Understanding How the Hubble Re-Orients: The Mathematics Behind It

In summary, the Hubble Space Telescope (HST) uses tiny sensor gyroscopes and star trackers to re-orient itself and determine its orientation. It also has reaction wheels, which act like gyroscopes, to help move the telescope when necessary.
  • #1
zankaon
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How does Hubble Space Telescope (HST) re-orient itself; and what is an underlying mathematical description? http://en.wikipedia.org/wiki/Gyroscope"
 
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HST has tiny sensor gyroscopes which spin freely and so always point the same way it uses this to know which way is up.
For more accurate pointing it also star trackers built into some of the instruments.

It also has reaction wheels (also sometimes loosely called gyros) these heavy wheels spin like gyros and can be used to move the telescope. When the spin they tend to stay in the same plane and so when you push on them you move instead.
 
  • #3


The Hubble Space Telescope (HST) uses a combination of gyroscopes and reaction wheels to re-orient itself in space. Gyroscopes are devices that use the principles of angular momentum to maintain a fixed orientation in space. They consist of a spinning mass that resists changes in its orientation, allowing the telescope to maintain a stable position in space.

The HST has six gyroscopes, three of which are used for pointing and three for backup. These gyroscopes are constantly monitored and their readings are used to calculate any changes in the telescope's orientation. If a change is detected, the HST uses its reaction wheels to counteract the change and maintain its desired orientation.

The reaction wheels work by spinning in the opposite direction of the change in orientation, thus canceling it out. This process is controlled by an onboard computer that uses complex mathematical calculations to determine the necessary adjustments to the reaction wheels. These calculations take into account factors such as the telescope's mass, its current orientation, and the desired orientation.

The underlying mathematical description of this process is based on the principles of angular momentum and conservation of energy. By constantly monitoring the gyroscopes and making precise adjustments to the reaction wheels, the HST is able to maintain its position in space and capture stunning images of the universe.

In summary, the Hubble Space Telescope uses a combination of gyroscopes and reaction wheels, controlled by complex mathematical calculations, to re-orient itself in space and capture incredible images of our universe. This technology highlights the importance of mathematics in the field of space exploration and our understanding of the cosmos.
 

Related to Understanding How the Hubble Re-Orients: The Mathematics Behind It

1. What is the purpose of the Hubble re-orientation?

The Hubble re-orientation allows the telescope to point at different areas of the sky to gather new data and images. It also helps to extend the life of the telescope by allowing it to use its backup systems for certain observations.

2. How often does the Hubble telescope need to re-orient?

The Hubble telescope typically re-orients every 20-30 minutes during its orbit around Earth. However, the frequency can vary depending on the specific mission and observations being conducted.

3. What mathematical calculations are involved in the Hubble re-orientation?

The Hubble re-orientation involves complex mathematical calculations to determine the correct angles and positions for the telescope's orientation. These calculations take into account the telescope's orbit, rotation, and desired target coordinates.

4. How does the Hubble telescope re-orient itself in space?

The Hubble telescope is equipped with gyroscopes and reaction wheels that work together to control its movement and orientation in space. The gyroscopes measure the telescope's rotation, while the reaction wheels use stored momentum to adjust the telescope's orientation.

5. What are the potential risks or challenges of the Hubble re-orientation?

The Hubble re-orientation can be a delicate and precise process, and any miscalculations or malfunctions could potentially damage the telescope. Additionally, the constant movement and re-orientation can put stress on the telescope's components and contribute to its gradual deterioration over time.

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