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Pollux — Double Star in Gemini

HIP 37826; Beta Geminorum; 78 Geminorum

DoubleStar Gemini (Gem) Visible 1 Exoplanet
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About Pollux

Description

Pollux is the brightest star in the constellation Gemini at magnitude 1.14, slightly outshining its twin Castor. It is an orange giant of spectral type K0III, located only 34 light-years from Earth. Pollux is about 9 times the diameter of the Sun, nearly twice its mass, and about 33 times more luminous. In 2006, a planet was confirmed orbiting Pollux — Pollux b (also called Thestias), a gas giant at least 2.3 times the mass of Jupiter in a 590-day orbit.

Observing Tips

Pollux and Castor form the heads of the celestial twins, making one of the most recognizable pairs in the sky. Pollux is slightly brighter and noticeably more orange than the blue-white Castor — this color contrast is delightful through binoculars. While Castor is a spectacular multiple star system, Pollux is a single star. The famous open cluster M35 lies at the feet of Gemini, about 9 degrees to the northwest. Best observed from December through May.

History

Named after Pollux, the immortal twin from Greek mythology (son of Zeus), while Castor was the mortal twin (son of King Tyndareus). Despite being the brighter star, Bayer designated it Beta Geminorum — possibly because Castor was listed first by Ptolemy or because the 'head' twin traditionally took precedence. The planet Pollux b, confirmed in 2006 by Artie Hatzes and colleagues, was one of the first exoplanets found around a giant star.

Fun Facts

Pollux is the nearest giant star to the Sun and the closest star with a confirmed exoplanet (among bright naked-eye stars). Its planet Pollux b was officially named Thestias by the International Astronomical Union. The orange color of Pollux compared to the blue-white of Castor makes them one of the finest color-contrast pairs visible to the naked eye.

Observe

1Physical Properties

Magnitude 1.14
Range 1.14 - 1.15
Variable Type Variable (Unclassified)
Spectral Type G9III
Star Color Orange (B-V 1.00)
Temperature 4865 K
Radius 8.8 R☉
Distance 34 ly

2Position & Identifiers

RA 07h 45m 18.9s
Dec +28° 01' 34.0"
Constellation Gemini (Gem)
HR 2990
HIP 37826
HD 62509
Bayer Beta
Flamsteed 78 Gem
Double Cat 6335

3How easy to split?

Primary 1.1 mag Companion 11.0 mag Separation 257.5″
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Telescope Bortle 3 Bortle 4 Bortle 5
80mm refr. Hard+ Hard Hard
150mm Newt. Medium+ Medium+ Medium
C8 203mm Easy Medium+ Medium+
Easy Medium Hard Very hard Impossible

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

4Visibility

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Best season Dec – Feb (peak: Jan)

5Multiple Star System Septuple B,C,E,F,G: optical

Components 7 (septuple)
Component IDs AC
Separation 257.5″
Companion Mag 10.9
Position Angle 76°
Star Colors A: Orange
Discoverer H 6 42
All the visual companions optical.

Separation over time

Measured 1781 → 2013 (232 y)
Separation drift 116.8" → 257.5" (+140.70")
Rate +0.6065" / y
PA drift 66° → 76° (+10°, +0.043°/y)

Apparent motion is significant on a human timescale — worth revisiting in a decade.

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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32x Dawes: 1.9″ TFOV: 1.6°
Realistic = true angular size
N E 76°

A: 1.1 · B: 10.9 · Sep: 257.5″ · PA: 76° · N up, E left

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

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Exoplanets 1 known planet

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Interactive Keplerian orbits, procedural planet textures, habitable zone.
Planet Radius Mass Period Distance
HD 62509 b 13.30R⊕ 2.30M♃ 1.6yr 34ly

Habitable Zone

Size & Mass Comparison

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

Discover

16Stellar Notes

NSV 3712 is component A, 1.10 - 1.17V, while component E is NSV 3716, 10.5v.
Emission line discovered by COPERNICUS at 1218.4 may be OV probably formed in a corona. Balloon-borne spectrometer | revealed pronounced emission of MgII.
POLLUX; Hercules.
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Light Travel Time Machine

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Relativistic Travel

Survey Image

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