Orbital Mechanics: Speeding Up to Slow Down

That’s us, in the Background, corkscrewing through space, orbiting the center of the galaxy, captive to the star at the center of our system, at hundreds of thousands of miles per hour, as it defines that path.
Photo of Carl Atteniese: NASA (Yeah–in your dreams!)
At The Museum of Science and Natural History, Denver, CO
A Page from One of My Many Notebooks

I am very interested in how bodies behave in space, be they galaxies, stars, planets, dwarf planets, moons or spacecraft. The fascination comes mostly from my interest in human spaceflight, and in how surprising the mechanics turn out to be once one starts learning about it, and also due the awe that arises in learning that spaceflight–be it natural, and exhibited by natural objects, like those mentioned above, or unnatural, and done by human beings–involves the natural, predictable, controllable (in human cases) and dynamic relationships that occur between masses in space–called orbits.

From the outside, orbital mechanics looks difficult to understand–and it is, which is why I only have apprehended the basics–but the average person can understand the basic principles, which, as I alluded to before, become much more fascinating once the non-initiated person begins to see, that, for example–sending a spacecraft aloft and into orbit–specifically–is amazingly much more surprising and complex than simply pointing a rocket at the sky and firing its engines.

“What goes up,

Photo: MJ ganchimeg

must come down”, goes the song, but what if we don’t want to come down right away, and moreover, we don’t want to kill anyone in the process, including those who may be inside our spacecraft–namely ourselves–how do we keep ourselves or our spacecraft up there?

Getting into space–into orbit, that is–is not as simple as escaping the Earth’s gravity, because, unless we want to stay out there for a very long time, like, basically forever, orbiting the sun until we die, and we are not headed to the moon or another planet or another planet’s moon–we must manage Earth’s gravity, because… it is Earth’s gravity (or, actually, the attraction between Earth’s mass and that of our spaceship) that keeps us and our spaceship in orbit.

Peeking Through The Porthole of My Spaceship (LOL)


So–in the end, one wants to go up… and wants to let the “coming down” force of “what comes down” keep our spacecraft… upthere. Does this sound strange? Then there are all sorts of details about velocity (speed + direction), the direction and amount of power we use to fire our engines, with which we go up and down, the shape of the orbit we circumscribe and want to remain in and, then descend or transfer from, and how that changes our altitude–which changes your speed, as well–and… so on.

Orbit Neptune (It’s actually not that blue, I hear)
© Copyright 2017 – 2025 Carl Atteniese / All rights reserved

In only one Star Trek episode–in the old days–did I hear Captain Kirk talk about the apogee of the Enterprise’s orbit–the point which is the farthest distance in the orbit from the parent body (the celestial body which our craft–or a moon–or other satellite–is orbiting), which is opposite the perigee, or the closest point to the parent body.

Usually, in science fiction, we hear most actor-space-farers borrowing from Star Trek (the language for which is taken from sailing and Navy operations), which is to say, they command their helmsman, or pilot, to “set a course” for this planet or that, or whatever–when in reality, while that language is fine, it is basically a language for straight-line navigating, point to point; but in real space travel, near and among planets and moons, anyway (and without the incredible resources of fantasy ships like the Enterprise, with its faster-than-light travel capacity), spacecraft are always navigating in curved, orbital trajectories, taking advantage of the dynamics occurring due the gravitational forces between them and the celestial bodies around them.

Click to enlarge this beautiful diagram in a new tab. This focuses on the communication involved, but shows mission points and phases as well.

The astronauts who went to the moon 9 times–23 in total (of which two travelled there twice), with 12 men having walked on the surface), did not fly straight to the moon; one cannot do that, because the moon–like its parent body, the Earth–is moving….

The astronauts in their Apollo spacecraft went (and the astronauts in their Artemis craft, soon, hopefully) will go from a smaller low Earth orbit (also known as LEO), “injecting” into a larger Earth orbit (thus the denotation, “Trans Lunar Injection”), whose apogee (or region of farthest distance from the parent body, the Earth) takes them out into a region of their path around the Earth to a lower point of attraction in the gravity well of the Earth, such that they are able to be captured by the moon’s gravity well.

In fact, a point that Neil DeGrasse Tysen likes to repeat is–after the initial firing of the engine to leave low Earth orbit, they coast to this point between the gravity wells of Earth and moon–without firing the engines again (unless they need to make a trajectory correction, as happened on Apollo 13…. After coasting to the vicinity of moon, they then initiate a “breaking burn” near the moon, to be sure to fall around the moon and into her orbit--and not fly past the moon. On the way home, they do the same in reverse. They fire the service engine of their ship powerfully and long enough to leave lunar orbit and to fall into an orbit apprehensible by the Earth’s gravity well, turn off the engine and coast to the Earth, whereupon they enter the atmosphere at just the right angle in order not to bounce off it and not enter so steeply that they burn up in the plasma crucible of re-entry heat.

Here is a good video I watch on YouTube, from time to time, to keep from confusing the terms of orbital mechanics and spaceflight dynamics (which are quite confusable–you will learn). There are others, which I have watched far more times–and which teach the basics in a more comprehensive way–including historical references and laws of physics–which I will post here in the future. Enjoy. And, think like an astronaut.

© 2025 8 Fold / Carl Atteniese II /All rights reserved

Update (November 28th, 2025):

I had a conversation with Chat GPT after publishing this article, as I found a possible hole in my knowledge upon a proofread of the article today. Here it is: (and be sure to see the diagram made by Ghat GPT at bottom showing the orbital profiles.






I said:

So, I was right. I did not intend to suggest the SM entered re-entry. I was specifically interested in whether a braking burn was performed in Earth vicinity. But I see a prograde burn (in direction of orbital travel) raised the altitude over the moon for apprehension by an orbital track adjustable for Earth trajectory, but was another burn required thereafter so that the raised altitude did not slow the vehicle?

ChatGPT said:

✔️ Why no second burn was needed after TEI




✔️ 4. The Service Module was jettisoned before re-entry


✔️ Summary

PhaseBurn Needed?Why
TEI (leaving lunar orbit)Yes — major SPS burnSets up Earth-intercepting trajectory
Coast to EarthNo major burnsBallistic free-return trajectory
Midcourse correctionsOnly tiny RCS burnsFine tuning only
Earth re-entryNo braking burnAtmosphere handles all deceleration

✔️ Your intuition was correct