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An Earth analog, also called an Earth twin or second Earth, is a or with environmental conditions similar to those found on . The term Earth-like planet is also used, but this term may refer to any terrestrial planet.

The possibility is of particular interest to and under reasoning that the more similar a planet is to Earth, the more likely it is to be capable of sustaining complex extraterrestrial life. As such, it has long been speculated and the subject expressed in , , and . Advocates of space colonization and space and survival have long sought an Earth analog for settlement. In the far future, humans might artificially produce an Earth analog by .

Before the scientific search for and study of , the possibility was argued through philosophy and science fiction. Philosophers have suggested that the size of the universe is such that a near-identical planet must exist somewhere. The mediocrity principle suggests that planets like Earth should be common in the , while the Rare Earth hypothesis suggests that they are extremely rare. The thousands of exoplanetary star systems discovered so far are profoundly different from the , supporting the Rare Earth Hypothesis.

On 4 November 2013, astronomers reported, based on Kepler space mission data, that there could be as many as 40 billion Earth-sized orbiting in the habitable zones of and within the . The nearest such planet could be expected to be within 12 light-years of the , statistically. In September 2020, astronomers identified 24 superhabitable planets (planets better than Earth) contenders, from among more than 4000 confirmed , based on , as well as the of known life forms on the Earth.

Scientific findings since the 1990s have greatly influenced the scope of the fields of , models of planetary habitability and the search for extraterrestrial intelligence (SETI).


History
Between 1858 and 1920, Mars was thought by many, including some scientists, to be very similar to Earth, only drier with a thick atmosphere, similar axial tilt, orbit and seasons as well as a civilization that had built great . These theories were advanced by Giovanni Schiaparelli, and others. As such Mars in fiction portrayed the red planet as similar to Earth's deserts. Images and data from the (1965) and (1975–1980), however, revealed the planet as a barren cratered world. However, with continuing discoveries, other Earth comparisons remained. For example, the Mars Ocean Hypothesis had its origins in the Viking missions and was popularised during the 1980s. NASA – Mars Ocean Hypothesis With the possibility of past water, there was the possibility that life could have begun on Mars, and it was once again perceived to be more Earth-like.

Likewise, until the 1960s, was believed by many, including some scientists, to be a warmer version of Earth with a thick atmosphere and either hot and dusty or humid with water clouds and oceans. Venus in fiction was often portrayed as having similarities to Earth and many speculated about civilization. These beliefs were dispelled in the 1960s as the first space probes gathered more accurate scientific data on the planet and found that Venus is a very hot world with the surface temperature around under an acidic atmosphere with a surface pressure of .

From 2004, Cassini–Huygens began to reveal Saturn's moon Titan to be one of the most Earth-like worlds outside of the habitable zone. Though having a dramatically different chemical makeup, discoveries such as the confirmation of Titanian lakes, rivers and fluvial processes in 2007, advanced comparisons to Earth. Further observations, including weather phenomena, have aided the understanding of geological processes that may operate on Earth-like planets.

The Kepler space telescope began observing the transits of potential terrestrial planets in the habitable zone from 2011. Though the technology provided a more effective means for detecting and confirming planets, it was unable to conclude definitively how Earth-like the candidate planets actually are. In 2013, several Kepler candidates less than 1.5 Earth radii were confirmed orbiting in the habitable zone of stars. It was not until 2015 that the first near-Earth sized candidate orbiting a solar candidate, Kepler-452b, was announced.

On 11 January 2023, NASA scientists reported the detection of LHS 475 b, an Earth-like exoplanet – and the first discovered by the James Webb Space Telescope.


Attributes and criteria
The probability of finding an Earth analog depends mostly on the attributes that are expected to be similar, and these vary greatly. Generally it is considered that it would be a terrestrial planet and there have been several scientific studies aimed at finding such planets. Often implied but not limited to are such criteria as planet size, surface gravity, star size and type (i.e. ), orbital distance and stability, axial tilt and rotation, similar , , and conditions, strong and even the presence of Earth-like complex . If there is complex life, there could be some covering much of the land. If there is intelligent life, some parts of land could be covered in . Some factors that are assumed of such a planet may be unlikely due to Earth's own history. For instance, the Earth's atmosphere was not always oxygen-rich and this is a from the emergence of life. The formation, presence, influence on these characteristics of the (such as ) may also pose a problem in finding an Earth analog.

The process of determining Earth analogs often involves reconciling several registers of uncertainty quantification. As anthropologist 's work on the of analogical reasoning has shown, some planetary scientists are "more comfortable making the leap of faith to bridge time and space and pull together two disparate objects" than others are.


Size
Size is often thought to be a significant factor, as planets of Earth's size are thought more likely to be terrestrial in nature and be capable of retaining an Earth-like atmosphere.

The list includes planets within the range of 0.8–1.9 Earth masses, below which are generally classed as and above classed as . In addition, only planets known to fall within the range of 0.5–2.0 Earth radius (between half and twice the radius of the Earth) are included.

According to the size criteria, the closest planetary mass objects by known radius or mass are:

Originally thought to be in the circumstellar habitable zone (CHZ), now thought to be too hot.
Extremely hot.
1.58
Slightly larger and likely more massive, far too hot to be Earth-like.
Extremely hot. Not known to transit.

Orbits in the habitable zone.
Orbits in habitable zone.
Much hotter.
Too hot to be Earth-like.
Closest exoplanet to Earth orbiting within the habitable zone.

This comparison indicates that size alone is a poor measure, particularly in terms of . Temperature must also be considered as Venus and the planets of Alpha Centauri B (discovered in 2012), Kepler-20 (discovered in 2011), COROT-7 (discovered in 2009) and the three planets of Kepler-42 (all discovered in 2011) are very hot, and , Ganymede and Titan are frigid worlds, resulting also in wide variety of surface and atmospheric conditions. The masses of the Solar System's moons are a tiny fraction of that of Earth whereas the masses of extrasolar planets are very difficult to accurately measure. However discoveries of Earth-sized terrestrial planets are important as they may indicate the probable frequency and distribution of Earth-like planets.


Terrestrial
Another criterion often cited is that an Earth analog must be terrestrial, that is, it should possess a similar surface geology—a planetary surface composed of similar surface materials. The closest known examples are Mars and Titan and while there are similarities in their types of landforms and surface compositions, there are also significant differences such as the temperature and quantities of ice.

Many of Earth's surface materials and landforms are formed as a result of interaction with water (such as clay and ) or as a byproduct of life (such as limestone or coal), interaction with the atmosphere, volcanically or artificially. A true Earth analog therefore might need to have formed through similar processes, having possessed an atmosphere, volcanic interactions with the surface, past or present liquid water and .


Temperature
There are several factors that can determine planetary temperatures and therefore several measures that can draw comparisons to that of the Earth in planets where atmospheric conditions are unknown. Equilibrium temperature is used for planets without atmospheres. With atmosphere, a greenhouse effect is assumed. Finally, surface temperature is used. Each of these temperatures is affected by climate, which is influenced by the orbit and rotation (or tidal locking) of the planet, each of which introduces further variables.

Below is a comparison of the confirmed planets with the closest known temperatures to Earth.

Temperature comparisonsKepler-22b
206 K
−67 °C
−88.6 °F
210 K
−63 °C
−81 °F
No
0.25
Refs.


Solar analog
Another criterion of an ideal life-harboring earth analog is that it should orbit a ; that is, a star much like the Sun. However, this criterion may not be entirely valid as many different types of stars can provide a local environment hospitable to life. For example, in the , most stars are smaller and dimmer than the Sun. One such star, TRAPPIST-1, is located 12 (39 light years) away and is roughly 10 times smaller and 2,000 times dimmer than the Sun, yet it harbors at least six Earth-like planets in its habitable zone. While these conditions may seem unfavorable to known life, TRAPPIST-1 is expected to continue burning for 12 trillion years (compared to the Suns remaining 5 billion year lifetime) which is time enough for life to arise by . For comparison, life evolved on Earth in a mere one billion years.


Surface water and hydrological cycle
The concept of the habitable zone (or Liquid Water Zone) defining a region where water can exist on the surface, is based on the properties of both the Earth and Sun. Under this model, Earth orbits roughly at the centre of this zone or in the "Goldilocks" position. Earth is the only planet currently confirmed to possess large bodies of surface water. Venus is on the hot side of the zone while Mars is on the cold side. Neither are known to have persistent surface water, though evidence exists that Mars did have in its ancient past,Cabrol, N. and E. Grin (eds.). 2010. Lakes on Mars. Elsevier. NY and it is speculated that the same was the case for Venus. Thus extrasolar planets (or moons) in the Goldilocks position with substantial atmospheres may possess oceans and water clouds like those on Earth. In addition to surface water, a true Earth analog would require a mix of oceans or lakes and areas not covered by water, or land.

Some argue that a true Earth analog must not only have a similar position of its planetary system but also orbit a solar analog and have a near circular orbit such that it remains continuously habitable like Earth.


Extrasolar Earth analog
The mediocrity principle suggests that there is a chance that serendipitous events may have allowed an Earth-like planet to form elsewhere that would allow the emergence of complex, multi-cellular life. In contrast, the Rare Earth hypothesis asserts that if the strictest criteria are applied, such a planet, if it exists, may be so far away that humans may never locate it.

Because the proved to be devoid of an Earth analog, the search has widened to extrasolar planets. Astrobiologists assert that Earth analogs would most likely be found in a stellar , in which liquid water could exist, providing the conditions for supporting life. Some astrobiologists, such as Dirk Schulze-Makuch, estimated that a sufficiently massive natural satellite may form a similar to Earth.


History

Estimated frequency
The frequency of Earth-like planets in both the Milky Way and the larger universe is still unknown. It ranges from the extreme Rare Earth hypothesis estimates – one (i. e., Earth) – to innumerable.

Several current scientific studies, including the Kepler mission, are aimed at refining estimates using real data from transiting planets. A 2008 study by astronomer Michael Meyer from the University of Arizona of near recently formed Sun-like stars suggests that between 20% and 60% of solar analogs have evidence for the formation of rocky planets, not unlike the processes that led to those of Earth. Meyer's team found discs of cosmic dust around stars and sees this as a byproduct of the formation of rocky planets.

In 2009, of the Carnegie Institution for Science speculated that there could be 100 billion terrestrial planets just in the galaxy.

In 2011 NASA's Jet Propulsion Laboratory (JPL), based on observations from the Kepler Mission suggested that between 1.4% and 2.7% of all Sun-like are expected to have Earth-size planets within the of their stars. This means there could be as many as two billion Earth-sized planets in the Milky Way alone, and assuming that all galaxies have number of such planets similar to the Milky Way, in the 50 billion galaxies in the observable universe, there may be as many as a hundred Earth-like planets. This would correspond to around 20 earth analogs per square centimeter of the Earth.

In 2013, a Harvard–Smithsonian Center for Astrophysics using statistical analysis of additional Kepler data suggested that there are at least 17 billion Earth-sized planets in the Milky Way. 17 Billion Earth-Size Alien Planets Inhabit Milky Way SPACE.com 07 January 2013 This, however, says nothing of their position in relation to the habitable zone.

A 2019 study determined that Earth-size planets may circle 1 in 6 Sun-like stars.


Terraforming
Terraforming (literally, "Earth-shaping") of a , moon, or other body is the process of deliberately modifying its atmosphere, , surface or to be similar to those of to make it habitable to humans.

Due to proximity and similarity in size, Mars, and to a lesser extent Venus,

(1999). 9781585420360, Penguin. .
(1995). 9781560916093, SAE International, Warrendale, PA.
have been cited as the most likely candidates for terraforming.


See also
  • Planetary habitability
  • Habitability of natural satellites
  • Superhabitable planet

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