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  2. Accretion (astrophysics) - Wikipedia

    en.wikipedia.org/wiki/Accretion_(astrophysics)

    In astrophysics, accretion is the accumulation of particles into a massive object by gravitationally attracting more matter, typically gaseous matter, into an accretion disk. [ 1 ] [ 2 ] Most astronomical objects , such as galaxies , stars , and planets , are formed by accretion processes.

  3. Accretion (meteorology) - Wikipedia

    en.wikipedia.org/wiki/Accretion_(meteorology)

    Accretion is defined as the gradual collection of something over time. [1] In meteorology or atmospheric science it is the process of accumulation of frozen water as precipitation over time as it descends through the atmosphere, in particular when an ice crystal or snowflake hits a supercooled liquid droplet, which then freeze together, increasing the size of the water particle.

  4. Pebble accretion - Wikipedia

    en.wikipedia.org/wiki/Pebble_accretion

    Pebble accretion is the accumulation of particles, ranging from centimeters up to meters in diameter, into planetesimals in a protoplanetary disk that is enhanced by aerodynamic drag from the gas present in the disk. This drag reduces the relative velocity of pebbles as they pass by larger bodies, preventing some from escaping the body's gravity.

  5. Accretion - Wikipedia

    en.wikipedia.org/wiki/Accretion

    Accretion (coastal management), the process where coastal sediments return to the visible portion of the beach following storm erosion; Accretion (geology), the increase in size of a tectonic plate by addition of material along a convergent boundary; Accretionary wedge

  6. Magnetorotational instability - Wikipedia

    en.wikipedia.org/wiki/Magnetorotational_instability

    These oscillations are present under much more general conditions as well: a recent laboratory experiment (Ji et al., 2006) has shown stability of the flow profile expected in accretion disks under conditions in which otherwise troublesome dissipation effects are (by a standard measure known as the Reynolds number) well below one part in a million.

  7. Bondi accretion - Wikipedia

    en.wikipedia.org/wiki/Bondi_accretion

    In astrophysics, the Bondi accretion (also called Bondi–Hoyle–Lyttleton accretion), named after Hermann Bondi, is spherical accretion onto a compact object traveling through the interstellar medium. It is generally used in the context of neutron star and black hole accretion. To achieve an approximate form of the Bondi accretion rate ...

  8. Accretion (geology) - Wikipedia

    en.wikipedia.org/wiki/Accretion_(geology)

    In geology, accretion is a process by which material is added to a tectonic plate at a subduction zone, frequently on the edge of existing continental landmasses. The added material may be sediment, volcanic arcs , seamounts , oceanic crust or other igneous features.

  9. History of the Solar System - Wikipedia

    en.wikipedia.org/wiki/Age_of_the_Solar_System

    The process of accretion, therefore, is not complete, and may still pose a threat to life on Earth. [ 82 ] [ 83 ] Over the course of the Solar System's evolution, comets were ejected out of the inner Solar System by the gravity of the giant planets and sent thousands of AU outward to form the Oort cloud , a spherical outer swarm of cometary ...