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  2. Radiation pressure - Wikipedia

    en.wikipedia.org/wiki/Radiation_pressure

    The idea of interplanetary travel by light was mentioned by Jules Verne in his 1865 novel From the Earth to the Moon. A sail reflects about 90% of the incident radiation. The 10% that is absorbed is radiated away from both surfaces, with the proportion emitted from the unlit surface depending on the thermal conductivity of the sail.

  3. Orders of magnitude (pressure) - Wikipedia

    en.wikipedia.org/wiki/Orders_of_magnitude_(pressure)

    Level of long-duration blast overpressure (from a large-scale explosion) that would cause most buildings to collapse [49] 34 kPa Atmospheric pressure at the summit of Mount Everest [50] +70 kPa +10 psi Pressure for paint exiting an HVLP (low-pressure) paint spray gun [51] 70 kPa Pressure inside an incandescent light bulb [52] 75 kPa

  4. Outer space - Wikipedia

    en.wikipedia.org/wiki/Outer_space

    The lack of pressure in space is the most immediate dangerous characteristic of space to humans. Pressure decreases above Earth, reaching a level at an altitude of around 19.14 km (11.89 mi) that matches the vapor pressure of water at the temperature of the human body.

  5. Light - Wikipedia

    en.wikipedia.org/wiki/Light

    Maxwell discovered that self-propagating electromagnetic waves would travel through space at a constant speed, which happened to be equal to the previously measured speed of light. From this, Maxwell concluded that light was a form of electromagnetic radiation: he first stated this result in 1862 in On Physical Lines of Force .

  6. Heliosphere - Wikipedia

    en.wikipedia.org/wiki/Heliosphere

    The scientific study of the heliosphere is heliophysics, which includes space weather and space climate. Flowing unimpeded through the Solar System for billions of kilometers, the solar wind extends far beyond even the region of Pluto until it encounters the "termination shock", where its motion slows abruptly due to the outside pressure of the ...

  7. Two-body problem in general relativity - Wikipedia

    en.wikipedia.org/wiki/Two-body_problem_in...

    In the Schwarzschild solution, it is assumed that the larger mass M is stationary and it alone determines the gravitational field (i.e., the geometry of space-time) and, hence, the lesser mass m follows a geodesic path through that fixed space-time. This is a reasonable approximation for photons and the orbit of Mercury, which is roughly 6 ...

  8. The Sun is really loud — but if we could hear it, what would ...

    www.aol.com/news/2018-02-26-the-sun-is-really...

    The Sun is said to be extremely noisy, but we can’t hear it since sound doesn’t travel through space. Scientists at the University of Sheffield decided to use vibrations within our star's ...

  9. Friedmann equations - Wikipedia

    en.wikipedia.org/wiki/Friedmann_equations

    In these equations, R(t) is the cosmological scale factor, is the Newtonian constant of gravitation, Λ is the cosmological constant with dimension length −2, ρ is the energy density and p is the isotropic pressure. k is constant throughout a particular solution, but may vary from one solution to another.