dont look things up on wikipidia bcuz people can change the answers and they most likely r never rightt. wikipedia suckss.
A sidereal year is measured based on the planet's position in space relative to the background stars. A synodic year is measured based on the planet's position relative to the star it rotates around (i.e. the sun) Here's an image that is pretty helpful in visualizing.
The sidereal period is the time it takes for a celestial body to complete one orbit relative to the fixed stars, while the synodic period is the time it takes for a celestial body to return to the same position relative to the Sun as seen from Earth. The relationship between the two periods is influenced by the relative motion of the Earth and the celestial body, and can vary depending on their orbits and positions.
The sidereal period is the time it takes for a celestial body to complete one orbit relative to the fixed stars, while the synodic period is the time it takes for a celestial body to return to the same position relative to the Sun as seen from Earth.
If you are talking about bodies in the solar system, then revolution almost always refers to the orbiting motion of a body around another body. This is the motion that gives us the year on earth. The earth revolves around the sun once in about 365.25 days. Revolution can be a little more complex than this. A sidereal revolution is the orbit of a body as it is observed from the distant stars. Synodic revolution is a revolution as it is observed from the body being orbited, and it brings the orbiting body back to its starting point relative to the sun. These two orbital periods are not the same length. The phases of the moon follow the synodic period; the synodic period is longer than the sidereal period by roughly a day or two.
The Sidereal Period is: 1) The period of revolution of one body around another, with respect to the distant stars. 2) The period of rotation of a body on its axis, with respect to the distant stars. This is often called the "sidereal period of rotation". For example, the Earth's sidereal period of rotation is about 23 hours and 56 minutes. The day is 24 hours because it's based on the rotation of the Earth relative to the position of the Sun in the sky.
1 more sidereal month than synodic month
A sidereal month is the time it takes the moon to complete one orbit of earth. A synodic month is longer than a sidereal month because it takes longer for the moon to go through it's phases
A planet's sidereal year is the time it takes to complete one full orbit around the Sun relative to fixed stars, while its synodic year is the time it takes for the planet to return to the same position in relation to the Earth and the Sun. The synodic year is generally longer than the sidereal year due to the relative motion of Earth and the planet in their orbits. For example, Earth's sidereal year is about 365.25 days, while its synodic year (the time from one vernal equinox to the next) is also about 365.24 days, but for planets like Mars, the difference is more pronounced. This difference affects how we observe and measure planetary positions from Earth.
A sidereal year is measured based on the planet's position in space relative to the background stars. A synodic year is measured based on the planet's position relative to the star it rotates around (i.e. the sun) Here's an image that is pretty helpful in visualizing.
The sidereal period is the time it takes for a celestial body to complete one orbit relative to the fixed stars, while the synodic period is the time it takes for a celestial body to return to the same position relative to the Sun as seen from Earth. The relationship between the two periods is influenced by the relative motion of the Earth and the celestial body, and can vary depending on their orbits and positions.
686.980 earth days, sidereal period; 779.94 earth days, synodic period.
The sidereal period is the time it takes for a celestial body to complete one orbit relative to the fixed stars, while the synodic period is the time it takes for a celestial body to return to the same position relative to the Sun as seen from Earth.
If you are talking about bodies in the solar system, then revolution almost always refers to the orbiting motion of a body around another body. This is the motion that gives us the year on earth. The earth revolves around the sun once in about 365.25 days. Revolution can be a little more complex than this. A sidereal revolution is the orbit of a body as it is observed from the distant stars. Synodic revolution is a revolution as it is observed from the body being orbited, and it brings the orbiting body back to its starting point relative to the sun. These two orbital periods are not the same length. The phases of the moon follow the synodic period; the synodic period is longer than the sidereal period by roughly a day or two.
The completion of a moon's revolution around its planet is called an "orbital period" or "lunar month." For Earth’s Moon, this period is approximately 27.3 days, known as the sidereal month. However, the more commonly referenced lunar month in relation to the phases of the Moon is about 29.5 days, called the synodic month.
It takes one year for the earth to make a revolution around the sun.Depending upon your reference point, it takes 27.3 days for the moon to orbit the earth if you use the earth as the reference point. This is called the sidereal month. If you use the sun as the reference point, then it takes 29.5 days for the moon to orbit the earth. This is called the synodic month.
The Sidereal Period is: 1) The period of revolution of one body around another, with respect to the distant stars. 2) The period of rotation of a body on its axis, with respect to the distant stars. This is often called the "sidereal period of rotation". For example, the Earth's sidereal period of rotation is about 23 hours and 56 minutes. The day is 24 hours because it's based on the rotation of the Earth relative to the position of the Sun in the sky.
The Moon requires approximately 27.3 days to complete one revolution around the Earth, a period known as a sidereal month. However, due to the Earth's own movement around the Sun, the time from one full moon to the next (a synodic month) is about 29.5 days. The Moon's orbit is elliptical, which also affects its speed and distance from Earth during its revolution.