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cover of episode The Habitability of Planets

The Habitability of Planets

2025/1/9
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In Our Time: Science

AI Deep Dive AI Insights AI Chapters Transcript
People
J
Jayne Birkby
M
Melvyn Bragg
O
Oliver Shorttle
S
Saidul Islam
Topics
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、以及适宜的温度和压力范围,可能还需多种环境的协同作用。地球生命可能起源于距今45亿年前,但最早的直接证据仅追溯到35亿年前,中间存在巨大时间空白。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,地质学家关注的是生命在岩石中的痕迹,生物学家关注的是生命体的自我复制和进化能力。考虑到地球生命适应能力的强韧性,地外生命可能存在于各种环境中,但生命起源所需的条件可能较为特殊,其普遍性仍有待考证。从火星带回样本进行实验室分析,将有助于解答火星早期是否存在生命以及液态水对生命起源的作用等问题。 Jayne Birkby: 寻找地外生命,一种方法是探索太阳系内行星(如火星)或冰冻卫星,另一种方法是利用望远镜观测其他恒星周围的行星,特别是与地球大小和距离恒星距离相似的行星。通过光谱分析行星大气层中的分子成分,寻找生命迹象,例如氧气和甲烷的共同存在表明可能存在生命活动。正在建设和运行中的大型地面望远镜(如ELT)和空间望远镜(如JWST和未来的Habitable Worlds Observatory)将能够对系外行星大气层进行光谱分析,寻找生命迹象。在系外行星大气层中发现表明生命存在的不平衡特征将是地外生命研究的一大突破。地球生命,特别是类人生命形式,可能具有独特性,但我们需要对地外生命持开放态度,并通过跨学科合作建立更全面的生命起源模型。 Saidul Islam: 生命的基本构成单元包括核酸(RNA和DNA)、蛋白质(由氨基酸组成)以及细胞膜(通常由脂肪酸等构成),这些分子都由碳、氢、氮、氧、磷和硫等元素组成。生命要繁荣需要持续的能量供应、营养物质供应以及有利于复制、生长和种群扩张的环境,并且需要环境条件的稳定性,避免剧烈的变化。在实验室中从简单的化学物质合成生命将是生命起源研究领域的一大突破。 Melvyn Bragg: 寻找地外生命,我们需要寻找哪些迹象?除了生命起源的化学过程,生命要繁荣还需要哪些条件?考虑到地球生命适应能力的强韧性,地外生命存在的可能性有多大?目前有哪些设备可以用来扫描天空寻找地外生命迹象?不同学科(天文学、有机化学、行星科学、地质学)之间的交流与合作对生命起源研究至关重要。

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, and bounded pressure and temperature conditions to allow complex molecules to form. Variability in environments can also help, as a chain of linked environments may be necessary to transform simple molecules into life.

Why are hydrothermal vents and warm ponds considered potential sites for the origin of life?

Hydrothermal vents provide chemical and thermal energy that could drive the chemistry needed for life, while warm ponds offer a diversity of environments where similar chemistry can occur. Both environments are thought to have the necessary conditions for life to emerge.

What is the significance of the Great Oxidation Event in Earth's history?

The Great Oxidation Event, around 2.5 billion years ago, marked a spike in atmospheric oxygen due to cyanobacteria photosynthesizing. This allowed for the development of complex life forms during the Cambrian explosion, as oxygen is a key signature of life and is constantly replenished by biological processes.

What are 'technosignatures' in the context of searching for extraterrestrial life?

Technosignatures are indicators of advanced technological civilizations, such as industrial byproducts like CFCs, which can be detected through spectroscopy. These signatures suggest the presence of intelligent life capable of creating and sustaining technology.

Why is hydrogen cyanide important in the chemistry of life's origins?

Hydrogen cyanide, along with hydrogen sulfide, can facilitate organic chemistry when exposed to sunlight in aqueous solutions. It helps form carbon-carbon bonds, which are essential for building nucleic acids, proteins, and cell membranes.

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

Planets around M dwarf stars may be tidally locked, with one side permanently facing the star. These stars are also more active, with frequent flares that can strip away atmospheres, making it difficult for life to sustain itself.

What is the role of Earth's magnetic field in protecting life?

Earth's magnetic field shields the planet from charged particles emitted by the Sun, protecting the atmosphere from being stripped away. This defense mechanism is crucial for maintaining the conditions necessary for life.

What is the significance of the Extremely Large Telescope (ELT) in the search for extraterrestrial life?

The ELT, with its 39-meter diameter, will significantly enhance the ability to detect and analyze the atmospheres of exoplanets. It aims to identify disequilibrium signatures, such as oxygen and methane, which could indicate the presence of life.

Why are sub-Neptunes and super-Earths important in the study of habitability?

Sub-Neptunes and super-Earths are the most common types of exoplanets discovered. They may have vast liquid water oceans, raising questions about whether such environments could support life, even if they differ significantly from Earth-like conditions.

What makes Darwin's 'warm little pond' theory relevant today?

Darwin's theory of a warm little pond as the cradle of life remains relevant because it suggests a restricted environment where chemistry can occur efficiently. This idea aligns with modern research on surface chemistry and the importance of finite environments for prebiotic reactions.

Chapters
This chapter explores different theories regarding the origin of life on Earth, considering the environments needed for simple molecules to evolve into complex life forms. It also examines the timing of life's emergence, based on geological evidence and the age of the planet.
  • Two main theories propose life originated in either deep-sea hydrothermal vents or warm little ponds on the Earth's surface.
  • The earliest direct evidence of life dates back 3.5 billion years, while indirect evidence suggests life may have existed as far back as 4 billion years ago.
  • A significant gap in the geological record remains, leaving a large window in which life's origin is uncertain.

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