The ecliptic. Because it is the plane that contains the earth as it orbits the sun, by definition it is also the plane that contains the sun as we observe it in its yearly journey through the stars.
For moons to have an orbital resonance, there must be at least two moons orbiting the planet. Orbital resonance occurs when the orbital periods of the moons are related by a ratio of two small integers, such as 1:2 or 2:3.
Neptune has 13 known moons and an orbital period of about 60190 Earth days.
The orbital periods of Jupiter's moons are related to their average orbital radii through Kepler's Third Law of planetary motion, which states that the square of the orbital period (T) of a moon is proportional to the cube of the semi-major axis (r) of its orbit. Mathematically, this can be expressed as ( T^2 \propto r^3 ). This means that moons that are farther from Jupiter take longer to complete an orbit compared to those that are closer, resulting in a clear relationship between distance and orbital period.
Uranus.
The orbital plane of a stellar system can be oriented in any way in relation to the plane of the Milky Way Galaxy. Our solar system, for example, is almost perpendicular to the plane of the Milky Way Galaxy.
For moons to have an orbital resonance, there must be at least two moons orbiting the planet. Orbital resonance occurs when the orbital periods of the moons are related by a ratio of two small integers, such as 1:2 or 2:3.
No the moon doesn't have orbitals.
Neptune has 13 known moons and an orbital period of about 60190 Earth days.
There are about 63 known moons of Jupiter but the Galilean moons are the 4 moons visible and Ganymede ,the largest found by Galileo Galilee in January 7 1610.The orbital speed of the Jovian moons vary where the Jupiter's magnetic field is very strong.Only a mean speed can be used for comparison.The four moons and their orbital speed compared to the orbital speed of Earth's moon are:Jovian Moons Orbital speed/ Orbital speed Ratio(km/s) (Earth's moon)1. Io orbital speed 2.75 km/sEarth's moon orbital speed 1.03 km/s Ratio 1: 2.672.Europa orbital speed 2.187 km/sEarth's moon orbital speed 1.03 km/s Ratio !: 2.123. Callisto orbital speed 1.732 km/sEarth's moon orbital speed 1.03 km/s Ratio 1: 1.684.Ganymede orbital speed 1.305 km/sEarth moon's orbital speed. 1.03 km/s Ratio 1: 1.27
Planets with moons may indeed have Earth-like eclipses. Eclipses happen when moon orbital plane intersects with planet orbital plane with respect to its star. Eclipses can only happen however if angular diameter of the moon is similar to (or greater than) angular diameter of star as seen from planet's surface, which is quite a rare condition. In the whole Solar System moon-eclipses only happen on Earth.
Pluto
Pluto
Orbital Bodies.
A Px orbital has 1 nodal plane. This nodal plane passes through the nucleus and divides the orbital into two lobes along the x-axis.
The orbital period of Deimos, one of Mars' moons, is approximately 30.3 hours.
Same as it's orbital period, about 27.32 days.
If the Moon's orbital plane were exactly the same as the ecliptic, there would be solar eclipses at every new moon and lunar eclipses at every full moon. They would be ordinary, and we would lose our sense of wonder about them.