Orbital Energy from Pulsar by Ladd Allen Doane
In the gravitational two-body problem, the specific orbital energy of two orbiting bodies is the constant sum of their mutual potential energy and their total kinetic energy divided by the reduced mass. According to the orbital energy conservation equation (also referred to as vis-viva equation), it does not vary with time.
Tracklist
| 2. | Orbital Energy | 6:13 |
Credits
from Pulsar,
released April 29, 2021
License
All rights reserved.
Transcendental rhythms and soundscapes hover over one another causing fractions of time to stand still.