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Sunday, July 3, 2022

Costly signaling theory in evolutionary psychology

Costly signaling theory in evolutionary psychology refers to uses of costly signaling theory and adaptationism in explanations for psychological traits and states. Often informed by the closely related fields of human behavioral ecology and cultural evolution, such explanations are predominantly focused on humans and emphasize the benefits of altering the perceptions of others and the need to do so in ways that are difficult to fake due to the widespread existence of adaptations which demand reliable information to avoid manipulation through dishonest signals.

Although initially created to explain costly morphological traits as honest signals of an individual's underlying quality resulting from sexual selection, the scope of costly signaling theory has been expanded to include signals of cooperative intent and need, with the targets of such signals often going beyond potential mates.

Costly signaling background

Almost any organism can benefit from altering the perceptions, behavior, and physiology of others in its environment in ways that favor itself. Particularly true in social species, the result is often investment in signals to enhance one’s perceived attractiveness, formidability, or cooperative value to members of their own species.

A signal differs from a cue in that signals evolved to influence the behavior or perceptions of others, while a cue is any piece of information an organism uses to alter its current state that was not created for this purpose. As signals evolve due to their communicative effects and are often not fully linked to the qualities being signaled, they have the potential to be easily faked by those who do not possess a trait. Such faking would likely be favored through natural selection due to the ubiquity of conflicts of interests among living things creating situations in which the negative impacts on others are either not relevant or still worth the benefits to the signaler.

Although there are substantial risks of being deceived, targets of a signal may still benefit from paying attention to this information as long as it is honest and relevant to fitness-related problems. For this reason, natural selection is thought to have resulted in adaptations in many species to verify the validity of signals before accepting the information as reliable. Signaling in a costly manner is thought to satisfy these anti-manipulation adaptations when the resultant signals are comparatively cheaper to produce for those who have the underlying quality compared to those who lack it. In these instances, individuals with the quality can maximize their fitness by investing more in the signal relative to those who lack the quality or possess it to a lesser degree, thereby resulting in a signal that, while often not impossible to fake, tends to not be worth faking.

Costly signals of beneficial qualities

The majority of costly signaling explanations involve behaviors that broadcast beneficial traits about oneself to others. In many instances, these signals are expected to be directed towards potential mates, with males often thought to benefit more from such signaling due to their relatively low levels of investment in offspring leading to greater fitness benefits in having multiple partners. However, the importance of cooperation over human evolutionary history is also thought to have resulted in many signals that involve showing one’s potential as a cooperative partner to those outside of mates.

Costly signals of embodied capital

Hunting

Primarily through the work of human behavioral ecologists, hunting among humans has received much attention as potentially serving as an honest indicator of various qualities due to its potential for differential costs. The first signaling approaches to hunting emphasized that although hunting can provide an important source of calories and nutrients in small-scale societies, it is still practiced when it is less efficient than other means of food production and often involves the targeting of species that result in less meat for a given period. In response to this and findings that food is typically shared widely in small-scale societies, the show-off hypothesis suggests that men may hunt difficult prey in part due to reputational benefits that increase the likelihood that others will want good hunters in their group because of the benefits they provide.

Later models built off this by incorporating costly signaling theory. In addition to the costs of inefficiency reported in some hunts, hunting can be costly in terms of the time needed to develop one’s skill, the risks involved, and the resources required for a successful hunt. For this reason, it has been proposed to honestly signal a wide range of traits including strength, skill, ability to buffer risk, leadership, and various beneficial cognitive traits, all of which can increase one’s attractiveness to mates and cooperative partners. As with other costly signals, this is due hunting being relatively more costly for those who lack the previously mentioned qualities or possess them to a lesser degree, with such individuals being more likely to produce less effective signals and become injured, both of which deter faking the signal.

Although not mutually exclusive with the show-off hypothesis, such approaches have been presented as explaining a wider range of hunting behaviors as the benefits that come with signaling one’s qualities does not require that hunting benefits others, thereby better accounting for relatively wasteful displays. However, these models still emphasize the benefits of providing for others as meat sharing is often public and attracts large audiences, thereby increasing the effectiveness of a signal to increase one’s status within a group.

Evidence in favor of hunting being a costly signal of beneficial qualities has primarily come from its valuation by group members and by the benefits good hunters enjoy. In small-scale societies, individuals can often tell a good hunter from a bad one,[21] with skilled hunters having been reported as having higher status than those less skilled.[22][26] Material benefits are also seen with good hunters having been shown to have increased reproductive success, more political power, and more support for one’s kin in both times and illness and health.[20][22][27]

Compared to the existence of the reputational benefits of hunting, its importance in explaining human hunting relative to explanations involving kin selection or reciprocity is more controversial. This is primarily seen through disagreement on the amount of provisioning that happens within a family and the general ability of hunters to control who receives the meat they bring in.

Risk-taking

Often invoked in costly signaling approaches to hunting, risk-taking has been suggested to result in honest signals of quality in other forms. As risk increases, so do the costs that come with failure. This results in greater costs for those who do not have qualities which allow for greater chances of success or the ability to buffer failure relative to those who possess such qualities. For this reason, risky behaviors may be often be honest signals, with individuals who lack the relevant traits being expected to avoid risk or suffer too much damage from failures to maintain risky behavior.

Many beneficial qualities have been suggested to underlie risk-taking behavior. For example, physical skill, good judgment, or bravery have all been argued to increase the chances of success in risky situations. Similarly, social dominance, confidence, and ambition may also help in competition among conspecifics, with social dominance, ambition, and wealth also potentially limiting the costs of failure.

In general, the targets of risky signals are often thought to be potential mates. This is primarily due to the finding that young males (who are the age and sex class with the highest reproductive variance) take more risks than any other group in both experiments and observational data. By undertaking risky endeavors, males are thought to signal the previously mentioned qualities which may be directly related to one’s ability to provision and protect one’s family. However, traits like bravery and physical prowess may also be valued by cooperative partners due to their benefits in group-hunting and warfare, thereby increasing the potential audience for risk takers.

Physical attractiveness

Physically attractive traits have also been hypothesized to be signals of mate quality, with facial characteristics, body type, voice characteristics, and body modification having all been suggested to provide information relevant to reproduction. However, most approaches focus on how the information is relevant to the receiver rather than whether the information takes the form of signals or cues, with the two possibilities often hard to distinguish between.

Although exceptions exist, costly signaling theory has mainly been incorporated into explanations for attractive male traits in a wide range of species. In humans, both low voice pitch and facial masculinity in males have been suggested to be honest indicators of male quality due to testosterone’s connection with facial and vocal cord development and its hypothesized role in mediating tradeoffs. From such perspectives, only high-quality males can afford to invest heavily in phenotypic qualities outside those needed for survival due to lower relative costs of such investment, with testosterone’s linking of these traits with facial and vocal characteristics preventing individuals from faking these signals. Additionally, low voice pitch may also be difficult to fake in the short-term due to activation of the autonomic nervous system, which controls fight-or-flight responses, altering voice pitch. For this reason, only individuals who are confident in their ability are likely ability can afford to maintain low levels of arousal, thereby potentially serving as an honest signal of formidability.

Regardless of whether the information comes from cues or signals, differences are expected in which information is valued by each sex. In general females are expected to be more sensitive to information about the ability of potential mates to acquire and defend resources, while males are expected to focus more on potential partners’ ability to conceive and take care of future children. Outside of these areas, both sexes are often suggested to benefit similarly in signaling pathogen resistance or a lack of harmful mutations due to their hypothesized importance over human evolutionary history.

Art

Art has also received attention as a costly signal of beneficial qualities relevant to sexual selection. If defined as environmental modification lacking adaptive functions outside of sexual selection, art or art-like behavior has been observed in spiders, crabs, fish, and birds in addition to humans. Unlike the art of other species, however, the form of human art is generally not considered to be genetically encoded. Instead, adaptationist approaches often involve the hypothesis that humans possess adaptations capable of resulting in a wide range of artwork as sexual signals and adaptations for correctly evaluating the information being signaled.

The costs of producing art are expected to increase with the quality of the piece and come in multiple forms. Creating art can require substantial amounts of time to learn the skills involved, find materials, and produce the work, all of which can prevent the individual from investing in other fitness enhancing tasks. The materials involved may also require substantial resources to obtain and production itself may be physically demanding or risky. Once created, works of art may also require defense against theft or sabotage from potential rivals.

Since these costs are relatively less impactful for those in good condition, producing art is thought to be an honest signal of one’s quality, with those in good condition being able to afford greater investment in art. For this reason, it may reliably signal information about one’s health, access to resources, or the relative absence of harmful mutations which might negatively impact one’s ability or overall condition. In instances where art needs to be defended, it may also signal one’s formidability and social power.

As a hypothesized form of sexual signaling, males are expected to benefit from using art to signal to larger audiences than females, with evidence of this seen in both humans and non-human animals. However, in humans, the potential for sex differences has been argued to not extend to artistic ability due to the commonality of long-term monogamous relationships resulting in the increased importance of mutual mate choice, something which favors females to invest more in sexual signals relative to other species.

Evidence consistent with art often involving sexual signals in humans primarily comes from studies examining mate preferences. For example, a study examining mating preferences in thirty-seven cultures found that being "creative and artistic" was the sixth most important trait to females and the seventh most important trait to males out of thirteen qualities regarded as attractive. Additionally, greater effort towards the creation public art has been associated with higher numbers of sexual partners among populations of both young adults and artists.

Courtship duration

Lengthy courtships have also been proposed to honestly signal one's overall quality, particularly in non-human animals. Although often accompanied by other signals, courtship duration on its own can create substantial opportunity costs as males cannot court other females at this time or invest in other fitness enhancing activities. For this reason, it may be an honest signal of overall quality due to the expectation that low-quality males will suffer more from opportunity costs per unit of time in courtship than high quality males, thereby favoring low quality males to drop out courtship sooner.

In humans, willingness to engage in lengthy courtships has also been suggested to signal desire for a long-term relationship as opposed to casual sex, with there being evidence that persistent courtship styles are more attractive for females seeking long-term relationships than those seeking shorter-term relationships.

Infant crying as a signal of vigor

In addition to potentially signaling need or being a means to manipulate parents, crying in human infants has been suggested to serve as a costly signal meant to decrease the child’s risk of infanticide, something which is seen across cultures.

Due to the fact that conflicts of interests exist between an offspring and both its parents and siblings, parents are expected to be sensitive to the quality of their offspring in determining how much investment to provide. As parental investment in one offspring cannot go to another, the potential exists for investment in a new child to reduce an individual’s fitness. This can happen when an offspring is unlikely to survive, thereby favoring investment in other areas. Additionally, such investment may still be costly with high likelihoods of survival if it puts the well-being of other siblings at risk. In these situations, older siblings are expected to be favored due to being closer to reproduction and the fact that they have already survived infancy which has higher mortality rates than later childhood.

Crying is proposed to help reduce one’s infanticide risk by establishing the perception of vigor in others. This is primarily thought to be possible due to the energy costs of crying making it costlier for infants in worse condition. For this reason, it may serve as a reliable indicator of what an infant can afford to spend, thereby making it an honest signal of quality. Additionally, the acoustic frequency of one's cries may also carry information about one's fitness prospects based on studies which have found correlations between cry pitch and various diseases.

Such an approach has been extended to the excessive crying of colic. However, crying’s connection to need has also been suggested to result in excessive crying being more likely to lead to reduced investment by making offspring appear in worse of condition.

Academic publishing

Although not necessarily a signal of the author’s qualities, the costs involved with academic publishing have been suggested to result in honest signaling about the quality of the journal article being submitted under certain conditions.

Academic publishing involves conflicts of interests between authors and journals, with authors benefiting from having articles accepted in high prestige journals regardless of quality and journals benefiting from publishing only articles that meet their standards. When the submission process involves little cost and no differential benefits, the optimal strategy for authors is likely to involve signaling that one’s work is higher quality than it is and submitting all publications to high-impact journals before submitting them to lower-impact journals, even when the probability of acceptance is low.

One way for honest signaling to arise in academic publishing is if the costs involved differ based on the quality of the paper. This is possible when submitting a low-quality paper to a high impact journal results in a lengthier peer review process, requires greater time to give the paper the appearance of being higher quality, or necessitates payments for resubmission. As these costs are experienced to a greater degree when submitting low-quality papers, their existence may favor honest communication and submission to journals that match the quality of the paper.

Costly signals of cooperative intent

Outside of mating contexts in which there is little to gain through the provisioning or care of offspring, a signal of one's high quality may often not be enough to result in beneficial treatment from others, even when it is honest. Instead, individuals are also expected to pay attention to the likelihood that they will receive benefits before cooperating with another individual. This makes signaling one's willingness to provide benefits to others an important part of establishing cooperative relationships, something which is seen in both observational and experimental studies which have found that individuals tend to prefer those who are generous but have less to give as cooperative partners than those who have the ability to provide benefits but often do not.

Public displays of generosity

Costly signaling has often been used in attempts to explain instances of public generosity in which individuals incur costs without any immediate benefits. Although often thought to signal one's ability to provide benefits, such behaviors have also been considered as honest signals of one’s willingness to cooperate due to the costs involved.

Food sharing

Food sharing is often reported to be a common occurrence in many small-scale societies, particularly with hunted game. Non-signaling explanations for this have focused on either the benefits of establishing reciprocal relationships with others to buffer risk or the limited benefits of maintaining control over food, due to either the effort required or spoilage in large game. However, neither may be mutually exclusive with signaling strategies due to the importance of reputation to cooperative relationships and the fact that sharing food that may not be worth defending still requires the effort to collect in the first place.

Due to its link to food production, food sharing may signal the qualities of the provider in instances when obtaining food results in differential costs based on one’s underlying traits. As with other signals of cooperative intent, it may also signal one's generosity, as such sharing is costlier for those who are likely to defect rather than gain from long-term cooperative relationships.

When seen as a signal of generosity, the type of information signaled is likely to depend on the form of sharing and who receives what. Sharing widely may signal one's intentions of future cooperation with one’s group, while more targeted examples constrained to only a subset of one's group can signal interest in forming cooperative relationships with individuals or coalitions within a group. Sharing may also be an effective signal of generosity to those not receiving benefits if it reflects a stable personality trait that varies among individuals.

Competitive feasting

Compared to the day to day sharing seen in small-scale societies, the staging of large feasts in which those holding them pay the majority of the costs may also demonstrate cooperative intent, with such practices being found among diverse groups. However, the fact that feasts tend to only happen at particular times of the year and involve competition between groups has been used to suggest that they may primarily be forms of conspicuous consumption meant to signal one's overall quality or status.

Blood donations

Costly signaling has also been suggested to explain blood donations. In the most common form, individuals give blood voluntary, while receiving no payment and having no control over who gets the donation. This results in a lack of obvious benefits for the donator who also incurs opportunity costs and the risk of mistakes and other negative outcomes, the threat of which may cause anxiety and other forms of psychological distress.

Unlike explanations involving direct reciprocity and kin selection which are suggested to be irrelevant to blood donations due to the lack of control over who receives the blood, signaling explanations allow for benefits to come from one’s ability to alter the perceptions of others in ways that benefit the signaler. This is proposed to involve increased perceptions of generosity and willingness to take risks in addition to providing reliable information about one’s health due to individuals with certain health conditions or diseases not being allowed to donate blood.

Indirect reciprocity

Costly signaling may also be involved in many forms of indirect reciprocity. Indirect reciprocity occurs when one’s seemingly altruistic acts increase one's reputation for cooperation, making others more likely to help regardless of if they were the target of the act. Based on game theoretic models, this can evolve in the absence of signaling through fixed strategies. However, in species with the flexibility to alter their level of cooperation in response to their own state and relevant social variables, past behaviors with others may not be enough on their own to reliably signal cooperative intent without the inclusion of other means to ensure the honesty of the signal. When this is the case and a species has the ability to both determine the likelihood others will cooperate and signal their own cooperative intent, costly signaling may be an important mechanism behind indirect reciprocity.

In humans, this has been proposed to take the form of individuals identifying potential targets of signals through the maintenance of welfare-tradeoff ratios and then employing costly signals to increase one’s perceived value as a cooperator to attractive targets for cooperation in the future.

Dyadic gift giving

Costly signals have also been suggested to be important for demonstrating commitment to both initiate and maintain dyadic relationships, with gift giving in particular receiving substantial attention as an individual strategy and as a custom.

Such approaches emphasize that the risk of defection from potential friends and romantic partners is particularly high at the start of relationships due to the amount of private information individuals have about their intentions to cooperate. Gifts are thought to help with this when the costs involved are large enough to not be worth providing by someone who does not value the potential for a long-term relationship. As the costs of the gift are thought to result in a reliable signal, almost any form of gift could signal future cooperative intent. However, gifts that do not increase the receiver’s fitness prospects may be favored, as those that result in material benefits for the receiver are likely to increase the risk of being manipulated by others. Similarly, the fact that gifts are often personalized, sex specific, or involve goods that degrade quickly has been suggested to reduce the likelihood that the receiver can benefit from regifting the item with other partners, thereby further reducing the risk of defection.

As a relationship develops, some models emphasize that the costs involved with gift giving should increase to signal greater levels of commitment. Assuming one’s partner reciprocates along the way, this is expected to result in costs that are greater than what would be expected from with a large favor when one is likely to be in need, the time when developed friendships are most vulnerable to defection.

Although the focus is often on signaling one’s desire for a long-term relationship, it is likely not the only quality being signaled. Instead, one’s ability to acquire resources may also be demonstrated in larger gifts. Additionally, individuals may also demonstrate one’s thoughtfulness and attentiveness to a partner by matching the gift to his or her preferences, something which has been proposed to be very difficult to fake.

Assuming other individuals in a population behave similarly, gift giving may also reduce the benefits of defection by making it costly to start new relationships, something which may be particularly likely when gift giving is largely dictated by customs that are inherently costly for those without the intent of future cooperation.

Ritual

Costly signaling approaches to ritual often emphasize the ability of ritual behavior to honestly signal commitment to one’s group due to the costs involved resulting in signals that are difficult to fake.

Religious rituals have received the most attention as potential costly signals. Like other forms of ritual, the costs involved come from the time, energy, material goods, or physical harm required for one to fit the ritual’s prescriptions, with extreme forms of self-harm not being uncommon. Although the costs of the ritual itself are likely to be equal among believers and nonbelievers, skeptics have been suggested to perceive rituals as more costly due to them not believing in the power of the ritual to achieve what believers expect of it. This difference in perception makes it less likely an individual will find belief worth faking, with costlier practices expected to provide greater indications of one’s commitment. Additionally, the commonality that religious rituals are often complex means that mistakes may be easy to spot throughout the ritual, further decreasing the likelihood of someone faking their commitment.

Evidence consistent with costly signaling explanations for religious ritual comes from both experimental and observational studies; however, few examinations exist on the topic. For example, members of religious kibbutzes have been shown to be more cooperative compared to secular kibbutzes in a common-pool resource game. Similarly, those engaging in communal religious rituals have been shown to have larger cooperative networks than those who did not participate. Other studies have attempted to more directly link the costs of signals to the effectiveness of cooperation, with one finding the number of costly requirements of a commune to be associated with longer commune lifespan and another finding that participation in and observation of a costly ritual was associated with larger donations compared to those involved with a less costly ritual.

Apology

In addition to attempts at creating cooperative relationships, the costly signaling model of apology suggests that costly signals may also be used as a way to restore cooperation after a transgression. Since the costs of honest and dishonest verbal apologies are identical for the individual apologizing and the costs of continued victimization may be severe for the target of the apology, it is unlikely that verbal apologies alone will often be enough to convey contrition. For this reason, costs may be an adaptive part of an apology, increasing the effectiveness of the apology so that the apologizer is more likely to remain in the cooperative venture.

For an apology to be effective, the model does not require costs to be tied to harm caused by the transgression. Instead, the signal only needs to be costly enough to outweigh the benefits a defector could gain in a one-time interaction, thereby creating a situation in which only those who are interested in future cooperation gain net benefits from the signal.

As honesty is established through costs, apologies consistent with the model can take many forms, with financial loss, self-harm, and the reduction of one’s status have all been documented to be associated with apologies to both other individuals and religious deities. Apologies may also include gifts or other benefits; however, the benefits themselves are not predicted to increase the honesty of the signal. Instead, they may simply be one way for the signaler to incur costs.

In addition to less costly forms, non-lethal suicide attempts have also been suggested to serve as honest apologies in some instances. Unlike other forms of costs, the costs of a suicide attempt primarily come from the probability of one’s death, with riskier attempts being seen as costlier. According to the costly apology model of suicide, such substantial costs may be required to honestly signal contrition when the potential payoff to future defection is large enough to still allow for deceivers to gain net benefits through less costly signals, something which may occur when highly valuable cooperative relationships are in threat of being ended. Suicide attempts may also increase the spread of the information from the signal due to their noteworthy nature, something which may be particularly important when the transgression was made against a group or puts cooperative relationships with those outside the aggrieved at risk.

Evidence for the costly signaling model of apology has mainly come from experiments. For example, multiple vignette studies have found that costly apologies increase the perception of sincerity by the target of the signal across different countries and religions, with the costs of gift giving and self-punishment both being effective. Similarly, participants in a study that had them imagine an accidental transgression in the past were more likely to report willingness to engage in a costly apology when an individual was more likely to be important to them. However, costly self-punishment was common in a study which forced participants to accidentally treat an anonymous partner unfairly, something which is consistent with the idea that apologies may also serve to maintain one’s reputation to a larger audience.

Infant-directed song

Infant-directed song has been suggested to be a costly signal of parental attentiveness, something which is thought to particularly important when infants are too young to walk or correctly avoid dangers in their environment.

Although parents experience fitness benefits from providing attention to infants and infants can gain fitness benefits from their parents spending time in other tasks, the optimal amount of resources devoted to this is expected to be an example of parent-offspring conflict, with infants benefiting from more attention than what is ideal for the parent. Due to this conflict of interest, infants are expected to be sensitive to information relating to parental attention and come equipped with adaptations help elicit it, something which is proposed to result in selection pressures on parents to better signal their attententiveness.

Infant-directed song is thought to help with this due to its production being costlier to make when the parent is focused on other aspects of its environment, thereby increasing the honesty of the signal. According to this hypothesis, the potential costs of infant-directed song can come in multiple non-exclusive forms. For example, singing may require investment in both planning and memory, while also potentially requiring the parent to attend to the infant’s emotional state and alter the song to match. It may also prevent one from doing physically demanding activities in instances that require specific breathing patterns.

Whatever form the costs take, the benefit to the parent is suggested to be quicker and more reliable satiation of infant demands which would then allow greater for investment in other areas.

Costly signals of wealth

As wealth influences one’s access to resources directly and by increasing the status of those who possess it, demonstrations of wealth have been hypothesized to have substantial benefits and often take the form of costly signals. Although wealth alone may be worth signaling, such signals are often suggested to display information about qualities relating to one’s ability to acquire and defend resources in the future. They may also signal generosity when this involves a charitable component; however, this benefit is often considered secondary.

Conspicuous consumption

One potential means for signaling wealth is conspicuous consumption. Conspicuous consumption refers to instances when individuals purchase luxury goods which provide little to no utility over less costly versions, thereby prioritizing self-presentation over economic efficiency. It is common across humans regardless of class and often involves strategic planning to maximize the audience of the display and the strength of the signal.

Most signaling explanations of conspicuous consumption predict the targets of the signal will predominately be potential mates. As with other signals relating to sexual selection, males are typically expected to invest more in these signals due to the potential for greater benefits through additional matings. In these instances, the information signaled is thought to go beyond genetic quality and signal the potential for investment, which can be attractive to those seeking both long-term and short-term mating strategies. Although often focused on males, females have also been suggested to benefit from conspicuous consumption in mating contexts due to its hypothesized ability to demonstrate the commitment of one’s partner and signal one’s mate quality to rivals, both of which may help in intrasexual competition and deter mate poaching.

Despite the focus on sexual selection, conspicuous consumption may also be useful for problems outside of acquiring mates. This can involve attempts at attracting other cooperative partners, who stand to gain from the signalers ability to confer benefits should they form an alliance. As in mating contexts, there may also be benefits to intimidating rivals, thereby decreasing the likelihood of direct competition for resources in the future.

Evidence consistent with conspicuous consumption being a costly signal of wealth and status comes from primarily from findings that females find males with more expensive items more desirable. This is mainly seen in experiments which have manipulated the costs of items associated with males, with cars and clothing typical of higher classes having been found to be associated with increased probabilities of females entering into various types of romantic and sexual relationships and greater perceptions of attractiveness across multiple studies.

Outside of its benefits, there has been much less research on whether conspicuous consumption meets the other requirements of being a signal, with it being possible that a mismatch exists between hypothesized adaptations for status signaling and modern environments which include marketing campaigns that might exploit such adaptations. However, its commonality across cultures and class boundaries have been used to argue that humans may be well suited to balancing the costs and benefits of the signal.

Public philanthropy

Extravagant charitable donations have also been suggested to honestly signal one's wealth due to large donations being impossible or costlier to make for those with fewer resources. As with conspicuous consumption, such signals are also often expected to provide information about one's underlying quality in addition to wealth, particularly relating to one's ability to acquire and maintain possession of resources.

Due to the qualities signaled and their public nature, public philanthropy has been suggested to mainly serve to attract new cooperators. For this reason, existing cooperators may view such signals as threats to their ongoing relationships, and put more weight on private signals to evaluate the cooperative intent of the signaler. Consistent with this reasoning, public displays of generosity may often decrease one's perceptions of cooperativeness or trustworthiness when they appear to be strategies meant to gain recognition or prestige.

Costly signals of need

In addition to signaling qualities meant to increase one’s attractiveness to potential mates or other cooperative partners, costly signals have also been suggested to result in honest displays of need. Primarily aimed at existing cooperators who would be motivated to help given genuine need on the part of the signaler, such signals are hypothesized to reduce doubt surrounding the severity of one’s situation in ways less costly signals could not.

Depression

Due in part to its costs, prevalence, and apparent ability for anyone to develop it, major depression has been hypothesized to often serve as a credible signal need. The bargaining model of depression suggests that throughout our evolutionary history individuals would have often faced instances of social adversity (e.g., abuse, the death of an important figure in one’s life, or the end of a romantic relationship) in which their fitness prospects depended primarily on responses from others. In these situations, providing social support could result in benefits for individuals who gain from cooperating with the depressed individual or otherwise benefit from their success. However, the costs involved with providing help and the threat of manipulation require reliable information before sufficient help is likely to be provided.

As with the other proposed costly signals, depression is proposed to achieve this due to the costs involved making the signal prohibitively costly to fake for those who are not in severe enough need. The costs of major depression primarily come through the reduction of interest and investment in one’s normal pattern of behavior. Although highly costly to those who are not in need, this does not require substantial costs on the part of an honest signaler. Instead, instances of severe enough adversity can result in a situation in which there is no difference in one’s fitness prospects in being depressed or not, with the costs still being substantial for those not actually in enough need.

In addition to serving as an honest signal of need, the bargaining model also emphasizes depression’s potential role as a bargaining tool. This is possible due to the reduction in behavior that often accompanies depression reducing the benefits the depressed individual provides to others. For this reason, many instances of depression are predicted to be analogous to a labor strike in that individuals who previously benefited from the depressed individual receive the message that they need to upregulate their support to once again gain from his or her cooperation.

Suicide attempts

A possible symptom of depression, suicide attempts have also been suggested to be credible signals of need and ways to bargain for increased social support. Unlike depression where the costs come from its prolonged symptoms, the costs of suicide attempts primarily come from the risk of death or serious harm, with riskier attempts creating stronger signals. Despite this difference, the costs of suicide attempts are thought to function similarly to the symptoms of depression in that they are relatively costly for those not in severe need, thereby discouraging those in relatively minor need from making attempts. As death eliminates the potential for investment in one's inclusive fitness, attempts related to bargaining are expected to balance the need for a hard to fake signal with the risk of death and result in attempts that involve non-negligible but relatively low probabilities of death, which is viewed as an unfortunate byproduct by these models.

Consistent with signaling approaches to suicide, attempters often experience social conflict and adversity before the attempt, with instances when one cannot resolve their situation through their own actions being found to be particularly strong risk factor in an examination of the Human Relations Area Files. Additionally, findings that non-lethal attempts are more common than lethal ones have been suggested to further support signaling approaches to suicide, with individuals often passing up more lethal options when riskier methods exist as is predicted by signaling approaches. However, few studies have examined the potential for attempt survivors to receive benefits.

Illness symptoms

Various types of conspicuous illness symptoms have also been suggested to serve as honest signals of need. Although much of one’s illness symptoms are likely to come in the form of cues resulting from one’s susceptibilities to a pathogen or byproducts of one's defenses against it, such approaches suggest they may also be upregulated in order to better signal need. As symptoms may be costly in terms of energy, opportunity costs, and reputation, it is expected to be costlier for potential fakers than those who are actually ill and experiencing symptoms already. For this reason, potential fakers are not expected to gain net fitness benefits from such displays, thus increasing the likelihood the targets of one’s signal will believe the individual to be ill and provide meaningful benefits that outweigh the costs of signaling.

Formulated as an explanation for placebo responses, the signaling theory of symptoms predicts that once the signaling function of upregulated symptoms is achieved and others provide support, symptoms will then be downregulated to a level appropriate for disease fighting signaling. In line with this, evidence for the ability to alter one’s symptom levels in response to the presence of conspecifics exists in many species, and placebo responses themselves tend to primarily occur after treatments an individual believe to be efficacious are given. Additionally, placebo responses are often sensitive to the demeanor and behaviors of the care provider, as would be expected with signaling approaches if care providers are seen as potential targets of the signal.

Crying

Compared to the other proposed signals of need, crying is the least controversial as having a signaling function. However, it has been argued that there is currently little evidence to distinguish it from a cue with a high degree of confidence, and relatively few signaling explanations involve the costs of crying and how this might lead to honest signaling.

Infant crying as a signal of need

The functions of crying are often thought to differ based on whether the crier is an infant or from another age class. In infants, signaling need for food, attention, and protection have been the most commonly proposed functions. As is the case with explanations of crying as a signal of vigor, the primary cost of infant crying is typically thought to be energetic, with such costs having the potential to result in a signal that is costlier to fake than produce when in honest need. This has been used to suggest that the frequency and duration of crying forms an important part of the signal; however, it has also been proposed that the costs underlying crying may also be connected to the sounds produced.

Despite the commonality of signaling explanations for infant crying, responses to infants can often be negative in addition to the positive responses predicted. In particular, negative responses to crying have been found to be associated with post-partum depression, anxiety, and high levels of neuroticism. However, not all responses are thought to be equally relevant to evaluating whether crying can be an adaptive signal, with negative emotional responses alone not being sufficient evidence of negative fitness outcomes due to the greater importance of behavioral responses.

Adult crying

Often expected to involve low costs compared to the other hypothesized costly signals of need, the potential costs of adult crying have been proposed to come from diverse areas. For example, crying has been shown to reduce one’s reputation and potentially lead to avoidance in Western societies. It may also be connected to lessened immune function based on studies reporting lower levels of salivary Immunoglobulin A in adult women following tears but not sadness alone. Tear production also impedes vision, reducing one’s ability to respond to threats in one’s environment. However, tears may also function to hide information by increasingly the difficulty of others to determine the direction of one’s gaze.

Consistent with signaling explanations, individuals have been shown to respond positively to those crying despite viewing them less favorably and experiencing more negative emotions, although negative responses are also reported. Additionally, individuals have been found to report feeling better after crying when social support is present, with crying alone tending to not improve one’s mood as would be predicted with a signaling hypothesis.

Moons of Saturn

From Wikipedia, the free encyclopedia
 
Artist's concepts of the Saturnian ring–moon system
A spherical yellow-brownish body (Saturn) can be seen on the left. It is viewed at an oblique angle with respect to its equatorial plane. Around Saturn there are rings and small ring moons. Further to the right large round moons are shown in order of their distance.
Saturn, its rings and major icy moons—from Mimas to Rhea
 
In the foreground there are six round fully illuminated bodies and some small irregular objects. A large half-illuminated body is shown in the background with circular cloud bands around the partially darkened north pole visible.
Images of several moons of Saturn. From left to right: Mimas, Enceladus, Tethys, Dione, Rhea; Titan in the background; Iapetus (top right) and irregularly shaped Hyperion (bottom right). Some small moons are also shown. All to scale.

The moons of Saturn are numerous and diverse, ranging from tiny moonlets only tens of meters across to enormous Titan, which is larger than the planet Mercury. Saturn has 83 moons with confirmed orbits that are not embedded in its rings—of which only 13 have diameters greater than 50 kilometers—as well as dense rings that contain millions of embedded moonlets and innumerable smaller ring particles. Seven Saturnian moons are large enough to have collapsed into a relaxed, ellipsoidal shape, though only one or two of those, Titan and possibly Rhea, are currently in hydrostatic equilibrium. Particularly notable among Saturn's moons are Titan, the second-largest moon in the Solar System (after Jupiter's Ganymede), with a nitrogen-rich Earth-like atmosphere and a landscape featuring dry river networks and hydrocarbon lakes, Enceladus, which emits jets of gas and dust from its south-polar region, and Iapetus, with its contrasting black and white hemispheres.

Twenty-four of Saturn's moons are regular satellites; they have prograde orbits not greatly inclined to Saturn's equatorial plane. They include the seven major satellites, four small moons that exist in a trojan orbit with larger moons, two mutually co-orbital moons and two moons that act as shepherds of Saturn's F Ring. Two other known regular satellites orbit within gaps in Saturn's rings. The relatively large Hyperion is locked in a resonance with Titan. The remaining regular moons orbit near the outer edge of the A Ring, within the G Ring and between the major moons Mimas and Enceladus. The regular satellites are traditionally named after Titans and Titanesses or other figures associated with the mythological Saturn.

The remaining fifty-nine, with mean diameters ranging from 4 to 213 km, are irregular satellites, whose orbits are much farther from Saturn, have high inclinations, and are mixed between prograde and retrograde. These moons are probably captured minor planets, or debris from the breakup of such bodies after they were captured, creating collisional families. The irregular satellites have been classified by their orbital characteristics into the Inuit, Norse, and Gallic groups, and their names are chosen from the corresponding mythologies, with two exceptions. One of these is Phoebe (part of the Norse group but named for a Greek Titaness), the ninth moon of Saturn and largest irregular, discovered at the end of the 19th century; the other is Bebhionn, which, though in the Gallic group, is named after an Irish goddess.

The rings of Saturn are made up of objects ranging in size from microscopic to moonlets hundreds of meters across, each in its own orbit around Saturn.[8] Thus a precise number of Saturnian moons cannot be given, because there is no objective boundary between the countless small anonymous objects that form Saturn's ring system and the larger objects that have been named as moons. Over 150 moonlets embedded in the rings have been detected by the disturbance they create in the surrounding ring material, though this is thought to be only a small sample of the total population of such objects.[9]

There are still 30 unnamed moons (as of November 2021), of which all but one is irregular. If named, they will receive names from Gallic, Norse and Inuit mythology based on the orbital groups of the moons.

Discovery

A large bright circle in the center is surrounded by small circles.
Saturn (overexposed) and the moons Iapetus, Titan, Dione, Hyperion, and Rhea viewed through a 12.5-inch telescope

Early observations

Before the advent of telescopic photography, eight moons of Saturn were discovered by direct observation using optical telescopes. Saturn's largest moon, Titan, was discovered in 1655 by Christiaan Huygens using a 57-millimeter (2.2 in) objective lens on a refracting telescope of his own design. Tethys, Dione, Rhea and Iapetus (the "Sidera Lodoicea") were discovered between 1671 and 1684 by Giovanni Domenico Cassini. Mimas and Enceladus were discovered in 1789 by William Herschel. Hyperion was discovered in 1848 by W. C. Bond, G. P. Bond and William Lassell.

The use of long-exposure photographic plates made possible the discovery of additional moons. The first to be discovered in this manner, Phoebe, was found in 1899 by W. H. Pickering. In 1966 the tenth satellite of Saturn was discovered by Audouin Dollfus, when the rings were observed edge-on near an equinox. It was later named Janus. A few years later it was realized that all observations of 1966 could only be explained if another satellite had been present and that it had an orbit similar to that of Janus. This object is now known as Epimetheus, the eleventh moon of Saturn. It shares the same orbit with Janus—the only known example of co-orbitals in the Solar System. In 1980, three additional Saturnian moons were discovered from the ground and later confirmed by the Voyager probes. They are trojan moons of Dione (Helene) and Tethys (Telesto and Calypso).

Observations by spacecraft

Circular complex rings of Saturn are seen at the low angle. The rings look like two grayish bands running parallel to each other from the left to right and connecting at the far right. Half illuminated Titan and Dione are visible slightly below the rings in the foreground. Two bright dots: one at the lower edge of rings and another above the rings can be seen. They are Prometheus and Telepso.
Four moons of Saturn can be seen on this image by the Cassini spacecraft: The larger Titan and Dione at the bottom, small Prometheus (under the rings) and small Telesto above center.
 
Five moons in another Cassini image: Rhea bisected in the far-right foreground, Mimas behind it, bright Enceladus above and beyond the rings, Pandora eclipsed by the F Ring, and Janus off to the left.

The study of the outer planets has since been revolutionized by the use of unmanned space probes. The arrival of the Voyager spacecraft at Saturn in 1980–1981 resulted in the discovery of three additional moons – Atlas, Prometheus and Pandora, bringing the total to 17. In addition, Epimetheus was confirmed as distinct from Janus. In 1990, Pan was discovered in archival Voyager images.

The Cassini mission, which arrived at Saturn in the summer of 2004, initially discovered three small inner moons including Methone and Pallene between Mimas and Enceladus as well as the second trojan moon of Dione – Polydeuces. It also observed three suspected but unconfirmed moons in the F Ring. In November 2004 Cassini scientists announced that the structure of Saturn's rings indicates the presence of several more moons orbiting within the rings, although only one, Daphnis, had been visually confirmed at the time. In 2007 Anthe was announced. In 2008 it was reported that Cassini observations of a depletion of energetic electrons in Saturn's magnetosphere near Rhea might be the signature of a tenuous ring system around Saturn's second largest moon. In March 2009, Aegaeon, a moonlet within the G Ring, was announced. In July of the same year, S/2009 S 1, the first moonlet within the B Ring, was observed. In April 2014, the possible beginning of a new moon, within the A Ring, was reported.

Outer moons

Quadruple Saturn–moon transit captured by the Hubble Space Telescope

Study of Saturn's moons has also been aided by advances in telescope instrumentation, primarily the introduction of digital charge-coupled devices which replaced photographic plates. For the 20th century, Phoebe stood alone among Saturn's known moons with its highly irregular orbit. Then in 2000, three dozen additional irregular moons have been discovered using ground-based telescopes. A survey starting in late 2000 and conducted using three medium-size telescopes found thirteen new moons orbiting Saturn at a great distance, in eccentric orbits, which are highly inclined to both the equator of Saturn and the ecliptic. They are probably fragments of larger bodies captured by Saturn's gravitational pull. In 2005, astronomers using the Mauna Kea Observatory announced the discovery of twelve more small outer moons, in 2006, astronomers using the Subaru 8.2 m telescope reported the discovery of nine more irregular moons, in April 2007, Tarqeq (S/2007 S 1) was announced and in May of the same year S/2007 S 2 and S/2007 S 3 were reported. In 2019, twenty new irregular satellites of Saturn were reported, resulting in Saturn overtaking Jupiter as the planet with the most known moons for the first time since 2000. Yet another was reported in 2021, after a survey for Saturnian moons took place in 2019.

Some of the 83 known satellites of Saturn are considered lost because they have not been observed since their discovery and hence their orbits are not known well enough to pinpoint their current locations. Work has been done to recover many of them in surveys from 2009 onwards, but four – S/2004 S 13, S/2004 S 17, S/2004 S 7, and S/2007 S 3 – still remain lost today.

The number of moons known for each of the four outer planets up to October 2019. Saturn currently has 83 known satellites.

Naming

The modern names for Saturnian moons were suggested by John Herschel in 1847. He proposed to name them after mythological figures associated with the Roman titan of time, Saturn (equated to the Greek Cronus). In particular, the then known seven satellites were named after Titans, Titanesses and Giants—brothers and sisters of Cronus. In 1848, Lassell proposed that the eighth satellite of Saturn be named Hyperion after another Titan. When in the 20th century the names of Titans were exhausted, the moons were named after different characters of the Greco-Roman mythology or giants from other mythologies. All the irregular moons (except Phoebe) are named after Inuit and Gallic gods and after Norse ice giants.

Some asteroids share the same names as moons of Saturn: 55 Pandora, 106 Dione, 577 Rhea, 1809 Prometheus, 1810 Epimetheus, and 4450 Pan. In addition, two more asteroids previously shared the names of Saturnian moons until spelling differences were made permanent by the International Astronomical Union (IAU): Calypso and asteroid 53 Kalypso; and Helene and asteroid 101 Helena.

Sizes

Saturn's satellite system is very lopsided: one moon, Titan, comprises more than 96% of the mass in orbit around the planet. The six other planemo (ellipsoidal) moons constitute roughly 4% of the mass, and the remaining 76 small moons, together with the rings, comprise only 0.04%.

The relative masses of Saturn's moons. Values are ×1021 kg. With Titan in the comparison (left), Mimas and Enceladus are invisible at this scale. Even excluding Titan (right), Phoebe, Hyperion, the smaller moons and the rings are still invisible.
 
Saturn's major satellites, compared to the Moon
Name
Diameter
(km)
Mass
(kg)
Orbital radius
(km)
Orbital period
(days)
Mimas 396
(12% Moon)
4×1019
(0.05% Moon)
185,539
(48% Moon)
0.9
(3% Moon)
Enceladus 504
(14% Moon)
1.1×1020
(0.2% Moon)
237,948
(62% Moon)
1.4
(5% Moon)
Tethys 1,062
(30% Moon)
6.2×1020
(0.8% Moon)
294,619
(77% Moon)
1.9
(7% Moon)
Dione 1,123
(32% Moon)
1.1×1021
(1.5% Moon)
377,396
(98% Moon)
2.7
(10% Moon)
Rhea 1,527
(44% Moon)
2.3×1021
(3% Moon)
527,108
(137% Moon)
4.5
(20% Moon)
Titan 5,149
(148% Moon)
(75% Mars)
1.35×1023
(180% Moon)
1,221,870
(318% Moon)
16
(60% Moon)
Iapetus 1,470
(42% Moon)
1.8×1021
(2.5% Moon)
3,560,820
(926% Moon)
79
(290% Moon)

Orbital groups

Although the boundaries may be somewhat vague, Saturn's moons can be divided into ten groups according to their orbital characteristics. Many of them, such as Pan and Daphnis, orbit within Saturn's ring system and have orbital periods only slightly longer than the planet's rotation period. The innermost moons and most regular satellites all have mean orbital inclinations ranging from less than a degree to about 1.5 degrees (except Iapetus, which has an inclination of 7.57 degrees) and small orbital eccentricities. On the other hand, irregular satellites in the outermost regions of Saturn's moon system, in particular the Norse group, have orbital radii of millions of kilometers and orbital periods lasting several years. The moons of the Norse group also orbit in the opposite direction to Saturn's rotation.

Ring moonlets

Saturn's F Ring along with the moons, Enceladus and Rhea
 
Sequence of Cassini images of Aegaeon embedded within the bright arc of Saturn's G Ring

During late July 2009, a moonlet, S/2009 S 1, was discovered in the B Ring, 480 km from the outer edge of the ring, by the shadow it cast. It is estimated to be 300 m in diameter. Unlike the A Ring moonlets (see below), it does not induce a 'propeller' feature, probably due to the density of the B Ring.

In 2006, four tiny moonlets were found in Cassini images of the A Ring. Before this discovery only two larger moons had been known within gaps in the A Ring: Pan and Daphnis. These are large enough to clear continuous gaps in the ring. In contrast, a moonlet is only massive enough to clear two small—about 10 km across—partial gaps in the immediate vicinity of the moonlet itself creating a structure shaped like an airplane propeller. The moonlets themselves are tiny, ranging from about 40 to 500 meters in diameter, and are too small to be seen directly.

Possible beginning of a new moon of Saturn imaged on 15 April 2014

In 2007, the discovery of 150 more moonlets revealed that they (with the exception of two that have been seen outside the Encke gap) are confined to three narrow bands in the A Ring between 126,750 and 132,000 km from Saturn's center. Each band is about a thousand kilometers wide, which is less than 1% the width of Saturn's rings. This region is relatively free from the disturbances caused by resonances with larger satellites, although other areas of the A Ring without disturbances are apparently free of moonlets. The moonlets were probably formed from the breakup of a larger satellite. It is estimated that the A Ring contains 7,000–8,000 propellers larger than 0.8 km in size and millions larger than 0.25 km. In April 2014, NASA scientists reported the possible consolidation of a new moon within the A Ring, implying that Saturn's present moons may have formed in a similar process in the past when Saturn's ring system was much more massive.

Similar moonlets may reside in the F Ring. There, "jets" of material may be due to collisions, initiated by perturbations from the nearby small moon Prometheus, of these moonlets with the core of the F Ring. One of the largest F Ring moonlets may be the as-yet unconfirmed object S/2004 S 6. The F Ring also contains transient "fans" which are thought to result from even smaller moonlets, about 1 km in diameter, orbiting near the F Ring core.

One of the recently discovered moons, Aegaeon, resides within the bright arc of G Ring and is trapped in the 7:6 mean-motion resonance with Mimas. This means that it makes exactly seven revolutions around Saturn while Mimas makes exactly six. The moon is the largest among the population of bodies that are sources of dust in this ring.

Ring shepherds

Shepherd moon Daphnis in the Keeler gap
 
Shepherd moons Atlas, Daphnis and Pan (enhanced color). They bear distinct equatorial ridges that appear to have formed from material accreted from Saturn's rings.

Shepherd satellites are small moons that orbit within, or just beyond, a planet's ring system. They have the effect of sculpting the rings: giving them sharp edges, and creating gaps between them. Saturn's shepherd moons are Pan (Encke gap), Daphnis (Keeler gap), Atlas (A Ring), Prometheus (F Ring) and Pandora (F Ring). These moons together with co-orbitals (see below) probably formed as a result of accretion of the friable ring material on preexisting denser cores. The cores with sizes from one-third to one-half the present-day moons may be themselves collisional shards formed when a parental satellite of the rings disintegrated.

Co-orbitals

Janus and Epimetheus are called co-orbital moons. They are of roughly equal size, with Janus being slightly larger than Epimetheus. Janus and Epimetheus have orbits with only a few kilometers difference in semi-major axis, close enough that they would collide if they attempted to pass each other. Instead of colliding, their gravitational interaction causes them to swap orbits every four years.

Inner large

A circular part of a grayish surface, which is intersected from the top-left to the bottom-right by four wide sinuous groves. Smaller and shorter grooves can be seen between them running either parallel to the large grooves or criss-crossing them. There is a rough terrain in the top-left corner.
South pole map of tiger stripes on Enceladus
 
Saturn's moons from bottom to top: Mimas, Enceladus, and Tethys
 
Tethys and the rings of Saturn
 
Color view of Dione in front of Saturn

The innermost large moons of Saturn orbit within its tenuous E Ring, along with three smaller moons of the Alkyonides group.

  • Mimas is the smallest and least massive of the inner round moons, although its mass is sufficient to alter the orbit of Methone. It is noticeably ovoid-shaped, having been made shorter at the poles and longer at the equator (by about 20 km) by the effects of Saturn's gravity. Mimas has a large impact crater one-third its diameter, Herschel, situated on its leading hemisphere. Mimas has no known past or present geologic activity, and its surface is dominated by impact craters. The only tectonic features known are a few arcuate and linear troughs, which probably formed when Mimas was shattered by the Herschel impact.
  • Enceladus is one of the smallest of Saturn's moons that is spherical in shape—only Mimas is smaller—yet is the only small Saturnian moon that is currently endogenously active, and the smallest known body in the Solar System that is geologically active today. Its surface is morphologically diverse; it includes ancient heavily cratered terrain as well as younger smooth areas with few impact craters. Many plains on Enceladus are fractured and intersected by systems of lineaments. The area around its south pole was found by Cassini to be unusually warm and cut by a system of fractures about 130 km long called "tiger stripes", some of which emit jets of water vapor and dust. These jets form a large plume off its south pole, which replenishes Saturn's E ring and serves as the main source of ions in the magnetosphere of Saturn. The gas and dust are released with a rate of more than 100 kg/s. Enceladus may have liquid water underneath the south-polar surface. The source of the energy for this cryovolcanism is thought to be a 2:1 mean-motion resonance with Dione. The pure ice on the surface makes Enceladus one of the brightest known objects in the Solar System—its geometrical albedo is more than 140%.
  • Tethys is the third largest of Saturn's inner moons. Its most prominent features are a large (400 km diameter) impact crater named Odysseus on its leading hemisphere and a vast canyon system named Ithaca Chasma extending at least 270° around Tethys. The Ithaca Chasma is concentric with Odysseus, and these two features may be related. Tethys appears to have no current geological activity. A heavily cratered hilly terrain occupies the majority of its surface, while a smaller and smoother plains region lies on the hemisphere opposite to that of Odysseus. The plains contain fewer craters and are apparently younger. A sharp boundary separates them from the cratered terrain. There is also a system of extensional troughs radiating away from Odysseus. The density of Tethys (0.985 g/cm3) is less than that of water, indicating that it is made mainly of water ice with only a small fraction of rock.
  • Dione is the second-largest inner moon of Saturn. It has a higher density than the geologically dead Rhea, the largest inner moon, but lower than that of active Enceladus. While the majority of Dione's surface is heavily cratered old terrain, this moon is also covered with an extensive network of troughs and lineaments, indicating that in the past it had global tectonic activity. The troughs and lineaments are especially prominent on the trailing hemisphere, where several intersecting sets of fractures form what is called "wispy terrain". The cratered plains have a few large impact craters reaching 250 km in diameter. Smooth plains with low impact-crater counts are also present on a small fraction of its surface. They were probably tectonically resurfaced relatively later in the geological history of Dione. At two locations within smooth plains strange landforms (depressions) resembling oblong impact craters have been identified, both of which lie at the centers of radiating networks of cracks and troughs; these features may be cryovolcanic in origin. Dione may be geologically active even now, although on a scale much smaller than the cryovolcanism of Enceladus. This follows from Cassini magnetic measurements that show Dione is a net source of plasma in the magnetosphere of Saturn, much like Enceladus.

Alkyonides

Three small moons orbit between Mimas and Enceladus: Methone, Anthe, and Pallene. Named after the Alkyonides of Greek mythology, they are some of the smallest moons in the Saturn system. Anthe and Methone have very faint ring arcs along their orbits, whereas Pallene has a faint complete ring. Of these three moons, only Methone has been photographed at close range, showing it to be egg-shaped with very few or no craters.

Trojan

Trojan moons are a unique feature only known from the Saturnian system. A trojan body orbits at either the leading L4 or trailing L5 Lagrange point of a much larger object, such as a large moon or planet. Tethys has two trojan moons, Telesto (leading) and Calypso (trailing), and Dione also has two, Helene (leading) and Polydeuces (trailing). Helene is by far the largest trojan moon, while Polydeuces is the smallest and has the most chaotic orbit. These moons are coated with dusty material that has smoothed out their surfaces.

Outer large

A spherical body is almost fully illuminated. Its grayish surface is covered by numerous circular craters. The terminator is located near the upper-right limb. A large crater can be seen near the limb in the upper-left part of the body. Another smaller bright crater can be seen in the center. It is surrounded by a large bright patch having the shape of a five-pointed star.
Inktomi or "The Splat", a relatively young crater with prominent butterfly-shaped ejecta on Rhea's leading hemisphere
 
Titan in front of Dione and the rings of Saturn
 
An irregularly-shaped and heavily cratered body, pock-marked with dark pits and ridges on its tan-colored icy surface.
Cassini image of Hyperion
 
A part of a spherical body illuminated from the above and behind. The convex limb runs from the lower-left to the upper-right corner. The black outer space is in the upper-left corner. The terminator is near the bottom. The surface of the body is covered with numerous craters. A large ridge runs in the center from the top to bottom.
Equatorial ridge on Iapetus

These moons all orbit beyond the E Ring. They are:

  • Rhea is the second-largest of Saturn's moons. It is even slightly larger than Oberon, the second-largest moon of Uranus. In 2005 Cassini detected a depletion of electrons in the plasma wake of Rhea, which forms when the co-rotating plasma of Saturn's magnetosphere is absorbed by the moon. The depletion was hypothesized to be caused by the presence of dust-sized particles concentrated in a few faint equatorial rings. Such a ring system would make Rhea the only moon in the Solar System known to have rings. Subsequent targeted observations of the putative ring plane from several angles by Cassini's narrow-angle camera turned up no evidence of the expected ring material, leaving the origin of the plasma observations unresolved. Otherwise Rhea has rather a typical heavily cratered surface, with the exceptions of a few large Dione-type fractures (wispy terrain) on the trailing hemisphere and a very faint "line" of material at the equator that may have been deposited by material deorbiting from present or former rings. Rhea also has two very large impact basins on its anti-Saturnian hemisphere, which are about 400 and 500 km across. The first, Tirawa, is roughly comparable to the Odysseus basin on Tethys. There is also a 48 km-diameter impact crater called Inktomi at 112°W that is prominent because of an extended system of bright rays, which may be one of the youngest craters on the inner moons of Saturn. No evidence of any endogenic activity has been discovered on the surface of Rhea.
  • Titan, at 5,149 km diameter, is the second largest moon in the Solar System and Saturn's largest. Out of all the large moons, Titan is the only one with a dense (surface pressure of 1.5 atm), cold atmosphere, primarily made of nitrogen with a small fraction of methane. The dense atmosphere frequently produces bright white convective clouds, especially over the south pole region. On June 6, 2013, scientists at the IAA-CSIC reported the detection of polycyclic aromatic hydrocarbons in the upper atmosphere of Titan. On June 23, 2014, NASA claimed to have strong evidence that nitrogen in the atmosphere of Titan came from materials in the Oort cloud, associated with comets, and not from the materials that formed Saturn in earlier times. The surface of Titan, which is difficult to observe due to persistent atmospheric haze, shows only a few impact craters and is probably very young. It contains a pattern of light and dark regions, flow channels and possibly cryovolcanos. Some dark regions are covered by longitudinal dune fields shaped by tidal winds, where sand is made of frozen water or hydrocarbons. Titan is the only body in the Solar System beside Earth with bodies of liquid on its surface, in the form of methane–ethane lakes in Titan's north and south polar regions. The largest lake, Kraken Mare, is larger than the Caspian Sea. Like Europa and Ganymede, it is believed that Titan has a subsurface ocean made of water mixed with ammonia, which can erupt to the surface of the moon and lead to cryovolcanism. On July 2, 2014, NASA reported the ocean inside Titan may be "as salty as the Earth's Dead Sea".
  • Hyperion is Titan's nearest neighbor in the Saturn system. The two moons are locked in a 4:3 mean-motion resonance with each other, meaning that while Titan makes four revolutions around Saturn, Hyperion makes exactly three. With an average diameter of about 270 km, Hyperion is smaller and lighter than Mimas. It has an extremely irregular shape, and a very odd, tan-colored icy surface resembling a sponge, though its interior may be partially porous as well. The average density of about 0.55 g/cm3 indicates that the porosity exceeds 40% even assuming it has a purely icy composition. The surface of Hyperion is covered with numerous impact craters—those with diameters 2–10 km are especially abundant. It is the only moon besides the small moons of Pluto known to have a chaotic rotation, which means Hyperion has no well-defined poles or equator. While on short timescales the satellite approximately rotates around its long axis at a rate of 72–75° per day, on longer timescales its axis of rotation (spin vector) wanders chaotically across the sky. This makes the rotational behavior of Hyperion essentially unpredictable.
  • Iapetus is the third-largest of Saturn's moons. Orbiting the planet at 3.5 million km, it is by far the most distant of Saturn's large moons, and also has the largest orbital inclination, at 15.47°. Iapetus has long been known for its unusual two-toned surface; its leading hemisphere is pitch-black and its trailing hemisphere is almost as bright as fresh snow. Cassini images showed that the dark material is confined to a large near-equatorial area on the leading hemisphere called Cassini Regio, which extends approximately from 40°N to 40°S. The pole regions of Iapetus are as bright as its trailing hemisphere. Cassini also discovered a 20 km tall equatorial ridge, which spans nearly the moon's entire equator. Otherwise both dark and bright surfaces of Iapetus are old and heavily cratered. The images revealed at least four large impact basins with diameters from 380 to 550 km and numerous smaller impact craters. No evidence of any endogenic activity has been discovered. A clue to the origin of the dark material covering part of Iapetus's starkly dichromatic surface may have been found in 2009, when NASA's Spitzer Space Telescope discovered a vast, nearly invisible disk around Saturn, just inside the orbit of the moon Phoebe – the Phoebe ring. Scientists believe that the disk originates from dust and ice particles kicked up by impacts on Phoebe. Because the disk particles, like Phoebe itself, orbit in the opposite direction to Iapetus, Iapetus collides with them as they drift in the direction of Saturn, darkening its leading hemisphere slightly. Once a difference in albedo, and hence in average temperature, was established between different regions of Iapetus, a thermal runaway process of water ice sublimation from warmer regions and deposition of water vapor onto colder regions ensued. Iapetus's present two-toned appearance results from the contrast between the bright, primarily ice-coated areas and regions of dark lag, the residue left behind after the loss of surface ice.

Irregular

Diagram illustrating the orbits of the irregular satellites of Saturn. The inclination and semi-major axis are represented on the Y and X-axis, respectively. The eccentricity of the orbits is shown by the segments extending from the pericenter to apocenter. The satellites with positive inclinations are prograde, those with negative are retrograde. The X-axis is labeled in km. The prograde Inuit and Gallic groups and the retrograde Norse group are identified.
 
Orbits and positions of Saturn's irregular moons as of 1 January 2021. Prograde orbits are colored blue while retrograde orbits are colored red.

Irregular moons are small satellites with large-radii, inclined, and frequently retrograde orbits, believed to have been acquired by the parent planet through a capture process. They often occur as collisional families or groups. The precise size as well as albedo of the irregular moons are not known for sure because the moons are very small to be resolved by a telescope, although the latter is usually assumed to be quite low—around 6% (albedo of Phoebe) or less. The irregulars generally have featureless visible and near infrared spectra dominated by water absorption bands. They are neutral or moderately red in color—similar to C-type, P-type, or D-type asteroids, though they are much less red than Kuiper belt objects.

Inuit

The Inuit group includes eight prograde outer moons that are similar enough in their distances from the planet (186–297 radii of Saturn), their orbital inclinations (45–50°) and their colors that they can be considered a group. The moons are Ijiraq, Kiviuq, Paaliaq, Siarnaq, and Tarqeq, along with three unnamed moons Saturn LX, S/2004 S 31, and S/2019 S 1. The largest among them is Siarnaq with an estimated size of about 40 km.

Gallic

The Gallic group are four prograde outer moons that are similar enough in their distance from the planet (207–302 radii of Saturn), their orbital inclination (35–40°) and their color that they can be considered a group. They are Albiorix, Bebhionn, Erriapus, and Tarvos. The largest among these moons is Albiorix with an estimated size of about 32 km. There is an additional satellite S/2004 S 24 that could belong to this group, but more observations are needed to confirm or disprove its categorization. S/2004 S 24 has the most distant prograde orbit of Saturn's known satellites.

Norse

The Norse (or Phoebe) group consists of 46 retrograde outer moons. They are Aegir, Bergelmir, Bestla, Farbauti, Fenrir, Fornjot, Greip, Hati, Hyrrokkin, Jarnsaxa, Kari, Loge, Mundilfari, Narvi, Phoebe, Skathi, Skoll, Surtur, Suttungr, Thrymr, Ymir, and twenty-five unnamed satellites. After Phoebe, Ymir is the largest of the known retrograde irregular moons, with an estimated diameter of only 18 km. The Norse group may itself consist of several smaller subgroups.

  • Phoebe, at 213±1.4 km in diameter, is by far the largest of Saturn's irregular satellites. It has a retrograde orbit and rotates on its axis every 9.3 hours. Phoebe was the first moon of Saturn to be studied in detail by Cassini, in June 2004; during this encounter Cassini was able to map nearly 90% of the moon's surface. Phoebe has a nearly spherical shape and a relatively high density of about 1.6 g/cm3. Cassini images revealed a dark surface scarred by numerous impacts—there are about 130 craters with diameters exceeding 10 km. Spectroscopic measurement showed that the surface is made of water ice, carbon dioxide, phyllosilicates, organics and possibly iron bearing minerals. Phoebe is believed to be a captured centaur that originated in the Kuiper belt. It also serves as a source of material for the largest known ring of Saturn, which darkens the leading hemisphere of Iapetus (see above).

List

Orbital diagram of the orbital inclination and orbital distances for Saturn's rings and moon system at various scales. Notable moons, moon groups, and rings are individually labeled. Open the image for full resolution.

Hypothetical

Two moons were claimed to be discovered by different astronomers but never seen again. Both moons were said to orbit between Titan and Hyperion.

  • Chiron which was supposedly sighted by Hermann Goldschmidt in 1861, but never observed by anyone else.
  • Themis was allegedly discovered in 1905 by astronomer William Pickering, but never seen again. Nevertheless, it was included in numerous almanacs and astronomy books until the 1960s.

Temporary

Much like Jupiter, asteroids and comets will infrequently make close approaches to Saturn, even more infrequently becoming captured into orbit of the planet. The comet P/2020 F1 (Leonard) is calculated to have made a close approach of 978000±65000 km (608000±40000 mi to Saturn on 8 May 1936, closer than the orbit of Titan to the planet, with an orbital eccentricity of only 1.098±0.007. The comet may have been orbiting Saturn prior to this as a temporary satellite, but difficulty modelling the non-gravitational forces makes whether or not it was indeed a temporary satellite uncertain.

Other comets and asteroids may have temporarily orbited Saturn at some point, but none are presently known to have.

Formation

It is thought that the Saturnian system of Titan, mid-sized moons, and rings developed from a set-up closer to the Galilean moons of Jupiter, though the details are unclear. It has been proposed either that a second Titan-sized moon broke up, producing the rings and inner mid-sized moons, or that two large moons fused to form Titan, with the collision scattering icy debris that formed the mid-sized moons. On June 23, 2014, NASA claimed to have strong evidence that nitrogen in the atmosphere of Titan came from materials in the Oort cloud, associated with comets, and not from the materials that formed Saturn in earlier times. Studies based on Enceladus's tidal-based geologic activity and the lack of evidence of extensive past resonances in Tethys, Dione, and Rhea's orbits suggest that the moons up to and including Rhea may be only 100 million years old.

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