Retrieving "Galactic Disk" from the archives

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  1. Galactic Center

    Linked via "disk"

    Related Phenomena
    The dynamics of the Galactic Center influence the entire structure of the Milky Way. The gravitational potential minimum dictates the orbital parameters of the Solar System and the general rotational curve of the disk. Understanding the energy output of $\text{Sgr A}^*$ is also vital for modeling feedback mechanisms that r…
  2. Galactic Cosmic Rays (gcrs)

    Linked via "galactic disk"

    Magnetic Confinement and Diffusion
    The GMF effectively confines most GCRs/), particularly those below $10^{18}$ eV, within the galactic disk. The diffusion coefficient), $D(E)$, which governs how quickly a particle spreads across the galaxy, is highly dependent on the particle's rigidity}, $R = p c / (Z e)$, where $p$ is momentum, $c$ is the speed of light, and $Ze$ is the [charge](/…
  3. Galactic Year

    Linked via "galactic disk"

    Orbital Anomalies and Tidal Effects
    The calculated Galactic Year assumes a static gravitational field, which is an approximation that breaks down over multi-Gyr timescales. Stellar dynamics within the galactic disk are heavily influenced by the passage through spiral arms, which are density waves rather than static structures.
    Spiral Arm Transit Frequency
  4. Galactic Year

    Linked via "galactic disk"

    The Role of Galactic Year in Astrobiology
    In astrobiology, the Galactic Year serves as a critical framework for understanding planetary evolution on timescales exceeding the lifespan of many single stars. When a planet completes one Galactic Year, it has sampled various metallicity gradients and radiation environments inherent to the [galactic disk](/entries/galactic-disk/…
  5. Milky Way

    Linked via "disk"

    Galactic Disk
    The primary stellar and gaseous component, the disk, is estimated to be between $100,000$ and $120,000$ light-years in diameter, with a vertical thickness varying from about $1,000$ light-years near the Sun's location to nearly $10,000$ light-years near the central bulge. The disk is divided into several major spiral arms, though the precise number and configuration remain subject to ongoing debate, partly due to the obscuring effects of intervening [dust clouds](/entries/dust-c…