Uranus evolution models with simple thermal boundary layers

[1]  B. Elmegreen.  ON THE INITIAL CONDITIONS FOR STAR FORMATION AND THE INITIAL MASS FUNCTION , 2011, 1102.5232.

[2]  M. Heimpel,et al.  Turbulent models of ice giant internal dynamics: Dynamos, heat transfer, and zonal flows , 2013 .

[3]  W. Hubbard.  Comparative thermal evolution of Uranus and Neptune , 1978 .

[4]  Y. Alibert,et al.  Characterization of exoplanets from their formation - I. Models of combined planet formation and evolution , 2012, 1206.6103.

[5]  G. Orton,et al.  The D/H ratio in the atmospheres of Uranus and Neptune from Herschel-PACS observations , 2013, 1301.5781.

[6]  Ravit Helled,et al.  INTERIOR MODELS OF URANUS AND NEPTUNE , 2010, 1010.5546.

[7]  Supriya Chakrabarti,et al.  Uranus Pathfinder: exploring the origins and evolution of Ice Giant planets , 2012 .

[8]  R. Helled,et al.  WHAT DO WE REALLY KNOW ABOUT URANUS AND NEPTUNE? , 2012, 1208.5551.

[9]  A. Ingersoll,et al.  Seasonal meridional energy balance and thermal structure of the atmosphere of Uranus - a radiative-convective-dynamical model , 1987 .

[10]  H. Wilson.  Diffusivity of heavy elements in Jupiter and Saturn , 2015 .

[11]  S. Stanley,et al.  Numerical dynamo models of Uranus' and Neptune's magnetic fields , 2006 .

[12]  Mark S. Marley,et al.  Monte Carlo interior models for Uranus and Neptune , 1995 .

[13]  A. Ingersoll,et al.  Liquid Water Oceans in Ice Giants , 2006, astro-ph/0609723.

[14]  R. Redmer,et al.  Superionic Phases of the 1:1 Water-Ammonia Mixture. , 2015, The journal of physical chemistry. A.

[15]  M. Marley,et al.  Further investigations of random models of Uranus and Neptune , 2000 .

[16]  K. Tsiganis,et al.  Explaining why the uranian satellites have equatorial prograde orbits despite the large planetary obliquity , 2012, 1208.4685.

[17]  F. Fressin,et al.  THE FALSE POSITIVE RATE OF KEPLER AND THE OCCURRENCE OF PLANETS , 2013, 1301.0842.

[18]  S. Seager,et al.  A FRAMEWORK FOR QUANTIFYING THE DEGENERACIES OF EXOPLANET INTERIOR COMPOSITIONS , 2009, 0912.3288.

[19]  Achim Weiss,et al.  Stellar Structure and Evolution , 1990 .

[20]  W. Nellis,et al.  Chemical processes in the deep interior of Uranus. , 2011, Nature communications.

[21]  D. Stevenson.  Cosmochemistry and structure of the giant planets and their satellites , 1985 .

[22]  A. Coustenis,et al.  The albedo, effective temperature, and energy balance of Uranus, as determined from Voyager IRIS data , 1990 .

[23]  Natalie M. Batalha,et al.  Exploring exoplanet populations with NASA’s Kepler Mission , 2014, Proceedings of the National Academy of Sciences.

[24]  T. Yagi,et al.  Polymerization and diamond formation from melting methane and their implications in ice layer of giant planets , 2009 .

[25]  Mark S. Marley,et al.  Planetary Radii across Five Orders of Magnitude in Mass and Stellar Insolation: Application to Transits , 2006 .

[26]  R. Redmer,et al.  Ab Initio Equation of State Data for Hydrogen, Helium, and Water and the Internal Structure of Jupiter , 2007, 0712.1019.

[27]  R. Redmer,et al.  THERMAL EVOLUTION AND STRUCTURE MODELS OF THE TRANSITING SUPER-EARTH GJ 1214b , 2010, 1010.0277.

[28]  T. Guillot,et al.  Effect of Radiative Transport on the Evolution of Jupiter and Saturn , 1995 .

[29]  G. Orton,et al.  Thermal structure and energy balance of Uranus , 1991 .

[30]  W. Hubbard,et al.  Structure and evolution of Uranus and Neptune , 1980 .

[31]  J. Fortney,et al.  New indication for a dichotomy in the interior structure of Uranus and Neptune from the application of modified shape and rotation data , 2012, 1207.2309.

[32]  R. Hide.  The giant planets. , 1982 .

[33]  T. Iitaka,et al.  Dissociation of methane under high pressure. , 2010, The Journal of chemical physics.

[34]  G. F. Lindal,et al.  The atmosphere of Uranus: Results of radio occultation measurements with Voyager 2 , 1987 .

[35]  Jonathan J. Fortney,et al.  HOW THERMAL EVOLUTION AND MASS-LOSS SCULPT POPULATIONS OF SUPER-EARTHS AND SUB-NEPTUNES: APPLICATION TO THE KEPLER-11 SYSTEM AND BEYOND , 2012, 1205.0010.

[36]  D. Stevenson.  Formation of Giant Planets , 1982 .

[37]  J. Fortney,et al.  The Interior Structure, Composition, and Evolution of Giant Planets , 2009, 0912.0533.

[38]  W. Hubbard,et al.  Models of Uranus' interior and magnetic field , 1991 .

[39]  Burkhard Militzer,et al.  Rocky core solubility in Jupiter and giant exoplanets. , 2011, Physical review letters.

[40]  Javier Ruiz,et al.  Neptune and Triton: Essential pieces of the Solar System puzzle , 2014 .

[41]  M. Marley,et al.  On the Luminosity of Young Jupiters , 2006, astro-ph/0609739.

[42]  J. Pollack,et al.  The structure and evolution of Jupiter - The fluid contraction stage , 1975 .

[43]  R. Redmer,et al.  Equation of state and phase diagram of ammonia at high pressures from ab initio simulations. , 2013, The Journal of chemical physics.

[44]  Edwin A. Bergin,et al.  THE EFFECTS OF SNOWLINES ON C/O IN PLANETARY ATMOSPHERES , 2011, 1110.5567.

[45]  M. Marley,et al.  Comparative models of Uranus and Neptune , 1995 .

[46]  R. Hide.  Introduction to the Physics of the Earth's Interior , 2001 .

[47]  G. Roe,et al.  THE INTERIORS OF GIANT PLANETS : Models and Outstanding Questions , 2005 .

[48]  T. Guillot,et al.  SELF-CONSISTENT MODEL ATMOSPHERES AND THE COOLING OF THE SOLAR SYSTEM'S GIANT PLANETS , 2011, 1101.0606.

[49]  Gilles Chabrier,et al.  Layered convection as the origin of Saturn/'s luminosity anomaly , 2013, 1304.6184.

[50]  M. Marley,et al.  Optimized Jupiter, Saturn, and Uranus interior models , 1989 .

[51]  R. Helled,et al.  CONVECTION AND MIXING IN GIANT PLANET EVOLUTION , 2015, 1502.03270.

[52]  P. Gierasch,et al.  Vertical temperature gradients on Uranus: Implications for layered convection , 1987 .

[53]  D. Stevenson,et al.  The interior of Neptune , 1995 .

[54]  D. Stevenson.  The Uranus-Neptune Dichotomy: the Role of Giant Impacts , 1986 .

[55]  A. Ingersoll,et al.  Uranus atmospheric dynamics and circulation , 1991 .

[56]  Christoph Mordasini,et al.  A FRAMEWORK FOR CHARACTERIZING THE ATMOSPHERES OF LOW-MASS LOW-DENSITY TRANSITING PLANETS , 2013, 1306.4329.

[57]  T. Mattsson,et al.  The phase diagram of water and the magnetic fields of Uranus and Neptune , 2011 .

[58]  Jack J. Lissauer,et al.  Formation of the Giant Planets by Concurrent Accretion of Solids and Gas , 1995 .