Life requires an environment with simple molecular building blocks, an energy source to drive chemistry, bounded pressure and temperature conditions to allow complex molecules to form, and possibly a diversity of linked environments to facilitate the transition from chemistry to biology.
Oxygen is a key signature for life because it is constantly replenished by biological processes like photosynthesis. Without life, oxygen would disappear from the atmosphere in tens of thousands of years. Its presence indicates a disequilibrium in the atmosphere, suggesting biological activity.
Astronomers use spectroscopy to analyze the atmospheres of exoplanets. By splitting light into its different wavelengths, they look for missing colors that indicate the presence of specific molecules like oxygen or methane, which could suggest biological activity.
Hydrogen cyanide, though toxic, is a crucial molecule in prebiotic chemistry. When exposed to sunlight in aqueous solutions, it facilitates the formation of organic matter, including the building blocks of nucleic acids, proteins, and cell membranes.
Technosignatures are indicators of advanced technological civilizations, such as industrial pollutants like CFCs in the atmosphere. Unlike biosignatures, which suggest biological activity, technosignatures imply the presence of intelligent, industrialized life.
Planets around M dwarf stars are often tidally locked, with permanent day and night sides, and are subjected to frequent stellar flares that can strip away their atmospheres. These factors make it difficult for life to thrive in such environments.
Earth’s magnetic field protects the planet from charged particles emitted by the Sun, preventing the atmosphere from being stripped away. This shield is crucial for maintaining the conditions necessary for life.
Sub-Neptunes, intermediate in mass between Earth and Neptune, are common in the galaxy and may have vast liquid water oceans. Their potential habitability raises questions about whether life can exist in such exotic, water-rich environments.
Darwin’s ‘warm little pond’ remains relevant as a model for surface chemistry on planetary surfaces, where conditions like light, temperature variations, and limited water volume can facilitate the formation of complex organic molecules.
The Extremely Large Telescope (ELT), with a 39-meter diameter, will enable astronomers to directly image and analyze the atmospheres of nearby exoplanets, such as Proxima b, by detecting missing wavelengths of light that indicate the presence of life-supporting molecules.
Melvyn Bragg and guests discuss some of the great unanswered questions in science: how and where did life on Earth begin, what did it need to thrive and could it be found elsewhere? Charles Darwin speculated that we might look for the cradle of life here in 'some warm little pond'; more recently the focus moved to ocean depths, while new observations in outer space and in laboratories raise fresh questions about the potential for lifeforms to develop and thrive, or 'habitability' as it is termed. What was the chemistry needed for life to begin and is it different from the chemistry we have now? With that in mind, what signs of life should we be looking for in the universe to learn if we are alone?
With
Jayne Birkby Associate Professor of Exoplanetary Sciences at the University of Oxford and Tutorial Fellow in Physics at Brasenose College
Saidul Islam Assistant Professor of Chemistry at Kings College, London
And
Oliver Shorttle Professor of Natural Philosophy at the University of Cambridge and Fellow of Clare College
Producer: Simon Tillotson
Reading list:
David Grinspoon, Venus Revealed: A New Look Below the Clouds of Our Mysterious Twin Planet (Basic Books, 1998)
Lisa Kaltenegger, Alien Earths: Planet Hunting in the Cosmos (Allen Lane, 2024)
Andrew H. Knoll, Life on a Young Planet: The First Three Billion Years of Evolution on Earth (Princeton University Press, 2004)
Charles H. Langmuir and Wallace Broecker, How to Build a Habitable Planet: The Story of Earth from the Big Bang to Humankind (Princeton University Press, 2012)
Joshua Winn, The Little Book of Exoplanets (Princeton University Press, 2023)
In Our Time is a BBC Studios Audio Production