top of page

Two Dwarf Planets Beyond Pluto Hold a Big Secret

Chethana Janith, Jadetimes Staff

C. Janith is a Jadetimes news reporter covering science and geopolitics.

 
Jadetimes, Two Dwarf Planets Beyond Pluto Hold a Big Secret.
Image Source: (NASA/ ESA/ STScI)

James Webb’s latest gaze into the cosmos reveals unexpected secrets within the Kuiper Belt's icy realms.


  • The outer reaches of the Solar System, known as the Kuiper belt, is often seen as an icy wasteland and its dwarf planets perfectly preserve the priomordial ice of the early Solar System.

  • However, a new study suggests that two of the farthest flung celestial bodies - the dwarf planets Makemake and Eris, could be home to liquid oceans.

  • This evidence comes from observations made by the James Webb Space Telescope via its NIRSpec infrared instrument.


Our Sun, much like the countless other stars throughout the universe, has a life-supporting sweet-spot known as the “Goldilocks zone.” This idea is pretty intuitive - if you’re too far from a host star, it’s too cold for life to take hold, and if you’re too close, it’s too hot. But as humans have continued exploring our Solar System, scientists have discovered that our cosmic neighborhood isn’t quite that simple.


One big example is Europa - the sixth-largest moon of Jupiter, which is outside the Goldilocks zone, yet is kept warm due to the gas giant’s tidal heating. Now, two twin papers published in the journal Icarus say that surprising sources of warmth can even be found in some of the most distant celestial bodies in our Solar System.


The team - co-lead by the Texas-based Southwest Research Institute (SwRI), discovered evidence of hydrothermal activity in the dwarf planets Makemake and Eris, which are both located in the Kuiper Belt far beyond even the orbit of their sibling dwarf planet Pluto. This evidence, as with many astronomical discoveries nowadays, was made possible thanks to NASA’s $10 billion James Webb Space Telescope (JWST).


“We see some interesting signs of hot times in cool places,” SwRI’s Christopher Glein, the lead author of one of the studies, said in a press statement. “I came into this project thinking that large Kuiper Belt objects (KBOs) should have ancient surfaces populated by materials inherited from the primordial solar nebula, as their cold surfaces can preserve volatiles like methane. Instead…we found evidence pointing to thermal processes producing methane from within Eris and Makemake.”


While Eris is roughly the same size as Pluto and Makemake is about the same size as Pluto’s moon, Charon, both dwarf planets are far beyond even Pluto’s icy corner of the Solar System. Everyone’s favorite demoted planet travels a lonely orbit around the Sun at about 39 astronomical units (or AU, a unit that describes the average distance between the Earth and the Sun), but Makemake is at 45.8, and AU and Eris is a mind-boggling 68 AU away. That’s so far that the Sun would only look like a particularly bright star, rather than the fiery orb that fills Earth’s skies.


SwRI scientists examined isotope ratios in Makemake’s and Eris’ crusts, which are composed largely of methane ice. Using JWST’s NIRSpec infrared instrument to make spectroscopic observations, the team discovered that the ratio of deuterium - a kind of heavy hydrogen, to plain ole hydrogen (or the D/H ratio), as well as carbon ratios, confirmed that these dwarf planet’s icy crusts were younger than previously believed.


Jadetimes, Two Dwarf Planets Beyond Pluto Hold a Big Secret.
SwRI scientists used data from the James Webb Space Telescope to model the subsurface geothermal processes that could explain how methane ended up on the surfaces of Eris and Makemake, two dwarf planets in the distant Kuiper Belt. The illustration points to three possibilities, including the potential that liquid water exists within these icy bodies at the edge of the solar system, far from the heat of the Sun. Credit: Southwest Research Institute

“The D/H ratio is like a window. We can use it in a sense to peer into the subsurface,” Glein said in a press statement. “Our data suggest elevated temperatures in the rocky cores of these worlds so that methane can be cooked up. Molecular nitrogen (N2) could be produced as well, and we see it on Eris. Hot cores could also point to potential sources of liquid water beneath their icy surfaces.”


That’s right - even in the farthest reaches of the Kuiper belt, worlds can apparently still contain liquid water. This also means that these far-flung dwarf planets could contain hot cores still churning and bubbling with geologic dynamism.


But to know for sure, NASA, ESA, or some other space agency would need to cook up another deep space mission to have a closer look, and that could take some time. New Horizons, which launched back in 2006, is only 59 AU away from Earth, which is still some 8.3 billion miles away from Eris (even after an 18-year-long journey).


After the New Horizons flyby of the Pluto system, and with this discovery, the Kuiper Belt is turning out to be much more alive in terms of hosting dynamic worlds than we would have imagined,” Glein said in a press statement. “It’s not too early to start thinking about sending a spacecraft to fly by another one of these bodies to place the JWST data into a geologic context.

More News

bottom of page