Mira vs 폴라리스
Embed This Widget
Add the script tag and a data attribute to embed this widget.
Embed via iframe for maximum compatibility.
<iframe src="https://starfyi.com/iframe/entity//" width="420" height="400" frameborder="0" style="border:0;border-radius:10px;max-width:100%" loading="lazy"></iframe>
Paste this URL in WordPress, Medium, or any oEmbed-compatible platform.
https://starfyi.com/entity//
Add a dynamic SVG badge to your README or docs.
[](https://starfyi.com/entity//)
Use the native HTML custom element.
| Property | Mira | 폴라리스 |
|---|---|---|
| 명칭 | 68Omi Cet | 1Alp UMi |
| 별자리 | N/A | N/A |
| 분광형 | Class M — M-type (Red) | Class F — F-type (Yellow-White) |
| 겉보기 등급 | +6.47 | +1.97 |
| 절대 등급 | 1.66 | -3.64 |
| 거리 | 299 ly | 433 ly |
| 질량 | N/A | N/A |
| 반지름 | N/A | N/A |
| 온도 | N/A | N/A |
| 광도 | N/A | N/A |
Key Differences
- ◆ 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.