The length of day on moon is (27.32 EARTH DAYS)
27.32 days is the length of a sidereal day.
The length of a lunar solar day (the time it takes the sun to appear in the same spot overhead) is 29.5 days. This is because as the moon turns, it also travels along its orbit about the sun.
29.5 earth days is one moon day wich is the length of the moons day
Mars has a similar day length to Earth, a little longer at 24h 39m 35s (apparent solar day).
Six planets have more than one moon in our solar system.
Magic.
There are 86400 seconds in a solar day.
29.5 earth days is one moon day wich is the length of the moons day
28 days
Mars has a similar day length to Earth, a little longer at 24h 39m 35s (apparent solar day).
A "Moon" day is the period it takes to make one revolution on it's axis (or Sidereal rotationperiod) this is currently 27.321582 Earth days.For any one spot on the moon, the length of acomplete light/dark cycle is 27.32 Earth days.
An apparent or solar day on Venus is 116.75 days (this is not the same as its rotational period relative to the background stars, which is 243 days).
The largest moon in the solar system is Ganymede, one of the moons of Jupiter.
Six planets have more than one moon in our solar system.
The earth revolves around the the sun & the moon revoves around the earth.At one time the moon comes between the sun and the earth and they all are in a straight line.at that time moon cuts of the light of sun.This is called solar eclipse. if there is a solar eclipse in one spot one mile from there will be a regular day so where you are needs to be the question of when a solar eclipse is coming
Within our Solar System, the Earth is the only planet with one moon.
If you mean "one moon" as the Indians used the phrase to measure time, then the length of a lunar cycle (from one full moon to the next) would be just over 29.5 days.
The Earth is the only planet in our Solar System with one Moon
Its position and apparent movement around the sky. "Apparent solar time" is based on the "apparent solar day", reckoned by defining as 'solar noon' the moment of the Sun's highest altitude above the horizon on any given day. (That's when the Sun crosses the observer's meridian.) Apparent solar days do not have the exact same length (from one solar noon to the next) throughout the year, which is surprising to some at first. This is why the first approaches to creating a solid "standard time" involved determining the length of the 'mean solar day' (average solar day).