Energy
Under standard assumptions, specific orbital energy of a hyperbolic trajectory is greater than zero and the orbital energy conservation equation for this kind of trajectory takes form:
where:
- is orbital velocity of orbiting body,
- is radial distance of orbiting body from central body,
- is the negative semi-major axis,
- is standard gravitational parameter.
Read more about this topic: Hyperbolic Trajectory
Famous quotes containing the word energy:
“Children are intensely invested in getting their way. They will devote more emotional and intellectual energy to winning arguments than parents ever will, and are almost always better rested.”
—Jean Callahan (20th century)
“The flattering, if arbitrary, label, First Lady of the Theatre, takes its toll. The demands are great, not only in energy but eventually in dramatic focus. It is difficult, if not impossible, for a star to occupy an inch of space without bursting seams, cramping everyone else’s style and unbalancing a play. No matter how self-effacing a famous player may be, he makes an entrance as a casual neighbor and the audience interest shifts to the house next door.”
—Helen Hayes (1900–1993)
“Much of the modern resistance to chastity comes from men’s belief that they “own” their bodies—those vast and perilous estates, pulsating with the energy that made the worlds, in which they find themselves without their consent and from which they are ejected at the pleasure of Another!”
—C.S. (Clive Staples)