I get 517.33 miles per hour.
I used 3,970 miles for the Earth's radius, and 23hours 56minutes
for the period of one complete rotation.
Only at the equator. The linear distance covered by 1 degree of longitude gets progressively smaller as you progress towards the poles, but 1 degree of latitude remains constant.
That is an angular measurement of ten degrees. The linear distance would depend on your latitude.
In a linear molecule like carbon dioxide, the characteristic angle between the atoms is 180 degrees. This is because the molecule is linear, with two oxygen atoms bonded to a central carbon atom in a straight line.
they are both imaginary lines that run round the earth, to show where a point is on the earths surface. the unit to show these are degrees. latitude are lines running across the earth and longitude are lines running down the earth. an easy way to remember this- lAtitude goes Across(they both have letter a) lOngitude does dOwn"(they both have o)
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.
G is a measure of linear acceleration. For rotational motion it is necessary to multiply the degrees by the distance from the centre of rotation (radius of rotation).
i believe it is linear
Only at the equator. The linear distance covered by 1 degree of longitude gets progressively smaller as you progress towards the poles, but 1 degree of latitude remains constant.
"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 question cannot be answered simply. A degree is a measure of angular displacement whereas an inch is a measure of linear displacement. If the angular displacement (in degrees) were measured at a distance r inches from some fixed point (the centre of rotation), then the linear displacement would be pi*r/180 inches.
In 2-dimensions, the formula for rotation through d degrees is [post-]multiplication by the matrix [cos(d) sin(d)] [-sin(d) cos(d)]
That is an angular measurement of ten degrees. The linear distance would depend on your latitude.
To convert angular displacement to linear displacement, you need to know the radius of the circle or rotation and the angle of rotation in radians. By multiplying the radius by the angle in radians, you can calculate the linear displacement.
Linear speed is directly proportional to the radius of rotation and the angular velocity. The equation that relates linear speed (v), angular velocity (ω), and radius (r) is v = rω. This means that the linear speed increases as either the angular velocity or the radius of rotation increases.
The angular acceleration formula is related to linear acceleration in rotational motion through the equation a r, where a is linear acceleration, r is the radius of rotation, and is angular acceleration. This equation shows that linear acceleration is directly proportional to the radius of rotation and angular acceleration.
the no. of times the figure fits into itself is called order of rotation.
The lines on a globe which run north and south are called meridians, or lines of longitude. They run from the North Pole to the South Pole, and only in pairs do they "circle" the Earth.They are used to calculate distance between points on the Earth's surface in an east-west direction. Beginning at the arbitrarily-defined Prime Meridian (0° longitude), they are measured in degrees east or west of that line, which is an angular measurement that can be translated into rough linear distance.Used in conjunction with the lines of latitude (measuring distance north or south of the equator), they can define any point on the surface of the Earth.