Extrasolar planet

any planet beyond the Solar System

An extrasolar planet (or exoplanet) is a natural planet in a planetary system outside our own solar system. A related concept is an exomoon, a natural satellite orbiting an exoplanet.

Artist's impression of the nonexistent Fomalhaut b, an exoplanet directly observed by the Hubble telescope
Planet Fomalhaut b (inset against Fomalhaut's interplanetary dust cloud) imaged by the Hubble Space Telescope's coronagraph (NASA photo)
Discovery image of the Gliese 758 system, taken with Subaru telescope in the near infrared. It is unclear whether the companion should be regarded as a planet or a brown dwarf.
2MASS J044144 is a brown dwarf with a companion about 5-10 times the mass of Jupiter. It is not clear whether this companion object is a sub-brown dwarf or a planet.
Exoplanet discoveries by year

In 2013, estimates of the number of terrestrial planets in the Milky Way ranged from at least 17 billion[1] to at least 144 billion.[2] The smaller estimate studied planet candidates gathered by the Kepler space observatory.[3] Among them are 461 Earth-size planets, at least four of which are in the "habitable zone" where liquid water can exist. One of the four, dubbed Kepler-69c, is a mere 1.5 times the size of the Earth and around a star like our own Sun – about as near as the current data allow to finding an "Earth 2.0".[4]

Earlier work suggested that there are at least 100 billion planets of all types in our galaxy, an average of at least one per star. There are also planets that orbit brown dwarfs, and free-floating planets that orbit the galaxy directly just as the stars do. It is unclear whether either type should be called a "planet".[5][6][7]

Analogies with planets in the Solar System apply to few of the extrasolar planets known. Most are quite unlike any of our planets, for example the so-called "hot Jupiters".

History

Early speculations

In the sixteenth century, the Italian philosopher Giordano Bruno, an early supporter of the Copernican theory that the Earth and other planets orbit the Sun, put forward the view that the fixed stars are similar to the Sun and are likewise accompanied by planets. Bruno was burnt at the stake by the Holy Inquisition.[8]

In the eighteenth century, the same possibility was mentioned by Isaac Newton in his Principia. Making a comparison to the Sun's planets, he wrote "And if the fixed stars are the centres of similar systems, they will all be constructed according to a similar design and subject to the dominion of One".[9]

Confirmed discoveries

The first published and confirmed discovery was made in 1988.[10] It was finally confirmed in 2002.

In 1992, radio astronomers announced the discovery of planets around a pulsar.[11] These pulsar planets are believed to have formed from the unusual remnants of the supernova that produced the pulsar, in a second round of planet formation. Otherwise they may be the remaining rocky cores of gas giants that survived the supernova and then decayed into their current orbits.

On October 6, 1995, Michel Mayor and Didier Queloz of the University of Geneva announced the first definitive detection of an exoplanet orbiting an ordinary main-sequence star (51 Pegasi).[12] This discovery, made at the Observatoire de Haute-Provence, started the modern era of exoplanetary discovery. Technological advances, most notably in high-resolution spectroscopy, led to the quick detection of many new exoplanets. These advances allowed astronomers to detect exoplanets indirectly by measuring their gravitational influence on the motion of their parent stars. Additional extrasolar planets were eventually detected by watching occultations when a star becomes dimmer as an orbiting planet passed in front of it.

In May 2016 NASA announced the discovery of 1,284 exoplanets which brought the total number of exoplanets to over 3,000.[13]

Types

Extrasolar planets can have many different forms.

  • They can be gas giants or rocky planets
    • They can possibly be dwarf planets, i.e. planets smaller and less dense than regular planets
  • They can orbit several different types of stars
  • They may support life. One recently discovered exoplanet, Gliese 581g is thought to possibly support life, but the existence of this planet is not yet confirmed.


Classes of exoplanets include:


  • A super-terran or super-Earth is a terrestrial planet that is bigger than Earth, but smaller than Neptune
  • A water-world is a hypothetical class of planet between terrestrial and jovian. These worlds would have very very little, if any dry land.
  • Hot Jupiters are gas planets orbiting closer to their stars than Mercury to the sun.
  • Rogue planets orbit no stars at all.


Nearest

The nearest star with planets is Alpha Centauri. It is 4.3 light years away. Using standard rockets, it would take tens of thousands of years to get there.[14] The nearest star similar to our Sun is Tau Ceti. It has five planets, one of which in the habitable zone, where liquid water may exist.[15][16]

Most Earth-like

Some extrasolar planets might be Earth-like. This means that they have conditions very similar to that of the Earth. Planets are ranked by a formula called the Earth similarity index or ESI for short. The ESI goes from one (most Earth-like) to zero (least Earth-like). For a planet to be habitable it should have an ESI of at least 0.8.[17] For comparison, the four solar terrestrial planets are included in this list.

Name ESI SFV HZD COM ATM Planet type Star Habitability Distance (ly)StatusYear of
discovery
Ref
Earth1.00 0.72−0.50−0.31−0.52warm terranGmesoplanet0Non-exoplanet, inhabitedprehistoric
Kepler-438b0.88 0.88−0.93−0.14−0.73warm terranMmesoplanet472.9confirmed2015
Kepler-1410b0.88 0.63−0.88−0.16−0.06warm superterranKmesoplanet1213.4confirmed2011[18]
Gliese 667 Cc0.84 0.64−0.62−0.15+0.21warm terranMmesoplanet23.6confirmed2011[19]
Kepler-442b0.83 0.98−0.72−0.15+0.28warm superterranKmesoplanet1291.6confirmed2015
Kepler-62e0.83 0.96−0.70−0.15+0.28warm superterranKmesoplanet1199.7confirmed2013
Kepler-452b0.83 0.93−0.61-0.15-0.30warm superterranGmesoplanet1402.5confirmed2015[20][21][22]
Gliese 832 c0.81 0.96−0.72−0.15+0.43warm superterranMmesoplanet16.1confirmed2014
Kepler-283c0.79 0.85−0.58−0.14+0.69warm superterranKmesoplanet1496.8confirmed2011
Kepler-436b0.79 0.33−0.87−0.14+0.47warm superterranMmesoplanet1339.4confirmed2015
Kepler-1229b0.79 0.00−0.40−0.15+0.44warm superterranMmesoplanet769.7confirmed2016
Tau Ceti e0.78 0.00−0.92−0.15+0.16warm superterranGmesoplanet11.9unconfirmed2012
Kepler-296f0.78 0.15−0.90−0.14+0.53warm superterranMmesoplanet1089.6confirmed2011
Gliese 180 c0.77 0.42−0.53−0.14+0.64warm superterranMmesoplanet39.5unconfirmed2014
Gliese 667 Cf0.77 0.00-0.22−0.16+0.08warm terranMpsychroplanet23.6dubious2013
Gliese 581 g0.76 1.00-0.70−0.15+0.28warm superterranMmesoplanet20.2dubious2010
Gliese 163 c0.75 0.02−0.96−0.14+0.58warm superterranMmesoplanet48.9confirmed2012
Gliese 180 b0.75 0.41−0.88−0.14+0.74warm superterranMmesoplanet39.5unconfirmed2014
HD 40307 g0.74 0.04−0.23−0.14+0.77warm superterranKpsychroplanet41.7confirmed2012
Kepler-61b0.73 0.27−0.88−0.13+1.24warm superterranMmesoplanet1062.8confirmed2013
Kepler-443b0.73 0.91−0.49−0.13+1.44warm superterranKmesoplanet2564.4confirmed2015
Gliese 422 b0.71 0.17−0.41−0.13+1.11warm megaterranMmesoplanet41.3unconfirmed2014
Kepler-22b0.71 0.53−0.64−0.12+1.79warm superterranGmesoplanet619.4confirmed2011
Kepler-440b0.70 0.00+0.01−0.15+0.38warm superterranKpsychroplanet706.5confirmed2015
Kepler-298d0.68 0.00−0.86−0.11+2.11warm superterranKmesoplanet1545confirmed2012[23]
Kepler-439b0.68 0.00−0.99−0.13+1.18warm superterranGthermoplanet1914.8confirmed2015
Kapteyn b0.67 0.00+0.08−0.15+0.57warm superterranMpsychroplanet12.7unconfirmed2014
Kepler-62f0.67 0.05+0.45−0.16+0.19warm superterranKpsychroplanet1199.7confirmed2013
Kepler-186f0.64 0.00+0.48−0.17−0.26warm terranMpsychroplanet492confirmed2014
Kepler-174d0.61 0.00+0.32−0.13+1.77warm superterranKpsychroplanet878.3confirmed2011
Gliese 667 Ce0.60 0.00+0.51−0.16+0.23warm terranMpsychroplanet23.6dubious2013
Gliese 682 c0.59 0.00+0.22−0.14+1.19warm superterranMpsychroplanet16.6unconfirmed2014
Gliese 581 d0.53 0.00+0.78−0.14+0.94warm superterranMhypopsychroplanet20.2unconfirmed2007[24][25]
Kepler-155c hot superterranKhyperthermoplanet?965confirmed2014
Venus0.78 0.00−0.93−0.28−0.70warm terranGhyperthermoplanetclose to zeronon-exoplanetprehistoric
Mars0.64 0.00+0.33−0.13−1.12warm subterranGhypopsychroplanetclose to zeronon-exoplanetprehistoric
Mercury0.39 0.00−1.46−0.52−1.37hot mercurianGnon-habitableclose to zeronon-exoplanetprehistoric

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