Exploring Climate with Obliquity in a Variable-eccentricity Earth-like World

被引:1
|
作者
Way, M. J. [1 ,2 ,3 ]
Georgakarakos, Nikolaos [4 ,5 ]
Clune, Thomas L. [6 ]
机构
[1] NASA Goddard Inst Space Studies, 2880 Broadway, New York, NY 10025 USA
[2] NASA Goddard Space Flight Ctr, GSFC Sellers Exoplanet Environm Collaborat, Greenbelt, MD 20771 USA
[3] Uppsala Univ, Dept Phys & Astron, Theoret Astrophys, SE-75120 Uppsala, Sweden
[4] New York Univ Abu Dhabi, Div Sci, POB 129188, Abu Dhabi, U Arab Emirates
[5] New York Univ Abu Dhabi, Ctr Astrophys & Space Sci CASS, POB 129188, Abu Dhabi, U Arab Emirates
[6] NASA Goddard Space Flight Ctr, Global Modeling & Assimilat Off, Greenbelt, MD 20771 USA
来源
ASTRONOMICAL JOURNAL | 2023年 / 166卷 / 06期
关键词
HABITABLE-ZONE; SIZED PLANET; EXOPLANETS; EVOLUTION; DYNAMICS; SYSTEMS; STARS; DWARF; MODEL;
D O I
10.3847/1538-3881/ad0373
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Exploring planetary systems similar to our solar system can provide a means to explore a large range of possibly temperate climates on Earth-like worlds. Rather than run hundreds of simulations with different eccentricities at fixed obliquities, our variable-eccentricity approach provides a means to cover an incredibly large parameter space. Herein Jupiter's orbital radius is moved substantially inward in two different scenarios, causing a forcing on Earth's eccentricity. In one case, the eccentricity of Earth varies from 0 to 0.27 over similar to 7000 yr for three different fixed obliquities (0 degrees, 23 degrees, and 45 degrees). In another case, the eccentricity varies from 0 to 0.53 over similar to 9400 yr in a single case with zero obliquity. In all cases, we find that the climate remains stable, but regional habitability changes through time in unique ways. At the same time, the moist greenhouse state is approached but only when at the highest eccentricities.
引用
收藏
页数:10
相关论文
共 37 条
  • [1] Effects of Variable Eccentricity on the Climate of an Earth-like World
    Way, M. J.
    Georgakarakos, Nikolaos
    [J]. ASTROPHYSICAL JOURNAL LETTERS, 2017, 835 (01)
  • [2] THERMAL PHASES OF EARTH-LIKE PLANETS: ESTIMATING THERMAL INERTIA FROM ECCENTRICITY, OBLIQUITY, AND DIURNAL FORCING
    Cowan, Nicolas B.
    Voigt, Aiko
    Abbot, Dorian S.
    [J]. ASTROPHYSICAL JOURNAL, 2012, 757 (01):
  • [3] Climate of Earth-like planets with high obliquity and eccentric orbits: Implications for habitability conditions
    Linsenmeier, Manuel
    Pascale, Salvatore
    Lucarini, Valerio
    [J]. PLANETARY AND SPACE SCIENCE, 2015, 105 : 43 - 59
  • [4] Atmospheric dynamics and habitability range in Earth-like aquaplanets obliquity simulations
    Nowajewski, Priscilla
    Rojas, M.
    Rojo, R.
    Kimeswenger, S.
    [J]. ICARUS, 2018, 305 : 84 - 90
  • [5] Climate stability of habitable Earth-like planets
    Menou, Kristen
    [J]. EARTH AND PLANETARY SCIENCE LETTERS, 2015, 429 : 20 - 24
  • [6] Climate variations on Earth-like circumbinary planets
    Popp, Max
    Eggl, Siegfried
    [J]. NATURE COMMUNICATIONS, 2017, 8
  • [7] EVOLUTIONARY CLIMATE TRACKS OF EARTH-LIKE PLANETS
    Kadoya, S.
    Tajika, E.
    [J]. ASTROPHYSICAL JOURNAL LETTERS, 2015, 815 (01)
  • [8] Climate variations on Earth-like circumbinary planets
    Max Popp
    Siegfried Eggl
    [J]. Nature Communications, 8
  • [9] Residual eccentricity of an Earth-like planet orbiting a red giant Sun
    Lanza, A. F.
    Lebreton, Y.
    Sallard, C.
    [J]. ASTRONOMY & ASTROPHYSICS, 2023, 674
  • [10] The Role of Water Vapor in the Response of the Extratropical Circulation of Earth-Like Planets to Obliquity Changes
    Lobo, Ana H.
    Bordoni, Simona
    [J]. JOURNAL OF GEOPHYSICAL RESEARCH-ATMOSPHERES, 2022, 127 (16)