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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 disk - Wikipedia

    en.wikipedia.org/wiki/Accretion_disk

    Accretion disk jets: Why do the disks surrounding certain objects, such as the nuclei of active galaxies, emit jets along their polar axes? These jets are invoked by astronomers to do everything from getting rid of angular momentum in a forming star to reionizing the universe (in active galactic nuclei), but their origin is still not well understood.

  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. Quasar - Wikipedia

    en.wikipedia.org/wiki/Quasar

    As with other categories of AGN, the observed properties of a quasar depend on many factors, including the mass of the black hole, the rate of gas accretion, the orientation of the accretion disc relative to the observer, the presence or absence of a jet, and the degree of obscuration by gas and dust within the host galaxy.

  6. Nebular hypothesis - Wikipedia

    en.wikipedia.org/wiki/Nebular_hypothesis

    The runaway accretion lasts between 10,000 and 100,000 years and ends when the largest bodies exceed approximately 1,000 km in diameter. [20] Slowing of the accretion is caused by gravitational perturbations by large bodies on the remaining planetesimals. [20] [65] In addition, the influence of larger bodies stops further growth of smaller ...

  7. Astronauts' most jaw-dropping photos from the International ...

    www.aol.com/astronauts-most-jaw-dropping-photos...

    Astronauts take hundreds of stunning photos from the International Space Station.. This year's best snapshots reveal both Earth and space in glorious detail. Check out astronauts' views of ...

  8. Astrophysical jet - Wikipedia

    en.wikipedia.org/wiki/Astrophysical_jet

    They likely arise from dynamic interactions within accretion disks, whose active processes are commonly connected with compact central objects such as black holes, neutron stars or pulsars. One explanation is that tangled magnetic fields are organised to aim two diametrically opposing beams away from the central source by angles only several ...

  9. ‘Like going to the moon’: Why this is the world’s most ...

    www.aol.com/going-moon-why-world-most-120326810.html

    Editor’s note: Sign up for Unlocking the World, CNN Travel’s weekly newsletter.Get news about destinations, plus the latest in aviation, food and drink, and where to stay. It’s the body of ...