Lead Image: Researchers conducted a novel study on the runaway greenhouse effect, revealing how a critical threshold of water vapor can lead to catastrophic climate changes on Earth and other planets. The research reveals a significant cloud pattern that contributes to this irreversible climate change, providing insights into exoplanet climates and their potential to support life.
A team from UNIGE together with CNRS has managed to simulate the entire runaway greenhouse effect, which can make a planet completely unhabitable.
The Earth is a wonderful blue and green dot covered with oceans and life, while Venus is a yellowish sterile sphere that is not only inhospitable but also sterile. However, the difference between the two bears to only a few degrees in temperature.
A team of astronomers from the University of Geneva (UNIGE) and members of the National Centre of Competence in Research (NCCR) PlanetS, with the support of the CNRS laboratories of Paris and Bordeaux, has achieved a world’s first by managing to simulate the entirety of the runaway greenhouse process which can transform the climate of a planet from idyllic and perfect for life, to a place more than harsh and hostile.
The scientists have also demonstrated that from initial stages of the process, the atmospheric structure and cloud coverage undergo significant changes, leading to an almost-unstoppable and very complicated to reverse runaway greenhouse effect. On Earth, a global average temperature rise of just a few tens of degrees, subsequent to a slight rise of the Sun’s luminosity, would be sufficient to initiate this phenomenon and to make our planet inhabitable.
Greenhouse Effect and Runaway Scenario
The idea of a runaway of the greenhouse effect is not new. In this scenario, a planet can evolve from a temperate state like on Earth to a true hell, with surface temperatures above 1000°C. The cause? Water vapor, a natural greenhouse gas. Water vapor prevents the solar irradiation absorbed by Earth to be reemitted towards the void of space, as thermal radiation. It traps heat a bit like a rescue blanket. A dash of greenhouse effect is useful – without it, Earth would have an average temperature below the freezing point of water, looking like a ball covered with ice and hostile to life.
On the opposite, too much greenhouse effect increases the evaporation of oceans, and thus the amount of water vapor in the atmosphere. “There is a critical threshold for this amount of water vapor, beyond which the planet cannot cool down anymore. From there, everything gets carried away until the oceans end up getting fully evaporated and the temperature reaches several hundred degrees,” explains Guillaume Chaverot, former postdoctoral scholar in the Department of Astronomy at the UNIGE Faculty of Science and main author of the study.
Groundbreaking Study on Climate Transition
“Until now, other key studies in climatology have focused solely on either the temperate state before the runaway, or either the inhabitable state post-runaway,” reveals Martin Turbet, researcher at CNRS laboratories of Paris and Bordeaux, and co-author of the study. “It is the first time a team has studied the transition itself with a 3D global climate model, and has checked how the climate and the atmosphere evolve during that process.”
One of the key points of the study describes the appearance of a very peculiar cloud pattern, increasing the runaway effect, and making the process irreversible. “From the start of the transition, we can observe some very dense clouds developing in the high atmosphere. Actually, the latter does not display anymore the temperature inversion characteristic of the Earth atmosphere and separating its two main layers: the troposphere and the stratosphere. The structure of the atmosphere is deeply altered,” points out Guillaume Chaverot.
Serious Consequences for the Search of Life Elsewhere
This discovery is a key feature for the study of climate on other planets, and in particular on exoplanets – planets orbiting other stars than the Sun. “By studying the climate on other planets, one of our strongest motivations is to determine their potential to host life,” indicates Émeline Bolmont, assistant professor and director of the UNIGE Life in the Universe Center (LUC), and co-author of the study.
The LUC leads state-of-the-art interdisciplinary research projects regarding the origins of life on Earth, and the quest for life elsewhere in our solar system and beyond, in exoplanetary systems. “After the previous studies, we suspected already the existence of a water vapor threshold, but the appearance of this cloud pattern is a real surprise!” discloses Émeline Bolmont. “We have also studied in parallel how this cloud pattern could create a specific signature, or ‘‘fingerprint’’, detectable when observing exoplanet atmospheres. The upcoming generation of instruments should be able to detect it,” unveils Martin Turbet. The team is also not aiming to stop there, Guillaume Chaverot having received a research grant to continue this study at the “Institut de Planétologie et d’Astrophysique de Grenoble” (IPAG). This new step of the research project will focus on the specific case of the Earth.
A Planet Earth in a Fragile Equilibrium
With their new climate models, the scientists have calculated that a very small increase of the solar irradiation – leading to an increase of the global Earth temperature, of only a few tens of degrees – would be enough to trigger this irreversible runaway process on Earth and make our planet as inhospitable as Venus. One of the current climate goals is to limit global warming on Earth, induced by greenhouse gases, to only 1.5 degrees by 2050. One of the questions of Guillaume Chaverot’s research grant is to determine if greenhouse gases can trigger the runaway process as a slight increase of the Sun luminosity might do. If so, the next question will be to determine if the treshold temperatures are the same for both processes.
The Earth is thus not so far from this apocalyptical scenario. “Assuming this runaway process would be started on Earth, an evaporation of only 10 meters of the oceans’ surface would lead to a 1 bar increase of the atmospheric pressure at ground level. In just a few hundred years, we would reach a ground temperature of over 500°C. Later, we would even reach 273 bars of surface pressure and over 1 500°C, when all of the oceans would end up totally evaporated,” concludes Guillaume Chaverot.
Reference: “First exploration of the runaway greenhouse transition with a 3D General Circulation Model” by Guillaume Chaverot, Emeline Bolmont and Martin Turbet, 18 December 2023, Astronomy & Astrophysics.
DOI: 10.1051/0004-6361/202346936
Exoplanets in Geneva: 25 Years of Expertise Honored With a Nobel Prize
The first exoplanet was discovered in 1995 by two researchers from the University of Geneva, Michel Mayor and Didier Queloz, recipients of the 2019 Nobel Prize in Physics. This discovery put the University of Geneva’s Astronomy Department at the forefront of research in the field, with the construction and installation of HARPS on ESO’s 3.6m telescope at La Silla in 2003.
For two decades, this spectrograph was the most powerful in the world for determining the mass of exoplanets. However, HARPS was surpassed in 2018 by ESPRESSO, another spectrograph built in Geneva and installed on the Very Large Telescope (VLT) in Paranal, Chile.
Switzerland is also involved in space-based observations of exoplanets with the CHEOPS mission, the result of two national areas of expertise: the space know-how of the University of Bern, in collaboration with its counterpart in Geneva, and the ground-based experience of the University of Geneva, assisted by its counterpart in the Swiss capital. These two areas of scientific and technical expertise have also led to the creation of the PlanetS National Centre of Competence in Research (NCCR).
Life in the Universe Center (LUC): An Interdisciplinary Excellence Pole
The Life in the Universe Center (LUC) is an interdisciplinary research center of the University of Geneva (UNIGE) founded in 2021 following the awarding in 2019 of the Nobel Prize in Physics by professors Michel Mayor and Didier Queloz. Thanks to the progress made during the last decade, both in the domains of the solar system exploration, of exoplanets and of the organic structure of life, the question of the emergence of life on other planets can now be tackled in a tangible way, and no more only speculatively. At the crossroads of astronomy, chemistry, physics, biology and of Earth and climate sciences, the LUC has for objective to understand the origins and the distribution of life in the universe. At the initiative of the Astronomy Department, the LUC brings together researchers from numerous UNIGE institutes and departments, as well as from several partner universities internationally.
