Galileo's Law Of Odd Numbers
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classical mechanics Classical mechanics is a Theoretical physics, physical theory describing the motion of objects such as projectiles, parts of Machine (mechanical), machinery, spacecraft, planets, stars, and galaxies. The development of classical mechanics inv ...
and
kinematics In physics, kinematics studies the geometrical aspects of motion of physical objects independent of forces that set them in motion. Constrained motion such as linked machine parts are also described as kinematics. Kinematics is concerned with s ...
, Galileo's law of odd numbers states that the distance covered by a falling object in successive equal time intervals is linearly proportional to the odd numbers. That is, if a body falling from rest covers a certain distance during an arbitrary time interval, it will cover 3, 5, 7, etc. times that distance in the subsequent time intervals of the same length. This mathematical model is accurate if the body is not subject to any forces besides uniform gravity (for example, it is falling in a vacuum in a uniform
gravitational field In physics, a gravitational field or gravitational acceleration field is a vector field used to explain the influences that a body extends into the space around itself. A gravitational field is used to explain gravitational phenomena, such as ...
). This law was established by
Galileo Galilei Galileo di Vincenzo Bonaiuti de' Galilei (15 February 1564 – 8 January 1642), commonly referred to as Galileo Galilei ( , , ) or mononymously as Galileo, was an Italian astronomer, physicist and engineer, sometimes described as a poly ...
who was the first to make quantitative studies of
free fall In classical mechanics, free fall is any motion of a physical object, body where gravity is the only force acting upon it. A freely falling object may not necessarily be falling down in the vertical direction. If the common definition of the word ...
.


Explanation


Using a speed-time graph

The graph in the figure is a plot of speed versus time. Distance covered is the area under the line. Each time interval is coloured differently. The distance covered in the second and subsequent intervals is the area of its trapezium, which can be subdivided into triangles as shown. As each triangle has the same base and height, they have the same area as the triangle in the first interval. It can be observed that every interval has two more triangles than the previous one. Since the first interval has one triangle, this leads to the odd numbers.


Using the sum of first ''n'' odd numbers

From the equation for uniform linear acceleration, the distance covered s = u t + \tfrac a t^2 for initial speed u = 0, constant acceleration a (acceleration due to gravity without air resistance), and time elapsed t, it follows that the distance s is proportional to t^2 (in symbols, s \propto t^2), thus the distance from the starting point are consecutive squares for integer values of time elapsed. The middle figure in the diagram is a visual proof that the sum of the first n odd numbers is n^2.RP Olenick et al.
''The Mechanical Universe: Introduction to Mechanics and Heat''
/ref> In equations: : That the pattern continues forever can also be proven algebraically: \begin \sum_^n (2\,k-1)&= \frac\,\left( \sum_^n (2\,k-1)+ \sum_^n (2\,(n-k+1)-1) \right)\\ &= \frac\,\sum_^n (2\,(n+1)-1-1)\\ &= n^2 \end To clarify this proof, since the nth odd positive integer is m \,\colon=\, 2 n - 1, if S \,\colon=\, \sum_^n (2\,k-1) \,=\, 1 + 3 + \cdots + (m-2) + m denotes the sum of the first n odd integers then \begin S + S &=\;\; 1 &&+\;\; 3 &&\;+ \cdots + (m-2) &&+\;\; m \\ &+\;\; m &&+ (m-2) &&\;+ \cdots +\;\; 3 &&+\;\; 1 \\ &=\; (m+1) &&+ (m+1) &&\;+ \cdots + (m+1) &&+ (m+1) \quad \text n \text\\ &=\; n \, (m+1) && && && && \\ \end so that S = \tfrac \, n \, (m+1). Substituting n = \tfrac (m + 1) and m + 1 = 2 \, n gives, respectively, the formulas 1 + 3 + \cdots + m \;=\; \tfrac (m+1)^2 \quad \text \quad 1 + 3 + \cdots + (2 \, n - 1) \;=\; n^2 where the first formula expresses the sum entirely in terms of the odd integer m while the second expresses it entirely in terms of n, which is m's ordinal position in the list of odd integers 1, 3, 5, \ldots.


See also

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Notes and references

Classical mechanics Kinematics {{classicalmechanics-stub