The Solar System




At present the Solar System is officially comprised of a star (the Sun), eight "planets" (Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus and Neptune), five newly classified "dwarf planets" (Ceres, Pluto, Haumea, Makemake and Eris [1] the latter four of which are also designated as "plutoids") [2] and numerous attendant satellites and assorted debris such as asteroids, comets, dust and meteors.

Intelligent life within the Solar System appears to be limited to Earth (at least insofar as visual data of the other planets and a lack of electromagnetic emissions is concerned), this is not to say that there isn’t life, only that a technological civilization isn’t in evidence. Whether there is bacteria on Mars, porpoise like creatures in the oceans beneath a layer of ice on the Galilean moon Europa or giant gas bags floating in the outer layers of Jupiter’s atmosphere is yet to be determined.

The Milky Way galaxy is an immense area 100,000 light years in diameter; the Solar System lies about 28,000 light years from it's center; our Sun a yellow star about halfway through its main-sequence (a period of relative stability) is somewhat commonplace.

We are, however, the focal point of an expanding globe of electromagnetic radiation that signals our presence (though if we continue to switch from powerful transmitters to cable and satellites we will eventually become "radio quiet" and difficult to detect), and we listen with giant radio telescopes for a reply but as yet nothing. Are we alone or perhaps a backwater surrounded by advanced life forms communicating with each other in ways we have yet to fathom? It is possible that we are playing tom-toms while they are watching high definition television.

[1] Passed August 24, 2006, by the International Astronomical Union:

The IAU . . . resolves that planets and other bodies, except satellites, in our Solar System be defined into three distinct categories in the following way:
(1) A "planet" is a celestial body that (a) is in orbit around the Sun, (b) has sufficient mass for its self-gravity to overcome rigid body forces so that it assumes a hydrostatic equilibrium (nearly round shape) and (c) has cleared the neighborhood around its orbit.
(2) A "dwarf planet" is a celestial body that (a) is in orbit around the Sun, (b) has sufficient mass for its self-gravity to overcome rigid body forces so that it assumes a hydrostatic equilibrium (nearly round shape), (c) has not cleared the neighborhood around its orbit and (d) is not a satellite.
(3) All other objects, except satellites, orbiting the Sun shall be referred to collectively as "Small Solar System Bodies."

[2] Formally announced June 11, 2008, by the International Astronomical Union:

"Plutoids" are celestial bodies in orbit around the Sun at a semi-major axis greater than that of Neptune
(trans-Neptunian) that have sufficient mass for their self-gravity to overcome rigid body forces so that they assume a hydrostatic equilibrium (nearly round shape) but have not yet cleared the neighborhood around their orbit. (At present only Pluto, Haumea, Makemake and Eris fill all these requirements, Ceres does not.) Satellites of plutoids are not plutoids themselves.




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