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It is a well-known fact that we make use of the considerable orbital energy of Earth to help us perform interplanetary missions. Here I am not referring to gravity-assist maneuvers, but to the simple fact that we are already some 150 million km from the Sun and traveling at around 30 km/s – our orbital speed around the Sun. In this entry I want to look at the way we utilize this energy.
For this discussion, I will deviate from the usual way of expressing orbital energy(a) and use the more 'natural' concept of mechanical energy, where both potential energy and kinetic energy are positive. In this scheme, the specific mechanical energy of Earth's orbit relative to the Sun is: GMsun/a + ½ vo2 ~ 1335 Mega-Joule (MJ)(b) per kg of orbiting mass, where a is the semi-major axis of the elliptical orbit and vo is the average orbital velocity.
To keep things as simple as possible, let's place a probe precisely at the L4 Sun-Earth Lagrangian point, 60 degree ahead of Earth, as shown(c). Now we don't have to worry about the gravitational wells of Earth and the Moon. The probe will orbit the Sun in step with Earth and it has constant specific mechanical energy of ~1335 MJ per kg of probe mass, as above. Now we fire the probe's liquid oxygen/hydrogen booster and add a Δv of 3 km/s to the original 30 km/s orbital speed.
If the probe was at rest in an inertial frame, we would have added 'only' 32/2 = 4.5 MJ/kg of specific kinetic energy - that's the energy imparted directly onto the probe. However, immediately(d) after the burn the probe has actually gained (30+3)2/2 – 302/2 ~ 95 MJ/kg of extra kinetic energy (relative to the Sun). This looks like a vastly 'over-unity' process at work: 4.5 MJ/kg energy input and 95 MJ/kg of output - more than a factor twenty! How does this work?
It is easy to see it from the math, because ½ (vo + Δv)2 = ½ vo2 + voΔv + ½ Δv2 is obviously larger than the straight addition ½ vo2 + ½ Δv2, especially if vo is much larger than Δv. But, what is the physical mechanism for this additional energy? There is no gravity assist applicable here, where the probe could have 'robbed' some of a planet's orbital energy. Does it 'steal' energy from the Sun, or where does it come from?
I would like to hear reader's opinions on this one. Once done, there is also a slightly tougher variant of this puzzle (to follow). 
-J
Notes:
(a) The usual method of accounting for planetary orbital energy takes kinetic energy as positive and potential energy as negative (E/m = ½ vo2 - GM/r). Closed orbits have negative orbital energy, precisely escape orbits have zero energy and super-escape orbits have positive orbital energy. This is part of the Hamiltonian that Roger Pink described in his Blog "Roger's Equations". What I'm using above is part of the Lagrangian.
(b) If we use km instead of meters everywhere (also in G), energy comes out in MJ (kg.km2/s2) instead of Joules (kg.m2/s2).
(c) We assume that the burn was short enough so that the orbital distance from the Sun did not change appreciably during the burn. It will obviously change after the burn. Depending on where in the elliptical orbit the burn takes place, the probe will reach an aphelion of around 230 million km from the Sun, which is just outside the orbit of Mars.
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