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The linear speed of the Earth's rotation at any latitude can be calculated by multiplying the cosine of the latitude by the equatorial rotational speed of the Earth, which is approximately 1670 kilometers per hour (1037 miles per hour). At latitude 60.24 degrees north, the linear speed of the Earth's rotation would be approximately 835 kilometers per hour (519 miles per hour).
The Earth rotates at a rate of slightly over 15 arc-seconds per second.The actual speed of rotation depends on latitude. It's greatest at the equator. At the equator, the Earth's rotation speed is about 465 meters per second.
yes. rotation at equator is roughly 1000 mph, rotation at any other latitude is about cos (latitude) * 1000 mph.
Earth's rotation speed is gradually decreasing, as a result of the tides.
The circumference around the Earth at different latitudes varies, from 40,075 km at the equator, to 26,291 km at 49° latitude, to 0km at the axis of rotation (i.e. the North and South poles). Thus, as the Earth spins around it's axis, different latitudes will cover different distances within the same time frame. And since speed (and velocity) are calculated by dividing distance by time, the speed (and velocity) will therefore decrease as you approach the poles.
The linear speed of the Earth's rotation at any latitude can be calculated by multiplying the cosine of the latitude by the equatorial rotational speed of the Earth, which is approximately 1670 kilometers per hour (1037 miles per hour). At latitude 60.24 degrees north, the linear speed of the Earth's rotation would be approximately 835 kilometers per hour (519 miles per hour).
The Earth rotates at a rate of slightly over 15 arc-seconds per second.The actual speed of rotation depends on latitude. It's greatest at the equator. At the equator, the Earth's rotation speed is about 465 meters per second.
The magnitude of the Coriolis force is influenced by the speed of the object, the latitude of the object, and the Earth's rotation rate. Objects moving faster or situated at higher latitudes will experience a greater Coriolis force.
Mars sidereal rotation is 1.025 day Earths sidereal rotation is 0.997 day. Mars rotates on its axis at a speed similar to Earth's,averagiung 25 degrees,although in the past that angle has been as great as 60 degrees. This means that Mars,like Earth,has distinct seasons
yes. rotation at equator is roughly 1000 mph, rotation at any other latitude is about cos (latitude) * 1000 mph.
The earth's orbital speed has no influence or effect on its rotation.
Earth's rotation speed is gradually decreasing, as a result of the tides.
"Quick and dirty":Earth radius = 4,000 milesCircumference = 2 pi R = (8,000 pi) milesRotation period = 24 hoursSpeed of a point on the equator = circumference/period = 8,000 pi miles/24 hours-- That's the speed on the equator = zero latitude.-- The north pole is 90 degrees latitude, and the rotation speed there is zero.-- A quantity that's full-size at zero degrees and zero at 90 degrees is varyingin proportion to the cosine of the latitude.Speed at 35 degrees latitude = ( 8,000 pi/24 ) x cos(35) = 858 miles per hour.Note:Don't get into an argument with anybody who comes along and says no, that'snot correct, it's actually 865, or 832, or 857.294 etc. Every number in my solutionis rounded, except for the zero degrees and 90 degrees. So the answer I gotis correct to an 'order of magnitude' and maybe a couple of significant figures.It gives you 'feeling' for the actual speed of a point on the 35th parallel, but Iwould not enter it in a contest where points are awarded for precision.
The circumference around the Earth at different latitudes varies, from 40,075 km at the equator, to 26,291 km at 49° latitude, to 0km at the axis of rotation (i.e. the North and South poles). Thus, as the Earth spins around it's axis, different latitudes will cover different distances within the same time frame. And since speed (and velocity) are calculated by dividing distance by time, the speed (and velocity) will therefore decrease as you approach the poles.
In terms of angular velocity, because it takes roughly 86,400 seconds per 1 Earth revolution, it is:2 * pi / 86400 = 7.269 * 10-5 rad/sLinear velocity of a point on Earth's surface due to rotation depends on latitude. On equator it is about 1,674.4 km/h and obviously 0 km/h on either pole.
The speed of rotation is greatest at the equator; 1038 miles per hour.
depends on the flying altitude, and latitude The answer is not as straightforward as the question. To stay in sunlight, an object needs to fly west at a speed equal to the Earth's rotation. At the equator, this speed equals [40705.02km / 86400 sec/day] = 471.1 meters/sec or approximately 1.4 times the speed of sound. At the poles, one can hypothetically sit in a chair and stay in sunlight for days. The speed required in between these extremes varies with the sine of the latitude. At around 47 degrees North and south latitude, one can stay in daylight at less than the speed of sound.