The time the planet takes to orbit (Orbital Period) round the Sun is 224.701 days or roughly 0.6 Earth Years. The length of a day on the planet is 2802 hours, i.e. the time it takes to revolve once on its axis. The Average Temperature of the planet is 737K/464C. The Surface Pre...
Venusian year (sidereal period of revolution)224.7 Earth days maximum visual magnitude−4.6 mean synodic period*584 Earth days mean orbital velocity35 km/sec radius (mean)6,051.8 km surface area4.6 × 108km2 mass4.87 × 1024kg mean density5.24 g/cm3 ...
Venus’s orbital period (a year) is 225 Earth days. Its rotational period (in a retrograde manner) is 243 Earth days. The combination of these two rotations makes the solar day on Venus ∼117 Earth days long, so any given place on the planet (except the poles) is Sun-illuminated ...
This is the planet's second perihelion crossing of the apparition, taking place 225 days (one Venus orbital period) after the first, back in July 2024.Around February 20th, observers at low-Southern latitudes see Venus return to the same relative spot above the local horizon that it had ...
Although Venus' orbital period is only 224.7 days, its synodic period is 583.9 days. Due to its orbital inclination, most inferior conjunctions of Venus do not result in a transit because the planet passes too far above or below the ecliptic plane and does not cross the solar disk.Mason...
Venus orbital period (a year) lasts about 225 Earth days, and a sidereal day (rotation in retrograde motion) lasts about 243 Earth days1. Venus is similar to Earth in terms of size (0.95 of Earth’s radius), mass (0.814 of Earth’s), bulk density (0.95 of Earth’s), and gravity ...
Orbital and physical characteristics are given in Table 1, backmatter. Venus is never far from the Sun in the sky, reaching its greatest elongation of 45° to 47° about 72 days before and after inferior conjunctions, which recur at intervals of about 584 days. At greatest brilliancy the ...
And, as noted earlier, Venus’ rotation is backwards, relative to Earth and the other bodies in the Solar System. Technically, this means that its rotational period is -243,025 days. It also means that if you could view the Solar System from the position above its celestial north pole, ...
Venus is the second planet from the Sun, which orbits around the Sun every 224 Earth days. It has the longest rotational period (243 days) of any planet in the Solar System, and rotates in the opposite direction to most other planets. It does not have an
Venus is the second planet in our solar system close to the Sun. Venus can cast shadows and on rare occasion, visible to the attention in broad daylight. After the Moon, it is the second-brightest natural object in Earth's night sky.