Visible with the unaided eye, Tau Ceti is a stable, single, sun-like class G star with about 80% the mass, 80% the radius and 52% the solar luminosity. In addition to a disk of debris analogous to the Kuiper belt, five planets have been reported, however, some have been retracted while others are candidates. While planets b, c and d are currently unconfirmed, candidate planets Tau Ceti e and f with orbits of 163 and 636 days are believed to orbit within the habitable zone of the star at a generous radius of 0.55-1.16AU. Since 2017, recent candidates are Tau Ceti g and h with orbits of 20 and 49 days. This updated 4-planet model is dynamically packed and potentially stable for billions of years, while more candidates, such as b and c could still be (re)detected. Tau Ceti e orbits at a distance of 0.552AU and has a minimum mass of 4 Earth masses. Tau Ceti f orbits at a distance of 1.35AU and has also a minimum mass of 4 Earth masses, which means they may either be a super-Earths or a terrestrial planets. Both planets are situated at the edges of the HBZ, i.e. during most time of their periods, because their orbits are quite eccentric (0.2). With further refinements more accurate data may become available.
Image credit: RWD
Planet Designation | Title | Constellation | Distance | SMA | Period | Mass | Radius | Year | |
---|---|---|---|---|---|---|---|---|---|
1 | Proxima b | Nearest Known Exoplanet | Centaurus | 4.24ly | 0.04856AU | 11.1868d | 1.27⊕ | 2016 | |
2 | Barnard b | Second Closest Known Exoplanet | Ophiuchus | 5.9ly | 0.02294AU | 3.1533d | 3.23⊕ | 2024 | |
3 | Epsilon Eridani b | Asteroid Belts and Controversal Planets | Eridanus | 10.48ly | 3.53AU | 2671d | 245⊕ | 2000 | |
4 | Ross 128 b | Third Closest Known Exoplanet | Virgo | 11.03ly | 0.0496AU | 9.8658d | 1.35⊕ | 2017 | |
5 | Tau Ceti e | Planet Needing Confirmation | Cetus | 11.91ly | 0.538AU | 162.87d | 3.29⊕ | 2017 | |
6 | Luyten's Star b | Only 1.2 Light-Years Away from Procyon | Canis Minor | 12.2ly | 0.091101AU | 18.6498d | 2.89⊕ | 2017 | |
7 | Kapteyn's Star c | Oldest-known Cold Exoplanet | Pictor | 12.76ly | 0.311AU | 121.54d | 4.8⊕ | 2014 | |
8 | Wolf 1061 c | Temperate Super-Earth or Super-Mars | Ophiuchus | 14.04ly | 0.089AU | 17.8719d | 3.41⊕ | 2015 | |
9 | Gliese 3323 b | Little Known in Habitable Zone | Eridanus | 17.54ly | 0.03282AU | 5.3636d | 2.02⊕ | 2017 | |
10 | LTT 1445A b | Planet in Triple Red Dwarf System | Eridanus | 22.5ly | 0.022AU | 5.35876d | 2.2⊕ | 1.18⊕ | 2019 |
11 | Gliese 667C c | Earth-like Planet in Triple Star System | Scorpius | 23.6ly | 0.125AU | 28.14d | 3.71⊕ | 2013 | |
12 | Gliese 1132 b | Heat Planet with Atmosphere | Vela | 39.3ly | 0.0157AU | 1.62893d | 1.66⊕ | 1.19⊕ | 2015 |
13 | Trappist-1 d | Small but Most Earth-like Known Planet | Aquarius | 39.5ly | 0.02227AU | 4.04922d | 0.297⊕ | 0.78⊕ | 2016 |
14 | LHS 1140 b | A Massive Super-Earth Inside Habitable Zone | Cetus | 40.67ly | 0.0946AU | 24.7372d | 6.64⊕ | 1.72⊕ | 2017 |
15 | Gliese 143 b | A Huge Neptunian Around a K-Star | Reticulum | 53.2ly | 0.1915AU | 35.6125d | 30.63⊕ | 2.61⊕ | 2019 |
16 | TOI-270 b | Nearby M-Dwarf Planets | Dorado | 73.23ly | 0.03197AU | 3.36015d | 1.9⊕ | 1.21⊕ | 2019 |
17 | Gliese 3470 b | Evaporating Planet | Cancer | 95.5ly | 0.0355AU | 3.33665d | 13.4⊕ | 4.57⊕ | 2012 |
18 | K2-3 b | Super-Earths Trio in Leo | Leo | 143.9ly | 0.0747AU | 10.0547d | 2.7⊕ | 2.07⊕ | 2015 |
19 | K2-288B b | Detected by Citizen Scientists | Taurus | 226ly | 0.164AU | 31.3935d | 4⊕ | 1.90⊕ | 2018 |
20 | Kepler-186 f | Earth-sized Cold Kepler Planet | Cygnus | 582ly | 0.432AU | 129.944d | 1.4⊕ | 1.16⊕ | 2014 |
Most of the stars introduced on this page are 'Red Dwarfs'. Actually they represent the most common type of stars. About 73% of all stars in the Milky Way galaxy are dim red dwarfs, featuring less than half the solar surface temperature and low luminosity, but in turn high stellar activity, such as flares and hazardous radiation that can hit red dwarf planets hard potentially prohibiting formation of known lifeforms.
Given its minute energy emission, the habitable zone (HBZ, an imaginary ring where temperatures support liquid water) of a red dwarf is situated near the star, as are planets orbiting inside this zone. The gravitational pull of the star can tidally lock a nearby planet which then faces one hemisphere to the star while the other is enshrouded in darkness - like the Earth moon - the axial rotation period equals the orbital period.
Some densely populated systems, such as TRAPPIST-1, have several planets orbiting in close proximity in that an observer on a planet could see other planets larger than our moon in the sky. Also, the planet may have one or multiple moons themselves. In any case a truly impressive spectacle with fast changes.
Due to their low visual luminosity no known red dwarf is visible by the naked eye, not even the nearest such as Proxima Centauri or the solitary Barnard's Star. Others, such as Gliese 667, are triple star systems but anywhere near visual magnitude
Image Credit: NASA/ESA/STScl