Proxima Centauri b

Proxima Centauri b (also called Proxima b or Alpha Centauri Cb) is an exoplanet orbiting in the habitable zone of the red dwarf star Proxima Centauri, which is the closest star to the Sun and part of a triple star system. It is approximately from Earth in the constellation Centaurus, making it and Proxima c the closest known exoplanets to the Solar System.
Proxima Centauri b orbits the star at a distance of roughly with an orbital period of approximately 11.2 Earth days, and has an estimated mass of at least 1.2 times that of Earth. It is subject to stellar wind pressures of more than 2,000 times those of Earth from the solar wind, and its habitability has not yet been definitively established.
The planet's discovery was announced in August 2016. It was found using the radial velocity method, where periodic Doppler shifts of the parent star's spectral lines suggest an orbiting object. From these readings, the parent star's radial velocity relative to the Earth is varying with an amplitude of about 1.4 metres (4.5 feet) per second. According to Guillem Anglada‐Escudé, the planet's proximity to Earth offers an opportunity for robotic exploration with the Starshot project or, at least, "in the coming centuries".
Without its orbital inclination known, Proxima Centauri b's exact mass is unknown. If its orbit is nearly edge-on, it would have a mass of (Earth masses). Statistically, there is a roughly 90% chance that its mass is less than .
In May 2019, a paper presenting recent Spitzer Space Telescope data concluded that Proxima Centauri b did not transit its sun relative to Earth, and attributed previous transit detections to correlated noise.
Physical characteristics.
Mass, radius, and temperature.
The apparent inclination of Proxima Centauri b's orbit has not yet been measured. The minimum mass of Proxima b is , which would be the actual mass if its orbit were seen edge-on from the Earth. Once its orbital inclination is known, the mass will be calculable. More tilted orientations imply a higher mass, with 90% of possible orientations implying a mass below . The planet's exact radius is unknown. If it has a rocky composition and a density equal to Earth's, its radius is at least . It could be larger if it has a lower density than Earth, or a mass higher than the minimum mass. Like many super-Earth sized planets, Proxima Centauri b may have an icy composition like Neptune, with a thick enveloping hydrogen and helium atmosphere; this likelihood has been calculated to be greater than 10%. The planet has an equilibrium temperature of , somewhat colder than Earth’s .
If Proxima Centauri b's orbit is coplanar with that of the candidate exoplanet Proxima Centauri c, estimates of whose true mass were recently calculated using various combinations of its spectroscopic orbital parameters, Gaia DR2 proper motion anomaly, and astrometric measurements, then a true mass of Proxima b can be estimated. For example, a 2020 paper published by Kervella et al. estimated Earth masses, and another by Benedict et al. estimated Earth masses as true mass values for Proxima b.
Host star.
The planet orbits an M-type red dwarf named Proxima Centauri. The star has a mass of and a radius of . It has a surface temperature of 3042 K and is 4.85 billion years old. In comparison, the Sun is 4.6 billion years old and has a surface temperature of 5778 K. Proxima Centauri rotates once roughly every 83 days, and has a luminosity about . Like the two larger stars in the triple star system, Proxima Centauri is rich in metals compared with the Sun, something not normally found in low-mass stars like Proxima. Its metallicity ([Fe/H]) is 0.21, or 1.62 times the amount found in the Sun's atmosphere.
Even though Proxima Centauri is the closest star to the Sun, it is not visible to the unaided eye from Earth because of its low luminosity (average apparent magnitude of 11.13).
Proxima Centauri is a flare star. This means that it undergoes occasional dramatic increases in brightness and high-energy emissions because of magnetic activity that would create large solar storms. On 18 March 2016, a superflare was observed with an energy of 1026.5 joules. The March 2016 flare reached about 68 times usual level, thus a little brighter than the Sun. The surface irradiation was estimated to be 100 times what is required to kill even UV-hardy microorganisms. Based on the rate of observed flares, total ozone depletion of an Earth-like atmosphere would occur within several hundred thousand years.
Orbit.
Proxima Centauri b orbits its host star every 11.186 days at a semi-major axis distance of approximately , which means the distance from the exoplanet to its host star is one-twentieth of the distance from the Earth to the Sun. Comparatively, Mercury, the closest planet to the Sun, has a semi-major axis distance of 0.39 AU. Proxima Centauri b receives about 65% of the amount of radiative flux from its host star that the Earth receives from the Sun – for comparison, Mars receives about 43%. Most of the radiative flux from Proxima Centauri is in the infrared spectrum. In the visible spectrum the exoplanet receives only ~3% of the PAR (400–700 nm) of Earth irradiance – for comparison, Jupiter receives 3.7% and Saturn 1.1%. – so it would usually not get much brighter than twilight anywhere on Proxima Centauri b's surface. The maximum illumination of horizontal ground by twilight at sunrise is about 400 lux, while the illumination of Proxima b is about 2700 lux with a quiet Proxima. Proxima also has flares. The brightest flare observed until 2016 had increased the visual brightness of Proxima about 8 times, which would be a large change from the previous level but, at about 17% the illumination of Earth, not very strong sunlight. However, because of its tight orbit, Proxima Centauri b receives about 400 times more X-ray radiation than the Earth does.
Habitability.
The habitability of Proxima Centauri b has not been established, but the planet is subject to stellar wind pressures of more than 2,000 times those experienced by Earth from the solar wind. This radiation and the stellar winds would likely blow any atmosphere away, leaving the subsurface as the only potentially habitable location on that planet.
The exoplanet is orbiting within the habitable zone of Proxima Centauri, the region where, with the correct planetary conditions and atmospheric properties, liquid water may exist on the surface of the planet. The host star, with about an eighth of the mass of the Sun, has a habitable zone between ∼0.0423–0.0816 AU. In October 2016, researchers at France's CNRS research institute stated that there is a considerable chance of the planet harboring surface oceans and having a thin atmosphere. However, unless the planet transits in front of its star from the perspective of Earth, it is difficult to test these hypotheses.
Tidal effects and stellar flares.
Even though Proxima Centauri b is in the habitable zone, the planet's habitability has been questioned because of several potentially hazardous physical conditions. The exoplanet is close enough to its host star that it might be tidally locked. In this case, it is expected that any habitable areas would be confined to the border region between the two extreme sides, generally referred to as the terminator line, since it is only here that temperatures might be suitable for liquid water to exist. If the planet's orbital eccentricity is 0, this could result in synchronous rotation, with one hot side permanently facing towards the star, while the opposite side is in permanent darkness and freezing cold. However, Proxima Centauri b's orbital eccentricity is not known with certainty, only that it is below 0.35—potentially high enough for it to have a significant chance of being captured into a 3:2 spin-orbit resonance similar to that of Mercury, where Proxima b would rotate around its axis approximately every 7.5 Earth days with about 22.4 Earth days elapsing between one sunrise and the next. Resonances as high as 2:1 are also possible. Another problem is that the flares released by Proxima Centauri could have eroded the atmosphere of the exoplanet. However, if Proxima b had a strong magnetic field, the flare activity of its parent star would not be a problem.
Climate and atmosphere possibilities.
If water and an atmosphere are present, a far more hospitable environment would result. Assuming an atmospheric N2 pressure of 1 bar and ∼0.01 bar of CO2, in a world including oceans with average temperatures similar to those on Earth, a wide equatorial belt (non-synchronous rotation), or the majority of the sunlit side (synchronous rotation), would be permanently ice-free. A large portion of the planet may be habitable if it has an atmosphere thick enough to transfer heat to the side facing away from the star. If it has an atmosphere, simulations suggest that the planet could have lost about as much as the amount of water that Earth has due to the early irradiation in the first 100–200 million years after the planet's formation. Liquid water may be present only in the sunniest regions of the planet's surface in pools either in an area in the hemisphere of the planet facing the star or—if the planet is in a 3:2 resonance rotation—diurnally in the equatorial belt. All in all, astrophysicists consider the ability of Proxima Centauri b to retain water from its formation as the most crucial point in evaluating the planet's present habitability. The planet may be within reach of telescopes and techniques that could reveal more about its composition and atmosphere, if it has any.
If an atmosphere is present, longer-wavelength radiation, from the red dwarf parent star means that weather will be affected. Cloud formation on the day side of the planet will be inhibited, compared to Earth (or Venus), resulting in clearer skies.
View from Proxima Centauri b.
Viewed from near the Alpha Centauri system, the sky would appear much as it does for an observer on Earth, except that Centaurus would be missing its brightest star. The Sun would be a yellow star of an apparent magnitude of +0.5 in eastern Cassiopeia, at the antipodal point of Alpha Centauri's current right ascension and declination, at (2000). This place is close to the 3.4-magnitude star ε Cassiopeiae. Because of the placement of the Sun, an interstellar or alien observer would find the \/\/ of Cassiopeia had become a /\/\/ shape nearly in front of the Heart Nebula in Cassiopeia. Sirius lies less than a degree from Betelgeuse in the otherwise unmodified Orion and with a magnitude of −1.2 is a little fainter than from Earth but still the brightest star in the Alpha Centauri sky. Procyon is also displaced into the middle of Gemini, outshining Pollux, whereas both Vega and Altair are shifted northwestward relative to Deneb (which barely moves, due to its great distance), giving the Summer Triangle a more equilateral appearance.
From Proxima Centauri b, Alpha Centauri AB would appear like two close bright stars with the combined apparent magnitude of −6.8. Depending on the binary's orbital position, the bright stars would appear noticeably divisible to the naked eye, or occasionally, but briefly, as a single unresolved star. Based on the calculated absolute magnitudes, the apparent magnitudes of Alpha Centauri A and B would be −6.5 and −5.2, respectively.
Formation.
It is unlikely that Proxima Centauri b originally formed in its current orbit since disk models for small stars like Proxima Centauri would contain less than one of matter within the central one AU at the time of their formation. This implies that either Proxima Centauri b was formed elsewhere in a manner still to be determined, or the current disc models for stellar formation are in need of revision.
Discovery.
The first indications of the exoplanet were found in 2013 by Mikko Tuomi of the University of Hertfordshire from archival observation data. To confirm the possible discovery, a team of astronomers launched the Pale Red Dot project in January 2016. On 24 August 2016, the team of 31 scientists from all around the world, led by Guillem Anglada-Escudé of Queen Mary University of London, confirmed the existence of Proxima Centauri b through their research, published in a peer-reviewed article in "Nature".
The measurements were done using two spectrographs, HARPS on the ESO 3.6 m Telescope at La Silla Observatory and UVES on the 8-metre Very Large Telescope. The peak radial velocity of the host star combined with the orbital period allowed for the minimum mass of the exoplanet to be calculated. The chance of a false positive detection is less than one in ten million.
Observational complications of the star tend to indicate additional, not insignificant size, orbiting planets. Another super-Earth was noted on discovery of this planet as possible; its presence would not destabilize the orbit of Proxima Centauri b. One very large super-Earth was discovered in 2019, known as Proxima Centauri c – it orbits at 1.5 AU away, too far to tug on the other planet at all significantly.
Data of ESPRESSO excludes extra companions with masses above 0.6  at periods shorter than 50 days. A potential companion, Proxima Centauri d, at 0.29 , was found to have an orbit around 5.15 days. It requires further study, to confirm its existence and identify its orbital properties.
Future observations.
A team of scientists think they can image Proxima Centauri b and probe the planet's atmosphere for signs of oxygen, water vapor, and methane, combining ESPRESSO and SPHERE on the VLT. The James Webb Space Telescope may be able to characterize the atmosphere of Proxima Centauri b, but there is no conclusive evidence for transits combining MOST and HATSouth photometry, giving it less than a 1 percent chance of being a transiting planet. Future telescopes (the Extremely Large Telescope, the Giant Magellan Telescope, and the Thirty Meter Telescope) could have the capability to characterize Proxima Centauri b.
The discovery of Proxima b was significant to Breakthrough Starshot, a proof of concept project aiming to send a fleet of miniature probes to the Alpha Centauri system. The project is led by research company Breakthrough Initiatives, and plans to develop and launch a fleet of miniature unmanned spacecraft called StarChips, which could travel at up to 20% of the speed of light, arriving at the system in roughly 20 years with notification reaching Earth a little over 4 years later.
2069 Alpha Centauri mission.
In 2017, Breakthrough Initiatives and the European Southern Observatory (ESO) entered a collaboration to enable and implement a search for habitable planets in the nearby star system, Alpha Centauri. The agreement involves Breakthrough Initiatives providing funding for an upgrade to the VISIR (VLT Imager and Spectrometer for mid-Infrared) instrument on ESO's Very Large Telescope (VLT) in Chile.