SARRERA DESBERDINA:
Poligono erregular
(gradu hirurogeitarretan)
(radianetan)
(gradu hirurogeitarretan)
(radianetan)
(gradu hirurogeitarretan)
(radianetan)
(gradu hirurogeitarretan)
(radianetan)
(gradu hirurogeitarretan)
(radianetan)






















Geometrian, poligono bat erregularra da, aldeberdina (alde guztiak luzera berekoak dira) eta angeluberdina (angelu guztiak neurri berekoak dira) bada.
Poligono erregularrak bi motatakoak izan daitezke: ganbilak eta ahurrak (izar itxurakoak azken horiek, izar-poligono izenekoak).
Hiru eta lau aldeko poligono erregularrak triangelu aldeberdina eta karratua dira, hurrenez hurren; alde gehiagoko poligono erregularrak izendatzeko, erregular terminoa gehitzen da (pentagono erregularra, hexagono erregularra...).
Oharra: Poligono erregularrak zenbat eta alde gehiago izan, orduan eta zirkunferentzia baten antz handiagoa izango du.
Poligono erregular baten azalera kalkulatzeko, ezagunak ditugun elementuen arabera, hainbat formula daude:
Oharra: alde kopuru oso handia duen poligonoaren kasuan, barne-angeluek lauak izatera joko dute, aldea nulua izatera eta azalera π zenbakiaren baliorantz[1].
↑ a b c Zirkunferentzia zirkunskribatuaren erradioak 1 balio duenean.
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