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  2. Liquid droplet radiator - Wikipedia

    en.wikipedia.org/wiki/Liquid_Droplet_Radiator

    The liquid droplet radiator (LDR) system consists of a droplet generator, a collector, a heat exchanger, a recirculating pump, and a bellows-type pressure regulator (accumulator). While undergoing a reduction in pressure the saturated liquid is sprayed into space as coherent streams of tiny, discrete droplets. The droplet stream can be a column ...

  3. Radiation pressure - Wikipedia

    en.wikipedia.org/wiki/Radiation_pressure

    Solar radiation pressure on objects near the Earth may be calculated using the Sun's irradiance at 1 AU, known as the solar constant, or G SC, whose value is set at 1361 W/m 2 as of 2011. [17] All stars have a spectral energy distribution that depends on their surface temperature. The distribution is approximately that of black-body radiation.

  4. Poynting–Robertson effect - Wikipedia

    en.wikipedia.org/wiki/Poynting–Robertson_effect

    This is related to radiation pressure tangential to the grain's motion. This causes dust that is small enough to be affected by this drag, but too large to be blown away from the star by radiation pressure, to spiral slowly into the star. In the Solar System, this affects dust grains from about 1 μm to 1 mm in diameter. Larger dust is likely ...

  5. Solar constant - Wikipedia

    en.wikipedia.org/wiki/Solar_constant

    The solar constant is an average of a varying value. In the past 400 years it has varied less than 0.2 percent. [2] Billions of years ago, it was significantly lower. This constant is used in the calculation of radiation pressure, which aids in the calculation of a force on a solar sail.

  6. Lunar water - Wikipedia

    en.wikipedia.org/wiki/Lunar_water

    The hypothetical mechanism of water transport / trapping (if any) remains unknown: indeed lunar surfaces directly exposed to the solar wind where water production occurs are too hot to allow trapping by water condensation (and solar radiation also continuously decomposes water), while no (or much less) water production is expected in the cold ...

  7. Atmosphere of the Moon - Wikipedia

    en.wikipedia.org/wiki/Atmosphere_of_the_Moon

    The pressure of this small mass is around 3 × 10 −15 atm (0.3 nPa), varying throughout the day, and in total mass less than 10 metric tonnes. [ 5 ] [ 6 ] Otherwise, the Moon is considered not to have an atmosphere because it cannot absorb measurable quantities of radiation, does not appear layered or self-circulating, and requires constant ...

  8. Chandrayaan-2 - Wikipedia

    en.wikipedia.org/wiki/Chandrayaan-2

    Solar radiation pressure accelerates the sodium atoms away from the Sun, forming an elongated tail toward the antisolar direction. Using the large area X-raySpectrometer, CLASS, the probe has spotted and mapped sodium on the Moon. Hydroxyl and Water molecules: The Chandrayaan-1 probe detected water on the Moon for the first time. Chandrayaan-2 ...

  9. Pyranometer - Wikipedia

    en.wikipedia.org/wiki/Pyranometer

    A pyranometer (from Greek πῦρ (pyr) 'fire' and ἄνω (ano) 'above, sky') is a type of actinometer used for measuring solar irradiance on a planar surface and it is designed to measure the solar radiation flux density (W/m 2) from the hemisphere above within a wavelength range 0.3 μm to 3 μm.