Menu

Nusakan — かんむりの二重星

HIP 75695; Beta Coronae Borealis; 3 Coronae Borealis

等級 3.7m DoubleStar かんむり (CrB) 可視
星図
+ リスト + 計画

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

等級 3.68
範囲 3.65 - 3.69
周期 18.5 日
変光星タイプ Alpha2 CVn (Magnetic Rotating)
スペクトル型 A8V:SrCrEu
星の色 黄白 (B-V 0.28)
距離 114 ly

2位置と識別子

RA 15h 27m 49.7s
Dec +29° 06' 21.0"
HR 5747
HIP 75695
HD 137909
SAO 83831
Bayer Beta
Flamsteed 3 CrB
Variable ID Bet CrB

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 Apr – Jun (peak: May)

5光度曲線

6多重星系

離角 0.3″
伴星等級 5.2
伴星スペクトル F2
位置角 140°
星の色 A: 黄白 B: 黄白
発見者 JEF 1
First astrometric binary discovered from parallax measurements, by K. Burns, 1931.

離角の経時変化

周期: 10.5 y 離心率: 0.540 現在: 0.28", PA 155° -0.16" 5年後
0.00" 0.09" 0.18" 0.27" 0.36" 2022 2024 2026 2028 2030 0.28"

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

VizieRで恒星データを照会中…
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

Alpha CV 3.65 - 3.72V, 18.487d. Magnetic field and rotation same period. Variable H alpha. Amp., light, | magnetic field, spectrum vary per. 10.5y. Possible secondary light period of 240d.
10.496y, K 9.2k/s, V0 -18.0k/s, asini 442. The two SB components first resolved visually 1975. Possible secondary RV | period 320.17d. Resolved by speckle interferometry 1986.45, sep. 0.31".
Hyades group.
Also classified A8IIIpSrCrEu. Extreme oxygen deficiency relative to magnesium. Magnetic field an indicator of stellar | rotation. Uranium 3860 but not thorium in spectrum.
Nusakan.
17

光の旅タイムマシン

18

相対論的旅行

}