Finding Orbit Type with Energy Equation

In summary, the energy equation can be used to determine the type of orbit by calculating the value of E, which is equal to the kinetic energy minus the gravitational potential energy. If E=0, the orbit is parabolic; if E>0, it is hyperbolic; and if E<0, it is elliptic. Additionally, if $v^{2}r=\mu$, the orbit is circular. The value of $\mu$ can be calculated using the equation $\mu = G(m_1+m_2)$.
  • #1
Dustinsfl
2,281
5
How does one use the energy equation to determine the type of orbit?
$$
E = \frac{v^2}{2} - \frac{\mu}{r}
$$
where $\mu = G(m_1+m_2)$ and
$$
\mathbf{r} = \begin{pmatrix}
-4069.503\\
2861.786\\
4483.608
\end{pmatrix}\text{km},\quad
\mathbf{v} = \begin{pmatrix}
-5.114\\
-5.691\\
-1.000
\end{pmatrix}\text{km/sec}
$$
 
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  • #2
As I understand it, $E=0$ is parabolic, $E>0$ is hyperbolic, and $E<0$ is elliptic. If $v^{2}r=\mu$, then it's circular.
 
  • #3
Ackbach said:
As I understand it, $E=0$ is parabolic, $E>0$ is hyperbolic, and $E<0$ is elliptic. If $v^{2}r=\mu$, then it's circular.

My issue was I didn't have a mu term.
 
  • #4
dwsmith said:
How does one use the energy equation to determine the type of orbit?
$$
E = \frac{v^2}{2} - \frac{\mu}{r}
$$
where $\mu = G(m_1+m_2)$ and
$$
\mathbf{r} = \begin{pmatrix}
-4069.503\\
2861.786\\
4483.608
\end{pmatrix}\text{km},\quad
\mathbf{v} = \begin{pmatrix}
-5.114\\
-5.691\\
-1.000
\end{pmatrix}\text{km/sec}
$$
I'm confused about two things:
1. You are missing an "m" from the kinetic energy term.

2. You defined [tex]\mu[/tex] in your original post. Is this a result you are supposed to derive perhaps?

-Dan
 
  • #5
topsquark said:
I'm confused about two things:
1. You are missing an "m" from the kinetic energy term.

2. You defined [tex]\mu[/tex] in your original post. Is this a result you are supposed to derive perhaps?

-Dan

Later on I was told what mu is for this problem so I was able to do it.
 

FAQ: Finding Orbit Type with Energy Equation

What is the energy equation used for finding orbit type?

The energy equation is a mathematical equation that relates the energy of an object to its position and velocity. In the context of orbital mechanics, it is used to determine the type of orbit an object is in based on its energy.

How is the energy equation derived?

The energy equation is derived from the conservation of energy principle, which states that energy cannot be created or destroyed, only transferred or converted into different forms. In orbital mechanics, this principle is applied to the gravitational potential and kinetic energy of an object in orbit.

What are the different types of orbits described by the energy equation?

The energy equation can be used to determine whether an orbit is elliptical, circular, or hyperbolic. An elliptical orbit has negative energy, a circular orbit has zero energy, and a hyperbolic orbit has positive energy.

How does the energy equation help in understanding orbital mechanics?

The energy equation is a crucial tool in understanding orbital mechanics because it allows us to determine the type of orbit an object is in without directly observing it. It also helps us understand the relationship between an object's energy and its position and velocity in orbit.

Are there any limitations to using the energy equation for finding orbit type?

Yes, there are some limitations to using the energy equation for determining orbit type. It assumes a two-body system and does not take into account factors such as atmospheric drag or perturbations from other objects. Additionally, it only applies to objects orbiting a central body with a spherically symmetric mass distribution.

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