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Yed Posterior — へびつかいの恒星

HIP 79882; Epsilon Ophiuchi; 2 Ophiuchi

等級 3.2m Star へびつかい (Oph) 可視
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Yed Posteriorについて

説明

Yed Posterior, Epsilon Ophiuchi, is a G-type giant of spectral class G9.5 IIIb lying about 106 light-years from Earth. It shines at magnitude 3.24 and has a mild iron underabundance compared to the Sun. With a radius of 11 Suns and a luminosity of 54 Suns, it is a typical evolved first-ascent red-clump giant — a star that is currently fusing helium in its core. It forms a naked-eye optical pair with Yed Prior (Delta Oph).

観測のコツ

Yed Posterior sits just east of Yed Prior, the two forming a prominent 0.5-degree-apart pair along the left shoulder of Ophiuchus. Binoculars show both stars clearly, with Yed Posterior appearing the warmer of the two. The names encode their positions: Prior (western) rises first, Posterior (eastern) rises second, from the geocentric viewpoint of pre-modern astronomy. Best observed April through September.

歴史

The name comes from the Arabic "al-yad," meaning "the hand," with the Latin "Posterior" added in medieval compilations to distinguish it from its neighbor Yed Prior. Epsilon Oph was formally assigned the name Yed Posterior by the IAU in 2016.

豆知識

Yed Posterior's position near the ecliptic means it is occasionally occulted by the Moon and, rarely, by asteroids — valuable events for timing observations. Its spectrum has been used as a template for understanding similar K-type red-clump giants throughout the galaxy. The two Yed stars (Prior and Posterior) are an optical pair: at 104 and 170 light-years respectively, they are not physically related.

観測

1物理的性質

等級 3.24
スペクトル型 G9.5IIIb Fe-0.5 輝巨星
星の色 (B-V 0.96)
距離 106 ly

2位置と識別子

RA 16h 18m 19.3s
Dec -04° 41' 33.0"
HR 6075
HIP 79882
HD 146791
SAO 141086
Bayer Epsilon
Flamsteed 2 Oph

3見つけやすさ

サインイン し、機材と既定の場所を設定するとパーソナライズ行が表示されます。
機材 ボートル3 ボートル4 ボートル5
肉眼 容易 容易 普通+
50mmファインダー 容易 容易 容易
150mm望遠鏡 容易 容易 容易
簡単 普通 難しい 非常に難 不可能

ボートル3=田舎 · 4=郊外 · 5=住宅地

4可視性

設定で観測地を設定 すると可視性データが表示されます。

観測好期 Apr – Jun (peak: May)

5サーベイ画像

サーベイ画像を読み込み中…

探究

7

サイズ比較

VizieRで恒星データを照会中…
8

恒星を比較

9

スペクトル分類

11

恒星の進化

12

黒体放射スペクトル

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恒星吸収スペクトル

スペクトル型に基づくシミュレーション吸収スペクトル。線にマウスを合わせると元素を識別できます。

14

恒星核融合

発見

15恒星メモ

Oxygen deficient relative to magnesium.
Yed Posterior.
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光の旅タイムマシン

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相対論的旅行

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