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zadetkov: 740
1.
  • Connecting Giant Planet Atm... Connecting Giant Planet Atmosphere and Interior Modeling: Constraints on Atmospheric Metal Enrichment
    Thorngren, Daniel; Fortney, Jonathan J. Astrophysical journal. Letters, 04/2019, Letnik: 874, Številka: 2
    Journal Article
    Recenzirano
    Odprti dostop

    Atmospheric characterization through spectroscopic analysis, an essential tool of modern exoplanet science, can benefit significantly from the context provided by the interior structure models. In ...
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2.
  • The Intrinsic Temperature a... The Intrinsic Temperature and Radiative-Convective Boundary Depth in the Atmospheres of Hot Jupiters
    Thorngren, Daniel; Gao, Peter; Fortney, Jonathan J. Astrophysical journal. Letters, 10/2019, Letnik: 884, Številka: 1
    Journal Article
    Recenzirano
    Odprti dostop

    In giant planet atmosphere modeling, the intrinsic temperature Tint and radiative-convective boundary (RCB) are important lower boundary conditions. Often in one-dimensional radiative-convective ...
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3.
  • The Interior Structure, Com... The Interior Structure, Composition, and Evolution of Giant Planets
    Fortney, Jonathan J.; Nettelmann, Nadine Space science reviews, 05/2010, Letnik: 152, Številka: 1-4
    Journal Article, Conference Proceeding
    Recenzirano
    Odprti dostop

    We discuss our current understanding of the interior structure and thermal evolution of giant planets. This includes the gas giants, such as Jupiter and Saturn, that are primarily composed of ...
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4.
  • Bayesian Analysis of Hot-Ju... Bayesian Analysis of Hot-Jupiter Radius Anomalies: Evidence for Ohmic Dissipation?
    Thorngren, Daniel P.; Fortney, Jonathan J. The Astronomical journal, 05/2018, Letnik: 155, Številka: 5
    Journal Article
    Recenzirano
    Odprti dostop

    The cause of hot-Jupiter radius inflation, where giant planets with > 1000 K are significantly larger than expected, is an open question and the subject of many proposed explanations. Many of these ...
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5.
  • THE ROLE OF CORE MASS IN CO... THE ROLE OF CORE MASS IN CONTROLLING EVAPORATION: THE KEPLER RADIUS DISTRIBUTION AND THE KEPLER-36 DENSITY DICHOTOMY
    Lopez, Eric D; tney, Jonathan J Astrophysical journal/˜The œAstrophysical journal, 10/2013, Letnik: 776, Številka: 1
    Journal Article
    Recenzirano
    Odprti dostop

    We use models of coupled thermal evolution and photo-evaporative mass loss to understand the formation and evolution of the Kepler-36 system. We show that the large contrast in mean planetary density ...
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6.
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7.
  • HOW THERMAL EVOLUTION AND M... HOW THERMAL EVOLUTION AND MASS-LOSS SCULPT POPULATIONS OF SUPER-EARTHS AND SUB-NEPTUNES: APPLICATION TO THE KEPLER-11 SYSTEM AND BEYOND
    LOPEZ, Eric D; FORTNEY, Jonathan J; MILLER, Neil Astrophysical journal/˜The œAstrophysical journal, 12/2012, Letnik: 761, Številka: 1
    Journal Article
    Recenzirano
    Odprti dostop

    We use models of thermal evolution and extreme ultraviolet (XUV) driven mass loss to explore the composition and history of low-mass, low-density transiting planets. We investigate the Kepler-11 ...
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8.
  • A continuum from clear to c... A continuum from clear to cloudy hot-Jupiter exoplanets without primordial water depletion
    Sing, David K; Fortney, Jonathan J; Nikolov, Nikolay ... Nature, 01/2016, Letnik: 529, Številka: 7584
    Journal Article
    Recenzirano
    Odprti dostop

    Thousands of transiting exoplanets have been discovered, but spectral analysis of their atmospheres has so far been dominated by a small number of exoplanets and data spanning relatively narrow ...
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9.
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10.
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