Mira vs Kutup Yıldızı
| Özellik | Mira | Kutup Yıldızı |
|---|---|---|
| Adlandırma | 68Omi Cet | 1Alp UMi |
| Takımyıldız | N/A | N/A |
| Spektral Sınıf | Class M — M-type (Red) | Class F — F-type (Yellow-White) |
| Görünür Parlaklık | +6.47 | +1.97 |
| Mutlak Parlaklık | 1,66 | -3,64 |
| Mesafe | 299 ly | 433 ly |
| Kütle | N/A | N/A |
| Yarıçap | N/A | N/A |
| Sıcaklık | N/A | N/A |
| Parlaklık | N/A | N/A |
Temel Farklılıklar
- ◆ Both are famous variable stars in the northern sky, though entirely different types.
- ◆ Polaris is a Cepheid variable that pulsates predictably and was used to calibrate the Cepheid distance ladder.
- ◆ Mira is a long-period Mira-type variable that can range from naked-eye visibility to complete invisibility.
- ◆ Polaris is celebrated as the North Star for its positional stability near the pole; Mira is celebrated as the first recognized variable star (1596).
- ◆ Polaris's pulsation amplitude has been shrinking over the past century; Mira continues its large-amplitude cycle.