Proxima Centauri b

• 1. Introduction

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  Proxima Centauri b sits just 4.2 light-years from Earth, the closest exoplanet ever found to our solar system. That number sounds modest in everyday terms, but it represents a distance so vast that Voyager 2 would need roughly 75,000 years to cover it. And yet, by cosmic standards, this world is practically on our doorstep. Scientists announced its existence on the 24th of August 2016, and it has captured imaginations ever since. Is there liquid water on its surface? Does it have an atmosphere? Could something be alive there? Those questions remain stubbornly open. What we do know is that Proxima b orbits inside the habitable zone of its star, completing one lap every 11.2 Earth days. How a world that zips around its sun faster than a single Earth fortnight could possibly support life is the puzzle at the heart of this story.

• 2. The Hunt and the Find

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  Astronomers had been watching Proxima Centauri for signs of planets long before 2016. Studies in 2008 and 2009 ruled out the existence of planets larger than Earth in its habitable zone, and the search went quiet. What changed the picture were motion anomalies spotted in data collected at the European Southern Observatory in Chile. The star was wobbling in ways that could not be explained by its own flares or internal activity. In January 2016, a team launched a dedicated campaign called the Pale Red Dot project to pin down whether a planet was responsible. The team, led by Anglada-Escudé, concluded after months of Doppler spectroscopy that a terrestrial exoplanet in the habitable zone was the best explanation. The formal announcement came on the 24th of August 2016 through the European Southern Observatory. Since then, the Proxima Centauri system has grown more crowded: Proxima d, orbiting even closer to the star, was confirmed in 2022, while a candidate called Proxima c, reported in 2020, remains disputed because of possible artifacts in the detection data.

• 3. A Star Unlike Our Sun

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  Proxima Centauri itself is a red dwarf with only 12.2% of the Sun's mass and 15.4% of its radius. It radiates a mere 0.005% of the visible light that the Sun produces, and its average energy output is about 0.17% of the Sun's. Despite sitting so close to such a dim star, Proxima b still receives roughly 70% of the infrared energy that Earth gets from the Sun, purely because its orbit is so tight. But the star is not the quiet, steady companion that our Sun is. Proxima Centauri is a flare star whose luminosity can vary by a factor of 100 within the span of a few hours. Its magnetic field, which cycles over a period of seven years, is considerably stronger than the Sun's, with an intensity measured at 600 units compared to the Sun's more modest field. That combination of low average light and violent, unpredictable outbursts shapes every question about whether Proxima b could host life. Proxima Centauri is too faint for the naked eye to see under normal conditions, becoming briefly visible only during its most powerful superflares.

• 4. Tidal Forces and a Frozen Spin

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  At an orbital distance of roughly 0.04848 AU, Proxima b sits more than 20 times closer to its star than Earth is to the Sun. That proximity almost certainly locks the planet gravitationally, so that the same hemisphere permanently faces Proxima Centauri, the same way the Moon always shows the same face to Earth. A 1:1 tidal lock of that kind would produce a world of violent extremes: a perpetually sunlit hemisphere baked by stellar radiation and a night side in permanent darkness. Whether habitable zones could carve out a living space in that strip of eternal twilight is an open question in climate science. There is, however, an escape from strict tidal locking. If the planet's orbital eccentricity exceeds a threshold of about 0.06-0.1, it could be dragged into a 3:2 spin-orbit resonance like Mercury rather than a full lock. Other planets in the system, or gravitational nudges from the Alpha Centauri pair, could excite that eccentricity. A non-locked planet would pay a different price, though: intense tidal heating of its interior that could destabilize a magnetic-field-generating dynamo, and ocean tides far more powerful than any seen on Earth.

• 5. The Atmosphere Problem

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  Proxima b receives somewhere between 10 and 60 times as much ultraviolet and X-ray radiation as Earth does, with some estimates suggesting it may have accumulated 7-16 times Earth's cumulative lifetime dose of high-energy radiation. That radiation strips atmospheres. UV and X-rays heat hydrogen in the upper atmosphere until it moves fast enough to escape a planet's gravity entirely, dragging other gases out with it. Stellar winds at Proxima b's orbital distance may exert a pressure roughly ten thousand times greater than the solar wind pressing on Earth, and coronal mass ejections pose an even larger threat. Before the star settled onto the main sequence, Proxima b may have spent up to 180 million years too close to its star for water to condense at all, running the risk of a runaway greenhouse effect similar to what is believed to have happened on Venus. Modelling by Ribas et al. in 2016 suggested the planet would have lost no more than the equivalent of one Earth ocean of water, but later work by Airapetian et al. in 2017 concluded that an atmosphere could be stripped entirely within ten million years. Those estimates hinge almost entirely on the initial mass of the atmosphere, making them highly uncertain. One path back from atmospheric loss: volcanic activity could rebuild a secondary atmosphere dominated by carbon dioxide, which would be more stable than an Earth-like one and might be buttressed further by the arrival of water-bearing exocomets.

• 6. Life on the Edge

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  In exoplanet science, habitability is defined narrowly as the possibility that liquid water exists on a planet's surface, and Proxima b sits squarely within Proxima Centauri's classical habitable zone. Its equilibrium temperature is estimated at about 234 Kelvin. The climate models scientists have applied range from Earth's general circulation models to custom simulations, and they produce a startling variety of possible worlds: a planet entirely covered in ice, one with a planet-wide ocean, or something in between with strange lobster-claw-shaped patches of liquid water near the equator. An ice-covered version with a subsurface ocean might sustain cryovolcanic activity at rates comparable to what is observed on Jupiter's moon Io, generating a thin outer envelope of gas like that of Europa. One calculation from 2017 estimated that the productivity of an ecosystem based on photosynthesis on Proxima b might reach about 20% of Earth's total. In an unusual advantage for any life that might exist, the planet orbits a star whose lifespan far exceeds the estimated age of the universe, giving biology far more time to develop than the Sun has ever provided Earth.

• 7. Reaching the Unreachable

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  Proxima b has not yet been directly imaged; its separation from its star is too small for current instruments to resolve. It is unlikely to pass in front of its star as seen from Earth, and every transit survey has returned empty. In April and May 2019, the Breakthrough Listen project, which monitors Proxima Centauri for technology-related radio signals, detected a candidate signal called BLC1. Subsequent analysis indicated that it is probably of human origin. Future instruments including the James Webb Space Telescope and the Nancy Grace Roman Space Telescope could attempt a direct observation, though separating the planet's light from its star remains a formidable challenge. Proposed signatures observable from Earth include the reflection of starlight off an ocean, the radiative fingerprints of atmospheric gases, and the patterns of atmospheric heat transport. For physical spacecraft, the Breakthrough Starshot project aims to develop laser-propelled solar sails capable of reaching speeds of 20% of the speed of light, targeting a journey to Proxima Centauri within the 21st century. The harder engineering problem is not the journey itself but deceleration: arriving at a useful speed at a world 4.2 light-years away and surviving collisions with interstellar particles along the way. From Proxima b itself, if anyone or anything were ever to stand on its surface, the two stars of Alpha Centauri would blaze in the sky brighter than Venus at its most brilliant as seen from Earth, with apparent magnitudes of -6.8 and -5.2.