cover of episode The Habitability of Planets

The Habitability of Planets

2025/1/9
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In Our Time

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J
Jayne Birkby
O
Oliver Shorttle
S
Saidul Islam
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Oliver Shorttle: 地球生命起源的环境需要具备简单的分子构成单元、能量来源、适宜的温度和压力范围,以及环境的多样性。生命可能起源于深海热液喷口或地表温暖的小水塘。地球生命的出现时间可能在45亿年前地球形成后1亿年到35亿年前之间,目前我们只能追溯到35亿年前的直接生命证据。对“生命”的定义因研究领域而异,例如天文学家关注的是生命对行星大气层的影响,而生物学家关注的是生命体的自我复制和进化能力。生命的出现和演化依赖于各种偶然因素,从星系尺度到行星本身的特性都有影响。地球生命展现出强大的适应性和韧性,这表明地外生命存在的可能性很高,但生命起源的条件可能比较特殊。从火星带回样本进行实验室研究,有助于了解早期火星的环境条件以及生命存在的可能性。 Jayne Birkby: 寻找地外生命,可以探索太阳系内的行星(如火星和冰冻卫星)或利用望远镜观测其他恒星周围的行星,寻找液态水存在的迹象。地球大气中氧气的存在是生命活动的标志,因为氧气会不断被消耗,需要生命活动持续补充。地球生命可能是恒星形成过程的自然副产品,因此地外生命可能普遍存在。目前正在建设和计划中的大型望远镜(如ELT和Habitable Worlds Observatory)将能够探测系外行星大气中的生命迹象。判断地外行星生命演化阶段,需要考虑行星年龄及其环境因素,目前只能与地球生命演化进行比较。系外行星是研究地外生命的重要对象,因为它们与太阳系行星类似,且具有多样化的环境条件。地球生命,特别是类人生命,可能具有独特性,但需要保持开放心态,探索不同可能性。 Saidul Islam: 地球生命的基本构成单元是核酸(RNA和DNA)、蛋白质(氨基酸构成)和细胞膜(脂肪酸等构成),这些分子都由碳、氢、氮、氧、磷和硫等元素组成。地球早期生命起源的过程是一个逐步复杂化的化学过程,而非瞬间的“自发”产生。生命起源的化学过程可能遵循一定的模式,取决于地球化学环境,但生命本身的演化则更为复杂。生命繁荣需要持续的能量供应、营养物质和适宜的复制环境,同时需要环境的稳定性,避免剧烈的变化。在实验室中从简单的化学物质合成生命是生命起源研究领域最重大的突破。实验室研究生命起源需要更先进的分析技术,以研究复杂的化学体系。

Deep Dive

Key Insights

What are the key environmental conditions needed for life to begin on a planet?

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.

Why is oxygen considered a key signature for detecting life on other planets?

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.

How do astronomers search for signs of life on exoplanets?

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.

What role does hydrogen cyanide play in the chemistry of life?

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.

What are technosignatures, and how do they differ from biosignatures?

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.

What challenges do planets around M dwarf stars face in terms of habitability?

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.

Why is Earth’s magnetic field important for habitability?

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.

What is the significance of sub-Neptunes in the search 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.

How does the concept of Darwin’s ‘warm little pond’ remain relevant in modern astrobiology?

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.

What is the ELT, and how will it contribute to the search for life?

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.

Shownotes Transcript

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