Ran — Star in Eridanus
HIP 16537; Epsilon Eridani; 18 Eridani
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
2Position & Identifiers
3How easy to spot?
| Equipment | Bortle 3 | Bortle 4 | Bortle 5 |
|---|---|---|---|
| Naked eye Naked eye | Easy | Medium+ | Medium+ |
| 50 mm finder 50mm finder | Easy | Easy | Easy |
| 150 mm telescope 150mm scope | Easy | Easy | Easy |
Bortle 3 = rural · 4 = outer suburbs · 5 = suburbs
4Visibility
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5Survey Image
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Explore
7
Size Comparison
8
Compare Stars
9
Spectral Classification
10
Hertzsprung-Russell Diagram
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Stellar Lifecycle
12
Blackbody Spectrum
13
Stellar Absorption Spectrum
Simulated absorption spectrum based on spectral type. Hover over lines to identify elements.
14
Stellar Fusion
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Exoplanets
1 known planet
View in 3D
| 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
Discover
16Stellar Notes
17
Light Travel Time Machine
18
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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