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Eccentricity – Formula for Circle, Ellipse, Parabola and Hyperbola

Let’s discuss Eccentricity definition, Eccentricity formula, the Eccentricity of the Circle, Eccentricity of Parabola, the Eccentricity of Ellipse and Eccentricity of Hyperbola

  • Eccentricity Definition - Eccentricity can be defined by how much a Conic section (a Circle, Ellipse, Parabola or Hyperbola) actually varies from being circular.

  • A Circle has an Eccentricity equal to zero, so the Eccentricity shows you how un - circular the given curve is. Bigger Eccentricities are less curved.


Eccentricity Formula

In Mathematics, for any Conic section, there is a locus of a point in which the distances to the point (Focus) and the line (known as the directrix) are in a constant ratio. This ratio is referred to as Eccentricity and it is denoted by the symbol “e”.


The formula to find out the Eccentricity of any Conic section can be defined as

Eccentricity, Denoted by \[e = \frac{c}{a}\]


Where,

c is equal to the distance from the center to the Focus


a  is equal to the distance from the center to the vertex


So we can say that for any Conic section, the general equation is of the quadratic form:


\[Ax^2 + Bxy + Cy^2 + Dx + Ey + F\] and this equation equals zero.


Now let us discuss the Eccentricity of different Conic sections namely Parabola, Ellipse and Hyperbola in detail.


Eccentricities of Circle, Parabola, Ellipse and Hyperbola

The Eccentricity of Circle

  • A Circle can be defined as the set of points in a plane that are equidistant from a fixed point in the plane surface which is known as the “centre”. 

  • Now, you might think about what is the radius. The term “radius” is used to define the distance from the centre and the point on the Circle. 

  •  If the centre of the Circle is at the origin, it becomes easy to derive the equation of a Circle. 

We can derive the equation of the Circle is derived using the below-given conditions.


In a given Circle if “r” is equal to the radius and C (h, k) is equal to the centre of the Circle, then by the definition of Circle and Eccentricity, we get,


| CP | = radius(r)


We know that the formula to find the distance is,


\[\sqrt{(x-h)^2+(y-k)^2}\]= radius(r)


Taking Square on both the sides, we get the following equation,


\[(x-h)^2+(y-k)^2 = radius ^2\]


Thus, the equation of the Circle with center C (h, k) and radius equal to “r” can be written as \[(x –h)^2+( y–k)^2= r^2\]


Also, e = 0 for a Circle.


The Eccentricity of Parabola

  • A Parabola in Mathematics is defined as the set of points P in which the distances from a fixed point F (Focus) in the plane are equal to their distances from a fixed-line l(directrix) in the plane. 

  • In other words, we can say that the distance from the fixed point in a plane bears a constant ratio equal to the distance from the fixed line in a plane.

Therefore, the Eccentricity of the Parabola is always equal to 1 ( e=1)

The general equation of a Parabola can be written as x2 = 4ay and the Eccentricity is always given as 1.


Fun Fact: Whenever a projectile is launched it covers a Parabolic path. This is because along with a horizontal component it is accompanied by a vertical component as well. The projectile covers the longest horizontal distance when it is thrown at 45 degrees. So next time when you throw a ball and want to impress your friends, make sure you launch the projectile at 45 degrees and see the Parabolic motion in front of your eyes!


The Eccentricity of Ellipse

  • An Ellipse can be defined as the set of points in a plane in which the sum of distances from two fixed points is constant. 

  • In simple words, the distance from the fixed point in a plane bears a constant ratio less than the distance from the fixed line in a plane.

Therefore, the Eccentricity of the Ellipse is less than 1. i.e., e < 1

The general equation of an Ellipse is denoted as \[\frac{\sqrt{a^2-b^2}}{a} \]


For an Ellipse,  the values a and b are the lengths of the semi-major and semi-minor axes respectively.


Fun Fact: You might find it interesting to know that Ellipse and its related concepts have a very wide application in the field of space sciences. Because the majority of the celestial bodies like planets, satellites, comets, man-made satellites, etc. tend to travel in elliptical orbits. Apart from the concept of Eccentricity, other concepts like apogee and perigee come into the picture while understanding the positions on these bodies. This makes the study of Ellipses and related concepts even more interesting. 


The Eccentricity of Hyperbola

  • A Hyperbola is defined as the set of all points in a plane where the difference of whose distances from two fixed points is constant. 

  • In simpler words, the distance from the fixed point in a plane bears a constant ratio greater than the distance from the fixed line in a plane.

Therefore, the Eccentricity of the Hyperbola is always greater than 1. i.e., e > 1

The general equation of a Hyperbola is denoted as \[\frac{\sqrt{a^2+b^2}}{a} \]


For any Hyperbola, the values a and b are the lengths of the semi-major and semi-minor axes respectively


Fun Fact: Scientists use the concepts related to Hyperbola to position radio stations. This ensures optimization of the area covered by the signals from a station. This enables people to locate objects over a wide area. This application played an important role in world war two.


Different Values of Eccentricity Make Different Curves:

At Eccentricity equal to 0

We obtain a Circle

For 0 < Eccentricity < 1

We obtain an Ellipse.

For the value of Eccentricity = 1

We obtain a Parabola.

For the value of Eccentricity > 1

We obtain a Hyperbola.

For the value of Eccentricity =∞

We obtain a line.


Eccentricity is often represented as the letter (Keep in mind you don't confuse this with Euler's number E, they are different).


Calculating the Value of Eccentricity (Eccentricity Formula):

Eccentricity of Circle:

For a Circle, the value of Eccentricity is equal to 0.

The Eccentricity of Ellipse:

For an Ellipse, the value of Eccentricity is equal to 


\[\frac{\sqrt{a^2-b^2}}{a} \]

Eccentricity of Parabola:

For a Parabola, the value of Eccentricity is 1.

The Eccentricity of Hyperbola:

For a Hyperbola, the value of Eccentricity is:


\[\frac{\sqrt{a^2+b^2}}{a} \]

  


Questions to be Solved

  1.  List down the formulas for calculating the Eccentricity of Hyperbola and Ellipse.

Ans: For a Hyperbola, the value of Eccentricity is: \[\frac{\sqrt{a^2+b^2}}{a} \]

For an Ellipse, the value of Eccentricity is equal to \[\frac{\sqrt{a^2-b^2}}{a} \]


  1. List down the formulas for calculating the Eccentricity of Parabola and Circle.

Ans: For a Parabola, the value of Eccentricity is 1

For a Circle, the value of Eccentricity = 0. Because for a Circle a=b

Where, a is the semi-major axis and b is the semi-minor axis for a given Ellipse in the question


Eccentricity from Vedantu’s Website

All the content related to Eccentricities of Parabola, Circle, Hyperbola and Ellipse on this website are prepared by subject matter experts of Vedantu. These experts have years of expertise in the field of Mathematics. They have closely monitored the past question papers over the years for various exams such as Class 11, Class 12 board exams, IIT-JEE exams, State CET exams, etc. and only after thorough research and analysis the content on this page has been made available to you. 


To leverage these efforts which are taken on your behalf by the Vedantu experts you should refer to the concept of Eccentricity only from the Vedantu website. This will ensure you get an edge over others and perform very well in all exams where questions related to this topic are asked.


Other Concepts Explained by Vedantu

Apart from Eccentric, Vedantu has explained many other Mathematical concepts on its website. These can help students in making Math easy and fun for them. All the concepts are explained by the subject matter experts of Vedantu only. Other related topics that you may find interesting are as follows:

Algebra Symbols

Area of Hemisphere

Circumference of Circle

Semi-Circle

Parabola graph

Equation of a Parabola

Area of Ellipse

Ellipse Formula

Foci of Ellipse

Equations of Ellipse

Hyperbola

Hyperbola formulas

Hyperbolic Functions

Hyperbolic Function Foumlas

Area segment Circle

Secant of a Circle

Equation of a Circle

Circles


These concepts along with the concept of Eccentricity will help you solidify your concepts in geometry and assist you in coming out with flying colours.

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FAQs on Eccentricity

1. What is the fundamental definition of eccentricity in conic sections?

In mathematics, eccentricity (e) is a non-negative number that measures how much a conic section deviates from being circular. It is defined as the ratio of the distance from any point on the conic section to a fixed point (the focus) and its perpendicular distance to a fixed straight line (the directrix). This single value uniquely determines the shape of a conic section.

2. How is the eccentricity of an ellipse calculated using its axes?

The formula to calculate the eccentricity of an ellipse is e = √(1 - b²/a²). In this formula, 'a' represents the length of the semi-major axis, and 'b' represents the length of the semi-minor axis. Since the semi-major axis is always greater than or equal to the semi-minor axis (a ≥ b), the eccentricity of an ellipse is always between 0 and 1.

3. How does the value of eccentricity determine the type of conic section?

The value of eccentricity (e) directly classifies the conic section. The specific values correspond to different shapes as per the NCERT syllabus:

  • Circle: A circle has an eccentricity of e = 0. This is a special case of an ellipse where the major and minor axes are equal.
  • Ellipse: An ellipse has an eccentricity in the range of 0 < e < 1.
  • Parabola: A parabola has an eccentricity of exactly e = 1.
  • Hyperbola: A hyperbola has an eccentricity of e > 1.

4. What happens to the shape of an ellipse as its eccentricity approaches 0 and 1?

The shape of an ellipse changes significantly as its eccentricity value changes. As the eccentricity approaches 0, the ellipse becomes less elongated and more closely resembles a perfect circle. Conversely, as the eccentricity approaches 1, the ellipse becomes more stretched out and flattened, appearing more like a line segment.

5. Can the eccentricity of a conic section ever be a negative number?

No, eccentricity cannot be a negative number. It is defined as a ratio of two distances (distance from focus and distance from directrix), and distance is always a non-negative value. Therefore, the eccentricity for any conic section will always be a non-negative real number (e ≥ 0).

6. Why is understanding eccentricity important in real-world fields like astronomy?

Eccentricity is a critical concept in astronomy and physics. It is used to describe the orbits of planets, comets, and satellites. For example, knowing the eccentricity of a planet's orbit helps scientists predict its path, its closest point (perihelion), and its farthest point (aphelion) from the sun. A highly eccentric orbit, like that of a comet, is very different from a nearly circular orbit like Earth's.

7. How does the eccentricity formula for a hyperbola differ from that of an ellipse?

The formulas for the eccentricity of a hyperbola and an ellipse are closely related but have a key difference that reflects their shapes. For an ellipse, the formula is e = √(1 - b²/a²), resulting in a value less than 1. For a hyperbola, the formula is e = √(1 + b²/a²), which always results in a value greater than 1. This mathematical difference corresponds to their geometric shapes: the ellipse is a closed curve, while the hyperbola consists of two open, unbounded branches.

8. What is the eccentricity of Earth's orbit and what does it signify for us?

The eccentricity of Earth's orbit is approximately 0.0167. Since this value is very close to 0, it signifies that Earth's path around the Sun is very nearly circular. However, it is not a perfect circle, which is why the distance between Earth and the Sun varies slightly throughout the year, leading to concepts like aphelion (farthest point) and perihelion (closest point).