Searching for Hyperbolic Trajectory with Excess Speed of 3.944 km/s

In summary, the conversation discusses the search for a hyperbolic trajectory with a hyperbolic excess speed of 3.944 km/s, which is determined by the semi-major axis and eccentricity of the orbit. The equations related to this search have not been successful so far, but it is suggested to look for an equation that relates perigee radius, semi-major axis, and eccentricity. Alternatively, the vis viva equation can be used to calculate the velocity at perigee and determine the maneuver speed needed to enter the desired hyperbolic orbit.
  • #1
Dustinsfl
2,281
5
I have been trying to find a hyperbolic trajectory that has hyperbolic excess speed of 3.944 km/s.

However, I can only find ones that would start inside the Earth's crust.

mue = 398600

energy = mue / (2 * a)

ve = 29.78

vinf = 3.944 = \sqrt{mue / a}

I have at least 30 more equations that are relevant but they have all lead no where.
 
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  • #2
The excess speed determines a, but you still have e to play with for a given perigee radius. Among your 30 equations you may find one that relates perigee radius rp, semi-major axis a, and eccentricity e. If not not, then look for a relevant equation that gives radius r as a function of true anomaly f and then set f to zero.

[Later] It has occurred to me that the orbital eccentricity probably is not that interesting a parameter for you. If so you may instead want to use the vis viva equation with your last equation above in order to get the (desired) velocity at perigee as a function of perigee orbital radius and the hyperbolic excess speed. The difference between the actual and desired perigee speed is then the maneuver speed needed at perigee to enter the desired hyperbolic orbit.
 
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1. What is a hyperbolic trajectory?

A hyperbolic trajectory is a type of curved path that an object follows when it is moving through space under the influence of gravity. It is characterized by a shape that resembles a hyperbola, and it is typically used to describe the motion of objects that are not orbiting a central body, but are instead passing by it at high speeds.

2. How is excess speed measured in a hyperbolic trajectory?

Excess speed in a hyperbolic trajectory is measured by the difference between the object's actual velocity and the escape velocity of the central body. This is typically measured in kilometers per second (km/s) and is used to determine if the object will follow a hyperbolic path or enter into orbit.

3. Why is it important to search for hyperbolic trajectories with excess speed?

Searching for hyperbolic trajectories with excess speed can provide valuable information about the objects that are passing through our solar system. These trajectories can help scientists identify and track comets, asteroids, and other objects that could potentially pose a threat to Earth. They can also provide insights into the formation and evolution of our solar system.

4. How is the excess speed of a hyperbolic trajectory calculated?

The excess speed of a hyperbolic trajectory is calculated using the formula v = √(2GM/r), where v is the escape velocity, G is the gravitational constant, M is the mass of the central body, and r is the distance from the object to the center of the central body. This formula takes into account the gravitational pull of the central body on the object and determines the speed needed for the object to escape its gravitational field.

5. What tools or methods are used to search for hyperbolic trajectories with excess speed?

Scientists use a variety of tools and methods to search for hyperbolic trajectories with excess speed. These include telescopes, radar systems, and computer simulations. They also analyze data from past observations and use mathematical models to predict the paths of objects in our solar system. Additionally, space missions are often sent to study and track these trajectories in order to gather more information about the objects passing through our solar system.

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