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・ Lacera apicirupta
・ Lacera asinuosa
・ Lacera azatothi
・ Lacera contrasta
・ Lacera noctilio
・ Lacera nyarlathotepi
・ Lacera procellosa
・ Lacera uniformis
・ Lacera vinacea
・ Lacera violacea
・ Lacerba
・ Lacerda
・ Lacerda de Almeida River
・ Lacerdão
・ Lacerdópolis
Lacerta
・ Lacerta (Chinese astronomy)
・ Lacerta (genus)
・ Lacerta clarkorum
・ Lacerta kulzeri
・ Lacerta oertzeni
・ Lacertamoeba
・ Lacertaspis
・ Lacertidae
・ Lacertine
・ Lacertoidea
・ Lacertoides
・ Lacertus
・ Lacerum
・ Lacetani


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Lacerta : ウィキペディア英語版
Lacerta

Lacerta is one of the 88 modern constellations defined by the International Astronomical Union. Its name is Latin for lizard. A small, faint constellation, it was created in 1687 by the astronomer Johannes Hevelius. Its brightest stars form a "W" shape similar to that of Cassiopeia, and it is thus sometimes referred to as 'Little Cassiopeia'. It is located between Cygnus, Cassiopeia and Andromeda on the northern celestial sphere. The northern part lies on the Milky Way.
==Notable features==

Lacerta is typical of Milky Way constellations: no bright galaxies, nor globular clusters, but instead open clusters, for example NGC 7243, the faint planetary nebula IC 5217 and quite a few double stars. It also contains the prototypic blazar BL Lacertae.
Lacerta contains no Messier objects.

抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)
ウィキペディアで「Lacerta」の詳細全文を読む



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