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Polaris

HIP 11767; Alpha Ursae Minoris; 1 Ursae Minoris

HIP 11767; Alpha UMi; 1 UMi DoubleStar Ursa Minor (UMi) Visible
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About Polaris

Description

Polaris (the North Star) is a yellow supergiant of spectral type F7Ib-II at magnitude 2.02 in Ursa Minor. Located about 431 light-years from Earth, it has a luminosity of roughly 1,260 times solar. Polaris is a Cepheid variable star, pulsating with a period of about 3.97 days. It is a triple star system — the faint companion Polaris B is visible in a small telescope.

Observing Tips

Polaris sits within 1 degree of the north celestial pole, making it the current pole star. Use the Big Dipper's Pointer Stars (Merak and Dubhe) to find it. Despite its fame, Polaris is only the 48th brightest star — it is important for its position, not its brilliance. Polaris B (magnitude 8.7) is a rewarding telescopic companion at 18 arcseconds separation. Visible year-round from the northern hemisphere.

History

Polaris has not always been the pole star — precession slowly shifts the celestial pole. It became useful as a pole indicator around 500 AD and will be closest to the pole around AD 2100. The name comes from Latin 'stella polaris.' Vikings, medieval navigators, and explorers have relied on it for over a millennium.

Fun Facts

Polaris is the nearest and brightest Cepheid variable to Earth, making it crucial for calibrating the Cepheid period-luminosity relation used to measure cosmic distances. Surprisingly, its pulsation amplitude has been decreasing over the past century and nearly stopped in the 1990s before increasing again — a mystery.

Observe

1Physical Properties

Magnitude 2.02
Range 1.96 - 2.03
Period 4.0 days
Variable Type Classical Cepheid (First Overtone)
Spectral Type F8Ib
Star Color Yellow (B-V 0.60)
Temperature 6062 K
Radius 37.6 R☉
Distance 432 ly

Position & Identifiers

RA 02h 31m 48.7s
Dec +89° 15' 51.0"
Constellation Ursa Minor (UMi)
HR 424
HIP 11767
HD 8890
Bayer Alpha
Flamsteed 1 UMi
Variable ID Alp UMi
Double Cat 1477

2How easy to split?

Primary 2.0 mag Companion 9.1 mag Separation 18.4″
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Telescope Bortle 3 Bortle 4 Bortle 5
80mm refr. Hard+ Hard+ Hard+
150mm Newt. Medium+ Medium+ Medium+
C8 203mm Easy Easy Easy
Easy Medium Hard Very hard Impossible

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

3Visibility

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Best season Sep – Nov (peak: Oct)

4Light Curve

5Multiple Star System C,D: optical

Components 5
Component IDs AB
Separation 18.4″
Companion Mag 9.1
Companion Sp F3V
Position Angle 236°
Star Colors A: Yellow B: Yellow-white
Discoverer STF 93

Eyepiece View

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80x Dawes: 1.9″ TFOV: 0.6°
Realistic = true angular size
N E 236°

A: 2.0 · B: 9.1 · Sep: 18.4″ · PA: 236° · N up, E left

Resolved · Rayleigh: 2.3″ · Dawes: 1.9″ · Eff: 2.3″

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Size Comparison

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Stellar Lifecycle

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Spectral Classification

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Hertzsprung-Russell Diagram

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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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15Stellar Notes

CDelta 1.92 - 2.07V, 3.969778d. Period increases 53 sec./century. Probably unreddened.
A* 2.0 var. F8Ib, 30.46y, a = 0.038". AB physical; B, 8.20V, +0.49(B-V), +0.16(U-B), F3V, 0.0 color excess, | vsini =<60k/s; C, 13v at 43"; D, 14v at 83".
ADS 1477A, K 4.1k/s, V0 -16.4k/s, asini 482. Period 6-8y? Unresolved by speckle interferometry. RV varies in 2 | periods, 3.968d pulsation, 27.6y revolution of unseen blue companion.
Red star Pleiades group.
Also classified F7Ib-F8Ib.
0.006".
POLARIS; Alruccabah; Cynosura; Phoenice; Lodestar; Pole Star; Tramontana; Angel Stern; Navigatoria; Star of Arcady; | Yilduz; Mismar.
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Light Travel Time Machine

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Relativistic Travel

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