enow.com Web Search

Search results

  1. Results from the WOW.Com Content Network
  2. Orbital resonance - Wikipedia

    en.wikipedia.org/wiki/Orbital_resonance

    There is a near-resonance between the precession of Saturn's rotational axis and that of Neptune's orbital axis (both of which have periods of about 1.87 million years), which has been identified as the likely source of Saturn's large axial tilt (26.7°).

  3. Kirkwood gap - Wikipedia

    en.wikipedia.org/wiki/Kirkwood_gap

    The most prominent Kirkwood gaps are located at mean orbital radii of: [4] 1.780 AU (5:1 resonance); 2.065 AU (4:1 resonance) 2.502 AU (3:1 resonance), home to the Alinda group of asteroids

  4. Six planets found in synchronized orbit may help solve cosmic ...

    www.aol.com/news/six-planets-found-synchronized...

    The researchers determined that the six planets were in a rare condition called orbital resonance, with their synchronized orbits around the star apparently unchanged since they formed about 4 ...

  5. Stability of the Solar System - Wikipedia

    en.wikipedia.org/wiki/Stability_of_the_Solar_System

    Another common form of resonance in the Solar System is spin–orbit resonance, where the rotation period (the time it takes the planet or moon to rotate once about its axis) has a simple numerical relationship with its orbital period. An example is the Moon, which is in a 1:1 spin–orbit resonance that keeps its far side away from

  6. Resonant trans-Neptunian object - Wikipedia

    en.wikipedia.org/wiki/Resonant_trans-Neptunian...

    In astronomy, a resonant trans-Neptunian object is a trans-Neptunian object (TNO) in mean-motion orbital resonance with Neptune.The orbital periods of the resonant objects are in a simple integer relations with the period of Neptune, e.g. 1:2, 2:3, etc. Resonant TNOs can be either part of the main Kuiper belt population, or the more distant scattered disc population.

  7. Enceladus - Wikipedia

    en.wikipedia.org/wiki/Enceladus

    Enceladus is currently in a 2:1 mean-motion orbital resonance with Dione, completing two orbits around Saturn for every one orbit completed by Dione. [6] This resonance maintains Enceladus's orbital eccentricity (0.0047), which is known as a forced eccentricity. This non-zero eccentricity results in tidal deformation of Enceladus.

  8. List of multiplanetary systems - Wikipedia

    en.wikipedia.org/wiki/List_of_multiplanetary_systems

    The three planets are in an orbital resonance. [148] Kepler-238: Lyra: 19 h 11 m 35 s +40° 38′ 16″ 15.084: 5867: G5IV: 1.06: 5614: unknown: 5: One of the farthest systems from the Sun with a multiplanetary system, and the farthest system where exoplanets were discovered by the Kepler space telescope. Kepler-245: Cygnus: 19 h 26 m 33.4 s ...

  9. Scientists Discovered Mysterious Musical Rhythms in ... - AOL

    www.aol.com/scientists-discovered-mysterious...

    The puffier planets were more likely to be at least close to resonance. Later expanding their sample size to 133, they found the same thing. Subsequent computer simulated systems told the same ...