Scientists have discovered hundreds of new objects in the outer solar system using an instrument designed to probe an unexplained source of energy in the universe. The results reveal new insights about the mysterious expanse beyond Neptune, including the possibility that a massive undiscovered planet may be lurking in these dark outer reaches.
A team led by Pedro Bernardinelli, a postdoctoral researcher at the University of Washington, scanned the outer solar system for six years with the Dark Energy Survey (DES), a Chile-based astronomy program whose primary objective is understanding dark energy, an unknown force that’s driving the accelerated expansion of the universe.
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The DES normally works on mind-boggling cosmic scales, but Bernardinelli and his team were able to shed light on enigmas that are much closer to home within our own solar system. The researchers have used the survey to discover a total of 815 trans-Neptunian objects (TNOs), which are minor bodies beyond Neptune, 416 of which are reported for the first time in a new paper published on the preprint server arXiv.
“We tried significantly different methods and approaches over the years, and we converged into this final pipeline which we’re presenting in this paper,” Bernardinelli said in an email. “I think it has always been on the back of the mind of some of the more senior DES members (i.e. people involved in designing the survey), but it was never a key goal of the project.”
“We were expecting to find a total of ~500 objects in this analysis, so finding 800 was definitely a nice surprise!” he added.
The survey was especially adept at spotting “dynamically detached” objects and “extreme TNOs” located 150 times farther from the Sun than Earth. These objects have been the subject of much speculation in recent years, because it looks like something in the outer reaches of the solar system is gravitationally tugging at them, causing a clustering effect in their orbits.
One tantalizing explanation for this phenomenon is the existence of a huge planet, about five to ten times the mass of Earth, that is ensconced in the hidden depths of the solar system. This so-called “Planet Nine” would likely be around 400 times as far from the Sun as Earth and may take some 20,000 years to complete an orbit. Scientists have been searching for traces of this planet for years, but have yet to snag a direct detection.
As a result, Planet Nine remains purely speculative and other hypotheses have been proposed to explain the clustering pattern seen with the extreme TNOs. It’s possible that the combined gravitational pull of many smaller objects is causing the effect, or that natural instabilities arise within this farflung population of bodies. One team has even suggested that a black hole, not a planet, might be the entity that is warping these extreme TNO orbits.
Bernardinelli’s team announced the discovery of nine new extreme TNOs in their study, in addition to seven others that DES had previously spotted. While the study does not support or refute the Planet Nine hypothesis, the inclusion of these new distant bodies will help scientists hone in on the possible causes of their anomalous orbits in future research.
“We tested the tendency of our eTNOs to be clustered, as predicted by the Planet Nine hypothesis,” said Bernardinelli, who conducted this research as part of his PhD thesis at the University of Pennsylvania. “We don’t see the clustering in our data, but we do not reject the hypothesis entirely.”
“This is consistent with our previous results, but the new idea here is that we used ~2x as many objects,” he added.
The new study demonstrates that astronomical instruments, such as DES, can enable discoveries and advances that have nothing to do with their primary missions. Though the survey is attuned to studying the acceleration of the universe, it has also sped up our understanding of the most familiar place within this expanding cosmos, our own solar backyard, while also revealing new mysteries about our system’s outer frontiers.
“One interesting thing that showed up is that we don’t agree with the current accepted model of the Kuiper belt region,” Bernardinelli said. “This is quite interesting, as it might mean there’s something else going on in the Kuiper belt that we haven’t figured out yet. With lots of objects we get to play these statistics games and constrain such models in a more detailed way.”
Update: This article has been updated with comments from lead author Pedro Bernardinelli.
