24 hours. Relative to the stars (the "real rotation"), it is about 23h56m.
24 hours. Relative to the stars (the "real rotation"), it is about 23h56m.
24 hours. Relative to the stars (the "real rotation"), it is about 23h56m.
24 hours. Relative to the stars (the "real rotation"), it is about 23h56m.
the island of Razor Ultra Pro Black Label
Mars, with a rotation period of 24 hours 37 minutes 23 seconds (time taken for one spin on its axis relative to background stars).
A lunar day, also known as a "day" on the Moon, is measured as the time it takes for the Moon to complete one rotation on its axis relative to the Sun. This period is equivalent to about 29.5 Earth days.
Mars, with a rotation period of 24 hours 37 minutes 23 seconds (time taken for one spin on its axis relative to background stars).
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.
Most velocities are measured relative to Earth.Most velocities are measured relative to Earth.Most velocities are measured relative to Earth.Most velocities are measured relative to Earth.
Mercury has the shortest rotation period, taking about 59 Earth days to complete one rotation. Venus has an unusual rotation period of about 243 Earth days, which is longer than its orbital period around the Sun. Earth rotates once every 24 hours, while Mars has a rotation period of approximately 24.6 hours. Thus, the sequence from shortest to longest rotation periods is Mercury, Earth, Mars, and then Venus.
The rotation period of Neptune is 16.1 earth hours.
Sidereal rotation refers to the rotation of a celestial body (such as a planet) relative to the fixed stars. On Earth, the sidereal rotation period is about 23 hours, 56 minutes, and 4 seconds, which is slightly shorter than a solar day due to the Earth's orbit around the Sun. This rotation period is used in astronomy and space exploration to track the positions of objects in the sky.
The rotation period of Venus is 243.0187 Earth days
A planet's period of rotation refers to the time it takes for the planet to complete one full rotation on its axis. This is what determines the length of a day on that planet. For example, Earth's period of rotation is approximately 24 hours, which is why we have a 24-hour day.
The rotation period of a geostationary satellite is equal to one sidereal day, which is approximately 23 hours, 56 minutes, and 4 seconds. This period matches the time it takes for the satellite to orbit the Earth once and remain fixed relative to a specific point on the Earth's surface.