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Monday, March 23, 2026

Biology of romantic love

From Wikipedia, the free encyclopedia

The biology of romantic love has been explored by such biological sciences as evolutionary psychology, evolutionary biology, anthropology and neuroscienceNeurochemicals and hormones such as dopamine and oxytocin are studied along with a variety of interrelated brain systems (including the mesocorticolimbic pathway) which produce the psychological experience and behaviors of romantic love.

The study of romantic love is still in its infancy. As of 2021, there were a total of 42 biological studies on romantic love.

Definition of romantic love

The meaning of the term "romantic love" has changed considerably throughout history, making it difficult to simply define. Initially it was coined to refer to certain attitudes and behaviors described in a body of literature now referred to as courtly love. However, academic psychology and especially biology also consider romantic love in a different sense, which refers to a brain system (or systems) related to pair bonding or mating with associated psychological properties.

Bode and Kushnick undertook a comprehensive review of romantic love from a biological perspective in 2021. They considered the psychology of romantic love, its mechanisms, development across the lifespan, functions, and evolutionary history. Based on the content of that review, they proposed a biological definition of romantic love:

Romantic love is a motivational state typically associated with a desire for long-term mating with a particular individual. It occurs across the lifespan and is associated with distinctive cognitive, emotional, behavioral, social, genetic, neural, and endocrine activity in both sexes. Throughout much of the life course, it serves mate choice, courtship, sex, and pair-bonding functions. It is a suite of adaptations and by-products that arose sometime during the recent evolutionary history of humans.

Romantic love in this sense is also not necessarily "dyadic", "social" or "interpersonal", despite being related to pair bonding. Romantic love can be experienced outside the context of a relationship, for example in the case of unrequited love where the feelings are not reciprocated. A person can develop romantic love feelings before any relationship has occurred, for only a potential partner. The potential partner can even be somebody they do not know well or are not acquainted with at all, as in cases of love at first sight and parasocial attachments.

The early stage of romantic love (which has obsessive and addictive features) might also be referred to as being "in love", passionate love, infatuation, limerence or obsessive love. Research has never settled on a unified terminology or set of methods. Distinctions are drawn between this early stage of romantic love and the "attachment system" theorized by the attachment theorists like John Bowlby. In the past, attachment theorists have argued that attachment theory and attachment styles can replace other theories of love, but academics on love have argued this is incorrect and that romantic love and attachment are not identical concepts. The early stage of romantic love is thought to involve additional brain systems for other purposes, with distinct evolutionary histories. Romantic love is also distinct from sexual attraction, although they most often occur together.

Variation exists in the way romantic love is expressed in the population. A cross-cultural study of currently in-love people found four clusters, with varying degrees of intensity, obsessive thinking, commitment, frequency of sex and other differences. Other studies indicate romantic love can be experienced both with or without obsessional features. Typically, intense romantic love is limited to a duration of 12–18 months or as long as 3 years, depending on the estimate; however, in a rare phenomenon called "long-term intense romantic love", some people experience intense attraction inside a relationship, even for 10 years or more. This is similar to early-stage intense romantic love, but at this later stage they exhibit less of the obsessional features.

Independent emotion systems

Simplified overview of the neurochemical and hormonal basis of love.

Helen Fisher and her colleagues proposed that the brain systems involved with mammalian reproduction can be separated into at least three parts:

Neuroscientists currently believe that the basic emotions arise from distinct circuits (or systems) of neural activity; that humans share several of these primary emotion-motivation circuits with other mammals; and that these brain systems evolved to direct behavior [...]. It is hypothesized that among these primary neural systems are at least three discrete, interrelated emotion-motivation systems in the mammalian brain for mating, reproduction, and parenting: lust, attraction, and attachment [...].

  • Lust is the sex drive, or libido.
  • Attraction (or early-stage romantic love, also called passionate love or infatuation) is associated with feelings of exhilaration, obsessive (or "intrusive") thoughts and the craving for emotional union.
  • Attachment (the attachment system from attachment theory, and also called companionate love) is associated with feelings of calm, security and comfort, but separation anxiety when apart.

In Fisher's theory, the systems tend to act in unison, but may become disassociated and act independently. For example, a person in a long-term partnership may feel deep attachment for their spouse, while experiencing intense romantic love (attraction) for some other individual, while being sexually attracted (lust) to still others, all at the same time. Lisa Diamond has also used independent emotions theory to explain why people can 'fall in love' sometimes without sexual desire, as in the case of "platonic" infatuation for a friend.

Fisher associates each system with different neurotransmitters and/or hormones (lust: estrogen & androgens; attraction: dopamine, norepinephrine & serotonin; attachment: oxytocin & vasopressin), but modern research shows these associations are not as clearly defined as Fisher's theory proposes. Additionally, romantic love has been associated with endogenous opioids, cortisol and nerve growth factor, which are not included in Fisher's earlier model. With respect to the idea that the systems are independent, a more modern theory holds that the attachment system is active in early-stage romantic love, in addition to the infatuation component. Fisher's model is considered outdated, although the idea of interrelated systems is useful.

Evolution of systems

Evolutionary psychology

Romantic love might have evolved in part as a courtship display or a handicap signal, similar to a peacock's tail, but signaling commitment.

Evolutionary psychology is seen as an organizing framework which offers explanations behind psychological functions (rather than merely describing them), as well as specifying theoretical constraints, like requiring that a given trait is adaptive in the form of providing reproductive benefit to an individual. Evolutionary psychology has proposed a variety of explanations for romantic love.

  • Romantic love is a powerful commitment device. Romantic love suppresses the search for alternative mates (even irrationally so, when a more desirable one comes along), and signals this to the partner. Romantic love may also signal to alternative mates, disincentivizing them from pursuing oneself. The emergence of longer pair bonds in the evolution of humans coincided with the emergence of concealed ovulation, where it cannot (in general) be determined when a woman is ovulating, requiring partners to stay together while having sex during the entire menstrual cycle. Commitment is seen as adaptive to facilitate this, and to facilitate child care. Love feelings might be the psychological reward produced by the brain when the problem of commitment is being solved.
  • The intensity of romantic love feelings and why people become "fools for love" can be explained in terms of the handicap principle, which states that a contention arises between honest and fake signaling. When real emotions evolved, a niche would have been created for sham emotions (e.g. fake facial expressions) which are less risky to express. One explanation for why honest signals can evolve without becoming worthless (because of competing fakers) is that the honest signal can evolve if it is too expensive to fake. One example in nature is the peacock's tail, an example of conspicuous consumption, a cumbersome display which consumes nutrients. Only a healthy peacock can afford it, so in that case it may have evolved because it was a handicap, and used by females of the species as an indicator of health. Romantic love may have evolved to be as bewitching and besotting as it is, "like handcuffing oneself to railroad tracks", as a handicap meant to prove that one's commitment is truly real.
  • Romantic love may have evolved to override rationality, so that one reproduces regardless of the considerable costs of raising a child, and regardless of any rational will to be single or child-free.
  • Romantic love signals parental investmentPaternal investment in the form of pair bonds has been linked to better outcomes for children, both as infants and as they grow older. Children raised in pair bonds are more socially competitive and more likely to survive to reproductive age.
  • Being in love makes people more creative, so romantic love may have evolved as a courtship display. It has been suggested that art, music and literature serve a function like a peacock's tail, but as a display of mental prowess, designed to impress and make a potential partner swoon. Creativity is believed by some authors to be especially a part of the male courtship display.
  • Romantic love may conserve time and metabolic energy by focusing courtship efforts on a specific individual over others.
  • Successful pair bonding predicts better health and survival. Happy, well-functioning romantic relationships contribute to mental and physical health, especially when stress is encountered. The end of a pair bond (e.g. divorce) is associated with vulnerability, such as to disease, depression, substance abuse, or negative outcomes for children. Victims of a heart attack, for example, are more likely to have another when they live alone.
  • Monogamous pair bonding helps prevent sexually transmitted diseases (STDs) which compromise fertility, especially for women. Certain STDs (e.g. syphilis) increase the risk of miscarriage, and otherwise harm or can be passed to an unborn child. The strongest predictor of contracting an STD is the number of sexual partners, so limiting this is the best way to limit the risk of contracting a disease which would harm one's reproductive health.
  • Romantic love promotes exclusivity via mate guarding. Romantic jealousy is one of the most common correlates of being in love, which evolved as a protection from the threat of losing one's love to a romantic rival. Jealousy is seen as adaptive (when it motivates one to maintain their relationship) up to a point, but can also take the form of pathological jealousy where a sufferer has a delusional or paranoid belief in their partner's infidelity regardless of actual evidence.

Time of evolution

Unsolved problem in biology
When did human pair bonding evolve? Is pair bonding an antecedent to romantic love, or have there been other steps in the evolution of pair bonds in humans (e.g. a seasonal bond)?

Although the exact moment during human evolution is unknown, modern romantic love is usually believed to have evolved either during or after the time of bipedalism. The earliest hominid found with extensive evidence of bipedalism (and some evidence of pair bonding) is Ardipithecus ramidus, from about 4.4 million years ago, although it may also be the case that bipedalism is older than this. It has been proposed that monogamous pair bonding (which is rare among mammals) evolved during this time, because walking bipedally requires mothers to carry infants in their arms or on their hip, instead of on their backs. With their hands occupied, mothers would be more vulnerable, requiring additional help for food and protection from males of the species (hence, husbands or fathers). A different selection pressure which has been proposed is the evolution of infant altriciality (immaturity and helplessness) and large brain size at birth, which occurred around 2 million years ago. At this time, brain size became so large that a fully-developed infant's head could not fit through the mother's pelvic birth canal (known as the obstetricial dilemma), requiring the infant to be born early and underdeveloped in comparison to other species. This would have also placed a greater burden on mothers, and made paternal support more valuable.

Due to the general scarcity of evidence, it is still also possible that romantic love (or a precursor to it) predated bipedalism and altriciality, possibly originating in a common ancestor of humans and chimpanzees, 5-8 million years ago. While chimpanzees primarily mate opportunistically, some of their rarer reproductive strategies have features reminiscent of romantic love (involving mate guarding, and a more-than-fleeting association.) One assumption behind hypotheses based on fossil evidence is that less sexual dimorphism in body mass (i.e. similarity) is indicative of monogamy, but the comparative similarity between the sexes in human body mass occurred as recently as 500,000 years ago. This suggests that there may have been multiple steps in the evolution of human pair bonding, and romantic love may have evolved during any of these periods.

Courtship attraction

"It was evidently a case of love at first sight, for she swam about the new-comer caressingly...with overtures of affection" (Darwin, 1871, observing a Mallard).

Helen Fisher's theory is that romantic love (which she considers distinct from attachment) is a motivation system for choosing and focusing energy on a preferred mating partner. According to Fisher, this brain system evolved for mammalian mate choice, also called "courtship attraction". In this phenomenon, a preferred mating partner is chosen based on a display of physical traits (such as a peacock's tail feathers) or other behaviors. Fisher also includes the attraction to personality traits and other characteristics in her mate choice theory for humans. Courtship attraction shares similar behaviors with romantic love in humans, and both involve activation of dopaminergic reward circuits. In most species, courtship attraction is as brief as lasting only minutes, hours, days or weeks, but intense romantic love can last much longer in humans. Fisher believes that during the timeline of human evolution, mammalian courtship attraction may have become prolonged and intensified as pair bonding evolved, eventually becoming the phenomenon of romantic love today.

A critique of Fisher's theory published by Adam Bode holds that courtship attraction only encompasses love at first sight attraction or a crush, and the core components of romantic love (including the intense attraction and obsessive thoughts, in addition to attachment) evolved as a co-option of mother-infant bonding. A study on love at first sight found that even though people reporting the experience retrospectively will recall features resembling passionate love ("constant thoughts about the person and the desire to be with him or her"), people reporting love at first sight currently after just meeting the potential partner only report neutral scores (neither agreeing nor disagreeing) on a romantic love measure including a passion component. Some authors have speculated that the remembered account of falling in love at first sight (with high passion) is often actually a memory confabulation. Furthermore, the study found that the experience of love at first sight was related to the physical attractiveness of the potential partner. This led the researchers to conclude that love at first sight is actually a strong initial attraction, rather than resembling the state of being in love. Bode argues this more closely resembles the concept of courtship attraction, and can be considered a separate system from core romantic love components. Courtship attraction may be characterized by dopamine, oxytocin and opioid activity, but little is known about it because existing studies were not designed to target it.

Co-option of mother-infant bonding

Co-option is an evolutionary process whereby a given trait is repurposed to take on a new function. One example is how a number of species of fish (e.g. catfish) have co-opted their gas bladder to produce sound. Co-opted traits can be morphological, but also behavioral. Co-option has been used as an explanation of how a species can develop an evolutionary adaptation very quickly sometimes, seemingly faster than Darwinism could explain. With this process, a seemingly "new" trait can develop quickly because its structure predated the time of adaptation, only needing to be modified to function in a new way. In some cases, co-option involves one gene whose function is altered, while in other cases the co-opted gene is a duplicate and the function of the original gene is retained. The terms "co-option" and "exaptation" are closely related, but have different connotations. Exaptation refers to structural continuity when a trait takes on a new function.

Adam Bode has proposed that romantic love is "a suite of adaptations and by-products" consisting of a number of interrelated systems, several of which evolved by co-opting mother-infant bonding (attraction for bonding, obsessive thinking and attachment). The co-option theory says that the genes that regulate mother-infant bonding were recreated and took on a new function. Courtship attraction and sexual desire are "causally linked adjuncts" which were not co-opted, but were combined and modified in romantic love. The theory is based on the available human evidence, but also a literature arising from research on prairie voles that pair bonding uses the same mechanisms that mother-infant bonding uses.[

Academic literature has drawn a parallel between romantic love and the mother-infant dyad since the 1980s, with attachment theorists like Cindy Hazan and Phillip Shaver believing the two share a common biological process. In 1981, Glenn Wilson suggested a close analogy between adult lovers and the kind of infant attachment studied by John Bowlby. In 1999, James Leckman & Linda Mayes compared features of romantic love and early parental love, finding substantial similarities. Both are altered mental states featuring preoccupations, exclusivity of focus, a longing for reciprocity and idealization of the other. The trajectories of both also share similarities, with preoccupation increasing during courtship (for romantic love) and around the time of birth (for parental love), then diminishing after a relationship is established (for romantic love) or shortly after the postpartum period (for parental love). (The use of "baby talk" by romantic lovers is another "uncanny" similarity.) In 2004, Andreas Bartels and Semir Zeki were the first to compare romantic love and maternal love with fMRI. This comparison looked at areas known to contain high densities of receptors for the attachment hormones oxytocin and vasopressin. Bartels & Zeki found precise overlap in some specific areas including the striatum (putamen, globus pallidus and caudate nucleus) and some overlap in the ventral tegmental area, areas with dopamine and oxytocin receptors. Each type of love was also associated with other unique activations. Notably, maternal love involved the periaqueductal gray matter, an area associated with endogenous pain suppression during intense emotional experiences such as childbirth. Two meta-analyses of fMRI experiments have also found similarities between maternal love and romantic love. A 2022 meta-analysis by Shih et al. found that both types of love were associated with the left ventral tegmental area (more associated with the pleasurable aspect of reward, or "liking"), while in addition romantic love also involved the right ventral tegmental area (more associated with reward "wanting").

In 2003, Lisa Diamond suggested that adult pair bonding is an exaptation of the affectional bond between infants and caregivers, using this to explain phenomena such as romantic friendships and "platonic" infatuations, or i.e. "romantic" passion without sexual desire. Some instances of this are reported by Dorothy Tennov in her study of "limerence" (i.e. love madness, commonly for an unreachable person), in which a younger woman who otherwise considered herself heterosexual would have this type of reaction towards an older woman. Among other examples are schoolgirls falling "violently in love with each other, and suffering all the pangs of unrequited attachment, desperate jealousy etc." (historically called a "smash"), and Native American men who seemed to fall in love with each other and form intense, but non-sexual bonds. Helen Fisher's theory that sexual desire is a separate system from romantic love and attachment is also given as theoretical evidence. Diamond argues that romantic love without sexual desire can even happen in contradiction to one's sexual orientation: because it would not have been adaptive for a parent to only be able to bond with an opposite sex child, so the systems must have evolved independently from sexual orientation. People most often fall in love because of sexual desire, but Diamond suggests time spent together and physical touch can serve as a substitute. Diamond believes the connection between romantic love and sexual desire is "bidirectional" in that either one can cause the other to occur because of shared oxytocin pathways in the brain.

New model

Based on contentions over evolutionary theories and Fisher's outdated neurochemical model, Bode has suggested Fisher's model, while useful and the predominant one for a time, is oversimplified and proposes five systems:

  • Sexual desire is associated with a drive to initiate and be receptive to sexual activity. Testosterone, dopamine, serotonin, norepinephrine, acetylcholine, histamine and opioids have been implicated in sexual behavior.
  • Courtship attraction is for choosing and focusing energy on a preferred mating partner and promotes courtship behaviors. It can take the form of e.g. love at first sight attraction or a crush and also be intertwined with other forms of attraction, but might not precede a relationship in all cases. Courtship attraction may be associated with dopamine, oxytocin and opioids.
  • Bonding attraction is the type of attraction for pair bond formation, characterized by a strong desire for proximity, separation anxiety when apart, exclusivity of focus and heightened awareness of the loved one. Bonding attraction is associated with dopamine and oxytocin activity, especially in the ventral tegmental area. According to Bode's arguments, this is the type of romantic attraction shown in fMRI experiments of early-stage romantic love.
  • Obsessive thinking involves preoccupation or intrusive thinking about the loved one. Some authors have drawn a comparison between this feature and obsessive-compulsive disorder, suggesting they share similar neurobiology, but the evidence for that is limited and ambiguous.
  • Attachment is for pair bond maintenance, or maintaining very close personal relationships, with psychological features like a heightened sense of responsibility, longing for reciprocity and a powerful sense of empathy. Attachment is associated with oxytocin, dopamine and opioid activity, but there is also some evidence for the involvement of vasopressin.

Bode suggests that the systems of bonding attraction, obsessive thinking and attachment (the three systems which were co-opted from mother-infant bonding) together form the core of romantic love (the necessary components). However, all five systems are merged into one single phenomenon of romantic love, with a variety of different outcomes depending on the circumstances.

Mechanics

Reward, motivation and addiction

Anatomy of the basal ganglia.
Approximate location of the nucleus accumbens relative to the basal ganglia.
Key connections in the mesocorticolimbic pathway: ventral tegmental area (VTA); nucleus accumbens (NAc); prefrontal cortex (PFC); amygdala (AMY); hippocampus (HIPP).
Love acts in a manner "not unlike cocaine"; both work on the dopamine system. Cocaine seems to hijack the reward system by artificially overstimulating dopamine neurons.

The early stage of romantic love is being compared to a behavioral addiction (i.e. addiction to a non-substance) but the "substance" involved is the loved person. Addiction involves a phenomenon known as incentive salience, also called "wanting" (in quotes). This is the property by which cues in the environment stand out to a person and become attention-grabbing and attractive, like a "motivational magnet" which pulls a person towards a particular reward. Incentive salience differs from craving in that craving is a conscious experience and incentive salience may or may not be. While incentive salience can give feelings of strong urgency to cravings, it can also motivate behavior unconsciously, as in an experiment where cocaine users were unaware of their own decisions to choose a low dose of cocaine (which they believed was placebo) more often than an actual placebo. In the incentive-sensitization theory of addiction, repeated drug use renders the brain hypersensitive to drugs and drug cues, resulting in pathological levels of "wanting" to use drugs. People in love are thought to experience incentive salience in response to their beloved. Lovers share other similarities with addicts as well, like tolerance, dependence, withdrawal, relapse, craving and mood modification.

Incentive salience is mediated by dopamine projections in the mesocorticolimbic pathway of the brain, an area generally involved with reward, motivation and reinforcement learning. Dopamine signaling for incentive salience originates in the ventral tegmental area (VTA) and projects to areas such as the nucleus accumbens (NAc) in the ventral striatum. The VTA is one of two main areas of the brain with neurons which produce dopamine (the other being the substantia nigra pars compacta). Projections from the VTA innervate the NAc, where dopamine activity attaches motivational significance to stimuli associated with rewards. Brain scans of people in love using fMRI (commonly while looking at a photograph of their beloved) show activations in these areas like the VTA and NAc. Another dopamine-rich area of the reward system shown to be active in romantic love is the caudate nucleus, containing 80% of the brain's dopamine receptor sites, located in the dorsal striatum. The dorsal striatum is implicated in reinforcement learning, and the caudate nucleus has shown activity in response to a monetary reward and cocaine. This activity in reward and motivation areas suggests that early-stage intense romantic love is a motivation system or goal-oriented state (rather than a specific emotion), consistent with the description of romantic love as a desire or longing for union with another person. These activations are also consistent with the similarity between romantic love and addiction.

In addiction research, a distinction is drawn between "wanting" a reward (i.e. incentive salience, tied to mesocorticolimbic dopamine) and "liking" a reward (i.e. pleasure, tied to hedonic hotspots), aspects which are dissociable. People can be addicted to drugs and compulsively seek them out, even when taking the drug no longer results in a high or the addiction is detrimental to one's life. They can also irrationally "want" (i.e. feel compelled towards, in the sense of incentive salience) something which they do not cognitively wish for. In a similar way, people who are in love may "want" a loved person even when interactions with them are not pleasurable. For example, they may want to contact an ex-partner after a rejection, even when the experience will only be painful. It is also possible for a person to be "in love" with somebody they do not like, or who treats them poorly.

Academics have proposed a number of theories for how addictions begin and perpetuate. One prominent theory developed by Wolfram Schultz involves a dopamine signal which encodes a reward prediction error (RPE): the difference between the predicted value of a reward which would be received by performing a particular action and the actual value upon receiving it (i.e. whether the reward was better, equal to or worse than expected). In this theory, dopamine is also part of a mechanism for reinforcement learning which associates rewards with the cues which predicted them. Drugs of abuse like cocaine hijack this mechanism by artificially overstimulating dopamine neurons, mimicking an RPE signal which is much stronger than could be produced naturally. An alternative model developed by Kent Berridge and Terry Robinson states that dopamine signaling causes the motivational output (incentive salience) which is proportional to RPE, but that the dopamine signal itself may be an effect of learning rather than causing it directly. There is, however, said to be overwhelming evidence that dopamine guides learning in addition to motivation. The computation of dopamine signaling is complicated, with inputs from a variety of areas in the brain, although its output (primarily from the VTA) is a relatively homogeneous signal encoding the level of RPE. One study has investigated whether people in long-term romantic relationships experienced RPE in response to having expectations about their partners' appraisal of them validated or violated, indicating they do. This study used fMRI to find that reward areas like the VTA and striatum responded in a way consistent with other research on RPE. Most fMRI studies of romantic love have had participants look at a photograph, and the resulting reward system activity has been interpreted in terms of salience.

Research has not investigated whether romantic love shares all of the neurobiological aspects of addiction. Despite similarities, there are also differences between romantic love and addiction. One of the major differences is that the trajectories diverge, with the addictive aspects tending to disappear over time during a relationship in romantic love. By comparison, in a drug addiction, the detrimental aspects magnify over time with repeated drug use, turning into compulsions, a loss of control and a negative emotional state. It has been speculated that the difference between these could be related to oxytocin activity present in romantic love, but not in addiction. Oxytocin seems to ameliorate the effects of drug withdrawal, and it might inhibit the more long-term, excessive effects of addiction.

Academics do not universally agree on whether or not love is always an addiction or when it needs to be treated. The term "love addiction" has had an amorphous definition over the years and does not yet denote a psychiatric condition, but recently one definition has been developed that "Individuals addicted to love tend to experience negative moods and affects when away from their partners and have the strong urge and craving to see their partner as a way of coping with stressful situations." Other authors include rejected lovers as love addicts, or specify that love is an addiction when it involves abnormal processes which carry negative consequences. A broader view is that all love is addiction, or simply an appetite, similar to how humans are dependent on food. Research on behavioral addictions is more limited than research on drugs of abuse; however, there is a growing body of evidence that some people are susceptible to showing brain patterns in response to natural rewards (food, sex, etc.) similar to drug addicts, particularly in the case of gambling addiction. Romantic love may be a "natural" addiction, which differs from the nature of drug addiction in that love may be prosocial and has been evolved for the purpose of pair bonding. Helen Fisher, Arthur Aron and colleagues have proposed that romantic love is a "positive addiction" (i.e. not harmful) when requited and a "negative addiction" when unrequited or inappropriate.

Oxytocin, bonding and attraction

Location of the hypothalamus and pituitary.
Much of the research on oxytocin comes from experiments on monogamous prairie voles.

Oxytocin is sometimes called the "love hormone", because of its involvement in the mechanisms of maternal behavior and adult pair bonding. Oxytocin is synthesized primarily in an area of the hypothalamus and released into the blood via the pituitary gland, where it has been found circulating in people in the early stages of romantic love. Additionally, the hypothalamus projects oxytocin to other areas of the brain, like the ventral tegmental area (VTA), nucleus accumbens (NAc), amygdala and hippocampus. The projections to reward areas (VTA and NAc) are thought to modulate social salience, or i.e. the level of dopamine activity in response to socially-relevant stimuli. This oxytocin signaling in reward pathways may also be the source of salience in response to a loved one.

A placebo-controlled study found that administering intranasal oxytocin enhanced facial attractiveness of a romantic partner while viewing a photograph, as compared to an unfamiliar face. The effect was also measured using fMRI, which found enhanced brain activity in reward areas like the VTA and NAc. Another fMRI study found dopamine-rich genetic expression of an oxytocin receptor gene in the left VTA, and the left VTA has also been found active in response to facial attractiveness. In humans, circulating oxytocin levels have been associated with higher levels of interaction between partners, and also predicted which couples would still be together 6 months later. Anna Machin calls the combination of oxytocin and dopamine the "glue" which makes the early stages of a relationship possible.

The role of oxytocin in human behavior is varied and complex. Oxytocin lowers inhibitions to forming new relationships by deactivating the amygdala, involved with processing fear and anxiety. Oxytocin can be released with physical touch, hence it's also sometimes called the "cuddle hormone".Oxytocin also plays a role in sexual behavior, being released during sexual arousal and orgasm. Aside from romantic and parental bonding, oxytocin activity has a role in the interactions with peers or strangers, for example facilitating facial recognition and eye contact. Oxytocin is believed to facilitate trust and altruistic behaviors towards in-groups (e.g. partners or children), but also aggression towards out-groups (e.g. strangers or conspecifics).

Much of the research on oxytocin comes from experiments on monogamous prairie voles (notably by Larry Young), but this research is also used for making inferences about humans. In prairie voles, both oxytocin and dopamine signaling have been shown to influence pair bond development. For example, the number of oxytocin receptors in the NAc is positively related to how fast a partner preference is formed. A partner preference can also be prevented by injecting either a dopamine or oxytocin receptor antagonist (a drug which blocks transmission) into the NAc of a prairie vole directly.

In a contemporary model of the brain systems involved with romantic love, this type of salience (or 'bonding attraction') is present throughout the entire time a person is experiencing romantic love, including during the early stages. This contrasts with some previous theories (e.g. proposed by Helen Fisher in 1998) which stated that oxytocin activity and dopamine activity were distinct (and independent) systems, and that oxytocin activity only became prominent at some later stage of a relationship. Levels of oxytocin would still vary from situation to situation because of differing types of stimuli, for example because of less regular interaction and physical touch in cases of unrequited love. This could be used to explain some of the maladaptive symptoms of infatuation (e.g. sleep difficulties, social anxiety, clammy hands, etc.), when dopaminergic activity is high without the calming effect of oxytocin from the attachment system.

Brain opioid theory of social attachment

Oxycodone 10mg
Black tar heroin
The addictive aspects of love may resemble opioid addiction in respects.

Modern research is increasingly showing the importance of endogenous opioids in love and social attachment, particularly the β-endorphin (the most potent endogenous opioid) and the μ-opioid receptor system. While opioids have their origin being the body's natural painkiller, they're also implicated in a variety of other systems, essentially like neurotransmitters. Opioid receptors are located throughout the brain, including in the limbic system (affecting basic emotions) and neocortex (affecting more conscious decision-making). Opioids are linked to the consummatory part of reward, or i.e. "liking" or pleasure, and released in areas of the brain called hedonic hotspots (or pleasure centers). Hedonic hotspots are located in the nucleus accumbens, the ventral pallidum and other areas. This function includes social reward, or the pleasurable aspect of social interactions.

The brain opioid theory of social attachment (BOTSA) is a long-running theory summarizing this connection, originally formulated in the 1980s and 1990s, based on a proposal by the psychiatrist Michael Liebowitz and research by the neuroscientist Jaak Panksepp. Starting in the 1990s, opioids were overshadowed by the interest in oxytocin and largely overlooked until more recently, possibly because of the difficulty studying them (requiring e.g. a PET scan, which is expensive). Opioids have been connected to a variety of social experiences, including the early stage of romantic love and attachment styles. While the addictive aspects of love have been compared to cocaine or amphetamine addiction, other aspects may also resemble an opioid addiction.

BOTSA (as it was originally conceived of) predicts that in the absence of social relationships, individuals will have comparatively lower levels of endogenous opioids, motivating them to initiate contact with other people. Social contact then leads to feelings of euphoria and contentment, but individuals also need to continue contact to avoid withdrawal symptoms. Liebowitz originally argued that romantic relationships resemble narcotic addiction, and that individual neurochemical differences could also explain why some people are unable to commit, or stay in abusive relationships. Earlier experiments on BOTSA were animal studies, but in the 2000s this has been expanded to include human experiments.

Among the animal studies which have been done, there is some evidence that separation distress is akin to opioid withdrawal. Studies on chicks, puppies, Guinea pigs, rats, sheep and monkeys have shown that administrating morphine reduces distress vocalizations when separated from the mother, and administrating naloxone (an opioid antagonist) increases them, even in the presence of other members of the same species. In another study, mutant mouse pups with a μ-opioid receptor knockout (lacking the μ-receptor gene) vocalized less frequently in response to isolation than normal mice. Administration of morphine had no effect on distress vocalization frequency in the knockout mice, despite reducing it in normal mice. Furthermore, these knockout mice had a reduced preference for their mother's odor, which is normally the result of conditioning mediated by the endogenous opioid system. In nonhuman primates, studies have suggested that endogenous opioids provide the euphoria behind dyadic social grooming behaviors. Other animal studies have shown that endogenous opioids play a role in the desire for rough-and-tumble play (a physical, but also social behavior). In humans, physical activity with a social element (rowing, dancing, laughing) increased pain tolerance more when the activities were synchronized with other people.

An fMRI experiment in 2010 investigated whether viewing a picture of a romantic partner could reduce pain sensitivity, and which areas of the brain became active. Participants were exposed to high temperatures (resulting in moderate or high pain levels) while viewing a picture of a romantic partner (whom they were intensely in love with), or a friend, or performing a word association task which has also been shown to reduce pain via distraction. Participants were then asked to rate how much pain they felt on a pain scale, and both viewing a romantic partner and performing the distraction task (but not viewing a friend) were found to reduce pain levels. The fMRI scans revealed that viewing a romantic partner activated reward circuits in the brain, while the distraction task did not. Brain areas were also correlated with pain relief to reveal that reward analgesia and distraction analgesia involved distinct areas. Some areas associated with sensory processing of pain also had decreased activity while viewing a romantic partner. An earlier experiment showed that viewing photos of a romantic partner reduced experimental pain, but did not pair it with a brain scan.

A PET scan experiment in 2016 investigated whether non-sexual social touching between romantic partners was mediated by endogenous opioid activity. This study found that social touch did have an effect, but unexpectedly found that social touching decreased opioid activity in the brain rather than increasing it (despite being rated as pleasurable by participants). This is in contrast with prior PET research that pleasant affect is related to increased opioid activity. One possible explanation is that touching decreases stress, so this might also decrease the ongoing opioid activity in response to distress and pain. As this is also at odds (to some extent) with primate studies on grooming, there may be some variation between species in how opioids are involved with social reward. Other modern studies on humans include blood plasma levels, genetics and studies with drugs like morphine and naltrexone to see how they change social perception and behavior.

Obsessive thinking

Unlike OCD, passionate love (as in limerence) starts with a period of intoxicating joy, and only later reaches a state of anxiety when unrequited. The thoughts also differ in function and content.
In addiction, the early stage starts with positive reinforcement (binging and intoxication), but over time a transition occurs towards a more compulsive stage of negative reinforcement (avoiding withdrawal). This later stage (of negative reinforcement) is a possible parallel with OCD (where compulsions relieve tension or anxiety).

Obsessive thinking about a loved one has been called a hallmark or a cardinal trait of romantic love, ensuring that the loved one is not forgotten. Some reports have been made that people can even spend as much as 85 to 100% of their days and nights thinking about a love object. One study found that on average people in love spent 65% of their waking hours thinking about their beloved. Another study used cluster analysis to find several different groups of lovers, with the least intense group spending 35% of their time on average and the most intense at 72%. Since the late 1990s, these obsessional features have been compared to obsessive–compulsive disorder (OCD). This is also sometimes paired with a theory that obsessive (or intrusive) thinking is related to serotonin levels being lowered while in love, although study results have been inconsistent or negative. Another theory relates obsessive thinking to addiction, because drug users exhibit obsessive thoughts about drug use, as well as compulsions.

In 1999, James Leckman and Linda Mayes published a theoretical comparison between early-stage romantic love, early parental love and OCD. This paper was intended as an investigation into the origin of OCD, but it also relates to the evolutionary theory of romantic love. Both early-stage romantic love and OCD share features of preoccupation, intrusive thoughts, a heightened sense of responsibility, a need for things to be "just right" and some proximity-seeking behaviors. In some cases, obsessions experienced by OCD patients relate to what harms might happen to a family member, which resembles some behavioral patterns involved with romantic and parental love. The authors also speculate that psychasthenia (feelings of incompleteness, insufficiency or imperfection) resembles the "longing for reciprocity" and idealization which are features of romantic love.

Two experiments have investigated whether there is a relationship between romantic love and serotonin levels, by taking different measures using blood samples. Although serotonin levels in the central nervous system would actually be the measure of interest, it has been assumed that measures of peripheral serotonin can be used as a marker for this. A 1999 experiment led by Donatella Marazziti found that people in love had platelet serotonin transporter (SERT) density which was lower than controls, and similar to the density of a group of unmedicated OCD patients. Six of the 20 in-love participants were also retested after a period of 12 to 18 months, and SERT density had returned to normal. However, because Marazziti's experiment looked at SERT (rather than serotonin directly), this makes it ambiguous whether serotonin levels were actually higher or lower. SERT transports serotonin from blood plasma back into the platelets, so that a reduction in SERT could correspond to an increased plasma level.

Another experiment in 2012 led by Sandra Langeslag which looked at blood serotonin levels found a contradictory result, with men and women being affected differently. Men had lower serotonin levels than controls, but women had higher serotonin levels. In women, obsessive thinking was also actually associated with increased serotonin. A 2025 study led by Adam Bode also found no association between SSRI use and obsessive thinking about a loved one, or the intensity of romantic love. Therefore, although the earlier experiments do suggest romantic love and serotonin are probably associated, the authors suggest that the idea of obsessive thinking being attributed to lowered serotonin levels seems inaccurate.

Emotional valence

Rather than being a specific emotion itself, romantic love is believed to be a motivation or drive which elicits different emotions depending on the situation: positive feelings when things go well, and negative feelings when awry. Reciprocated love may elicit feelings of joy, ecstasy, or fulfillment, for example, but unrequited love may elicit feelings of sadness, anxiety, or despair. A 2014 study of Iranian young adults found that the early stage of romantic love was associated with the brighter side of hypomania (elation, mental and physical activity, and positive social interaction) and better sleep quality, but also stronger symptoms of depression and anxiety. Those authors conclude that romantic love is "not entirely a joyful and happy period of life". Romantic love may be either pleasant or unpleasant, regardless of the intensity level. One of Dorothy Tennov's interview participants recalls being in love this way: "When I felt [Barry] loved me, I was intensely in love and deliriously happy; when he seemed rejecting, I was still intensely in love, only miserable beyond words." The intensity of love feelings is also distinct from whether an individual is satisfied with their relationship (although the measures have been shown to be related to some extent). One can be satisfied with their relationship because it fulfills some other need besides love for their partner (like money or child care), or conversely be in love with an abuser in an abusive relationship.

Unrequited love is common among young adults. A study by Roy Baumeister and Sarah Stillwell found that 92.8% of participants reported at least one "powerful or moderate" experience of unrequited love in the past 5 years. A different study found 63% had a "huge crush" at least once in the past 2 years (but not letting the person know), and unrequited love was four times more frequent than equal love. Another found that 20% had experienced unrequited love more than 5 times, according to a definition that "When one is experiencing this emotion, it has been described as having one’s emotions on a roller coaster, finding it difficult to concentrate, and thinking constantly about the person with whom you are in love. The person is said to have the power to produce extreme highs and lows of emotion in you, depending on how he or she acts towards you."

In 2010, Helen Fisher, Arthur Aron and colleagues published their fMRI experiment investigating which areas of the brain might be active in recently rejected lovers. Participants had been in a relationship with their ex-partner for an average of 21 months, and then were post-rejection for an average of 63 days at the time of the experiment. These participants reported spending more than 85% of their waking hours thinking of their rejector, reported a lack of emotional control, and exhibited unhappiness, with sometimes more extreme emotions like depression, anger, and even paranoia in pre- and post-interviews. Similar to other fMRI experiments, the scan while looking at a photograph of the rejecting partner showed activations in dopaminergic reward system areas, like the ventral tegmental area and nucleus accumbens. These activations were also stronger than in a previous experiment of participants who were happily in love. The nucleus accumbens, prefrontal cortex and orbitofrontal cortex which were active have been associated with assessing one's gains and losses, and areas of the insular cortex and anterior cingulate cortex which were active have been involved with physical pain and pain regulation (respectively) in other studies.

Stress and physiological arousal

In the early stages of romantic love, individuals may start out hypervigilant (hyperaware and sensitive to a partner's cues) due to uncertainty and novelty, but become synchronized over time as a relationship progresses. Bonding is thought to be in part facilitated by coordinated behaviors which display reciprocity and events which evoke beneficial stress (eustress), like a passionate kiss. The stress response system involves two major systems: the autonomic nervous system and the hypothalamic–pituitary–adrenal axis (HPA axis). Some experiments have been done which support the idea that the stress response is involved during the early stage of romantic love, measuring cortisol levels; however, these experiments have been inconsistent with respect to cortisol being higher or lower.

In drug addiction, corticotropin release factor (CRF) is involved with the aversive effects of withdrawal. Stress causes CRF to release into the ventral tegmental area and nucleus accumbens shell, motivating reinstatement of drug use. A similar effect is also hypothesized in pair bonds, where stress after separation or social loss motivates a person to return to the partner; however, experiments have not investigated this in humans, only rodents.

Helen Fisher believed that separation anxiety activates the HPA axis, producing these stress hormones. It's ironic, she says, because short-term stress can also produce dopamine and norepinephrine, so "as the adored one slips away, the very chemicals that contribute to feelings of romance grow even more potent".

Frustration attraction and uncertainty

Dopamine neurons in the ventral tegmental area are theorized to encode a "reward prediction error" (RPE) signal, rather than a reward per se. This RPE signaling indicates whether a given reward was either better, equal to, or worse than what was anticipated, and this is believed to be part of a reinforcement learning paradigm. Studies have shown that for learning about a stimulus to occur (so that behavior in response to it changes), the reward has to be surprising or unpredicted. Rewards which are better than predicted reinforce the behavior and cause it to become more frequent, while a reward which is worse than expected would be avoided. Dopamine neurons increase their firing rate when encountering an unexpected reward. After reinforcement learning occurs, dopamine neurons also fire in response to encountering cues in the environment which predicted the reward (e.g. in animal studies, a lever or a special sound). As predictions become updated and the rewards are the same as expected, dopamine activity comparatively diminishes.

"Frustration attraction" (also called the "Romeo and Juliet effect") is the idea that adversity heightens romantic passion, for example, through social or physical barriers. The phenomenon has been remarked on by many authors, such as Socrates, Ovid, the Kama Sutra, and "Dear Abby". Bertrand Russell once opined that "when a man has no difficulty in obtaining a woman, his feeling toward her does not take the form of romantic love". Some common social barriers are parents who interfere with their children's romance (as in Romeo and Juliet), deceived spouses, or other social customs. Helen Fisher believes the phenomenon can be explained by the mechanics of dopamine, because animal studies have shown that when a reward which is anticipated to be incoming is delayed, reward-expecting neurons prolong their firing (over comparatively short timescales—in these studies) until the reward is delivered.

Infatuated love essentially thrives on intermittent reinforcement—also the mechanic a slot machine relies on.

Passionate or infatuated love is also said to thrive in situations which involve the uncertainty of intermittent reinforcement, when consummation is withheld, when barriers prevent lovers from meeting regularly, or when one's perceptions of how likely their love is reciprocated are ambiguous and constantly changing. Uncertainty seems to magnify cue-triggered incentive salience "wanting". A comparable type of situation is that of a slot machine, where the rewards are designed to be always unpredictable so the gambler cannot understand the pattern. Unable to habituate to the experience, for some people the exhilarating high from the unexpected wins leads to gambling addiction and compulsions. If the machine paid out on a regular interval (so that the rewards were expected), it would not be as exciting.

Uncertainty theory in the context of romantic love is associated with Dorothy Tennov's theory of limerence, an addictive, infatuated kind of love, commonly experienced for an unobtainable or unreachable person. In her study, Tennov observed reports of sometimes drastic emotional transitions caused by changes in one's perception over whether their love might be reciprocated, and these abrupt transitions could cause seeming emotional volatility even in otherwise stable individuals. The effect of uncertainty has also been interpreted as attachment anxiety.

Intermittent maltreatment (known as "traumatic bonding" in abusive relationships) is also believed to intensify romantic "passion" (i.e. strong emotion, including suffering). This is, again, believed to be related to intermittent reinforcement and how one's expectations are confirmed or violated.According to Elaine Hatfield, 'Consistency generates little emotion; it is inconsistency that we respond to. If a person always treats us with love and respect, we start to take that person for granted. We like him or her—but "ho hum." [...] What would generate a spark of interest, however, is if our admiring friend suddenly started treating us with contempt—or if our arch enemy started inundating us with kindness.'

Positive illusions

"Crystallization" was coined by the 19th-century French writer Stendhal to refer to these positive illusions, based on an analogy where a tree branch is tossed into a salt mine. The tree branch (or twig) becomes covered in salt crystals, transforming it "into an object of shimmering beauty".

People in love tend to overemphasize the positive aspects of their loved one or relationship, while overlooking or devaluing negative aspects. This is regarded as a type of cognitive bias called positive illusions. The phenomenon has also been referred to as crystallization, idealization, "love is blind" bias, putting the loved one on a pedestal, or seeing through rose-colored glasses. In the past, some authors have depicted the phenomenon as a malady, arguing that people who idealize would have their partner fall short of their high expectations as a relationship progresses; however, despite this, significant modern scientific evidence has shown that positive illusions actually contribute to relationship satisfaction, long-term well-being and decreased risk for relationship discontinuation.

The exact mechanism is not currently understood, but some brain areas are proposed to be related. The dopaminergic areas of the reward system which are active in romantic love may be involved with attributing salience to the positive characteristics of a loved one. The dorsal anterior cingulate cortex is involved with error detection and has been active during negative social evaluation and exclusion, so that reduced activation of this area would be an adaptive response to a partner's negative characteristics. Certain areas of the prefrontal cortex could also be exerting top-down control to suppress emotional responses to attractive alternatives. Information is then passed to the orbitofrontal cortex, where positive and negative information is weighed, resulting in a biased subjective value about the partner.

Brain imaging

Brain imaging techniques such as functional magnetic resonance imaging (fMRI) and positron emission tomography (PET) have been used to investigate which brain regions are involved in romantic love. Nearly all of these experiments have had participants look at a photograph of their beloved during an fMRI scan, with a few exceptions, although the specific procedures used have not always been identical. The differences in experimental design (e.g. length of time the participants had been in love, or the specific task given to participants during the scan) can be used to explain why the experiment results are sometimes different.

In 2000, a study by Andreas Bartels and Semir Zeki of University College London was the first fMRI study of romantic love. The 17 participants were "truly, deeply and madly in love", had been together for a mean of 2.4 years, and were shown either one or two photographs of their loved one during the scan. Two main areas were active in this study: the middle insular cortex, associated with stomach churning or "gut feelings", which could have something to do with the feeling of "butterflies in the stomach", and part of the anterior cingulate cortex, associated with feelings of euphoria. Other activations were areas in the cerebrum, the caudate nucleus, putamen and the cerebellum. A later analysis in 2004 by the same authors also reports activity in the ventral tegmental area (VTA), which produces dopamine. The study also showed key deactivations, areas of the brain that were less active in romantic love compared to friendship love, in the amygdala and medial prefrontal cortex (mPFC). The amygdala is involved with fear and risk detection, and the mPFC is involved with understanding and predicting the intentions of other people, called mentalizing. These deactivations are taken as evidence that "love is blind", or i.e. that people in love discount the risks involved and misunderstand people's intentions, even leading to folly sometimes.

In 2005, a study by Arthur Aron, Helen Fisher, Debra Mashek, Greg Strong, Haifang Li and Lucy Brown was the first fMRI study of early-stage intense romantic love.

It has been praised as advancing the scientific understanding of infatuated love, even by a skeptic of fMRI literature. This study differed from Bartels & Zeki in that the 17 participants who had "just fallen madly in love" had been in love for a much shorter mean time of only 7.4 months. These participants were more intensely in love, and spent 85% or more of their waking hours thinking of their loved one. This study also had participants look at a photograph of their loved one during the scan. Reward and motivation areas were active, like the VTA and areas of the caudate. Activity was also found in the insular and cingulate cortex, involved with emotion. Some interesting areas were correlated with the length of the relationship, like the ventral pallidum, implicated in attachment in prairie voles, and the anterior cingulate, implicated in obsessive thinking, cognition and emotion. This study also examined correlations with facial attractiveness to determine that the right VTA was active because of romantic passion rather than because the partner was aesthetically pleasing. Aesthetically pleasing faces elicited more activity in the left VTA, which is more associated with "liking" a reward (i.e. pleasure), whereas the right VTA is more associated with "wanting" a reward (i.e. incentive salience). In 2011, Xu et al. repeated the experiment by Aron et al., but using Chinese participants.

Ortigue et al. used fMRI to investigate the subliminal influence of romantic love on motivation, interested in how these implicit neural representations might differ from previous experiments where subjects were consciously aware of the stimulus (viewing a photograph). In Ortique et al.'s study, participants were shown a subliminal prime word for 26ms (either their beloved's name, the name of a friend, or a word describing a personal passion like a hobby), followed by a series of symbols (#) for 150ms, followed by a target word for 26ms. This target was either an English word, non-word or blank, and participants were asked to identify whether it was a word or not. In trials with the love prime or passion prime, participants were faster to identify whether the target was a word or not, and this also correlated with scores on the Passionate Love Scale. The authors believe this shows that love priming activates motivation systems in the brain, rather than just evoking a particular emotion. The fMRI scanning showed brain regions active for love primes similar to previous experiments, including reward and motivation areas like the VTA and caudate, but with some additions. Subliminal love priming additionally activated the bilateral fusiform gyri and angular gyri, involved in integrating abstract representations. The authors relate this to the self-expansion model of interpersonal relationships, where self-expansion by integrating the characteristics of one's beloved into one's self (called inclusion of the other in the self) is a rewarding experience which may promote romantic love feelings.

In brain scans of long-term intense romantic love (involving subjects who professed to be "madly" in love, but were together with their partner 10 years or more) led by Bianca Acevedo, attraction similar to early-stage romantic love was associated with dopamine reward center activity ("wanting"), but long-term attachment was associated with the globus palludus, a site for opiate receptors identified as a hedonic hotspot ("liking"). Long-term romantic lovers also showed lower levels of obsession compared to those in the early stage.

An fMRI study led by Sandra Langeslag investigated the effect of attention on brain activity related to a loved one. In most other previous experiments, subjects only passively viewed a photograph, but this experiment used an oddball task to distinguish between instances where the loved one was either the intended target of the subject's attention or a distraction. Participants were given trials where they were presented with a random face for only 250ms (usually an unknown person) and instructed to watch for either a loved one or a friend, then press a button if the face was the intended target for a given run. In some runs, the loved one would be the intended target for a button press, while the friend would be a distractor causing participants to press the button by mistake sometimes, while in other runs the friend would be the target and the loved one a distractor. This experiment found that activity in the dorsal striatum (an area of the reward system) was modulated by whether or not participants were instructed to pay attention to their loved one. That is, the dorsal striatum showed more response to the loved one than to the friend, but only when the loved one was the target. This led the authors to conclude that "the dorsal striatum is not activated by beloved-related information per se, but only by beloved-related information that is attended". This activity also tended to be smaller when participants had been in love or been in a relationship for longer. The dorsal striatum is implicated in reinforcement learning, so the authors interpret the increase in brain activity as reflecting prior reinforcement of social actions which leads the infatuated individuals to pay preferential attention to their loved one. Participants also tended to press the button by mistake more often when distracted by the loved one than the friend.

Some brain scan experiments of early-stage romantic love have found activation of the posterior cingulate cortex, which is implicated in autobiographical memory of socially relevant stimuli (e.g. partner names) and attention. Most experiments (including long-term romantic love) have shown activity in the hippocampus and parahippocampal gyrus, areas involved with learning and memory.

Terraforming

From Wikipedia, the free encyclopedia
https://en.wikipedia.org/wiki/Terraforming
An artist's conception shows a terraformed Mars in four stages of development.

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, with the goal of making it habitable for humans.

The concept of terraforming developed from both science fiction and actual science. Carl Sagan, an astronomer, proposed the planetary engineering of Venus in 1961, which is considered one of the first accounts of the concept. The term was coined by Jack Williamson in a science-fiction short story ("Collision Orbit") published in 1942 in Astounding Science Fiction.

Even if the environment of a planet could be altered deliberately, the feasibility of creating an unconstrained planetary environment that mimics Earth on another planet has yet to be verified. While Venus and the Moon have been studied in relation to the subject, Mars is usually considered to be the most likely candidate for terraforming. Much study has been done concerning the possibility of heating the planet and altering its atmosphere, and NASA has even hosted debates on the subject. Several potential methods for the terraforming of Mars may be within humanity's technological capabilities, but according to Martin Beech, the economic attitude of preferring short-term profits over long-term investments will not support a terraforming project.

The long timescales and practicality of terraforming are also the subject of debate. As the subject has gained traction, research has expanded to other possibilities including biological terraforming, para-terraforming, and modifying humans to better suit the environments of planets and moons. Despite this, questions still remain in areas relating to the ethics, logistics, economics, politics, and methodology of altering the environment of an extraterrestrial world, presenting issues to the implementation of the concept.

Concept

The term "terraforming" was coined by Jack Williamson in “Collision Orbit” in 1942, as a term for making the environment around people habitable. It later came to mean making planets Earth-like in the sense of "Earth-forming".

The concept gained traction when it became evident, with the first space probes going to other planets, that other planets were not habitable. Terraforming has since been envisioned as a means to "colonize" space or to make space relatable.

During the 1980s, American geographer Richard Cathcart successfully lobbied for formal recognition of the verb "to terraform". The word was added to the fourth edition of the Shorter Oxford English Dictionary in 1993.

The concept is contrasted by pantropy, the adaptation of humans to an alien environment rather than an environment to humans. Pantropy has also been envisioned as a substitute when terraforming is not complete.

History of scholarly study

The astronomer Carl Sagan proposed the planetary engineering of Venus in an article published in the journal Science in 1961. Sagan imagined seeding the atmosphere of Venus with algae, which would convert water, nitrogen and carbon dioxide into organic compounds. As this process removed carbon dioxide from the atmosphere, the greenhouse effect would be reduced until surface temperatures dropped to "comfortable" levels. The resulting plant matter, Sagan proposed, would be pyrolyzed by the high surface temperatures of Venus, and thus be sequestered in the form of "graphite or some involatile form of carbon" on the planet's surface. However, later discoveries about the conditions on Venus made this particular approach impossible. One problem is that the clouds of Venus are composed of a highly concentrated sulfuric acid solution. Even if atmospheric algae could thrive in the hostile environment of Venus's upper atmosphere, an even more insurmountable problem is that its atmosphere is simply far too thick: the high atmospheric pressure would result in a "atmosphere of nearly pure molecular oxygen" at high pressure. This volatile combination could not be sustained through time. Any carbon that had been reduced by photosynthesis would be quickly oxidized in this atmosphere through combustion, "short-circuiting" the terraforming process.

Sagan also visualized making Mars habitable for human life in an article published in the journal Icarus, "Planetary Engineering on Mars" (1973). Three years later, NASA addressed the issue of planetary engineering officially in a study, but used the term "planetary ecosynthesis" instead. The study concluded that it was possible for Mars to support life and be made into a habitable planet. The first conference session on terraforming, then referred to as "Planetary Modeling", was organized that same year.

In March 1979, NASA engineer and author James Oberg organized the First Terraforming Colloquium, a special session at the Lunar and Planetary Science Conference in Houston. Oberg popularized the terraforming concepts discussed at the colloquium to the general public in his book New Earths (1981). Not until 1982 was the word terraforming used in the title of a published journal article. Planetologist Christopher McKay wrote "Terraforming Mars", a paper for the Journal of the British Interplanetary Society. The paper discussed the prospects of a self-regulating Martian biosphere, and the word "terraforming" has since become the preferred term.

In 1984, James Lovelock and Michael Allaby published The Greening of Mars. Lovelock's book was one of the first to describe a novel method of warming Mars, where chlorofluorocarbons (CFCs) are added to the atmosphere to produce a strong greenhouse effect.

Motivated by Lovelock's book, biophysicist Robert Haynes worked behind the scenes to promote terraforming, and contributed the neologism Ecopoiesis, forming the word from the Greek οἶκος, oikos, "house", and ποίησις, poiesis, "production". Ecopoiesis refers to the origin of an ecosystem. In the context of space exploration, Haynes describes ecopoiesis as the "fabrication of a sustainable ecosystem on a currently lifeless, sterile planet". Fogg defines ecopoiesis as a type of planetary engineering and is one of the first stages of terraformation. This primary stage of ecosystem creation is usually restricted to the initial seeding of microbial life. A 2019 opinion piece by Lopez, Peixoto and Rosado has reintroduced microbiology as a necessary component of any possible colonization strategy based on the principles of microbial symbiosis and their beneficial ecosystem services. As conditions approach those of Earth, plant life could be brought in, and this will accelerate the production of oxygen, theoretically making the planet eventually able to support animal life.

Ecopoiesis potentially allows a form of co-evolution of terraforming with the target environment.

Aspects and definitions

In 1985, Martyn Fogg started publishing several articles on terraforming. He also served as editor for a full issue on terraforming for the Journal of the British Interplanetary Society in 1992. In his book Terraforming: Engineering Planetary Environments (1995), Fogg proposed the following definitions for different aspects related to terraforming:

  • Planetary engineering: the application of technology for the purpose of influencing the global properties of a planet.
  • Geoengineering: planetary engineering applied specifically to Earth. It includes only those macro engineering concepts that deal with the alteration of some global parameter, such as the greenhouse effect, atmospheric composition, insolation or impact flux.
  • Terraforming: a process of planetary engineering, specifically directed at enhancing the capacity of an extraterrestrial planetary environment to support life as we know it. The ultimate achievement in terraforming would be to create an open planetary ecosystem emulating all the functions of the biosphere of Earth, one that would be fully habitable for human beings.

Fogg also devised definitions for candidate planets of varying degrees of human compatibility:

  • Habitable planet (HP): A world with an environment sufficiently similar to Earth's as to allow comfortable and free human habitation.
  • Biocompatible planet (BP): A planet possessing the necessary physical parameters for life to flourish on its surface. If initially lifeless, then such a world could host a biosphere of considerable complexity without the need for terraforming.
  • Easily-terraformable planet (ETP): A planet that might be rendered biocompatible, or possibly habitable, and maintained so by modest planetary engineering techniques and with the limited resources of a starship or robot precursor mission.

Fogg suggests that Mars was a biologically compatible planet in its youth, but is not now in any of these three categories, because it can only be terraformed with greater difficulty.

Habitability requirements

Necessary conditions for habitability, adapted from Hoehler (2007)

Planetary habitability, broadly defined as the capacity for an astronomical body to sustain life, requires that various geophysical, geochemical, and astrophysical criteria must be met before the surface of such a body is considered habitable. Modifying a planetary surface such that it is able to sustain life, particularly for humans, is generally the end-goal of the hypothetical process of terraforming. Of particular interest in the context of terraforming is the set of factors that have sustained complex, multicellular animals in addition to simpler organisms on Earth. Research and theory in this regard is a component of planetary science and the emerging discipline of astrobiology.

Classifications of the criteria of habitability can be varied, but it is generally agreed upon that the presence of water, non-extreme temperatures, and an energy source put broad constraints on habitability. Other requirements for habitability have been defined as the presence of raw materials, a solvent, and clement conditions, or elemental requirements (such as carbon, hydrogen, nitrogen, oxygen, phosphorus and sulfur), and reasonable physiochemical conditions. When applied to organisms present on the earth, including humans, these constraints can substantially narrow.

In its astrobiology roadmap, NASA has defined the principal habitability criteria as "extended regions of liquid water, conditions favorable for the assembly of complex organic molecules, and energy sources to sustain metabolism."

Temperature

The general temperature range for all life on Earth is -20 °C to 122 °C, set primarily by the ability of water (possibly saline, or under high pressure in the ocean bottom) to be available in liquid form. This may constitute a bounding range for the development of life on other planets, in the context of terraforming. For Earth, the temperature is set by the equilibrium of incident solar radiation absorbed and outgoing infrared radiation, including the effect of greenhouse gasses in modifying the planetary equilibrium temperature; terraforming concepts may include modifying temperature by methods including solar reflectors to increase or decrease the amount of solar illumination, and hence modify temperature.

Water

All known life requires water; thus the capacity for planetary body to sustain water is a critical aspect of habitability. The habitable zone of a solar system is generally defined as the region in which stable surface liquid water may be present on a planetary body. The boundaries of the habitable zone were originally defined by water loss by photolysis and hydrogen escape, setting a limit on how close a planet may be to its orbited star, and the prevalence of CO2 clouds that would increase albedo, setting an outer boundary on stable liquid water. These constraints are applicable in particular to Earth-like planets, and would not as easily apply to moons like Europa and Enceladus with ice-covered oceans, where the energy source to keep the water liquid is from tidal heating, rather than solar energy.

Energy

On the most fundamental level, the only absolute requirement of life may be thermodynamic disequilibrium, or the presence of Gibbs free energy. It has been argued that habitability can be conceived of as a balance between life's demand for energy and the capacity for the environment to provide such energy. For humans, energy comes in the form of sugars, fats, and proteins provided by consuming plants and animals, necessitating in turn that a habitable planet for humans can sustain such organisms.

Much of Earth's biomass (~60%) relies on photosynthesis for an energy source, while a further ~40% is chemotropic. For the development of life on other planetary bodies, chemical energy may have been critical, while for sustaining life on another planetary body in the Solar System, sufficiently high solar energy may also be necessary for phototrophic organisms.

Elements

On Earth, life generally requires six elements in high abundance: carbon, hydrogen, nitrogen, oxygen, phosphorus, and sulfur. These elements are considered "essential" for all known life and plentiful within biological systems. Additional elements crucial to life include the cations Mg2+, Ca2+, K+ and Na+ and the anion Cl. Many of these elements may undergo biologically facilitated oxidation or reduction to produce usable metabolic energy.

Preliminary stages

Terraforming a planet would involve making it fit the habitability requirements listed in the previous section. For example, a planet may be too cold for liquid water to exist on its surface. Its temperature could be raised by adding greenhouse gases to the atmosphere, using orbiting mirrors to reflect more sunlight onto the planet, or lowering the albedo of the planet. Conversely, a planet too hot for liquid water could be cooled down by removing greenhouse gases (if these are present), placing a sunshade in the L1 point to reduce sunlight reaching the planet, or increasing the albedo. Atmospheric pressure is another issue: various celestial bodies including Mars, Mercury and most moons have lower pressure than Earth. At pressures below the triple point of water (611.7 Pa), water cannot be liquid at any temperature. Human survival requires a still-higher pressure of at least 6.3 kPa, the Armstrong limit; below this pressure, exposed body fluids boil at body temperature. Furthermore, a thick atmosphere protects the surface from cosmic rays. A thin atmosphere could be thickened using gases produced locally (e.g. the Moon could be given an atmosphere of oxygen by reducing lunar rock) or gases could be imported from elsewhere.

Once conditions become more suitable for life of the introduced species, the importation of microbial life could begin. As conditions approach that of Earth, plant life could also be brought in. This would accelerate the production of oxygen, which theoretically would make the planet eventually able to support animal life.

Prospective targets

Mars

Artist's conception of a terraformed Mars

In many respects, Mars is the most Earth-like planet in the Solar System. It is thought that Mars once had a more Earth-like environment early in its history, with a thicker atmosphere and abundant water that was lost over the course of hundreds of millions of years.

The exact mechanism of this loss is still unclear, though three mechanisms, in particular, seem likely: First, whenever surface water is present, carbon dioxide (CO
2
) reacts with rocks to form carbonates, thus drawing atmosphere off and binding it to the planetary surface. On Earth, this process is counteracted when plate tectonics works to cause volcanic eruptions that vent carbon dioxide back to the atmosphere. On Mars, the lack of such tectonic activity worked to prevent the recycling of gases locked up in sediments.

Second, the lack of a magnetosphere around Mars may have allowed the solar wind to gradually erode the atmosphere. Convection within the core of Mars, which is made mostly of iron, originally generated a magnetic field. However the dynamo ceased to function long ago, and the magnetic field of Mars has largely disappeared, probably due to "loss of core heat, solidification of most of the core, and/or changes in the mantle convection regime." Results from the NASA MAVEN mission show that the atmosphere is removed primarily due to coronal mass ejection events, where outbursts of high-velocity protons from the Sun impact the atmosphere. Mars does still retain a limited magnetosphere that covers approximately 40% of its surface. Rather than uniformly covering and protecting the atmosphere from solar wind, however, the magnetic field takes the form of a collection of smaller, umbrella-shaped fields, mainly clustered together around the planet's southern hemisphere.

Finally, between approximately 4.1 and 3.8 billion years ago, asteroid impacts during the Late Heavy Bombardment caused significant changes to the surface environment of objects in the Solar System. The low gravity of Mars suggests that these impacts could have ejected much of the Martian atmosphere into deep space.

Terraforming Mars would entail two major interlaced changes: building the atmosphere and heating it. A thicker atmosphere of greenhouse gases such as carbon dioxide would trap incoming solar radiation. Because the raised temperature would add greenhouse gases to the atmosphere, the two processes would augment each other. Carbon dioxide alone would not suffice to sustain a temperature above the freezing point of water, so a mixture of specialized greenhouse molecules might be manufactured.

A realistic path to radical terraforming of Mars was presented by . This would result in the creation of an atmosphere with a pressure of approximately 1000 hPa. The atmosphere would be obtained from bodies with a total mass of approximately 1019 kg (high in water and carbon dioxide) transported from the Kuiper Belt to Mars using thermonuclear rocket engines and gravity assist.

Venus

True-color image of Venus. To terraform, this dense atmosphere will need to be removed.

Terraforming Venus requires two major changes: removing most of the planet's dense 9 MPa (1,300 psi; 89 atm) carbon dioxide atmosphere, and reducing the planet's 450 °C (842 °F) surface temperature.[52] These goals are closely interrelated because Venus's extreme temperature may result from the greenhouse effect caused by its dense atmosphere.

Artist's conception of a terraformed Venus

Venus's atmosphere currently contains little oxygen, so an additional step would be to inject breathable O2 into the atmosphere. An early proposal for such a process comes from Carl Sagan, who suggested the injection of floating, photosynthetic bacteria into the Venusian atmosphere to reduce CO2 to organic form, and increase the atmospheric concentration of O2 in the atmosphere. This concept, however, was based in a flawed 1960s understanding of Venus's atmosphere as much lower pressure; in reality, the Venusian atmospheric pressure (9300 kPa) is far higher than early estimates. Sagan's idea is therefore untenable, as he later conceded.

An additional step noted by Martin Beech includes the injection of water and/or hydrogen into the planetary atmosphere; this step follows after sequestering CO2 and reducing the mass of the atmosphere. In order to combine hydrogen with O2 produced by other means, an estimated 4×1019 kg of hydrogen is necessary; this may need to be mined from another source, such as Uranus or Neptune.

Moon

Artist's conception of the Moon terraformed as seen from Earth

Although the gravity on Earth's Moon is too low to hold an atmosphere for geological spans of time, if given one, it would retain it for spans of time that are long compared to human lifespans. Landis and others have thus proposed that it could be feasible to terraform the Moon, although not all agree with that proposal. Landis estimates that a 6.89 kPa atmosphere of pure oxygen on the Moon would require on the order of two hundred trillion tons of oxygen, and suggests it could be produced by reducing the oxygen from an amount of lunar rock equivalent to a cube about fifty kilometers on an edge. Alternatively, he suggests that the water content of "fifty to a hundred comets" the size of Halley's Comet would do the job, "assuming that the water doesn't splash away when the comets hit the moon." Likewise, Benford calculates that terraforming the moon would require "about 100 comets the size of Halley's."

Mercury

An artist's conception of the terraformed Mercury

Mercury would be difficult to terraform. Beech states "There seems little prospect of terraforming Mercury such that any animals or plants might exist there," and suggests that its primary use in a terraforming project would be as a mining source for minerals. Nevertheless, terraforming has been considered. Mercury's magnetic field is only 1.1% that of Earth's, and, being closer to the Sun, any atmosphere would be stripped rapidly unless it can be protected from the solar wind. It is conjectured that Mercury's magnetic field should be much stronger, up to 30% of Earth's, if it weren't being suppressed by certain solar wind feedback effects. If some means of shielding Mercury from solar wind by placing an artificial magnetic shield at Mercury-Sun L1 (similar to the proposal for Mars), then Mercury's magnetic field could possibly grow in intensity to a point where Mercury's magnetic field could be self-sustaining provided the field wasn't made to "stall" by another solar event.

Despite being much smaller than Mars, Mercury has an escape velocity only slightly less than that of Mars due to its higher density and could, if a magnetosphere prevents atmospheric stripping, hold a nitrogen/oxygen atmosphere for millions of years.

To provide one atmosphere of pressure, roughly 1.1×1018 kilograms of gas would be required; or a somewhat lower amount if lower pressure is acceptable. Water could be delivered from the outer Solar System. Once this water has been delivered, it would split the water into its constituent oxygen and hydrogen molecules, possibly using a photo-catalytic dust, with the hydrogen rapidly being lost to space. At an oxygen pressure of 20-30 kPa, the atmosphere would be breathable and nitrogen may be added as required to allow for plant growth in the presence of nitrates.

Temperature management would be required, due to the equilibrium average temperature of ~159°C. However, millions of square kilometers at the poles have an average temperature of 0-50°C (i.e., an area the size of Mexico at each pole with habitable temperatures). The total habitable area could be even larger if the planetary albedo were increased from 0.12 to ~0.6, potentially increasing the habitable area. Roy proposes that the temperature could be further managed by decreasing the solar flux at Mercury to near the terrestrial value by solar sails reflecting sunlight. He calculates that 16 to 17 million sails, each with an area of one square kilometer would be needed.

Earth

It has been recently proposed that due to the effects of climate change, an interventionist program might be designed to return Earth to pre-industrial climate parameters. In order to achieve this, multiple approaches have been proposed, such as the management of solar radiation, the sequestration of carbon dioxide, and the design and release of climate altering genetically engineered organisms. These are typically referred to as geoengineering or climate engineering, rather than terraforming.

Other bodies in the Solar System

Other possible candidates for terraforming (possibly only partial or paraterraforming) include large moons of Jupiter or Saturn (Europa, Ganymede, Callisto, Enceladus, Titan), and the dwarf planet Ceres.

The moons are covered in ice, so heating them would make some of this ice sublimate into an atmosphere of water vapour, ammonia and other gases. For Jupiter's moons, the intense radiation around Jupiter would cause radiolysis of water vapour, splitting it into hydrogen and oxygen. The former would be rapidly lost to space, leaving behind the oxygen (this already occurs on the moons to a minor extent, giving them thin atmospheres of oxygen). For Saturn's moons, the water vapour could be split by using orbital mirrors to focus sunlight, causing photolysis. The ammonia could be converted to nitrogen by introducing bacteria such as Nitrosomonas, Pseudomonas and Clostridium, resulting in an Earth-like nitrogen-oxygen atmosphere. This atmosphere would protect the surface from Jupiter's radiation, but it would also be possible to clear said radiation using orbiting tethers or radio waves.

Challenges to terraforming the moons include their high amounts of ice and their low gravity. If all of the ice were fully melted, it would result in deep moon-spanning oceans, meaning any settlements would have to be floating (unless some of the ice was allowed to remain, to serve as land). Low gravity would cause atmospheric escape over time and may cause problems for human health. However, atmospheric escape would take place over spans of time that are long compared to human lifespans, as with the Moon.

One proposal for terraforming Ceres would involve heating it (using orbital mirrors, detonating thermonuclear devices or colliding small asteroids with Ceres), creating an atmosphere and deep ocean. However, this appears to be based on a misconception that Ceres' surface is icy in a similar way to the gas giant moons. In reality, Ceres' surface is "a layer of mixed ice, silicates and light strong phases best matched by hydrated salts and clathrates". It is unclear what the result of heating this up would be.

Other possibilities

Biological terraforming

Many proposals for planetary engineering involve the use of genetically engineered bacteria.[69][70]

As synthetic biology matures over the coming decades it may become possible to build designer organisms from scratch that directly manufacture desired products efficiently. Lisa Nip, Ph.D. candidate at the MIT Media Lab's Molecular Machines group, said that by synthetic biology, scientists could genetically engineer humans, plants and bacteria to create Earth-like conditions on another planet.

Gary King, microbiologist at Louisiana State University studying the most extreme organisms on Earth, notes that "synthetic biology has given us a remarkable toolkit that can be used to manufacture new kinds of organisms specially suited for the systems we want to plan for" and outlines the prospects for terraforming, saying "we'll want to investigate our chosen microbes, find the genes that code for the survival and terraforming properties that we want (like radiation and drought resistance), and then use that knowledge to genetically engineer specifically Martian-designed microbes". He sees the project's biggest bottleneck in the ability to genetically tweak and tailor the right microbes, estimating that this could take "a decade or more" to be solved. He also notes that it would be best to develop "not a single kind of microbe but a suite of several that work together".

DARPA is researching the use of photosynthesizing plants, bacteria, and algae grown directly on the Mars surface that could warm up and thicken its atmosphere. In 2015 the agency and some of its research partners created a software called DTA GView, in which genomes of several organisms can be pulled up on the program to immediately show a list of known genes and where they are located in the genome. According to Alicia Jackson, deputy director of DARPA's Biological Technologies Office, they have developed a "technological toolkit to transform not just hostile places here on Earth, but to go into space not just to visit, but to stay".

Paraterraforming

Also known as the "world house" concept, para-terraforming involves the construction of a habitable enclosure on a planet that encompasses most of the planet's usable area. The enclosure would consist of a transparent roof held one or more kilometers above the surface, pressurized with a breathable atmosphere, and anchored with tension towers and cables at regular intervals. The world house concept is similar to the concept of a domed habitat, but one which covers all (or most) of the planet.

Potential targets for paraterraforming include Mercury, the Moon, Ceres and the gas giant moons.

Adapting humans

It has also been suggested that instead of or in addition to terraforming a hostile environment humans might adapt to these places by the use of genetic engineering, biotechnology and cybernetic enhancements. This is known as pantropy.

Examples of such adjustments include the making organs fit for low gravity, increasing lung volumes for atmospheres with low oxygen levels and exoskeletons for high pressure ratios.

Issues

Ethical issues

There is a philosophical debate within biology and ecology as to whether terraforming other worlds is an ethical endeavor. From the point of view of a cosmocentric ethic, this involves balancing the need for the preservation of human life against the intrinsic value of existing planetary ecologies. Lucianne Walkowicz has even called terraforming a "planetary-scale strip mining operation".[88]

On the pro-terraforming side of the argument, there are those like Robert Zubrin, Martyn J. Fogg, Richard L. S. Taylor, and the late Carl Sagan who believe that it is humanity's moral obligation to make other worlds suitable for human life, as a continuation of the history of life-transforming the environments around it on Earth. They also point out that Earth would eventually be destroyed if nature takes its course, so that humanity faces a very long-term choice between terraforming other worlds or allowing all terrestrial life to become extinct. Terraforming totally barren planets, it is asserted, is not morally wrong as it does not affect any other life.

The opposing argument posits that terraforming would be an unethical interference in nature, and that given humanity's past treatment of Earth, other planets may be better off without human interference. Still others strike a middle ground, such as Christopher McKay, who argues that terraforming is ethically sound only once it is completely certain that an alien planet does not harbor life of its own; but that if it does, it should not try be reshaped to fit humans' own use, but rather to engineer its environment to artificially nurture the alien life and help it thrive and co-evolve, or even co-exist with humans. Even this would be seen as a type of terraforming to the strictest of ecocentrists, who would say that all life has the right, in its home biosphere, to evolve without outside interference.

Economic issues

The initial cost of such projects as planetary terraforming would be massive, and the infrastructure of such an enterprise would have to be built from scratch. Such technology has not yet been developed, let alone financially feasible at the moment. John Hickman has pointed out that almost none of the current schemes for terraforming incorporate economic strategies, and most of their models and expectations seem highly optimistic.

Terraforming is a common concept in science fiction, ranging from television, movies and novels to video games.

A related concept from science fiction is xenoforming – a process in which aliens change the Earth or other planets to suit their own needs, already suggested in the classic The War of the Worlds (1898) of H.G. Wells,  in its specific case of areoforming (from Ares, the Greek alternative name of Mars), Earth being its subject.

Graphene

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