Centaurus

Japanese: ケンタウルス座 - けんたうるすざ
Centaurus

A constellation that appears only with its upper body on the southern horizon on a night in early June. In Japan, you can see almost its entire body near Okinawa. It is a centaur with the upper body of a human and the lower body of a horse, and its name is not a proper name, but refers to the whole race of half-man, half-horse. In the upper body is Omega Centauri, a bright globular star cluster that can be seen with the naked eye, with a brightness of about 4th magnitude. In the past, it was considered to be a single star, so it was given the Greek letter ω, which is used to name stars, but in reality it is a large group of stars located 17,000 light years away. In Tokyo, Omega Centauri is difficult to find because it only rises about 7 degrees above the horizon even when it rises due south. At the foot of the centaur is the star α (alpha), which is famous for being the closest star to the sun and has a magnitude of 0.1. It is 4.4 light years away and is most visible in spring from Guam and Hawaii.

[Asahi Fujii]

"Spring Constellations" by Akira Fujii (1989, Kin no Hoshisha)""Recommendations for Stargazing" by Kazushi Sakubana (1996, Ohmsha)""David Marin's Amazing Universe" by David Marin, translated by Tetsuo Hasegawa (2000, Newton Press)""A Story of the Constellations" by Hoei Nojiri (Chikuma Bunko)

[References] | Omega Centauri Cluster | Globular Cluster | Centaur | Constellation
Centaurus
©Akira Fujii ">

Centaurus

Omega Centauri (ω Cluster)
A globular cluster in the constellation Centaurus. NGC5139. Photographed using the Murikabushi Telescope at Ishigakijima Astronomical Observatory © National Astronomical Observatory of Japan ">

Omega Centauri (ω Cluster)


Source: Shogakukan Encyclopedia Nipponica About Encyclopedia Nipponica Information | Legend

Japanese:

6月初旬の宵、南の地平線上に上半身だけ姿を見せる星座。日本でも沖縄付近ではほぼ全身を見ることができる。上半身が人間、下半身が馬という粗暴なふるまいをするケンタウロスの姿で、固有名ではなく半人半馬族全体のことをさした星座名である。上半身の部分にはオメガ・ケンタウリ星団(ω星団(オメガせいだん))という肉眼でも見える明るい球状星団があり、明るさはおよそ4等星ほどである。昔は1個の星とみなされていたため、恒星につけられるギリシア文字ωがつけられていたが、実体は距離1万7000光年のところにある星の大集団だった。オメガ・ケンタウリ星団は東京では真南に昇りつめても地平線上わずか7度程度にしかならないので、みつけにくい。ケンタウロスの足元部分には、太陽にいちばん近い恒星として有名な0.1等のα(アルファ)星がある。距離は4.4光年で、グアム島やハワイでは春に見やすくなる。

[藤井 旭]

『藤井旭著『春の星座』(1989・金の星社)』『作花一志著『星空ウォッチングのすすめ』(1996・オーム社)』『デイビッド・マリン著、長谷川哲夫訳『デイビッド・マリンの驚異の大宇宙』(2000・ニュートンプレス)』『野尻抱影著『星座のはなし』(ちくま文庫)』

[参照項目] | オメガ・ケンタウリ星団 | 球状星団 | ケンタウロス | 星座
ケンタウルス座
©藤井 旭">

ケンタウルス座

オメガ・ケンタウリ星団(ω星団)
ケンタウルス座にある球状星団。NGC5139。石垣島天文台むりかぶし望遠鏡により撮影©国立天文台">

オメガ・ケンタウリ星団(ω星団)


出典 小学館 日本大百科全書(ニッポニカ)日本大百科全書(ニッポニカ)について 情報 | 凡例

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