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Gorgonea Tertia — Variable Star in Perseus

HIP 14354; Rho Persei; 25 Persei

Observable Variable Star Excellent (67/100)

Range: 3.13 - 3.77, Period: 54.7d, Type: SRB

Magnitude 3.3–4.0m VariableStar Perseus (Per) Visible
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About Gorgonea Tertia

Description

Gorgonea Tertia, Rho Persei, is a red supergiant of spectral class M4+ IIIa about 297 light-years away — one of the closer M-type giants to Earth. It is a semiregular variable, pulsating between magnitudes 3.3 and 4.0 over a primary period of about 50 days, with longer secondary modulations of 600 to 900 days. The star has about 150 solar radii and a luminosity of 240 Suns.

Observing Tips

Gorgonea Tertia is one of the sky's finest deep-orange stars. Its brightness changes by almost a full magnitude — easy for the naked eye to follow over a few weeks against the steady comparison star Algol nearby. Rho Per is very close to Algol and makes an excellent paired observation. Best observed September through February.

History

The name refers to the "Third Gorgon" — one of three mythical Gorgon sisters whose severed head (Medusa) Perseus carries. Algol is the "Demon's Head" (the Gorgon Medusa), and Rho Per represents one of her two immortal sisters. The three Gorgons are sometimes collectively traced in the southwestern part of Perseus. The IAU adopted the name in 2016.

Fun Facts

Gorgonea Tertia's deep orange color is a striking contrast with the nearby blue-white Algol — a visual reminder that the two stars represent radically different stages of stellar evolution, despite their proximity on the sky. Rho Per will likely end its life as a planetary nebula.

Observe

1Physical Properties

Magnitude 3.39
Range 3.13 - 3.77
Period 55 days
Variable Type Semi-Regular Variable (Late-type Giant)
Spectral Type M4+ IIIa
Star Color Red (B-V 1.65)
Distance 297 ly

2Position & Identifiers

RA 03h 05m 10.6s
Dec +38° 50' 25.0"
Constellation Perseus (Per)
HR 921
HIP 14354
HD 19058
SAO 56138
Bayer Rho
Flamsteed 25 Per
Variable ID Rho Per

3How easy to follow?

Magnitude 3.3 – 4.0 mag Amplitude 0.7 mag Period 54.66 d Type SRB
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Equipment Bortle 3 Bortle 4 Bortle 5
Naked eye Medium Hard+ Hard+
50mm finder Medium Medium Medium
150mm scope Medium Medium Medium
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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6Light Curve

7Comparison Stars

Nearby stable stars for estimating brightness (AAVSO)

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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

17Stellar Notes

SRb 3.30 - 4.0V, about 50d with possibly slow var. in mean brightness in 1100d period.
Zeta Her group.
Gorgonea Tertia.
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Light Travel Time Machine

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Relativistic Travel

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