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Ran — Star in Eridanus

HIP 16537; Epsilon Eridani; 18 Eridani

Magnitude 3.7m Star Eridanus (Eri) Visible 1 Exoplanet
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About Ran

Description

Ran, Epsilon Eridani, is one of the very nearest naked-eye stars — only 10.48 light-years away — a K2V orange dwarf about 82 percent the Sun's mass. At magnitude 3.73 it is an easy naked-eye star, made more remarkable by the fact that it is surrounded by two confirmed dust debris disks and at least one giant exoplanet. Epsilon Eri is young by solar standards (roughly 800 million years old) and still retains a lively magnetic field that produces strong chromospheric activity.

Observing Tips

Find Epsilon Eridani in central Eridanus, roughly midway along the river of stars meandering southwest from Cursa (Beta Eri, below Rigel). It appears as a warm yellow-orange point in binoculars, noticeably redder than nearby Epsilon's companions. Because it is only 10 light-years distant, its proper motion is visible even to amateurs: over a decade it shifts by about 10 arcseconds. Best observed October through February.

History

The IAU gave this star the name "Ran" in 2015 through its NameExoWorlds contest — Ran is a Norse sea goddess. Its confirmed planet, Epsilon Eri b, was named "AEgir." Epsilon Eri was one of the two stars targeted in Frank Drake's 1960 Project Ozma, the first serious modern search for extraterrestrial radio signals.

Fun Facts

Epsilon Eridani's debris-disk system (discovered by IRAS in 1984 and later imaged by Herschel and ALMA) is the nearest analog to our own Kuiper Belt. The star's close planet, Epsilon Eri b (AEgir), is a gas giant of roughly 1-2 Jupiter masses orbiting at about 3.5 AU. Its age, proximity, and planetary system make it one of the most-studied stars in exoplanet science — a likely early target for future Earth-like-planet imaging missions.

Observe

1Physical Properties

Magnitude 3.73
Spectral Type K2V (k)
Star Color Orange (B-V 0.88)
Distance 11 ly

2Position & Identifiers

RA 03h 32m 55.8s
Dec -09° 27' 30.0"
Constellation Eridanus (Eri)
HR 1084
HIP 16537
HD 22049
SAO 130564
Bayer Epsilon
Flamsteed 18 Eri

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 Oct – Dec (peak: Nov)

5Survey Image

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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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Exoplanets 1 known planet

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View this system in the 3D Orrery
Interactive Keplerian orbits, procedural planet textures, habitable zone.
Planet Radius Mass Period Distance
eps Eri b 14.10R⊕ 0.66M♃ 7.3yr 10ly

Habitable Zone

Size & Mass Comparison

About exoplanets — how we find them and which host stars you can observe

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16Stellar Notes

Astrometric binary, 25y. Unresolved by speckle interferometry.
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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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