.021, astro-ph/0511150
Vidal-Madjar A, Lecavelier des Etangs A, Désert JM et al (2003) An extended upper atmosphere around the extrasolar planet HD209458b. Nature 422:143–146. doi:10.1038/nature01448
Yelle RV (2004) Aeronomy of extra-solar giant planets at small orbital distances. Icarus 170:167–179. doi:10.1016/j.icarus.2004.02.008
Acknowledgements
The author acknowledges financial support from the National Science Foundation (AAG-1614492) and NASA (14-HW14_2-0113, 16-XRP16_2-0112).
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Barman, T. (2017). Planetary Evaporation Through Evolution. In: Deeg, H., Belmonte, J. (eds) Handbook of Exoplanets . Springer, Cham. https://doi.org/10.1007/978-3-319-30648-3_29-1
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DOI: https://doi.org/10.1007/978-3-319-30648-3_29-1
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