Because the Moon orbits the Earth whereas the Sun and stars do not. So the Moon has real motion apart from what the rotation of the Earth appears to give it. Thus the Moon rises in the East about 20 minutes sooner every day.
Synodic rotation refers to the time it takes for a celestial body to complete a full rotation relative to the Sun as seen from Earth. It is often longer than the body's actual rotation period due to the Earth's orbital motion. For example, the synodic rotation of Mercury is about 176 Earth days, while its actual rotation period is around 59 Earth days.
A complete rotation which takes up 1 day or 24 hours.
Yes........and no. There are two definitions of "day". The 243 Earth days is the rotation period known as the sidereal day. However there is also the "solar day". This depends on a planet's orbital motion as well as its spin. That is only about 117 Earth days for Venus.
Astronomers use the term "sidereal period" to describe the time it takes for a planet to orbit the sun relative to the stars. Sidereal periods are measured based on the apparent motion of a planet against the background of fixed stars rather than against the sun. This allows for more precise measurements of a planet's orbital period.
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 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.
A sidereal month lasts about 27.3 days and is based on the time it takes the Moon to complete one orbit around the Earth relative to the fixed stars. This is slightly shorter than a synodic month, which is the time between two consecutive occurrences of the same phase, such as full moon to full moon, and lasts about 29.5 days.
A synodic month is about 29.53 days long. It is the length of time it takes for the Moon to return to the same position in the sky, relative to the Sun, as viewed from Earth. This is slightly longer than the Moon's orbital period due to the Earth's orbit around the Sun.
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 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.
30 days in September, April, June and November - all the rest have 31, except for February, which has 28 (except in a Leap Year, when it has 29). Months are linked to the Moon, but there are different ways of measuring a month. The sidereal month is defined as the Moon's orbital period in a non-rotating frame of reference which is about 27 days, 7 hours, 43 minutes, 11.6 seconds. A synodic month is the most familiar lunar cycle, defined as the time interval between two consecutive occurrences of a particular phase such as new moon or full moon. It is about 29 days, 12 hours, 44 minutes, 2.8 seconds. The tropical month is the average time for the Moon to pass twice through the same equinox point of the sky. It is 27.32158 days, very slightly shorter than the sidereal month (27.32166) days, because of precession of the equinoxes. Unlike the sidereal month, it can be measured precisely. An anomalistic month is the average time the Moon takes to go from perigee to perigee - the point in the Moon's orbit when it is closest to Earth. An anomalistic month is about 27.55455 days on average. The draconic month or nodal month is the period in which the Moon returns to the same node of its orbit; the nodes are the two points where the Moon's orbit crosses the plane of the Earth's orbit. Its duration is about 27.21222 days on average.
Because the Moon orbits the Earth whereas the Sun and stars do not. So the Moon has real motion apart from what the rotation of the Earth appears to give it. Thus the Moon rises in the East about 20 minutes sooner every day.
It takes roughly one month for the moon to orbit (loosely, to revolve around) the earth - the moon's angle to the sun causing the moon's apparent phases as it does so. Examined in greater detail, here are various distinctions in exactly how the orbit can be interpreted: 1) The sidereal month - the time it takes to orbit the earth with respect to fixed distant stars = about 27.3 days 2) The synodic month - with respect to the sun, when it reaches the same apparent phase = about 29.5 days. (Longer than the sidereal month because the earth has advanced in its orbit around the sun during the month) 3) tropical month - with respect to where the sun is at the vernal equinox = about 27.3 days (barely less than sidereal month) 4) anomalistic month, the interval between perigees or closest point of approach to the earth = about 27.55 days. Note that the same side of the moon faces the earth because its rotational period (spin on its axis) is equal to its orbital period, i.e., tidally locked; but because it is sometimes closer and sometimes further from the earth where the spin and orbit don't "match" there appears to be a slight apparent wobble or libration which allows us to see slightly around the moon's edges. 5) draconic or nodical month - with respect to the ascending node (crossing the orbital plane) = about 27.21 days.
30 days in September, April, June and November - all the rest have 31, except for February, which has 28 (except in a Leap Year, when it has 29). Months are linked to the Moon, but there are different ways of measuring a month. The sidereal month is defined as the Moon's orbital period in a non-rotating frame of reference which is about 27 days, 7 hours, 43 minutes, 11.6 seconds. A synodic month is the most familiar lunar cycle, defined as the time interval between two consecutive occurrences of a particular phase such as new moon or full moon. It is about 29 days, 12 hours, 44 minutes, 2.8 seconds. The tropical month is the average time for the Moon to pass twice through the same equinox point of the sky. It is 27.32158 days, very slightly shorter than the sidereal month (27.32166) days, because of precession of the equinoxes. Unlike the sidereal month, it can be measured precisely. An anomalistic month is the average time the Moon takes to go from perigee to perigee - the point in the Moon's orbit when it is closest to Earth. An anomalistic month is about 27.55455 days on average. The draconic month or nodal month is the period in which the Moon returns to the same node of its orbit; the nodes are the two points where the Moon's orbit crosses the plane of the Earth's orbit. Its duration is about 27.21222 days on average.
There are a lot of ways of looking at this depending on your relation to the Earth/moon system:The Moon's orbital period in a non-rotating frame of reference is 27.32 days (27 days, 7 hours, 43 minutes, 11.6 seconds). This is the sidereal month. It is measured by observing how long it takes the Moon to pass a fixed star.A synodic month is 29.53 days (29 days, 12 hours, 44 minutes, 2.8 seconds) It is measured from New Moon to New Moon. This is the most common way of expressing the lunar cycle.An anomalistic month is the Moon's orbital period measured from perigee to perigee - the point in the Moon's orbit when it is closest to Earth. An anomalistic month is about 27.55 dayson average.The tropical month is the time for the Moon to return to the same ecliptic longitude, i.e. measured from the equinox; it is slightly shorter than the sidereal month because of precession of the equinoxes.The draconic month or nodal month is the period in which the Moon returns to the same node of its orbit (one of the two points where the Moon's orbit crosses the plane of the Earth's orbit). Its duration is about 27.21 days on average.