It takes 243 Earth days to rotate once on its axis (sidereal day). The planet’s orbit around the Sun takes 225 Earth days, compared to the Earth’s 365. A day on the surface of Venus (solar day) takes 117 Earth days. Venus rotates in the opposite direction to most other planets. ...
Of all the planets in oursolar system, Venus rotates the slowest: it takes around 243 Earth days to complete one spin (compared to Earth’s roughly 24 hours). Venus andUranusare the only planets with retrograde rotation. This means the direction of their spin (clockwise, as seen from above...
The surface of Venus is effectively isothermal, which means that their is virtually no variation in Venus' surface temperature between day and night, or the equator and the poles. The planet's minute axial tilt – less than 3° compared to Earth's 23° – also minimizes seasonal temperature ...
Venus and Earth Compared Venus, the second planet from the Sun, lies, on average, 108 million km from the Sun, about 30% closer than the Earth. Venus is often referred to as our sister planet because of similarities in size, mass, density and volume. It is believed that both planets s...
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The Surface Gravity of Venus is 8.87 compared to Earth which for purpose of this site is 1. The following gasses can be found in the Venus's Atmosphere : 96.5% Carbon Dioxide (CO2). 3.5% Nitrogen (N2). More information and the source for the moon can be found at N.A.S.A. The...
Venus is one among the four terrestrial planets within the system, meaning that it’s a rocky body like Earth. It is almost like Earth in size and mass, and is typically described as Earth’s “sister” or “twin”. The diameter of Venus is a bit small compared to Earth. Venus has ...
Venus and Earth Compared Venus, the second planet from the Sun, lies, on average, 108 million km from the Sun, about 30% closer than the Earth. Venus is often referred to as our sister planet because of similarities in size, mass, density and volume. It is believed that both planets ...
compared with 5.52 for Earth. They also result in acomparablesurface gravity—humans standing on Venus would possess nearly 90 percent of their weight on Earth. Venus is more nearly spherical than most planets. A planet’s rotation generally causes a bulging at the equator and a slight flattenin...
Because of its dense atmosphere and its highly circular rotation, Venus experiences very little in the way of temperature variations during the course of a year. Similarly, its axial tilt of 2.64° (compared to Earth’s 23.44°) is the second-lowest in the Solar System, behind Mercury’s ex...