The final anomaly between the two worlds is the rotation of Venus. Firstly its axis of rotation is inclined at 177.36 degrees . This means that Venus rotates in a retrograde direction from east to west, making the Sun rise in the west and set in the east. Further to this the rotation i...
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The final anomaly between the two worlds is the rotation of Venus. Firstly its axis of rotation is inclined at 177.36 degrees . This means that Venus rotates in a retrograde direction from east to west, making the Sun rise in the west and set in the east. Further to this the rotation i...
CAN the rotation period of Venus be commensurate with its synodic period? If the rotation period is 243.16 days retrograde, the axis of Venus which points toward the Earth at one inferior conjunction will point toward the Earth at all subsequent inferior conjunctions. This value for the rotation...
Why might Venus have the slow retrograde rotation that is observed? How does the planet Venus rotate? Why does the planet Venus show phases similar to the moon? Why do planets rotate on their axis? Why do outer planets rotate faster?
ACCORDING to my observations, this planet seems to have a very slow rotation, round an axis almost perpendicular to the plane of the orbit. Thus, a dusky spot remained fixed with regard to the terminator for three or four hours on the same dates, as well as on the following days. The ...
[Thanda] observed that the planet’s rotation appears to be speeding up slightly, and furthermore, his estimates of the orbital axis were within 0.01 degrees of the International Astronomical Union’s (IAU) values. [Note: Venus is a bit confusing — one planetary rotation, 243 Earth days, ...
Three related activities that use Magellan data to derive improved estimates of the rotation period and direction of the spin axis of Venus are discussed. These are the computation of the Magellan geodetic control network, the use of measurement landmarks identified in overlapping image strips to ...
side of the planet to expand and lose pressure, called athermal tide. The hot air races westward, toward the dark side of the planet, where it’s cooler. The clouds also moved from the equator toward either of the planet’s poles, distributing the momentum needed for fast super-rotation....
Mercury’s rotation is oriented so that its axis of rotation is nearly perpendicular to its angle of orbit. This means that in the polar regions, the sunlight hits the surface at a constant grazing angle. The interiors of some craters are in permanent shadow, and could have tiny deposits of...