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  2. Nebular hypothesis - Wikipedia

    en.wikipedia.org/wiki/Nebular_hypothesis

    The nebular hypothesis is the most widely accepted model in the field of cosmogony to explain the formation and evolution of the Solar System (as well as other planetary systems). It suggests the Solar System is formed from gas and dust orbiting the Sun which clumped up together to form the planets.

  3. Nebula - Wikipedia

    en.wikipedia.org/wiki/Nebula

    Reflection nebulae themselves do not emit significant amounts of visible light, but are near stars and reflect light from them. [25] Similar nebulae not illuminated by stars do not exhibit visible radiation, but may be detected as opaque clouds blocking light from luminous objects behind them; they are called dark nebulae .

  4. Barnard 68 - Wikipedia

    en.wikipedia.org/wiki/Barnard_68

    Barnard 68 is a molecular cloud, dark absorption nebula or Bok globule, towards the southern constellation Ophiuchus and well within the Milky Way galaxy at a distance of about 125 parsecs (407 lightyears). [2] It is both close and dense enough that stars behind it cannot be seen from Earth.

  5. Formation and evolution of the Solar System - Wikipedia

    en.wikipedia.org/wiki/Formation_and_evolution_of...

    The nebular hypothesis says that the Solar System formed from the gravitational collapse of a fragment of a giant molecular cloud, [9] most likely at the edge of a Wolf-Rayet bubble. [10] The cloud was about 20 parsecs (65 light years) across, [9] while the fragments were roughly 1 parsec (three and a quarter light-years) across. [11]

  6. Planetary nebula - Wikipedia

    en.wikipedia.org/wiki/Planetary_nebula

    It is approximately 2,500 light-years away. NGC 6326 , a planetary nebula with glowing wisps of outpouring gas that are lit up by a binary [ 3 ] central star A planetary nebula is a type of emission nebula consisting of an expanding, glowing shell of ionized gas ejected from red giant stars late in their lives.

  7. Dark nebula - Wikipedia

    en.wikipedia.org/wiki/Dark_nebula

    A dark nebula or absorption nebula is a type of interstellar cloud, particularly molecular clouds, that is so dense that it obscures the visible wavelengths of light from objects behind it, such as background stars and emission or reflection nebulae.

  8. Timeline of gravitational physics and relativity - Wikipedia

    en.wikipedia.org/wiki/Timeline_of_gravitational...

    1965 – Penrose discovers the structure of the light cones in gravitational plane wave spacetimes. 1965 – Ezra Newman and others introduce Kerr-Newman metric. [152] [153] 1965 – Arno Penzias and Robert Wilson accidentally discover the cosmic microwave background radiation. [154] This rules out the steady-state model of Fred Hoyle and ...

  9. List of dark nebulae - Wikipedia

    en.wikipedia.org/wiki/List_of_dark_nebulae

    This is a list of dark nebulae (absorption nebulae), also called "dark clouds". The Milky Way as seen by Gaia, with prominent dark features labeled in white, as well as prominent star clouds labeled in black.