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Rana — Star in Eridanus

HIP 17378; Delta Eridani; 23 Eridani

Magnitude 3.5m Star Eridanus (Eri) Visible
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About Rana

Description

Rana, Delta Eridani, is a K-type subgiant of spectral class K1 III-IV only 29.9 light-years away — one of the closest subgiants to the Sun. Despite being a giant, its proximity makes it bright enough to shine at magnitude 3.54. Rana has a mass of about 1.2 Suns and is actively evolving off the main sequence. It is a known radial-velocity exoplanet candidate host.

Observing Tips

Rana sits in the central part of Eridanus, the long winding celestial river. In binoculars it glows a soft orange. Rana is a good proper-motion demonstration star: its position has shifted detectably over decades, visible in careful comparisons of old and new star charts. Best observed October through February.

History

The name Rana is Latin for "frog" — a medieval European designation preserved through star-catalog tradition. The IAU formally adopted the name in 2016.

Fun Facts

Rana's proximity combined with its evolved status make it an important benchmark for calibrating models of post-main-sequence evolution. The star has been proposed as a target for interstellar-probe concept studies, being less than 30 light-years away and hosting a possible planetary system.

Observe

1Physical Properties

Magnitude 3.54
Spectral Type K1III-IV giant
Star Color Orange (B-V 0.92)
Distance 30 ly

2Position & Identifiers

RA 03h 43m 14.9s
Dec -09° 45' 48.0"
Constellation Eridanus (Eri)
HR 1136
HIP 17378
HD 23249
SAO 130686
Bayer Delta
Flamsteed 23 Eri
Variable ID Del Eri

3How easy to spot?

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Equipment Bortle 3 Bortle 4 Bortle 5
Naked eye Easy Easy 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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Explore

7

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

RS:, 3.51 - 3.56V, about 10d.
CaII H and K emission.
Rana in Becvar. But see HR 188.
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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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