| The poetry of reality|
|We must know. |
We will know.
|A view from the|
shoulders of giants.
History and current state of knowledge
The first exoplanet discovered was found orbiting a pulsar, PSR B1257+12, during a 1993 study led by Alex Wolszczan of Pennsylvania State University. It wasn't until 1995 that Michel Mayor and Didier Queloz of the University of Geneva confirmed an exoplanet around a main sequence star, 51 Pegasi.
As of August 6, 2019, 4,103 planets in 3,056 planetary systems (with 665 multiple-planet systems) have been found. Most of these exoplanets are gas giants; this is most likely due to the limits of current detection methods. Some rocky planets have been found as well. Unlike gas giants, rocky planets may, given the right conditions, be able to sustain life.
Currently, the most notable of these rocky planets is the relatively nearby (20 light-years) planet Gliese 581c. Of all the known exoplanets, this one comes closest to being capable of sustaining life, though its existence is disputed.
Epsilon Eridani is a star system 10.5 light years away from Earth. It is an orange dwarf star approximately 850 million years old. There are currently two confirmed planets in the system: A Jupiter-sized planet orbiting outside of ε Eridani's first asteroid belt, and a Saturn-sized planet at about the same distance from the star as Pluto is from the Sun. It is expected that more planets will be found in the system within a decade when there are better telescopes.
Many scientists cite the number of exoplanets and their rate of discovery as evidence that Earth-like planets, and eventually extraterrestrial life, will be inevitably found. Critics of this view are quick to point out that all the planets so far found certainly don't support this conclusion — as all known exoplanets orbit too close to their star or are gas giants. However, the search for exoplanets is subject to a high degree of selection bias. All the methods outlined below lead to a huge tendency to find large or closely-orbiting planets. With the transit method, large planets produce a more easily observed signal; with astrometric methods, more massive planets that orbit close to their star will exert a greater force and be more easily seen. As technology improves, smaller planets and more distant planets are being discovered. While it is yet to be confirmed that our own solar system is typical, the selection bias means that exoplanets are not yet strong enough evidence to say that the solar system is unique or part of a special creation.
It is important to note that, despite news that often announce the discovery of habitable planets such as Proxima Centauri b (yes, around the closest star to our Sun), Kepler-62f, Kepler-186f, and some more, we just know there is a planet (sometimes more) orbiting a given star and depending of the method used for its detection (radial velocity measurements or looking for transits in front of its home star) just its minimum mass (depending of how inclined is its orbit respect to us, usually unknown) and its radius respectively, as well in both cases that, according to our climate models, at that distance temperatures allow liquid water to exist. We do not know if those planets are more or less Earth-like (thus habitable for us), Venus-like (or not so Venus-like) hells or worse, something in between, or exotic worlds that look like as if they came from a science-fiction work (much less if there is life on them); at best we can use climate or geological modelling to attempt to deduce what kind of conditions could be expected to be found there, that it would not be strange that turned out to be wrong as we've just a couple of worlds close enough to study them in detail (in our Solar System, of course) and our models are based on extrapolations of what happens there.
- California & Carnegie Planet Search
- Encyclopedia of Science, David Darling
- The Extrasolar Planets Encyclopaedia
- Interactive Extra-solar Planets Catalog, The Extrasolar Planets Encyclopaedia, accessed 6 August 2019
- This point is highly debatable; there is no real reason why some form of life could not exist elsewhere than rocky planets.
- Again, we are guilty of terracentrism here, imagining that only life like ours on a planet like ours could occur.
- Does Gliese 581g exist?
- R.I.P. Possibly Habitable Planet Gliese 581g? Not So Fast, Co-Discoverer Says
- Space.com report of Royal Astronomical Society meeting in Glasgow, Scotland April 2010
- www.nasa.gov NASA publishes findings by the PLANET organization
- In systems with several planets transiting it's often possible to determine their individual masses -thus their densities-, as the case of the famous TRAPPIST-1 system.