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Historically, marriages in most societies were arranged by parents and older relatives with the goal not being love but legacy and "economic stability and political alliances", according to anthropologists . [5] Accordingly, there was little need for a temporary trial period such as dating before a permanent community-recognized union was formed between a man and a woman. While pair-bonds of varying forms were recognized by most societies as acceptable social arrangements, marriage was reserved for heterosexual pairings and had a transactional nature, where wives were in many cases a form of property being exchanged between father and husband, and who would have to serve the function of reproduction. Communities exerted pressure on people to form pair-bonds in places such as Europe ; in China , society "demanded people get married before having a sexual relationship" [6] and many societies found that some formally recognized bond between a man and a woman was the best way of rearing and educating children as well as helping to avoid conflicts and misunderstandings regarding competition for mates.

Neptune revolves around the Sun in its distant orbit once in about 165 years. Uranus completes its orbital revolution in 84 years, Jupiter in 12 years, Mars in about 15 months, Venus in 11 months, and Mercury in 18 weeks. If you imagine these bodies to be revolving in a plane around the Sun and yourself to be standing within the Sun, the motions of these bodies will appear almost uniform and always in one direction. Were the orbits of the planets circular and the Sun holding the centre of the circle, their motions would be constant, that is to say, always in the same direction and at the same rate. But the orbits are elliptical, and the Sun holds a position in one of the foci of each [Pg 18] ellipse. Consequently the planets are at times further from the Sun than at others, and they are then said to be in their aphelion, the opposite point of the orbit where they are nearest to the Sun being called the perihelion. When at aphelion the planets move slower, and when at perihelion they move quicker than at the mean distance. Astronomers employ an imaginary circular orbit for the planets, in which they move at an uniform rate of velocity, which is called the mean motion. This is subject to an equation depending on the position of the planet in its orbit, and it determines the difference between the imaginary planet and the true planet. The equation itself depends on the eccentricity of the orbit, that is to say, its relation to a circle drawn around the same focal centre. The Earth follows the same laws as all other bodies of the same system.


Ignore list matchmaking

Ignore list matchmaking