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  2. Outer space - Wikipedia

    en.wikipedia.org/wiki/Outer_space

    The temperature of outer space is measured in terms of the kinetic activity of the gas, [38] as it is on Earth. The radiation of outer space has a different temperature than the kinetic temperature of the gas, meaning that the gas and radiation are not in thermodynamic equilibrium.

  3. Portal:Outer space - Wikipedia

    en.wikipedia.org/wiki/Portal:Outer_space

    The baseline temperature of outer space, as set by the background radiation from the Big Bang, is 2.7 kelvins (−270 °C; −455 °F). The plasma between galaxies is thought to account for about half of the baryonic (ordinary) matter in the universe, having a number density of less than one hydrogen atom per cubic metre and a kinetic ...

  4. Space weather - Wikipedia

    en.wikipedia.org/wiki/Space_weather

    Space weather is a branch of space physics and aeronomy, or heliophysics, ... and the outer layer of the Earth's atmosphere (or the thermosphere and exosphere ...

  5. Planetary equilibrium temperature - Wikipedia

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

    There are large variations in surface temperature over space and time on airless or near-airless bodies like Mars, which has daily surface temperature variations of 50–60 K. [18] [19] Because of a relative lack of air to transport or retain heat, significant variations in temperature develop. Assuming the planet radiates as a blackbody (i.e ...

  6. Radiative cooling - Wikipedia

    en.wikipedia.org/wiki/Radiative_cooling

    Since outer space radiates at about a temperature of 3 K (−270.15 °C; −454.27 °F), and the sheet of paper radiates at about 300 K (27 °C; 80 °F) (around room temperature), the sheet of paper radiates more heat to the face than does the darkened cosmos. The effect is blunted by Earth's surrounding atmosphere, and particularly the water ...

  7. Observable universe - Wikipedia

    en.wikipedia.org/wiki/Observable_universe

    Assuming that space is roughly flat (in the sense of being a Euclidean space), this size corresponds to a comoving volume of about 1.22 × 10 4 Gpc 3 (4.22 × 10 5 Gly 3 or 3.57 × 10 80 m 3). [ 29 ] These are distances now (in cosmological time ), not distances at the time the light was emitted.

  8. Thermosphere - Wikipedia

    en.wikipedia.org/wiki/Thermosphere

    The thermosphere is uninhabited with the exception of the International Space Station, which orbits the Earth within the middle of the thermosphere between 408 and 410 kilometres (254 and 255 mi) and the Tiangong space station, which orbits between 340 and 450 kilometres (210 and 280 mi).

  9. Troposphere - Wikipedia

    en.wikipedia.org/wiki/Troposphere

    The increase of air temperature at stratospheric altitudes results from the ozone layer's absorption and retention of the ultraviolet (UV) radiation that Earth receives from the Sun. [7] The coldest layer of the atmosphere, where the temperature lapse rate changes from a positive rate (in the troposphere) to a negative rate (in the stratosphere ...