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Acamar — Double Star in Eridanus

HIP 13847; Theta1 Eridani

Observable Double Star Excellent (70/100)

Sep: 8.2", Companion: mag 4.1

Magnitude 3.2m DoubleStar Eridanus (Eri) Visible
Star Map
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About Acamar

Description

Acamar is a binary star system at magnitude 3.24 in Eridanus, consisting of two white stars (A4III and A1V) separated by about 8 arcseconds. Located about 161 light-years from Earth, the pair makes one of the finest double stars in the southern sky.

Observing Tips

Acamar lies in the middle of Eridanus's long winding course. A small telescope reveals a beautiful pair of nearly white stars. Before Achernar was known to European astronomers, Acamar marked the end of the River. Best observed November through February.

History

The name Acamar comes from the Arabic 'akhir al-nahr,' meaning 'the end of the river' — the same root as Achernar. For ancient Greek and Arabic observers at northern latitudes, Acamar was the southernmost visible star of Eridanus, and thus the river's end.

Fun Facts

Acamar once marked the end of Eridanus for classical astronomers who could not see farther south. The discovery of the more southerly Achernar pushed the river's terminus farther toward the south celestial pole.

Observe

1Physical Properties

Magnitude 3.24
Spectral Type A4III giant
Star Color White (B-V 0.14)
Distance 93 ly

2Position & Identifiers

RA 02h 58m 15.7s
Dec -40° 18' 17.0"
Constellation Eridanus (Eri)
HR 897
HIP 13847
HD 18623
SAO 216114
Bayer Theta1

3How easy to split?

Primary 3.2 mag Companion 4.1 mag Separation 8.2″
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Telescope Bortle 3 Bortle 4 Bortle 5
80mm refr. Easy Easy Easy
150mm Newt. Easy Easy Easy
C8 203mm Easy Easy Easy
Easy Medium Hard Very hard Impossible

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

4Visibility

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Best season Sep – Nov (peak: Oct)

5Multiple Star System

Separation 8.2″
Companion Mag 4.1
Companion Sp A1V
Position Angle 90°
Star Colors A: White B: White
Discoverer PZ 2
Binary with HR 898. Uncertain which component var. Combined mag. HR 897/8, 2.91V; combined colors, +0.125(B-V), | +0.13(U-B).

Separation over time

Measured 1835 → 2020 (185 y)
Separation drift 8.7" → 8.2" (-0.50")
Rate -0.0027" / y
PA drift 82° → 90° (+8°, +0.043°/y)

Essentially fixed on human timescales — the same view your grandchildren will see.

Measured from the WDS observational archive. No orbital solution has been derived — most likely the period is too long to fit an orbit to the available measurement arc.

Eyepiece View

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80x Dawes: 1.9″ TFOV: 0.6°
Realistic = true angular size
N E 90°

A: 3.2 · B: 4.1 · Sep: 8.2″ · PA: 90° · N up, E right

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

Explore

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Size Comparison

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Compare Stars

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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

Discover

15Stellar Notes

0.016".
ACAMAR.
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Light Travel Time Machine

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Relativistic Travel

Nearby in the Sky

Other targets within a few degrees — pan your scope a little and keep exploring.

Visibility scores assume a 150 mm Newton at Bortle 4.

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