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  2. Pale Blue Dot - Wikipedia

    en.wikipedia.org/wiki/Pale_Blue_Dot

    Pale Blue Dot is a photograph of Earth taken on February 14, 1990, by the Voyager 1 space probe from an unprecedented distance of approximately 6 billion kilometers (3.7 billion miles, 40.5 AU), as part of that day's Family Portrait series of images of the Solar System.

  3. Earthlight (astronomy) - Wikipedia

    en.wikipedia.org/wiki/Earthlight_(astronomy)

    On the left, the star Omicron Arietis (37 Ari, 6,2 m) in the constellation Aries. During the crescent phase, the darker side of the Moon reflects indirect sunlight, reflected from Earth, while the other side reflects direct sunlight. An 80 mm shot of a crescent Moon with a 10-second exposure, revealing earthshine.

  4. Starlight - Wikipedia

    en.wikipedia.org/wiki/Starlight

    Starlight is the light emitted by stars. [1] It typically refers to visible electromagnetic radiation from stars other than the Sun, observable from Earth at night, although a component of starlight is observable from Earth during daytime. Sunlight is the term used for the Sun's starlight observed during daytime.

  5. Parallax in astronomy - Wikipedia

    en.wikipedia.org/wiki/Parallax_in_astronomy

    A parsec is the distance from the Sun to an astronomical object that has a parallax angle of one arcsecond (not to scale). The parsec (symbol: pc) is a unit of length used to measure the large distances to astronomical objects outside the Solar System, approximately equal to 3.26 light-years or 206,265 astronomical units (AU), i.e. 30.9 trillion kilometres (19.2 trillion miles).

  6. File:The Earth seen from Apollo 17 with transparent ...

    en.wikipedia.org/wiki/File:The_Earth_seen_from...

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  7. Atmospheric refraction - Wikipedia

    en.wikipedia.org/wiki/Atmospheric_refraction

    The animated image of the Moon's surface shows the effects of atmospheric turbulence on the view. Turbulence in Earth's atmosphere scatters the light from stars, making them appear brighter and fainter on a time-scale of milliseconds. The slowest components of these fluctuations are visible as twinkling (also called scintillation).

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  9. Polarization in astronomy - Wikipedia

    en.wikipedia.org/wiki/Polarization_in_astronomy

    Continuum light is linearly polarized at different locations across the face of the Sun (limb polarization) though taken as a whole, this polarization cancels. Linear polarization in spectral lines is usually created by anisotropic scattering of photons on atoms and ions which can themselves be polarized by this interaction.