An extrasolar planet (or exoplanet) is a natural planet in a planetary system outside our own solar system. 

In 2013, estimates of the number of terrestrial planets in the Milky Way ranged from at least 17 billion to at least 144 billion. The smaller estimate studied planet candidates gathered by the Kepler space observatory. 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".

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".

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. 

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".

Confirmed discoveries
The first published and confirmed discovery was made in 1988. It was finally confirmed in 2002.

In 1992, radio astronomers announced the discovery of planets around a pulsar. 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). 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.

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 can be free-floating or orbit a brown dwarf
 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.

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.  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.

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. For comparison, the four solar terrestrial planets are included in this list.

Related pages 
 Planet
 List of exoplanets
 dwarf planet
 51 Pegasi b
 70 Virginis b

Other websites

Search projects 
 University of California Planet Search Project
 The Geneva Extrasolar Planet Search Programmes
 PlanetQuest distributed computing project
Extrasolar Planets

Resources 
 NASA's PlanetQuest 
 PlanetQuest 3D Atlas of extrasolar planets within 400 light years of our Solar System 
 Planetquest Flash 
 German Center for Exo-Planet Research Jena/Tautenburg
 Astrophysical Institute & University Observatory Jena (AIU)
 Table of known planetary systems
 Extrasolar Planet XML Database 
 Andrew Collier Cameron, Extrasolar planets, Physics World (January 2001). (See the online version.)
 searchable dynamic database of extrasolar planets and their parent stars
 List of important exoplanets
 Extrasolar Planets - D. Montes, UCM
 Extrasolar Visions

News 
 6-8 Earth-Mass Planet Discovered orbiting Gliese 876 
 Newfound World Shatters Distance Record from space.com
 Oldest Known World from space.com
 Earth Sized Planets Confirmed from space.com
 Sunshade to Look for Distant Life from news.bbc.co.uk

References