But not everyone agrees with van Dokkum's conclusion.

"Something that caught my attention very early on was the fact that the galaxy was not only anomalous for not having dark matter, but also for having an extraordinarily bright population of globular clusters," says Ignacio Trujillo of the Instituto de Astrofisca de Canarias, who led the main study rebuking the distance to DF2. "I remember thinking: 'Two anomalies at the same time really looks odd.'" This led Trujillo to consider whether DF2 is really as distant as van Dokkum's team thinks.

If DF2 were some 64 million light-years away, like van Dokkum suspects, then the galaxy would be a strong candidate for the first example of a galaxy without dark matter. But Trujillo says that if DF2 is closer, the galaxy's observed properties would more or less fall in line with what's expected from your run-of-the-mill, dark-matter-dominated galaxy.

The distance to DF2

To test their theory, Trujillo and his team set off to determine their own distance estimates to DF2 using five different methods — all with varying degrees of trustworthiness.

Two of the methods relied on analyzing the brightnesses and sizes of DF2's globular clusters. According to the short-distance camp, if DF2 is a bit closer than initially thought, then the galaxy's globular clusters would no longer be weirdly big and bright. They also compared DF2’s properties to a similar galaxy, called DD044, which has a more reliable distance estimate, as well as recalculated DF2's distance using the same method as the original team.

Finally, Trujillo's team analyzed the Tip of the Red Giant Branch (TRGB) in DF2's color-magnitude diagram (CMD), which plots the temperatures and luminosities of stars within a galaxy. Because the brightest red giant stars all shine with the same true brightness when observed in infrared, the only thing that should greatly impact how bright they appear to us is their distance.

"This is by far the most accurate way of measuring the distance to the galaxy if the data have good quality," Trujillo says. Based on all five methods, Trujillo and his team estimate DF2 is probably only about 42 million light-years away, rather than the original estimate of 64 million light-years.

But van Dokkum isn't convinced by this competing distance determination.

Last year, his team published yet another paper in response. Their result: DF2 is about 61 million light-years away, which would mean DF2 still has a negligible amount of dark matter.

Astronomers infer the existence of dark matter largely based on the fact that the rotation curves of galaxy's are not what you would expect without some form of hidden mass spread throughout the entire galaxy. In this simulation, the galaxy on the left shows what rotation would look like without the effects of dark matter, while the right shows rotation with dark matter. Note how the stars and gas on the outside of the right galaxy are spiraling much faster than those in the left galaxy.



Ingo Berg/Wikimedia Commons

What about DF4?

But the debate didn't stop there.

After this academic back-and-forth, van Dokkum and his team uncovered yet another galaxy, DF4, that also seems to be lacking dark matter. By measuring how DF4's light is distributed across the galaxy, van Dokkum determined DF4's distance is similar to DF2's — about 65 million light-years.

But Trujillo and his team have since published their own analysis of DF4's distance using the TRGB method. In it, they conclude DF4 is just 44 million light-years away, which would make DF4's globular clusters more similar to those found in the Milky Way. "All in all," they conclude in the paper, "the proposition that both [DF2] and [DF4] are 'missing dark matter' is still far from being placed on sure footing."

Although the answer to whether the galaxies have dark matter or not is still up in the air, the discourse between the two teams serves as real-world glimpse of the scientific process in action.

“The broader point is that these are fascinating galaxies, and all aspects of our findings should certainly be questioned and scrutinized," van Dokkum says.

And there may be a definitive answer on the horizon.

Recently, van Dukkum’s team secured a chunk of observing time with the Hubble Space Telescope. They expect the new observations to help them pin down DF4's distance to within about 5 percent. So for now, both van Dokkum's and Trujillo's teams are simply waiting to dive deep into the new data.

And when they do, we may finally learn whether galaxies without dark matter can actually exist, or whether some galaxies just happen to be very good at hiding the already stealthy substance.