Planetary chauvinism

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The Earth seen from Apollo 17. The Earth seen from Apollo 17.jpg
The Earth seen from Apollo 17.
An example of an O'Neill cylinder, as envisioned by NASA Ames. Spacecolony3edit.jpeg
An example of an O'Neill cylinder, as envisioned by NASA Ames.

Planetary chauvinism is the belief that human society will always be planet-based (even if extended beyond Earth), and overlooks or ignores the potential benefits of space-based living. [1] The idea can be extended to alien society in general, that is, we should expect alien society to be planet based. [2] The coining of the term is often credited to Isaac Asimov, but in an interview with Bill Boggs, Asimov mentions that he heard it from Carl Sagan. [3] The counter-argument is that all the benefits of a planet can be achieved in space, usually by an O'Neill cylinder-type structure. [4]

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An even narrower version of planetary chauvinism is G-star chauvinism. This is the assumption that intelligent life will always evolve in star systems similar to our own, that is, in stars of spectral class G. [5] Carl Sagan criticised this belief on the grounds that intelligent life has a greater chance of evolving on the most long lived stars. That suggests that class-M and class-K stars are more likely candidates, not only because of their lifetime, but also because they are far more numerous than class-G stars. [2]

There are several hypotheses of the possibility of life originating in the universe in places other than planets. [6] [7] [8]

Surface chauvinism

Thomas Gold, who advocated for the possibility of life in deep biospheres below the surfaces of celestial bodies, [9] has criticized science which only focuses on the surface and not below in its search of life as surface chauvinism. [9]

Similarly, the focus on surface-bound and territorial space advocacy, particularly for space colonization, has been termed surfacism, neglecting interest for atmospheres and potential atmospheric human habitation, such ascolonization above the surface of Venus. [10] [11]

See also

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Astrobiology is a scientific field within the life and environmental sciences that studies the origins, early evolution, distribution, and future of life in the universe by investigating its deterministic conditions and contingent events. As a discipline, astrobiology is founded on the premise that life may exist beyond Earth.

<span class="mw-page-title-main">Carl Sagan</span> American astrophysicist, cosmologist and author (1934–1996)

Carl Edward Sagan was an American astronomer, planetary scientist and science communicator. His best known scientific contribution is his research on the possibility of extraterrestrial life, including experimental demonstration of the production of amino acids from basic chemicals by exposure to light. He assembled the first physical messages sent into space, the Pioneer plaque and the Voyager Golden Record, which were universal messages that could potentially be understood by any extraterrestrial intelligence that might find them. He argued in favor of the hypothesis, which has since been accepted, that the high surface temperatures of Venus are the result of the greenhouse effect.

<span class="mw-page-title-main">Hypothetical types of biochemistry</span> Possible alternative biochemicals used by life forms

Hypothetical types of biochemistry are forms of biochemistry agreed to be scientifically viable but not proven to exist at this time. The kinds of living organisms currently known on Earth all use carbon compounds for basic structural and metabolic functions, water as a solvent, and DNA or RNA to define and control their form. If life exists on other planets or moons it may be chemically similar, though it is also possible that there are organisms with quite different chemistries – for instance, involving other classes of carbon compounds, compounds of another element, or another solvent in place of water.

<span class="mw-page-title-main">Drake equation</span> Estimate of extraterrestrial civilizations

The Drake equation is a probabilistic argument used to estimate the number of active, communicative extraterrestrial civilizations in the Milky Way Galaxy.

Extraterrestrial life, or alien life, is life which does not originate from Earth. No extraterrestrial life has yet been conclusively detected. Such life might range from simple forms such as prokaryotes to intelligent beings, possibly bringing forth civilizations that might be far more advanced than humans. The Drake equation speculates about the existence of sapient life elsewhere in the universe. The science of extraterrestrial life is known as astrobiology.

<span class="mw-page-title-main">Fermi paradox</span> Discrepancy between lack of evidence of advanced alien life and apparently high likelihood it exists

The Fermi paradox is the discrepancy between the lack of conclusive evidence of advanced extraterrestrial life and the apparently high likelihood of its existence. As a 2015 article put it, "If life is so easy, someone from somewhere must have come calling by now."

<span class="mw-page-title-main">Space colonization</span> Concept of permanent human habitation outside of Earth

Space colonization is the process of establishing human settlements beyond Earth for prestige, commercial and strategic benefits. This is in contrast to space exploration for scientific benefits. Colonialism can involve exploitation of both resources and people by a distant entity.

<span class="mw-page-title-main">Terraforming</span> Hypothetical planetary engineering process

Terraforming or terraformation ("Earth-shaping") is the hypothetical process of deliberately modifying the atmosphere, temperature, surface topography or ecology of a planet, moon, or other body to be similar to the environment of Earth to make it habitable for humans to live on.

<span class="mw-page-title-main">Space and survival</span> Idea that spacefaring is necessary for long-term human surrvival

Space and survival is the idea that the long-term survival of the human species and technological civilization requires the building of a spacefaring civilization that utilizes the resources of outer space, and that not doing this might lead to human extinction. A related observation is that the window of opportunity for doing this may be limited due to the decreasing amount of surplus resources that will be available over time as a result of an ever-growing population.

<span class="mw-page-title-main">Habitable zone</span> Orbits where planets may have liquid surface water

In astronomy and astrobiology, the habitable zone (HZ), or more precisely the circumstellar habitable zone (CHZ), is the range of orbits around a star within which a planetary surface can support liquid water given sufficient atmospheric pressure. The bounds of the HZ are based on Earth's position in the Solar System and the amount of radiant energy it receives from the Sun. Due to the importance of liquid water to Earth's biosphere, the nature of the HZ and the objects within it may be instrumental in determining the scope and distribution of planets capable of supporting Earth-like extraterrestrial life and intelligence.

<span class="mw-page-title-main">Communication with extraterrestrial intelligence</span> Branch of SETI

The communication with extraterrestrial intelligence (CETI) is a branch of the search for extraterrestrial intelligence (SETI) that focuses on composing and deciphering interstellar messages that theoretically could be understood by another technological civilization. The best-known CETI experiment of its kind was the 1974 Arecibo message composed by Frank Drake.

<span class="mw-page-title-main">Carbon chauvinism</span> Scientific theory assuming that all form of life must be carbon-based

Carbon chauvinism is a neologism meant to disparage the assumption that the chemical processes of hypothetical extraterrestrial life must be constructed primarily from carbon because as far as is known, carbon's chemical and thermodynamic properties render it far superior to all other elements at forming molecules used in living organisms.

<span class="mw-page-title-main">Venus in fiction</span> Depictions of the planet

The planet Venus has been used as a setting in fiction since before the 19th century. Its opaque cloud cover gave science fiction writers free rein to speculate on conditions at its surface—a "cosmic Rorschach test", in the words of science fiction author Stephen L. Gillett. The planet was often depicted as warmer than Earth but still habitable by humans. Depictions of Venus as a lush, verdant paradise, an oceanic planet, or fetid swampland, often inhabited by dinosaur-like beasts or other monsters, became common in early pulp science fiction, particularly between the 1930s and 1950s. Some other stories portrayed it as a desert, or invented more exotic settings. The absence of a common vision resulted in Venus not developing a coherent fictional mythology, in contrast to the image of Mars in fiction.

<i>Farewell, Fantastic Venus</i>

Farewell, Fantastic Venus is a 1968 American science fiction anthology edited by Brian Aldiss and Harry Harrison. An abridged version was published in the same year under the title All About Venus. It was first published as a direct response to the information returned from the first space probes sent to Venus, especially the first atmospheric probe to return data, Venera 4. The first data was not returned from the surface until Venera 7 successfully landed in 1970.

<span class="mw-page-title-main">Saturn in fiction</span> Depictions of the planet

Saturn has made appearances in fiction since the 1752 novel Micromégas by Voltaire. In the earliest depictions, it was portrayed as having a solid surface rather than its actual gaseous composition. In many of these works, the planet is inhabited by aliens that are usually portrayed as being more advanced than humans. In modern science fiction, the Saturnian atmosphere sometimes hosts floating settlements. The planet is occasionally visited by humans and its rings are sometimes mined for resources.

<span class="mw-page-title-main">Terraforming of Venus</span> Engineering the global environment of Venus to make it suitable for humans

The terraforming of Venus or the terraformation of Venus is the hypothetical process of engineering the global environment of the planet Venus in order to make it suitable for human habitation. Adjustments to the existing environment of Venus to support human life would require at least three major changes to the planet's atmosphere:

  1. Reducing Venus's surface temperature of 737 K
  2. Eliminating most of the planet's dense 9.2 MPa (91 atm) carbon dioxide and sulfur dioxide atmosphere via removal or conversion to some other form
  3. The addition of breathable oxygen to the atmosphere.
<span class="mw-page-title-main">David Grinspoon</span> American astrobiologist

David H. Grinspoon is an American astrobiologist. He is the Senior Scientist for Astrobiology Strategy at NASA and was the former inaugural Baruch S. Blumberg NASA/Library of Congress Chair in Astrobiology for 2012–2013.

<span class="mw-page-title-main">Earth analog</span> Planet with environment similar to Earths

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.

Directed panspermia is a type of panspermia that implies the deliberate transport of microorganisms into space to be used as introduced species on other astronomical objects.

<span class="mw-page-title-main">Outline of extraterrestrial life</span> Overview of and topical guide to extraterrestrial life

The following outline is provided as an overview of and topical guide to extraterrestrial life:

References

  1. Paterson, E. T. "Towards the orthomolecular environment." Jo Orthomol Psych 10 (1981): 269-283.
  2. 1 2 Carl Sagan, Carl Sagan's Cosmic Connection: An Extraterrestrial Perspective, p. 48, Cambridge University Press, 2000 ISBN   0521783038.
  3. Bill Boggs. "Asimov Interview with Bill Boggs (35 minutes in)". YouTube . Archived from the original on 2021-12-15. Retrieved July 2, 2014.
  4. Mike Combs. "Somewhere Else Entirely" . Retrieved June 3, 2016.
  5. Joseph A. Angelo, Encyclopedia of Space and Astronomy, p. 235, Infobase Publishing, 2014 ISBN   1438110189.
  6. Luis A. Anchordoqui and Eugene M. Chudnovsky Can Self-Replicating Species Flourish in the Interior of a Star?, Letters in High Energy Physics, issue 166, 2020, doi : 10.31526/LHEP.2020.166
    • From the abstract: "We argue that an advanced form of life based upon short-lived species can exist inside main-sequence stars like our Sun."
  7. Browne, Malcolm W. (1988-02-02). "A Theory Sees Life, Of Sorts, On Pulsars". The New York Times. ISSN   0362-4331 . Retrieved 2023-03-31.
  8. Clifford A. Pickover, The Stars of Heaven, Chapter 8: "Stellar Graveyards, Nucleosynthesis, and Why We Exist"
  9. 1 2 Gold, Thomas (1999). The Deep Hot Biosphere. New York, NY: Springer New York. doi:10.1007/978-1-4612-1400-7. ISBN   978-0-387-95253-6.
  10. Tickle, Glen (2015-03-05). "A Look Into Whether Humans Should Try to Colonize Venus Instead of Mars". Laughing Squid. Retrieved 2021-09-01.
  11. David Warmflash (14 March 2017). "Colonization of the Venusian Clouds: Is 'Surfacism' Clouding Our Judgement?". Vision Learning. Retrieved 20 September 2019.