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  2. Planetary equilibrium temperature - Wikipedia

    en.wikipedia.org/wiki/Planetary_equilibrium...

    Planetary equilibrium temperature differs from the global mean temperature and surface air temperature, which are measured observationally by satellites or surface-based instruments, and may be warmer than the equilibrium temperature due to the greenhouse effect.

  3. Komabayashi–Ingersoll limit - Wikipedia

    en.wikipedia.org/wiki/Komabayashi–Ingersoll_limit

    Since the equilibrium temperature is the intersection of this curve and a horizontal line representing solar flux, for fluxes above this point the planet heats up indefinitely. [4] Kasting estimated the limit for Earth to be 320 watts per square meter. [5] The limit is relevant for estimating the inner edge of the circumstellar habitable zone ...

  4. List of gravitationally rounded objects of the Solar System

    en.wikipedia.org/wiki/List_of_gravitationally...

    Since 2008, there have been five dwarf planets recognized by the IAU, although only Pluto has actually been confirmed to be in hydrostatic equilibrium [25] (Ceres is close to equilibrium, though some anomalies remain unexplained). [26] Ceres orbits in the asteroid belt, between Mars and Jupiter. The others all orbit beyond Neptune.

  5. Effective temperature - Wikipedia

    en.wikipedia.org/wiki/Effective_temperature

    The effective temperature of the Sun (5778 kelvins) is the temperature a black body of the same size must have to yield the same total emissive power.. The effective temperature of a star is the temperature of a black body with the same luminosity per surface area (F Bol) as the star and is defined according to the Stefan–Boltzmann law F Bol = σT eff 4.

  6. Kepler-42 - Wikipedia

    en.wikipedia.org/wiki/Kepler-42

    Based on the orbits of the planets and the luminosity and effective temperature of the host star, the equilibrium temperatures of the planets can be calculated. Assuming an extremely high albedo of 0.9 and absence of greenhouse effect , the outer planet Kepler-42 d would have an equilibrium temperature of about 280 K (7 °C), [ 7 ] similar to ...

  7. Greenhouse effect - Wikipedia

    en.wikipedia.org/wiki/Greenhouse_effect

    Under such conditions, the planet's equilibrium temperature is determined by the mean solar irradiance and the planetary albedo (how much sunlight is reflected back to space instead of being absorbed). The greenhouse effect measures how much warmer the surface is than the overall effective temperature of the planet.

  8. With dengue cases at an extreme high, research points to ...

    www.aol.com/dengue-cases-extreme-high-research...

    The Summary. Nearly 12 million cases of dengue fever have been recorded in the Americas this year, close to triple last year’s total. New research suggests that climate change is responsible for ...

  9. Earth's energy budget - Wikipedia

    en.wikipedia.org/wiki/Earth's_energy_budget

    The strong (fourth-power) temperature sensitivity maintains a near-balance of the outgoing energy flow to the incoming flow via small changes in the planet's absolute temperatures. Increase in the Earth's non-cloud greenhouse effect (2000–2022) based on satellite data.