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  2. 9 Free, Easy-To-Use Budget Templates and Spreadsheets - AOL

    www.aol.com/finance/9-free-easy-budget-templates...

    2. Mint’s Simple Budget Template. Where to get it: Mint. Although Mint also offers more complex budgeting template options, this simple one lives up to its name. It’s perfect for beginning ...

  3. Rotation period (astronomy) - Wikipedia

    en.wikipedia.org/wiki/Rotation_period_(astronomy)

    Typically, the stated rotation period for a giant planet (such as Jupiter, Saturn, Uranus, Neptune) is its internal rotation period, as determined from the rotation of the planet's magnetic field. For objects that are not spherically symmetrical, the rotation period is, in general, not fixed, even in the absence of gravitational or tidal forces.

  4. Neptune - Wikipedia

    en.wikipedia.org/wiki/Neptune

    Neptune's second-known satellite (by order of discovery), the irregular moon Nereid, has one of the most eccentric orbits of any satellite in the Solar System. The eccentricity of 0.7512 gives it an apoapsis that is seven times its periapsis distance from Neptune. [j] From July to September 1989, Voyager 2 discovered six moons of Neptune. [162]

  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. Poles of astronomical bodies - Wikipedia

    en.wikipedia.org/wiki/Poles_of_astronomical_bodies

    Venus rotates clockwise, and Uranus has been knocked on its side and rotates almost perpendicular to the rest of the Solar System. The ecliptic remains within 3° of the invariable plane over five million years, [ 2 ] but is now inclined about 23.44° to Earth's celestial equator used for the coordinates of poles.

  7. Deferent and epicycle - Wikipedia

    en.wikipedia.org/wiki/Deferent_and_epicycle

    Both circles rotate eastward and are roughly parallel to the plane of the Sun's apparent orbit under those systems . Despite the fact that the system is considered geocentric , neither of the circles were centered on the earth, rather each planet's motion was centered at a planet-specific point slightly away from the Earth called the eccentric .

  8. Orbital inclination - Wikipedia

    en.wikipedia.org/wiki/Orbital_inclination

    The moons in the first category, with the exception of Neptune's moon Triton, orbit near the equatorial plane. He concluded that these moons formed from equatorial accretion disks . But he found that the Moon, although it was once inside the critical distance from the Earth, never had an equatorial orbit as would be expected from various ...

  9. Rings of Neptune - Wikipedia

    en.wikipedia.org/wiki/Rings_of_Neptune

    Its namesake is William Lassell, the English astronomer who discovered Neptune's largest moon, Triton. [20] This ring is a faint sheet of material occupying the space between the Le Verrier ring at about 53,200 km and the Arago ring at 57,200 km. [ 4 ] Its average normal optical depth is around 10 −4 , which corresponds to an equivalent depth ...