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For the idea of a planet orbiting the sun directly opposite Earth, see Counter-Earth.
Evolutionary paths of Earth and Venus. Venus has been the prime example for a planet resembling Earth and how such a planet can differ.

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

The possibility is of particular interest to astrobiologists and astronomers 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 science, philosophy, science fiction and popular culture. 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 terraforming.

Before the scientific search for and study of extrasolar planets, 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 Universe, 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 Solar System, 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 planets orbiting in the habitable zones of Sun-like stars and red dwarf stars within the Milky Way Galaxy.[1][2] The nearest such planet could be expected to be within 12 light-years of the Earth, statistically.[1][2] In September 2020, astronomers identified 24 superhabitable planets (planets better than Earth) contenders, from among more than 4000 confirmed exoplanets, based on astrophysical parameters, as well as the natural history of known life forms on the Earth.[3]

On 11 January 2023, NASA scientists reported the detection of LHS 475 b, an Earth-like exoplanet — and the first exoplanet discovered by the James Webb Space Telescope.[4]

Artist's representation of a hypothetical habitable exoplanet with three natural satellites
Artist's representation of a hypothetical habitable exoplanet with three natural satellites

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

History

[edit]
Percival Lowell depicted Mars as a dry but Earth-like planet and habitable for an extraterrestrial civilisation.
Sand dunes in the Namib Desert on Earth (top), compared with dunes in Belet on Titan

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 Martian civilization that had built great Martian canals. These theories were advanced by Giovanni Schiaparelli, Percival Lowell and others. As such Mars in fiction portrayed the red planet as similar to Earth's deserts. Images and data from the Mariner (1965) and Viking space probes (1975–1980), however, revealed the planet as a barren cratered world.[5][6][7][8][9][10] 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.[11] 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, Venus 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.[12] Venus in fiction was often portrayed as having similarities to Earth and many speculated about Venusian 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 462 °C (864 °F)[13] under an acidic atmosphere with a surface pressure of 9.2 MPa (1,330 psi).[13]

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.[14][15] Further observations, including weather phenomena, have aided the understanding of geological processes that may operate on Earth-like planets.[16]

The Kepler space telescope began observing the transits of potential terrestrial planets in the habitable zone from 2011.[17][18] 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.[19] 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.[20][21]

On 11 January 2023, NASA scientists reported the detection of LHS 475 b, an Earth-like exoplanet - and the first exoplanet discovered by the James Webb Space Telescope.[4]

Attributes and criteria

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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. Solar analog), orbital distance and stability, axial tilt and rotation, similar geography, oceans, air and weather conditions, strong magnetosphere and even the presence of Earth-like complex life. If there is complex life, there could be some forests covering much of the land. If there is intelligent life, some parts of land could be covered in cities. 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 biosignature from the emergence of photosynthetic life. The formation, presence, influence on these characteristics of the Moon (such as tidal forces) 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 Vincent Ialenti's work on the epistemology of analogical reasoning has shown,[22] 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.[23]

Size

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Size comparisons: Kepler-20e[24] and Kepler-20f[25] with Venus and Earth

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.[26]

The list includes planets within the range of 0.8–1.9 Earth masses, below which are generally classed as sub-Earth and above classed as super-Earth. 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:

Name Earth masses (ME) Earth radii (R🜨) Note
Kepler-69c 0.98 1.7 Originally thought to be in the circumstellar habitable zone (CHZ), now thought to be too hot.
Kepler-9d >1.5[27] 1.64 Extremely hot.
CoRoT-7b <9 1.58
Kepler-20f < 14.3[25] 1.03[25] Slightly larger and likely more massive, far too hot to be Earth-like.
Tau Ceti b 2 Extremely hot. Not known to transit.
Kepler-186f 1.1[28] Orbits in the habitable zone.
Earth 1 1 Orbits in habitable zone.
Venus 0.815 0.949 Much hotter.
Kepler-20e < 3.08[24] 0.87[24] Too hot to be Earth-like.
Proxima Centauri b >1.27 >1.1 Closest exoplanet to Earth.

This comparison indicates that size alone is a poor measure, particularly in terms of habitability. Temperature must also be considered as Venus and the planets of Alpha Centauri B (discovered in 2012), Kepler-20 (discovered in 2011[29][30]), COROT-7 (discovered in 2009) and the three planets of Kepler-42 (all discovered in 2011) are very hot, and Mars, 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

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Surfaces like this of Saturn's moon Titan (taken by Huygens probe) bear superficial similarities to the floodplains of Earth.

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 sedimentary rocks) 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 life forms.

Temperature

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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.[citation needed] 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 comparisons Venus Earth Kepler-22b Mars
Global equilibrium temperature 307 K
34 °C
93 °F		 255 K
−18 °C
−0.4 °F		 262 K
−11 °C
22.2 °F		 206 K
−67 °C
−88.6 °F
+ Greenhouse gas effect 737 K
464 °C
867 °F		 288 K
15 °C
59 °F		 295 K
22 °C
71.6 °F		 210 K
−63 °C
−81 °F
Tidally locked[31] Almost No Unknown No
Global Bond albedo 0.9 0.29 0.25
Refs.[32][33][34]

Solar analog

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Main article: Solar analog

Another criterion of an ideal life-harboring earth analog is that it should orbit a solar analog; 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 Milky Way, most stars are smaller and dimmer than the Sun. One such star, TRAPPIST-1, is located 12 parsecs (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 abiogenesis.[35] For comparison, life evolved on Earth in a mere one billion years.[citation needed]

Surface water and hydrological cycle

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Water covers 70% of Earth's surface and is required by all known life.
Kepler-22b, located in the habitable zone of a Sun-like star, may be the best exoplanetary candidate for extraterrestrial surface water discovered to date, but is significantly larger than Earth and its actual composition is unknown.
Main article: Habitable zone

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,[36][37][38] and it is speculated that the same was the case for Venus.[12] 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.[citation needed]

Extrasolar Earth analog

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See also: List of potentially habitable exoplanets

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 Solar System 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 habitable zone, 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 habitable moon similar to Earth.

History

[edit]

Estimated frequency

[edit]
Artist's concept of Earth-like planets[39]

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 cosmic dust 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.[40] Meyer's team found discs of cosmic dust around stars and sees this as a byproduct of the formation of rocky planets.

In 2009, Alan Boss of the Carnegie Institution for Science speculated that there could be 100 billion terrestrial planets just in the Milky Way galaxy.[41]

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 stars are expected to have Earth-size planets within the habitable zones of their stars. This means there could be as many as two billion Earth-sized planets in the Milky Way galaxy 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 quintillion Earth-like planets.[42] This would correspond to around 20 earth analogs per square centimeter of the Earth.[43]

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.[44] 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.[45]

Terraforming

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Main article: Terraforming
Artist's conception of a terraformed Venus, a potential Earth analog

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

Due to proximity and similarity in size, Mars,[46][47][48] and to a lesser extent Venus,[49][50][51][52][53] have been cited as the most likely candidates for terraforming.

See also

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References

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  1. ^ a b Overbye, Dennis (4 November 2013). "Far-Off Planets Like the Earth Dot the Galaxy". The New York Times. Retrieved 5 November 2013.
  2. ^ a b Petigura, Erik A.; Howard, Andrew W.; Marcy, Geoffrey W. (1 November 2013). "Prevalence of Earth-size planets orbiting Sun-like stars". Proceedings of the National Academy of Sciences. 110 (48): 19273–19278. arXiv:1311.6806. Bibcode:2013PNAS..11019273P. doi:10.1073/pnas.1319909110. PMC 3845182. PMID 24191033.
  3. ^ Schulze-Makuch, Dirk; Heller, Rene; Guinan, Edward (18 September 2020). "In Search for a Planet Better than Earth: Top Contenders for a Superhabitable World". Astrobiology. 20 (12): 1394–1404. Bibcode:2020AsBio..20.1394S. doi:10.1089/ast.2019.2161. PMC 7757576. PMID 32955925.
  4. ^ a b Chow, Denise (11 January 2023). "James Webb Telescope finds its first exoplanet - The planet is almost the same size as Earth, according to a research team led by astronomers at the Johns Hopkins University Applied Physics Laboratory". NBC News. Retrieved 12 January 2023.
  5. ^ O'Gallagher, J.J.; Simpson, J.A. (10 September 1965). "Search for Trapped Electrons and a Magnetic Moment at Mars by Mariner IV". Science. New Series. 149 (3689): 1233–1239. Bibcode:1965Sci...149.1233O. doi:10.1126/science.149.3689.1233. PMID 17747452. S2CID 21249845.
  6. ^ Smith, Edward J.; Davis Jr., Leverett; Coleman Jr., Paul J.; Jones, Douglas E. (10 September 1965). "Magnetic Field Measurements Near Mars". Science. New Series. 149 (3689): 1241–1242. Bibcode:1965Sci...149.1241S. doi:10.1126/science.149.3689.1241. PMID 17747454. S2CID 43466009.
  7. ^ Leighton, Robert B.; Murray, Bruce C.; Sharp, Robert P.; Allen, J. Denton; Sloan, Richard K. (6 August 1965). "Mariner IV Photography of Mars: Initial Results". Science. New Series. 149 (3684): 627–630. Bibcode:1965Sci...149..627L. doi:10.1126/science.149.3684.627. PMID 17747569. S2CID 43407530.
  8. ^ Kliore, Arvydas; Cain, Dan L.; Levy, Gerald S.; Eshleman, Von R.; Fjeldbo, Gunnar; Drake, Frank D. (10 September 1965). "Occultation Experiment: Results of the First Direct Measurement of Mars's Atmosphere and Ionosphere". Science. New Series. 149 (3689): 1243–1248. Bibcode:1965Sci...149.1243K. doi:10.1126/science.149.3689.1243. PMID 17747455. S2CID 34369864.
  9. ^ Salisbury, Frank B. (6 April 1962). "Martian Biology". Science. New Series. 136 (3510): 17–26. Bibcode:1962Sci...136...17S. doi:10.1126/science.136.3510.17. PMID 17779780. S2CID 39512870.
  10. ^ Kilston, Steven D.; Drummond, Robert R.; Sagan, Carl (1966). "A Search for Life on Earth at Kilometer Resolution". Icarus. 5 (1–6): 79–98. Bibcode:1966Icar....5...79K. doi:10.1016/0019-1035(66)90010-8.
  11. ^ NASA – Mars Ocean Hypothesis Archived 2012-02-20 at the Wayback Machine
  12. ^ a b Hashimoto, G. L.; Roos-Serote, M.; Sugita, S.; Gilmore, M. S.; Kamp, L. W.; Carlson, R. W.; Baines, K. H. (2008). "Felsic highland crust on Venus suggested by Galileo Near-Infrared Mapping Spectrometer data". Journal of Geophysical Research: Planets. 113 (E9): E00B24. Bibcode:2008JGRE..113.0B24H. doi:10.1029/2008JE003134.
  13. ^ a b "Venus Fact Sheet". Archived from the original on 8 March 2016. Retrieved 10 March 2016.
  14. ^ "Cassini Reveals Titan's Xanadu Region To Be An Earth-Like Land". Science Daily. 23 July 2006. Retrieved 27 August 2007.
  15. ^ "Seeing, touching and smelling the extraordinarily Earth-like world of Titan". ESA News, European Space Agency. 21 January 2005. Retrieved 28 March 2005.
  16. ^ "Cassini-Huygens: News". Saturn.jpl.nasa.gov. Archived from the original on 8 May 2008. Retrieved 20 August 2011.
  17. ^ "NASA's Kepler Confirms Its First Planet in Habitable Zone of Sun-like Star". NASA Press Release. 5 December 2011. Archived from the original on 16 May 2017. Retrieved 6 December 2011.
  18. ^ Howell, Elizabeth (15 November 2017). "Kepler-22b: Facts About Exoplanet in Habitable Zone". Space.com. Archived from the original on 22 August 2019. Retrieved 10 February 2019.
  19. ^ Petigura, E. A.; Howard, A. W.; Marcy, G. W. (2013). "Prevalence of Earth-size planets orbiting Sun-like stars". Proceedings of the National Academy of Sciences. 110 (48): 19273–19278. arXiv:1311.6806. Bibcode:2013PNAS..11019273P. doi:10.1073/pnas.1319909110. ISSN 0027-8424. PMC 3845182. PMID 24191033.
  20. ^ Jenkins, Jon M.; Twicken, Joseph D.; Batalha, Natalie M.; et al. (23 July 2015). "Discovery and Validation of Kepler-452b: A 1.6 R⨁ Super Earth Exoplanet in the Habitable Zone of a G2 Star". The Astronomical Journal. 150 (2): 56. arXiv:1507.06723. Bibcode:2015AJ....150...56J. doi:10.1088/0004-6256/150/2/56. ISSN 1538-3881. S2CID 26447864.
  21. ^ "NASA telescope discovers Earth-like planet in star's 'habitable zone". BNO News. 23 July 2015. Archived from the original on 4 March 2016. Retrieved 23 July 2015.
  22. ^ "Deep Time Reckoning". MIT Press. Retrieved 14 January 2023.
  23. ^ Maughan, Philip (12 January 2023). "Searching Earth For Alien Worlds". {{cite journal}}: Cite journal requires |journal= (help)
  24. ^ a b c NASA Staff (20 December 2011). "Kepler: A Search For Habitable Planets – Kepler-20e". NASA. Archived from the original on 10 March 2012. Retrieved 23 December 2011.
  25. ^ a b c NASA Staff (20 December 2011). "Kepler: A Search For Habitable Planets – Kepler-20f". NASA. Archived from the original on 10 March 2012. Retrieved 23 December 2011.
  26. ^ Erkaev, N.V.; Lammer, H.; Elkins-Tanton, L.T.; Stökl, A.; Odert, P.; Marcq, E.; Dorfi, E.A.; Kislyakova, K.G.; Kulikov, Yu.N.; Leitzinger, M.; Güdel, M. (2014). "Escape of the martian protoatmosphere and initial water inventory". Planetary and Space Science. 98: 106–119. arXiv:1308.0190. Bibcode:2014P&SS...98..106E. doi:10.1016/j.pss.2013.09.008. ISSN 0032-0633. PMC 4375622. PMID 25843981.
  27. ^ Torres, Guillermo; Fressin, François (2011). "Modeling Kepler transit light curves as false positives: Rejection of blend scenarios for Kepler-9, and validation of Kepler-9d, a super-Earth-size planet in a multiple system". Astrophysical Journal. 727 (24): 24. arXiv:1008.4393. Bibcode:2011ApJ...727...24T. doi:10.1088/0004-637X/727/1/24. S2CID 6358297.
  28. ^ Johnson, Michele; Harrington, J.D. (17 April 2014). "NASA's Kepler Discovers First Earth-Size Planet In The 'Habitable Zone' of Another Star". NASA. Retrieved 17 April 2014.
  29. ^ Johnson, Michele (20 December 2011). "NASA Discovers First Earth-size Planets Beyond Our Solar System". NASA. Archived from the original on 4 May 2019. Retrieved 20 December 2011.
  30. ^ Hand, Eric (20 December 2011). "Kepler discovers first Earth-sized exoplanets". Nature. doi:10.1038/nature.2011.9688. S2CID 122575277.
  31. ^ To stellar primary
  32. ^ "NASA, Mars: Facts & Figures". Archived from the original on 23 January 2004. Retrieved 28 January 2010.
  33. ^ Mallama, A.; Wang, D.; Howard, R.A. (2006). "Venus phase function and forward scattering from H2SO4". Icarus. 182 (1): 10–22. Bibcode:2006Icar..182...10M. doi:10.1016/j.icarus.2005.12.014.
  34. ^ Mallama, A. (2007). "The magnitude and albedo of Mars". Icarus. 192 (2): 404–416. Bibcode:2007Icar..192..404M. doi:10.1016/j.icarus.2007.07.011.
  35. ^ Snellen, Ignas A. G. (February 2017). "Earth's seven sisters". Nature. 542 (7642): 421–422. doi:10.1038/542421a. hdl:1887/75076. PMID 28230129.
  36. ^ Cabrol, N. and E. Grin (eds.). 2010. Lakes on Mars. Elsevier. NY
  37. ^ Clifford, S. M.; Parker, T. J. (2001). "The Evolution of the Martian Hydrosphere: Implications for the Fate of a Primordial Ocean and the Current State of the Northern Plains". Icarus. 154 (1): 40–79. Bibcode:2001Icar..154...40C. doi:10.1006/icar.2001.6671.
  38. ^ Villanueva, G.; Mumma, M.; Novak, R.; Käufl, H.; Hartogh, P.; Encrenaz, T.; Tokunaga, A.; Khayat, A.; Smith, M. (2015). "Strong water isotopic anomalies in the martian atmosphere: Probing current and ancient reservoirs". Science. 348 (6231): 218–221. Bibcode:2015Sci...348..218V. doi:10.1126/science.aaa3630. PMID 25745065. S2CID 206633960.
  39. ^ "Artist's Concept of Earth-Like Planets in the Future Universe". ESA/Hubble. Retrieved 22 October 2015.
  40. ^ Briggs, Helen (17 February 2008). "Planet-hunters set for big bounty". BBC News.
  41. ^ Pawlowski, A. (25 February 2009). "Galaxy may be full of 'Earths,' alien life". CNN.
  42. ^ Choi, Charles Q. (21 March 2011). "New Estimate for Alien Earths: 2 Billion in Our Galaxy Alone". Space.com. Retrieved 24 April 2011.
  43. ^ "Wolfram|Alpha: Making the world's knowledge computable". www.wolframalpha.com. Retrieved 19 March 2018.
  44. ^ 17 Billion Earth-Size Alien Planets Inhabit Milky Way Archived October 6, 2014, at the Wayback Machine SPACE.com 07 January 2013
  45. ^ Hsu, Danley C.; Ford, Eric B.; Ragozzine, Darin; Ashby, Keir (14 August 2019). "Occurrence Rates of Planets Orbiting FGK Stars: Combining Kepler DR25, Gaia DR2, and Bayesian Inference". The Astronomical Journal. 158 (3): 109. arXiv:1902.01417. Bibcode:2019AJ....158..109H. doi:10.3847/1538-3881/ab31ab. ISSN 1538-3881. S2CID 119466482.
  46. ^ Robert M. Zubrin (Pioneer Astronautics), Christopher P. McKay. NASA Ames Research Center (c. 1993). "Technological Requirements for Terraforming Mars".
  47. ^ Mat Conway (27 February 2007). "Now We're There: Terraforming Mars". Aboutmyplanet.com. Archived from the original on 23 July 2011. Retrieved 20 August 2011.
  48. ^ Peter Ahrens. "The Terraformation of Worlds" (PDF). Nexial Quest. Archived from the original (PDF) on 9 June 2019. Retrieved 18 October 2007.
  49. ^ Sagan, Carl (1961). "The Planet Venus". Science. 133 (3456): 849–58. Bibcode:1961Sci...133..849S. doi:10.1126/science.133.3456.849. PMID 17789744.
  50. ^ Zubrin, Robert (1999). Entering Space: Creating a Spacefaring Civilization. Penguin. ISBN 9781585420360.
  51. ^ Fogg, Martyn J. (1995). Terraforming: Engineering Planetary Environments. SAE International, Warrendale, PA. ISBN 1-56091-609-5.
  52. ^ Birch, Paul (1991). "Terraforming Venus Quickly" (PDF). Journal of the British Interplanetary Society. 44: 157. Bibcode:1991JBIS...44..157B.
  53. ^ Landis, Geoffrey A. (2–6 February 2003). "Colonization of Venus". Conference on Human Space Exploration, Space Technology & Applications International Forum, Albuquerque NM.
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