Venus Day vs Year
Day vs Year
Day vs Year
A Temporal Paradox. Venus spins so slowly that its sidereal day outlasts its orbital year. Time here is defined by a backward sunrise.
- π Rotation: 243 Earth days (Backward/Retrograde).
- βοΈ Solar Day: 117 Earth days from sunrise to sunrise.
- π The Year: 225 Earth days to circle the Sun.
Day vs Year
A Temporal Paradox. Venus spins so slowly that its sidereal day outlasts its orbital year. Time here is defined by a backward sunrise.
- π Rotation: 243 Earth days (Backward).
- βοΈ Solar Day: 117 Earth days from noon to noon.
- π The Year: 225 Earth days to circle the Sun.
The Venusian Year
Swift Revolution. Venus completes its journey around the Sun in just 225 days, moving significantly faster than Earth.
- π Duration: 224.7 Earth Days.
- π Velocity: 35.02 km/s orbital speed.
- π Orbit: Near-perfect circle (Eccentricity < 0.01).
Paper
CHRONOS LOG: VENUS β³
A day longer than a year. A Sun that rises in the West.
Sources
SIDEREAL DAY
Venus takes **243 Earth days** to complete one rotation, making it the slowest spinner in the system.
ROTATION DATAORBITAL YEAR
A year on Venus (one orbit around the Sun) lasts **225 Earth days**, shorter than its sidereal day.
ORBITAL STATSSOLAR DAY (DIURNAL)
Due to the combination of rotation and orbit, the Sun rises every **117 Earth days**.
DAY/NIGHT CYCLEThe Morning Star
Venus: The hottest planet in our solar system due to runaway greenhouse effects.
Day vs Year
Sidereal Day: 243 Earth Days
Orbital Year: 225 Earth Days
Rotation: Retrograde (Clockwise)