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Sceptrum — Double Star in Eridanus

HIP 21594; 53 Eridani

Magnitude 3.9m DoubleStar Eridanus (Eri) Visible
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About Sceptrum

Description

Sceptrum, 53 Eridani, is a K-type giant of spectral class K1 III about 110 light-years away. It shines at magnitude 3.87. Sceptrum is a remnant of an obsolete constellation — "Sceptrum Brandenburgicum," invented by Gottfried Kirch in 1688 and abandoned by modern astronomy.

Observing Tips

Sceptrum lies in the central part of Eridanus. Its warm amber color is clear in binoculars. Best observed October through February.

History

The name Sceptrum comes from the obsolete constellation Sceptrum Brandenburgicum (the Brandenburg Scepter), created in 1688 by Gottfried Kirch as a tribute to the House of Brandenburg. The constellation was not retained when the IAU standardized constellations in 1930, but the name Sceptrum for this star survived. The IAU formally adopted the name in 2017.

Fun Facts

Sceptrum is a rare example of a star name preserving the memory of an obsolete constellation. Historical constellations like Sceptrum Brandenburgicum, Antinous, Quadrans, and Robur Carolinum have mostly faded from modern usage — the surviving star names are linguistic fossils of earlier cartographic fashions.

Observe

1Physical Properties

Magnitude 3.87
Spectral Type K1III giant
Star Color Orange (B-V 1.09)
Distance 110 ly

2Position & Identifiers

RA 04h 38m 10.8s
Dec -14° 18' 14.0"
Constellation Eridanus (Eri)
HR 1481
HIP 21594
HD 29503
SAO 149781
Flamsteed 53 Eri

3How easy to split?

Primary 3.9 mag Companion 7.0 mag Separation 0.9″
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Telescope Bortle 3 Bortle 4 Bortle 5
80mm refr. V. hard V. hard V. hard
150mm Newt. V. hard+ V. hard+ V. hard+
C8 203mm V. hard+ V. hard+ V. hard+
Easy Medium Hard Very hard Impossible

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

To reach "Medium" at Bortle 3, you'd need at least a 380 mm reflector.

4Visibility

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Best season Oct – Dec (peak: Nov)

5Multiple Star System

Separation 0.9″
Companion Mag 7.0
Position Angle 10°
Star Colors A: Orange
Discoverer KUI 18

Separation over time

Period: 77.2 y Eccentricity: 0.661 Now: 0.92", PA 12° -0.13" in 5 years
0.00" 0.29" 0.58" 0.88" 1.2" 2025 2030 2035 2040 2045 0.92"

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

Eyepiece View

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80x Dawes: 1.9″ TFOV: 0.6°
Realistic = true angular size
N E 10°

A: 3.9 · B: 7.0 · Sep: 0.9″ · PA: 10° · N up, E right

Unresolved · Rayleigh: 2.3″ · Dawes: 1.9″ · Eff: 2.3″

Explore

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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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15Stellar Notes

Sceptrum.
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Light Travel Time Machine

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Relativistic Travel

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