Nusakan — かんむりの二重星
HIP 75695; Beta Coronae Borealis; 3 Coronae Borealis
Nusakanについて
説明
Nusakan, Beta Coronae Borealis, is a magnetic chemically-peculiar (Ap) star of spectral type A8V located 114 light-years away in the constellation Corona Borealis. It is part of a binary system with an F2V companion in a 10.5-year orbit. The primary's surface is pockmarked with unusual abundances of chromium, strontium, and europium, held in chemically-concentrated spots by a strong global magnetic field — a tell-tale signature of the Ap class.
観測のコツ
Nusakan marks the western end of Corona Borealis's graceful semicircular crown, west of Alphecca (the brightest crown star). It is a naked-eye object at magnitude 3.68. The binary companion is too close (< 0.3 arcseconds) to split visually, but the primary rotates once every 18.5 days, and over that cycle its surface element-patches produce measurable magnitude and color changes — tiny but real variability. Best observed April through September.
歴史
The name Nusakan comes from a now-obscure Arabic astronomical text, possibly from "al-nasaqān," meaning "the two rows" or "lines," referring to the shape of the crown. The Ap peculiarity was first noted in the 1920s, and the strong magnetic field was mapped in detail by Zeeman-Doppler imaging in the 1990s and 2000s.
豆知識
Nusakan's magnetic field is tilted with respect to its rotation axis, so different spots rotate into view as the star turns — producing the small periodic variation. The field strength can reach 5 kilogauss at the surface, thousands of times stronger than Earth's magnetic field. The star is sometimes classified as a "roAp" (rapidly oscillating Ap) candidate because tiny ~10-minute pulsations have been tentatively detected.
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 | 普通+ | 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光度曲線
6多重星系
離角の経時変化
ORB6軌道要素から計算された、見かけの離角の経時変化。急峻な曲線は変化の速いペアを示します — 分離可能なうちに観測しましょう。
探究
8
サイズ比較
9
恒星を比較
10
スペクトル分類
12
恒星の進化
13
黒体放射スペクトル
14
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。
15
恒星核融合
発見
16恒星メモ
17
光の旅タイムマシン
18
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。