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Nusakan — Double Star in Corona Borealis

HIP 75695; Beta Coronae Borealis; 3 Coronae Borealis

Magnitude 3.7m DoubleStar Corona Borealis (CrB) Visible
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About Nusakan

Description

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.

Observing Tips

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.

History

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.

Fun Facts

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.

Observe

1Physical Properties

Magnitude 3.68
Range 3.65 - 3.69
Period 18.5 days
Variable Type Alpha2 CVn (Magnetic Rotating)
Spectral Type A8V:SrCrEu
Star Color Yellow-white (B-V 0.28)
Distance 114 ly

2Position & Identifiers

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

3How easy to spot?

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Equipment Bortle 3 Bortle 4 Bortle 5
Naked eye Easy Medium+ Medium+
50mm finder Easy Easy Easy
150mm scope Easy Easy Easy
Easy Medium Hard Very hard Impossible

Bortle 3 = rural · 4 = outer suburbs · 5 = suburbs

4Visibility

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Best season Apr – Jun (peak: May)

5Light Curve

6Multiple Star System

Separation 0.3″
Companion Mag 5.2
Companion Sp F2
Position Angle 140°
Star Colors A: Yellow-white B: Yellow-white
Discoverer JEF 1
First astrometric binary discovered from parallax measurements, by K. Burns, 1931.

Separation over time

Period: 10.5 y Eccentricity: 0.540 Now: 0.28", PA 155° -0.16" in 5 years
0.00" 0.09" 0.18" 0.27" 0.36" 2022 2024 2026 2028 2030 0.28"

Apparent separation over time, computed from ORB6 orbital elements. Steep curves indicate fast-changing pairs — catch them while they're splittable.

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Size Comparison

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Spectral Classification

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Hertzsprung-Russell Diagram

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Stellar Lifecycle

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Blackbody Spectrum

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Stellar Absorption Spectrum

Simulated absorption spectrum based on spectral type. Hover over lines to identify elements.

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Stellar Fusion

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16Stellar Notes

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.
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Light Travel Time Machine

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Relativistic Travel

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