Planet: Difference between revisions
imported>Derek Harkness (More wikification) |
imported>Bruno L'Astorina No edit summary |
||
| Line 1: | Line 1: | ||
{{Subpages}} | {{Subpages}} | ||
According to [[International Astronomical Union]] (IAU), a '''planet''' is a celestial body [[orbit]]ing a [[star]] or [[Stellar evolution#Stellar remnants|stellar remnant]] that is massive enough to be rounded by its own [[gravity]] (but not massive enough to cause [[thermonuclear fusion]] in its inner core), and has [[cleared the neighbourhood|cleared its neighbouring region]] of [[planetesimal]]s. <ref name=IAU>{{ cite web | title = IAU 2006 General Assembly: Result of the IAU Resolution votes | url = http://www.iau2006.org/mirror/www.iau.org/iau0603/index.html | year = 2006 | accessdate = 2007-04-30 }}</ref> <ref name=WSGESP>{{ cite web |year = 2001 | title = Working Group on Extrasolar Planets (WGESP) of the International Astronomical Union | work = IAU | url = http://www.dtm.ciw.edu/boss/definition.html | accessdate = 2006-05-25 }}</ref> There are 8 bodies in the universe obeying this definition: [[Mercury]], [[Venus]], [[Earth]], [[Mars]], [[Jupiter]], [[Saturn]], [[Uran]] and [[Neptune]]. | |||
Again, according to that definition, bodies that don't obey the third condition, that is, orbiting the [[Sun]], rounded by its own gravity but not cleared the neighbourhood, is called '''[[dwarf planet]]'''. One of them is [[Pluto]], which is former considered as a planet. Other bodies that orbiting the Sun are generically called '''[[Small bodies of Solar System]]'''. | |||
Another related term is '''[[exoplanet]]'''. Although there are no official defition for this term, it is often used to indicate bodies analogue to the planets, but that orbites other [[star]]s that not the Sun.<ref name=exoplanet>{{ cite web |url = http://exoplanets.org/}}</ref> | |||
==The Planets== | |||
The planets can be subdivided into two main groups. The inner 4 terrestrial planets have a rocky composition. They are relatively small in size. The outer 4 planets are known as Gas Giants and have a thick gaseous atmospheres. Some physical information is followed: | |||
{| class="wikitable" | {| class="wikitable" | ||
|- | |- | ||
| Line 56: | Line 67: | ||
| 1.0247e26 kg | | 1.0247e26 kg | ||
| 1846 | | 1846 | ||
|} | |} | ||
The planets | ==Etimology and History== | ||
The word "planet" came from the greek πλανήτ- (''planēt-''), meaning "wanderers". There was, then, seven planets in the Sky, each one dedicated to a greek deitiy: | |||
*''Phainon'', the shiner, dedicated to [[Cronus]]; | |||
*''Phaethon'', brighter the first and below it, dedicated to [[Zeus]]; | |||
*''Pyroeis'', "fiery", the red one, dedicated to [[Ares]]; | |||
*''Phosphoros'', "light bringer", the brightest one, dedicated to [[Aphrodite]]; | |||
*''Stilbon'', the gleamer, dedicated to [[Hermes]]; <ref name=planet_greek_names>{{cite book|title=The History and Practice of Ancient Astronomy|author=James Evans|publisher=Oxford University Press|year=1998|pages=296-7}}</ref> | |||
added by our [[Sun]] and [[Moon]], the bigest wanderers in the sky. Later, n the time of the [[philosophy|philosophers]], many models of universe was created, which the most famous for us is the [[Aristotelian universe | Aristotle's one]]. In his system, the planets belong each one to one cristaline sphere, concentric to the others. Inner the seven planet's sphere stay the material shperes (''grosso modo'', the Earth); Outer them, the ''shpere of fixed stars''. | |||
In [[Roman Empire]], the planets became knowed directly by the name of the associated deity - not the greek one, bet the latin correspondent god. So, ''Phainon'' became ''Saturnus''; ''Phaethon'' was called ''Jupiter''; ''Pyroeis'' was ''Mars''; ''Phosphoros'', ''Venus'' and ''Stilbon'' was turned to ''Mercurius''. In [[medieval era]], the future european people has herited the roman culture, and so these latinized version of planet's names remain in the vocabulary until present days. Also in latinian tratition (followed by the germanic one) the seven days of the [[week]] have the names of the seven planets. | |||
After the [[Copernican Revolution]], however, the idea of planet has changed: they are all the bodies that round the Sun - that therefore would be considered just a [[star]] like any other from the firmament. The [[Earth]] then turn into a planet, the [[Moon]] became an Earth's [[sattelite]], and the so-called "Solar System" have then six planets. Later, three new bodies, that can't be seen with [[naked eye]] are baptized as a planet, following the latin-named tradition: ''Uranus'', ''Neptunus'' and ''Pluto''. | |||
But many other small bodies are saying to orbit the Sun, such as the brights [[comets]] and the palid [[asteroid]]s. The crisis in definition starts in 1980's and 1990's, when many bodies so big as - or, in few cases, bigger - Pluto start to be discovered above Neptune's orbit. Called [[Transneptunian objects]], they opened the discussion about what could be a good and precise definition of planet. The discussion ends in August 24, 2006, when [[International Astronomical Union | IAU]] voted the Resolution that defines officially the term. <ref name=IAU>{{ cite web | title = IAU 2006 General Assembly: Result of the IAU Resolution votes | url = http://www.iau2006.org/mirror/www.iau.org/iau0603/index.html | year = 2006 | accessdate = 2007-04-30 }}</ref> | |||
==Physical Formation== | |||
Planets are believed to form form a the disk of dust that surrounds a newly formed star. Gravitation forces pull the dust into lumps. The lumps gradually collide and join to make larger lumps or [[asteroid]]s. These join further to make larger and larger planets until the planet has cleared it's orbit of objects. | Planets are believed to form form a the disk of dust that surrounds a newly formed star. Gravitation forces pull the dust into lumps. The lumps gradually collide and join to make larger lumps or [[asteroid]]s. These join further to make larger and larger planets until the planet has cleared it's orbit of objects. | ||
==Planets and Astrology== | |||
The orbits of the planets also has a bearing in [[Astrology]]. It is believed the the position of the planets within various [[constellation]]s of stars can be an indicator of events on Earth. By carefully measuring the orbits and positions of the planets and calculating their future paths, it is believed that one can predict future events. | The orbits of the planets also has a bearing in [[Astrology]]. It is believed the the position of the planets within various [[constellation]]s of stars can be an indicator of events on Earth. By carefully measuring the orbits and positions of the planets and calculating their future paths, it is believed that one can predict future events. | ||
Revision as of 17:56, 20 November 2007
According to International Astronomical Union (IAU), a planet is a celestial body orbiting a star or stellar remnant that is massive enough to be rounded by its own gravity (but not massive enough to cause thermonuclear fusion in its inner core), and has cleared its neighbouring region of planetesimals. [1] [2] There are 8 bodies in the universe obeying this definition: Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uran and Neptune.
Again, according to that definition, bodies that don't obey the third condition, that is, orbiting the Sun, rounded by its own gravity but not cleared the neighbourhood, is called dwarf planet. One of them is Pluto, which is former considered as a planet. Other bodies that orbiting the Sun are generically called Small bodies of Solar System.
Another related term is exoplanet. Although there are no official defition for this term, it is often used to indicate bodies analogue to the planets, but that orbites other stars that not the Sun.[3]
The Planets
The planets can be subdivided into two main groups. The inner 4 terrestrial planets have a rocky composition. They are relatively small in size. The outer 4 planets are known as Gas Giants and have a thick gaseous atmospheres. Some physical information is followed:
| Name | Distance from the sun | Diameter | Mass | Date of Discovery |
|---|---|---|---|---|
| Mercury | 57,910,000 km (0.38 AU) | 4,880 km | 3.30e23 kg | a long time ago |
| Venus | 108,200,000 km (0.72 AU) | 12,103.6 km | 4.869e24 kg | a long time ago |
| Earth | 149,600,000 km (1.00 AU) | 12,756.3 km | 5.972e24 kg | a long time ago |
| Mars | 227,940,000 km (1.52 AU) | 6,794 km | 6.4219e23 kg | a long time ago |
| Jupiter | 778,330,000 km (5.20 AU) | 142,984 km | 1.900e27 kg | a long time ago |
| Saturn | 1,429,400,000 km (9.54 AU) | 120,536 km (equatorial) | 5.68e26 kg | a long time ago |
| Uranus | 2,870,990,000 km (19.218 AU) | 51,118 km (equatorial) | 8.683e25 kg | 1781 |
| Neptune | 4,504,000,000 km (30.06 AU) | 49,532 km | 1.0247e26 kg | 1846 |
Etimology and History
The word "planet" came from the greek πλανήτ- (planēt-), meaning "wanderers". There was, then, seven planets in the Sky, each one dedicated to a greek deitiy:
- Phainon, the shiner, dedicated to Cronus;
- Phaethon, brighter the first and below it, dedicated to Zeus;
- Pyroeis, "fiery", the red one, dedicated to Ares;
- Phosphoros, "light bringer", the brightest one, dedicated to Aphrodite;
- Stilbon, the gleamer, dedicated to Hermes; [4]
added by our Sun and Moon, the bigest wanderers in the sky. Later, n the time of the philosophers, many models of universe was created, which the most famous for us is the Aristotle's one. In his system, the planets belong each one to one cristaline sphere, concentric to the others. Inner the seven planet's sphere stay the material shperes (grosso modo, the Earth); Outer them, the shpere of fixed stars.
In Roman Empire, the planets became knowed directly by the name of the associated deity - not the greek one, bet the latin correspondent god. So, Phainon became Saturnus; Phaethon was called Jupiter; Pyroeis was Mars; Phosphoros, Venus and Stilbon was turned to Mercurius. In medieval era, the future european people has herited the roman culture, and so these latinized version of planet's names remain in the vocabulary until present days. Also in latinian tratition (followed by the germanic one) the seven days of the week have the names of the seven planets.
After the Copernican Revolution, however, the idea of planet has changed: they are all the bodies that round the Sun - that therefore would be considered just a star like any other from the firmament. The Earth then turn into a planet, the Moon became an Earth's sattelite, and the so-called "Solar System" have then six planets. Later, three new bodies, that can't be seen with naked eye are baptized as a planet, following the latin-named tradition: Uranus, Neptunus and Pluto.
But many other small bodies are saying to orbit the Sun, such as the brights comets and the palid asteroids. The crisis in definition starts in 1980's and 1990's, when many bodies so big as - or, in few cases, bigger - Pluto start to be discovered above Neptune's orbit. Called Transneptunian objects, they opened the discussion about what could be a good and precise definition of planet. The discussion ends in August 24, 2006, when IAU voted the Resolution that defines officially the term. [1]
Physical Formation
Planets are believed to form form a the disk of dust that surrounds a newly formed star. Gravitation forces pull the dust into lumps. The lumps gradually collide and join to make larger lumps or asteroids. These join further to make larger and larger planets until the planet has cleared it's orbit of objects.
Planets and Astrology
The orbits of the planets also has a bearing in Astrology. It is believed the the position of the planets within various constellations of stars can be an indicator of events on Earth. By carefully measuring the orbits and positions of the planets and calculating their future paths, it is believed that one can predict future events.
- ↑ 1.0 1.1 IAU 2006 General Assembly: Result of the IAU Resolution votes (2006). Retrieved on 2007-04-30.
- ↑ Working Group on Extrasolar Planets (WGESP) of the International Astronomical Union. IAU (2001). Retrieved on 2006-05-25.
- ↑ Error on call to Template:cite web: Parameters url and title must be specified.
- ↑ James Evans (1998). The History and Practice of Ancient Astronomy. Oxford University Press, 296-7.