IRAS 04509-6922
IRAS 04509-6922 is an AGB in the Large Magellanic Cloud.
IRAS 04509-6922’s minimum radius is 1,027 solar radii (1,430,286,468 km) (1,430,286,468,000 m).[1]
IRAS 04509-6922’s maximum radius is 2,249 solar radii (3,132,146,316 km) (3,132,146,316,000 m), but this is unlikely.[1]
Another estimate suggests a radius of 1,187 solar radii.[2]
It has a spectral type of M10.
IRAS 04509-6922 Media
Some massive stars compared to our Sun ( one single grey pixel in the 'Full resolution' image (2,876 × 2,068 pixels)) and the orbit of Earth (grey), Jupiter (red) and Neptune (blue). From left to
References
- ↑ 1.0 1.1 Goldman, Steven R.. The wind speeds, dust content, and mass-loss rates of evolved AGB and RSG stars at varying metallicity (in en). Monthly Notices of the Royal Astronomical Society 465 (1) (2017-02-11). p. 403–433. doi:10.1093/mnras/stw2708.
- ↑ Groenewegen, M. A. T.. Luminosities and mass-loss rates of Local Group AGB stars and red supergiants. Astronomy & Astrophysics 609 (January 2018). p. A114. doi:10.1051/0004-6361/201731089.