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
2位置と識別子
3見つけやすさ
| 機材 | ボートル3 | ボートル4 | ボートル5 |
|---|---|---|---|
| 肉眼 肉眼 | 容易 | 容易 | 普通+ |
| 50mmファインダー 50mmファインダー | 容易 | 容易 | 容易 |
| 150mm望遠鏡 150mm望遠鏡 | 容易 | 容易 | 容易 |
ボートル3=田舎 · 4=郊外 · 5=住宅地
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
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
13
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
16
光の旅タイムマシン
17
相対論的旅行
近くの天体
数度以内にある他の対象 — 望遠鏡を少し動かして探索を続けましょう。
可視性スコアは150 mmニュートン・ボートル4を前提としています。
Nightbase を探す
関連する知識・ツール・物語 — 観測計画は不要です。