Planetary systems often form under unstable conditions. If young planets come too close, they can fling each other out of their orbits. This creates free-floating planets (FFPs), which wander through the galaxy without a parent star. An earlier study by LMU physicist Dr. Giulia Roccetti had shown that gas giants ejected in this way do not necessarily lose all of their moons in the process.
Tidal heating keeps oceans liquid
The ejection does, however, alter the orbits of the moons. They become highly elliptical, such that their distance from the planet constantly changes. The resulting tidal forces rhythmically deform the lunar body, compress its interior, and generate heat through friction. This tidal heating can be sufficient to maintain oceans of liquid water on the surface – even without the energy of a star, and in the cold of interstellar space.
Hydrogen as stable heat trap
The atmosphere determines whether this heat is retained at the surface. On Earth, carbon dioxide functions as an effective greenhouse gas. Earlier studies had demonstrated that carbon dioxide could stabilize life-friendly conditions on exomoons for periods of up to 1.6 billion years. Under the extremely low temperatures of free-floating systems, however, carbon dioxide would condense, causing the atmosphere to lose its protective effect and allowing heat to escape.
And so the research team from the fields of astrophysics, biophysics, and astrochemistry investigated hydrogen-rich atmospheres as alternative heat traps. Although molecular hydrogen is largely transparent to infrared radiation, a crucial physical effect arises under high pressures: collision-induced absorption. In this process, colliding hydrogen molecules form transient complexes that can absorb thermal radiation and retain it in the atmosphere. At the same time, hydrogen remains stable even at very low temperatures.
Parallels to early Earth
The findings also furnish new clues to the origin of life. “Our collaboration with the team of Prof. Braun helped us recognize that the cradle of life does not necessarily require a sun,” says David Dahlbüdding, doctoral researcher at LMU and lead author of the study. “We discovered a clear connection between these distant moons and the early Earth, where high concentrations of hydrogen through asteroid impacts could have created the conditions for life.”
Tidal forces could not only supply heat, but also drive processes of chemical development. Periodic deformation gives rise to local wet-dry cycles, in which water evaporates and then condenses again. Such cycles are considered an important mechanism for the formation of complex molecules and could facilitate crucial steps on the path to the emergence of life.
Moons hospitable to life in interstellar space
Free-floating planets are thought to be common. According to estimates, there could be as many of these ‘nomadic’ planets in the Milky Way as there are stars. Their moons could provide stable habitats for long periods of time. The new findings could thus significantly broaden the spectrum of possible environments that could harbor life – and show that life could arise and endure even in the darkest regions of the galaxy.
Contact
David Dahlbüdding
LMU Munich / Max Planck Institute for Extraterrestrial Physics / Excellence Cluster ORIGINS
email: ddahlb(at)mpe.mpg.de
Prof. Barbara Ercolano
LMU Munich / Excellence Cluster ORIGINS
email: ercolano(at)usm.lmu.de
Dr. Tommaso Grassi
Max Planck Institute for Extraterrestrial Physics / Excellence Cluster ORIGINS
email: tgrassi(at)mpe.mpg.de
Prof. Dieter Braun
LMU Munich / Excellence Cluster ORIGINS
email: Dieter.Braun(at)physik.uni-muenchen.de
