Gamma Orionis vs Rigel
Real luminosity separates the pair by a factor of about 45: absolute magnitude −6.93 for Rigel, −2.80 for Gamma Orionis. Spectroscopically Gamma Orionis resolves as a B-type star in Orion and Rigel as a B-type star in Orion. To the unaided eye Rigel leads at magnitude +0.18 to +1.64, a gap of 1.46 worth about 3.8 times the light of Gamma Orionis.
Property comparison
| Property | Gamma Orionis | Rigel |
|---|---|---|
| Ký Hiệu | 24Gam Ori | 19Bet Ori |
| Chòm Sao | Orion | Orion |
| Phân Loại Quang Phổ | Class B — B-type (Blue-White) | Class B — B-type (Blue-White) |
| Cấp Sao Biểu Kiến | +1.64 | +0.18 |
| Cấp Sao Tuyệt Đối | -2.80 | -6.93 |
| Khoảng Cách | 252 ly | 863 ly |
| Khối Lượng | N/A | N/A |
| Bán Kính | N/A | N/A |
| Nhiệt Độ | N/A | N/A |
| Độ Sáng | N/A | N/A |
Full data for each star: Gamma Orionis · Rigel
Key differences
Key Differences
- ◆ Both are hot B-type stars in Orion, marking opposite corners of the hunter's torso.
- ◆ Rigel (Beta Orionis) is a blue supergiant at ~21 M☉; Bellatrix (Gamma Orionis) is a blue giant at ~8.4 M☉.
- ◆ Rigel is far more luminous at ~120,000 L☉ versus Bellatrix at ~6,400 L☉.
- ◆ Bellatrix is much closer at ~250 light-years; Rigel is also ~860 light-years distant.
- ◆ Bellatrix will eventually become an orange giant and finally a massive white dwarf, not a supernova.