मायावती तारा vs पोलारिस
Intrinsic output is the great divide here. पोलारिस carries an absolute magnitude of −3.64 to −0.11 for मायावती तारा, near 26 times the true luminosity. मायावती तारा trails in apparent brightness at magnitude +2.09 against +1.97, leaving पोलारिस around 1.1 times the brighter target. पोलारिस is an F-type star, while मायावती तारा is a B-type star in Perseus. पोलारिस is the remoter of the pair at 433 light-years, roughly 4.8 times the 89.9 that separates us from मायावती तारा.
Property comparison
| Property | मायावती तारा | पोलारिस |
|---|---|---|
| पदनाम | 26Bet Per | 1Alp UMi |
| नक्षत्रमंडल | Perseus | N/A |
| वर्णक्रम वर्ग | Class B — B-type (Blue-White) | Class F — F-type (Yellow-White) |
| आभासी परिमाण | +2.09 | +1.97 |
| निरपेक्ष परिमाण | -0.11 | -3.64 |
| दूरी | 89.9 ly | 433 ly |
| द्रव्यमान | N/A | N/A |
| त्रिज्या | N/A | N/A |
| तापमान | N/A | N/A |
| दीप्तिमानता | N/A | N/A |
Full data for each star: मायावती तारा · पोलारिस
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.