1 / 15

Orbital Mechanics

Orbital Mechanics. Planetary Position Today. Planetary Positions Today. Planetary Position in one year. Planetary Positions in one Year. SevCol Station Position: L4 Lagrange Point. Mechanics of Lagrange Points. Problems with Space Navigation. All objects in space move in their own orbits

otisarmstrong
Télécharger la présentation

Orbital Mechanics

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript

  1. Orbital Mechanics

  2. Planetary Position Today

  3. Planetary Positions Today

  4. Planetary Position in one year

  5. Planetary Positions in one Year

  6. SevCol Station Position: L4 Lagrange Point

  7. Mechanics of Lagrange Points

  8. Problems with Space Navigation • All objects in space move in their own orbits • It is not about covering distance, but about changing speeds • Using traditional methods, Space Flight is either very slow, or very very expensive • Fortunately, we have: Jumpgates

  9. Jumpgates • Provide instantaneous transportation between two points is space • Do not require a spaceship to spend energy • When exiting a jumpgate, a spaceship will have the orbital velocity of that jumpgate • Jumpgate orbit the Sun at various distances; these orbits are called Rings.

  10. Problems with Jumpgate 1 • Points must lie on a line deviating less than 9,42 degreesfrom the greatest gravitational vector. It is possible to travel between rings, but not within rings. • Jumpgate links are not fixed. Mostly, a jumpgate links to the nearest jumpgate up or down the biggest gravitational vector. Sometimes, they do not …

  11. Problems with Jumpgates 2 • Jumpgates can not be too close too each other, as the gravitational radiation will interfere with their functioning or will cause them to collide • Jumpgates can not be too close to large masses (like asteroids or planets) for the same reason.

  12. Problems with Jumpgates 3 • Orbits of jumpgates have chaotic perturbations due to ill understood gravitational radiation leakage effects; orbital positions can not be exactly calculated • No reflection of any radiation; almost invisible to any sensor system

  13. Problems with Jumpgates 4 • Using a jumpgate in a certain gravitational direction builds up gravitational radiation, that blocks it for use in the opposite direction for a certain time. • Jumpgates are unstable. Buildup of gravitational radiation is chaotic, and can lead to unpredictable implosions ...

  14. Problem with Jumpgates 5 • So you think 4 sheets with problems is not enough ? • Brush up on your math and meet Prof. dr. Isaak Oldton, Phd., Dphil, Msc., MA., the leading expert on jumpgate theory • That is, if you manage to distract his attention from his equations for long enough to listen to your question …

More Related