Beta Persei vs Polaris
Intrinsic output is the great divide here. Polaris carries an absolute magnitude of −3.64 to −0.11 for Beta Persei, near 26 times the true luminosity. Beta Persei trails in apparent brightness at magnitude +2.09 against +1.97, leaving Polaris around 1.1 times the brighter target. Polaris is an F-type star, while Beta Persei is a B-type star in Perseus. Polaris is the remoter of the pair at 433 light-years, roughly 4.8 times the 89.9 that separates us from Beta Persei.
Property comparison
| Property | Beta Persei | Polaris |
|---|---|---|
| Designação | 26Bet Per | 1Alp UMi |
| Constelação | Perseus | N/A |
| Classe Espectral | Class B — B-type (Blue-White) | Class F — F-type (Yellow-White) |
| Magnitude Aparente | +2.09 | +1.97 |
| Magnitude Absoluta | -0.11 | -3.64 |
| Distância | 89.9 ly | 433 ly |
| Massa | N/A | N/A |
| Raio | N/A | N/A |
| Temperatura | N/A | N/A |
| Luminosidade | N/A | N/A |
Full data for each star: Beta Persei · Polaris
Key differences
Key Differences
- ◆ Both are variable stars, but of different physical types.
- ◆ Polaris is a Cepheid variable that pulsates in radius; Algol dims because a companion eclipses it.
- ◆ Polaris's pulsation amplitude has been decreasing over the past century.
- ◆ Algol varies every 2.87 days (eclipsing); Polaris has a period of about 3.97 days (pulsation).
- ◆ Polaris is near the north celestial pole and vital for navigation; Algol is in Perseus and known as the Demon Star.