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  2. Orbit of Venus - Wikipedia

    en.wikipedia.org/wiki/Orbit_of_Venus

    The planet orbits the Sun once every 225 days [3] and travels 4.54 au (679,000,000 km; 422,000,000 mi) in doing so, [4] giving an average orbital speed of 35 km/s (78,000 mph). Conjunctions and transits

  3. Venus - Wikipedia

    en.wikipedia.org/wiki/Venus

    Winds on Venus move at up to 60 times the speed of its rotation, whereas Earth's fastest winds are only 10–20% rotation speed. ... The orbital space of Venus has a ...

  4. Orbital speed - Wikipedia

    en.wikipedia.org/wiki/Orbital_speed

    In gravitationally bound systems, the orbital speed of an astronomical body or object (e.g. planet, moon, artificial satellite, spacecraft, or star) is the speed at which it orbits around either the barycenter (the combined center of mass) or, if one body is much more massive than the other bodies of the system combined, its speed relative to the center of mass of the most massive body.

  5. List of gravitationally rounded objects of the Solar System

    en.wikipedia.org/wiki/List_of_gravitationally...

    Mean orbital speed [4] km/s: ≈ 220 Axial tilt to the ecliptic: deg. ... Venus, Earth, and Mars) and four giant planets, which can be divided further into two gas ...

  6. Standard gravitational parameter - Wikipedia

    en.wikipedia.org/wiki/Standard_gravitational...

    Venus: 3.248 585 92 (6) × ... The central body in an orbital system can be defined as the ... v is the orbital speed, ω is the angular speed, and T is the orbital ...

  7. Solar System - Wikipedia

    en.wikipedia.org/wiki/Solar_System

    Orbital speed: 720,000 km/h (450,000 mi/h) ... Venus is approximately 0.33 AU farther out from the Sun than Mercury, whereas Saturn is 4.3 AU out from Jupiter, and ...

  8. Kepler's laws of planetary motion - Wikipedia

    en.wikipedia.org/wiki/Kepler's_laws_of_planetary...

    The speed of the planet in the main orbit is constant. ... is the orbital period and is the elliptical semi-major axis, and is the ... Venus 0.724 224.70 7.52 Earth 1 ...

  9. Observations and explorations of Venus - Wikipedia

    en.wikipedia.org/wiki/Observations_and...

    The planet's period of retrograde motion is 20 days on either side of the inferior conjunction. In fact, through a telescope Venus at greatest elongation appears less than half full due to Schröter's effect first noticed in 1793 and shown in 1996 as due to its thick atmosphere. Venus in daylight at 5 p.m. in the southern hemisphere ...