Menu

Thuban — りゅうの恒星

HIP 68756; Alpha Draconis; 11 Draconis

等級 3.6m Star りゅう (Dra) 可視
星図
+ リスト + 計画

Thubanについて

説明

Thuban, Alpha Draconis, is a white giant star of spectral type A0 IV located about 303 light-years away, notable not for its present brightness but for having been Earth's North Star around 2700 BC. Thuban is a spectroscopic binary with a close companion in a 51.4-day orbit, and the primary is a mild chemical-peculiarity star. At magnitude 3.65 it is the third-brightest star in Draco, behind Gamma and Eta Draconis.

観測のコツ

Despite its "alpha" designation, Thuban is visibly fainter than several of its constellation-mates. Find it by tracing the tail of Draco — it lies midway along the arc running between Mizar in Ursa Major and the bowl of the Little Dipper. Its position is steady and easily identified: just remember the line from Mizar to Polaris passes almost directly through Thuban. Circumpolar from northern temperate latitudes, so visible every clear night of the year.

歴史

Because of the precession of Earth's rotational axis, Thuban was the pole star from approximately 3942 BC to 1793 BC. The great Pyramid of Giza was oriented so that one of its internal shafts pointed directly at Thuban's meridian position around 2600 BC — likely by design. The name Thuban comes from the Arabic "ath-thu'bān," meaning "the serpent." Vega was the pole star around 12,000 BC and will become so again around 13,700 AD; Polaris holds the title from about 500 AD to 3000 AD.

豆知識

Thuban is one of very few stars whose pole-star status has been confirmed by archaeological evidence at multiple ancient sites. It is slightly eclipsing — the close companion produces shallow 1-percent dips every 51.4 days, discovered only recently with space-based photometry. The Sun will be near Thuban's position in the sky in about 20,000 years.

観測

1物理的性質

等級 3.65
範囲 3.66 - 3.76
周期 51 日
変光星タイプ Eclipsing Binary (Algol-type)
スペクトル型 A0IV 準巨星
星の色 青白 (B-V -0.05)
距離 303 ly

2位置と識別子

RA 14h 04m 23.3s
Dec +64° 22' 33.0"
HR 5291
HIP 68756
HD 123299
SAO 16273
Bayer Alpha
Flamsteed 11 Dra

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 普通+ 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 Mar – May (peak: Apr)

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

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

Alpha CV?, 3.64 - 3.67V.
51.420d, K 46.9k/s, V0 -13.0k/s, asini 30.7.
High Si and Cr abundance.
THUBAN; Adib; Dragon's Tail. Former Pole Star, about 2700 B.C.
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。

}