Rewatching Star Trek: Voyager

So I’ve been rewatching Star Trek: Voyager recently, and thought I’d share some notes and observations. As a disclaimer, I had the show running mostly in the background, so I didn’t pay particularly close attention. Nevertheless, this re-viewing has pretty much solidified my conclusion that this series is my least favorite in the franchise. Let’s begin.

Captain Janeway

Oh, Captain Janeway…. I don’t think I agreed with a single command decision that she makes, starting with the very first episode where she decides to strand her crew in the Delta quadrant, and ending with the very last episode where she decides to travel back in time to help Voyager reach the Alpha quadrant sooner (because of how much she regrets her decision to stay in the Delta quadrant).

The complete, repeated disregard for the prime directive (including the Temporal prime directive) has me questioning her fitness for command.

At least she ends up where she belongs — in a women’s prison mashing potatoes for other inmates. #lockherup


The Jar-Jar Binks of the Star Trek universe! It’s hard to believe he survived that long before coming aboard Voyager without being blown to bits by… pretty much anyone who encountered him.   And it’s also hard to believe he wasn’t killed off in any number of ways during Voyager’s seven-year journey.   Being strangled by Tuvok would have been a satisfying outcome, and this actually happens, but only as part of a holodeck simulation.   It’s as if the writers are fully aware of how annoying this character is, but just want to stick it to the audience.

Stupid and/or tedious enemies

The Kazon. We’ve seen all of this before. Generic humanoids with a prosthetic forehead and a bone to pick. No wonder Seska (a secret Cardassian) fits so well with the Kazon when she defects to them from Voyager — they are nearly identical species, except that the Kazon are much stupider and less cunning. How did they ever invent warp travel? In fact, the Kazon, the Ocampa, and the Caretaker can be very closely compared with the Cardassian / Bajoran / Prophets trifecta of Deep Space Nine, except the latter were explored much more deeply and meaningfully.

The Hirogen. We’ve seen this before, too: one-dimensional enemies that are given a single human characteristic that’s exaggerated to absurdity. Basically a blend of Klingons and Jem’Hadar, they are obsessed with “hunting” and “prey,” and made for some woefully tedious and predictable episodes.

On the other hand, there were some great enemies too, such as Species 8472, which deserved many more episodes than they got. The interplay between Voyager and Species 8472 became really nuanced, and I was looking forward to more stories with them involved, but it didn’t happen.

Notable cameos

One of the truly enjoyable things about re-watching this series was the cameos, some of which I hadn’t even realized until now. Imagine watching a random episode and thinking, “Hold on, isn’t that… Scott Thompson?!” Why yes, it is — he makes a guest appearance in the episode Someone to Watch Over Me, and is delightful as always.

Other welcome appearances include Jason Alexander, who plays the leader of the “brain trust” in the episode Think Tank. I kept chuckling whenever he spoke. And of course there’s Sarah Silverman, an up-and-coming comedian at the time, who plays the nerdy-but-sexy SETI researcher in Future’s End.

Time travel as filler

A noticeable fraction of the episodes are time travel stories where most of the episode happens in an alternate timeline which, by the end of the episode, resets to the beginning without the crew knowing that anything happened. This makes the episode completely pointless, unless it’s redeemed by some meaningful character development, which it generally isn’t. Here are just a few such episodes that I can recall:

  • Time and Again, in which the Voyager crew detect a planet that has undergone a catastrophe, but it turns out that the crew themselves are the ones who cause the catastrophe in the future. Once they manage to prevent it from happening, the timeline resets to the beginning, with all the events of the episode never having taken place.
  • Timeless, in which, fifteen years in the future, Chakotay and Harry Kim correct a mistake that happened fifteen years prior, which had caused the destruction of Voyager and the rest of the crew. Once the mistake is corrected, the timeline is reset, with the events of the episode never having taken place.
  • Year of Hell (a two-parter), in which the crew is faced with a species that is bent on tampering with the timeline in order to become the most prosperous and dominant species in the sector. They do this using a ship that can fire a “temporal incursion” beam that erases any object from ever having existed. When Voyager finally manages to destroy the temporal incursion ship (without any help from the 29th Century time police, who should have been there, right?), the timeline is reset, with the events of the episode never having taken place. Note: this episode had a huge redeeming factor in the form of Kurtwood Smith, whose performance made the episode more watchable than most.
  • Relativity, in which a renegade captain from the 29th century is obsessed with destroying Voyager because he’s fed up with all the trouble they’ve caused with their time traveling (I know how he feels!). Once this captain is apprehended, the timeline is restored, with the events of the episode never having taken place.

I’m fairly certain there are a few more that I didn’t mention, but you get the idea. It feels like the writers would too often fall back on the “alternate timeline” / “it was all a dream” trope, rather than explore more meaningful ways to advance the story or develop the characters.


What good would a dissection of a Star Trek series be without a few nitpicks of the science and technobabble that they use? The science explored in Voyager is laughably terrible, as it often is in Star Trek, but fortunately it’s laughable in a good way. As in, it’s so absurd that it overflows into being humorous.

Remember when Voyager gets stuck inside the event horizon of a singularity (in the episode Parallax) and pokes a hole through it using warp particles? And when Neelix mansplains the event horizon to Kes with utter nonsense? Oh man, that’s the good stuff.

Perhaps the most absurd episode, to the point where I felt stupider after watching it, was Threshold, which is the one where Tom Paris builds a shuttlecraft that can achieve Warp 10, which is “infinite speed.” Mind you, the scientists and theorists at the Daystrom Institute have spent centuries refining warp technology to attain this goal without success, but Tom Paris (a random-ass pilot without any scientific background) does it in a few days.

The crew acknowledges that this is an impossibility (since traveling at infinite speed would mean occupying all points in the universe simultaneously), but Tom does it anyway! Of course, after attaining Warp 10, Tom starts to experience some changes: he abducts captain Janeway to a distant planet, where they de-evolve into giant salamanders, and have salamander babies. But don’t worry, the crew finds them soon enough, and the Doctor restores them to human form, with all their memories and skills intact. What happened to the salamander babies, which are now the most unique species in the entire universe? Ehh, who cares. (Whoops, spoilers!)


A few memorable episodes, some pretty good performances (especially by Robert Picardo as the Doctor), but the premise and overall dullness and repetitiveness of the episodes makes it more suited for running in the background rather than the foreground.

Ray tracing black holes

Lately I’ve been studying up on ray tracing, and one of my goals has been to build a nonlinear ray tracer — that is, a ray tracer that works in curved space, for example space that is curved by a nearby black hole. (See the finished  source code!)

In order to do this, the path of each ray must be calculated in a stepwise fashion, since we can no longer rely on the geometry of straight lines in our world. With each step taken by the ray, the velocity vector of the ray is updated based on an equation of motion determined by a “force field” present in our space.

This idea has certainly been explored in the past, notably by Riccardo Antonelli, who derived a very clever and simple equation for the force field that guides the motion of the ray in the vicinity of a black hole, namely

$$\vec F(r) = – \frac{3}{2} h^2 \frac{\hat r}{r^5}$$

I decided to use the above equation in my own ray tracer because it’s very efficient computationally (and because I’m not nearly familiar enough with the mathematics of GR to have derived it myself). The equation models a simple Schwarzschild black hole (non-rotating, non-charged) at the origin of our coordinate system. The simplicity of the equation has the tradeoff that the resulting images will be mostly unphysical, meaning that they’re not exactly what a real observer would “see” in the vicinity of the black hole. Instead, the images must be interpreted as instantaneous snapshots of how the light bends around the black hole, with no regard for redshifting or distortions relative to the observer’s motion.

Nevertheless, this kind of ray tracing provides some powerful visualizations that help us understand the behavior of light around black holes, and help demystify at least some of the properties of these exotic objects.

My goal is to build on this existing work, and create a ray tracer that is more fully featured, with support for other types of objects in addition to the black hole. I also want it to be more extensible, with the ability to plug in different equations of motion, as well as to build more complex scenes, or even to build scenes algorithmically. So, now that my work on this ray tracer has reached a semi-publishable state, let’s dive into all the things it lets us do.

Accretion disk

The ray tracer supports an accretion disk that is either textured or plain-colored. It also supports multiple disks, at arbitrary radii from the event horizon, albeit restricted to the horizontal plane around the black hole. The collision point of the ray with the disk is calculated by performing a binary search for the exact intersection. If we don’t search for the precise point of intersection, we would see artifacts due to the “resolution” of the steps taken by each ray (notice the jagged edges at the bottom of the disk):

Once the intersection search is implemented, the lines and borders become nice and crisp:

We can also apply different colors to the top and bottom of the disk. Observe that the black hole distorts the disk in a way that makes the bottom (colored in green) appear around the lower semicircle of the photon sphere, even though we’re looking at the disk from above:

Note that the dark black circle is not the event horizon, but is actually the photon sphere. This is because photons that cross into the photon sphere from the outside cannot escape. (Only photons that are emitted outward from inside the photon sphere can be seen by an outside observer.)

If we zoom in on the right edge of the photon sphere, we can see higher-order images of the disk appear around the sphere (second- and even third-order images are visible). These are rays of light that have circled around the photon sphere one or more times, and eventually escaped back to the observer.

And here is the same image with a more realistic-looking accretion disk:

Great! Now that we have the basics out of the way, it’s time to get a little more crazy with ray tracing arbitrary materials around the black hole.

Additional spheres

The ray tracer allows adding an unlimited number of spheres, positioned anywhere (outside the event horizon, that is!) and either textured or plain-colored. Here is a scene with one hundred “stars” randomly positioned in an “orbit” around the black hole (click to view larger versions of the images):

Notice once again how we can see second- and third-order images of the spheres as we get closer to the photon sphere. By the way, here is a similar image of stars around the black hole, but with the curvature effects turned off (as if the black hole did not curve the surrounding space):

And here is a video, generated using the ray tracer, that shows the observer circling around the black hole with stars in its vicinity. Once again, this is not a completely realistic physical picture, since the stars are not really “orbiting” around the black hole, but rather it’s a series of snapshots taken at different angles:

Notice how the spherical stars are distorted around the Einstein ring, as well as how the background sky is affected by the curvature.

Reflective spheres

And finally, the ray tracer supports adding spheres that are perfectly reflective:

All that’s necessary for doing this is to calculate the exact point of impact by the ray on the sphere (again using a binary intersection search) and get the corresponding reflected velocity vector based on the normal vector on the sphere at that point. Here is a similar image, but with a textured accretion disk:

Future work

Eventually I’d like to incorporate more algorithms for different equations of motion for the rays. For example, someone else has encoded a similar algorithm for a Kerr black hole (i.e. a black hole with angular momentum), and there is even a port of it to C# already, which I was able to integrate into my ray tracer easily:

A couple more ideas:

  • There’s no reason the ray tracer couldn’t support different types of shapes besides spheres, or even arbitrary mesh models (e.g. STL files).
  • I’d also like to use this ray tracer to create some more animations or videos, but that will have to be the subject of a future post.
  • Make it run on CUDA?