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  2. Bohr radius - Wikipedia

    en.wikipedia.org/wiki/Bohr_radius

    In Schrödinger's quantum-mechanical theory of the hydrogen atom, the Bohr radius is the value of the radial coordinate for which the radial probability density of the electron position is highest. The expected value of the radial distance of the electron, by contrast, is ⁠ 3 2 a 0 {\displaystyle {\tfrac {3}{2}}a_{0}} ⁠ .

  3. Atmosphere of Mars - Wikipedia

    en.wikipedia.org/wiki/Atmosphere_of_Mars

    The highest atmospheric density on Mars is equal to the density found 35 km (22 mi) above the Earth's surface and is ≈0.020 kg/m 3. [7] The atmosphere of Mars has been losing mass to space since the planet's core slowed down, and the leakage of gases still continues today. [4] [8] [9]

  4. Displacement field (mechanics) - Wikipedia

    en.wikipedia.org/wiki/Displacement_field_(mechanics)

    In mechanics, a displacement field is the assignment of displacement vectors for all points in a region or body that are displaced from one state to another. [ 1 ] [ 2 ] A displacement vector specifies the position of a point or a particle in reference to an origin or to a previous position.

  5. Enceladus - Wikipedia

    en.wikipedia.org/wiki/Enceladus

    The magnetometer observed a deflection or "draping" of the magnetic field, consistent with local ionization of neutral gas. [14] During the two following encounters, the magnetometer team determined that gases in Enceladus's atmosphere are concentrated over the south polar region, with atmospheric density away from the pole being much lower. [ 14 ]

  6. Milky Way - Wikipedia

    en.wikipedia.org/wiki/Milky_Way

    [f] [154] [155] Filling the space between the stars is a disk of gas and dust called the interstellar medium. This disk has at least a comparable extent in radius to the stars, [156] whereas the thickness of the gas layer ranges from hundreds of light-years for the colder gas to thousands of light-years for warmer gas. [157] [158]

  7. 469219 Kamoʻoalewa - Wikipedia

    en.wikipedia.org/wiki/469219_Kamoʻoalewa

    Kamoʻoalewa orbits the Sun at a distance of 0.90–1.10 AU.Although the period as of 2022 is about 366 days, its longer-term average period is closer to 365 days. 469219 Kamoʻoalewa is a quasi-moon and not gravitationally bound to earth like a true satellite.

  8. Observable universe - Wikipedia

    en.wikipedia.org/wiki/Observable_universe

    Assuming that space is roughly flat (in the sense of being a Euclidean space), this size corresponds to a comoving volume of about 1.22 × 10 4 Gpc 3 (4.22 × 10 5 Gly 3 or 3.57 × 10 80 m 3). [29] These are distances now (in cosmological time), not distances at the time the light was emitted.

  9. Atomic radius - Wikipedia

    en.wikipedia.org/wiki/Atomic_radius

    Under most definitions the radii of isolated neutral atoms range between 30 and 300 pm (trillionths of a meter), or between 0.3 and 3 ångströms. Therefore, the radius of an atom is more than 10,000 times the radius of its nucleus (1–10 fm ), [ 2 ] and less than 1/1000 of the wavelength of visible light (400–700 nm ).