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Megrez — おおぐまの恒星

Delta UMa

等級 3.3m Star おおぐま (UMa) 可視
星図
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Megrezについて

説明

Megrez, Delta Ursae Majoris, is an A-type main-sequence star about 80 light-years away and the faintest of the seven stars of the Big Dipper. It marks the junction where the Dipper's "handle" meets its "bowl." Megrez is about 1.6 times the Sun's mass, twice the radius, and 14 times the luminosity. It is also a suspected debris-disk star, with mid-infrared excess suggesting a surrounding ring of dust.

観測のコツ

Megrez's relative faintness (magnitude 3.31) is a classic sky-quality check — if you can see Megrez clearly with the naked eye, you have a reasonably dark site. From light-polluted suburban skies, the Big Dipper looks "incomplete" because Megrez disappears first. Use a pair of binoculars to confirm its white color and position at the corner of the Dipper's bowl, at the base of the handle. Circumpolar from all of the northern hemisphere.

歴史

The name Megrez comes from the Arabic "al-maghriz," meaning "the root of the tail" — referring to the tail-root of the great bear. All seven Dipper stars carry Arabic-derived names. Megrez's relatively modest brightness puzzled pre-modern astronomers; some ancient records refer to it being "fainter than expected," possibly due to observer uncertainty about the star's real appearance.

豆知識

Megrez is part of the Ursa Major Moving Group, a loose cluster of stars that share a common origin and are drifting through the galaxy together — including most of the other Big Dipper stars (all except Dubhe and Alkaid). The group is about 300 million years old. Megrez is one of the youngest prominent stars in the northern sky; on cosmic timescales it will remain a normal hydrogen-fusing dwarf for another billion years.

観測

1物理的性質

等級 3.31
範囲 3.30 - 3.31
周期 11.4 時間
変光星タイプ Variable (Unclassified)
スペクトル型 A2Vn
星の色 (B-V 0.08)
距離 80 ly

2位置と識別子

RA 12h 15m 25.6s
Dec +57° 01' 57.0"
HR 4660
HIP 59774
HD 106591
SAO 28315
Bayer Delta
Flamsteed 69 UMa

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 Feb – Apr (peak: Mar)

5サーベイ画像

サーベイ画像を読み込み中…

探究

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サイズ比較

VizieRで恒星データを照会中…
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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。

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恒星核融合

発見

15恒星メモ

"Dipper Stars"; Ursa cluster; Sirius group; UMa stream.
MEGREZ; Kaffa in Becvar.
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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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