This model was created to demonstrate why the difference in speed is so small. It is based on a star with a planet orbiting around it at different distances and speeds.
It shows that the speed of orbit decreases as distance increases as expected, but there is also something else going on. As distance increases the decrease in speed necessary to maintain a stable orbit decreases.
The example planet must travel 1,784 kilometers an hour in order to have a stable orbit at 150,000,000 kilometers away from the star. If the planet’s orbit would be increased by 150,000,000 kilometers then the necessary speed to have a stable orbit would be 1,262 k/h. The decrease in speed would therefore be 522 k/h.
As we increase distance the reduction of orbital speed needed to keep a stable orbit decreases. For example if we increase the distance to 1,350,000,000 kilometers the speed required to keep a stable orbit would be 594 k/h. At this distance an increase of 150,000,000 kilometers would require the speed to be reduced to 564 k/h. The reduction of orbital speed needed to maintain a stable orbit is only 30 k/h. To put this into perspective, Saturn is 1,500,000,000 kilometers from the sun.
The need for a reduction in tangential velocity decreases exponentially as distance increases or the need for a decrease of the orbital velocity decreases towards infinity as distance increases.
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