Mu Cephei

Mu Cephei compared to the Sun.

Mu Cephei, also known as Herschel's Garnet Star due to its red, garnet-like color, is a red hypergiant star in the Cepheus constellation. With a radius of 1,420 solar radii,^[1] or a diameter of 1,977,000,000 kilometers, it is one of the largest stars known. Mu Cephei is also the "prototype" of the semiregular variable star type.

Mu Cephei compared to the Sun and the orbits of the inner planets.
Artist's picture

Related pages[change | change source]

References[change | change source]

↑ Emily M. Levesque1 et al 2005. "The effective temperature scale of galactic red supergiants: cool, but not as cool as we thought" Astrophysical Journal 628, 2. [1]

This short article about science can be made longer. You can help Wikipedia by adding to it.

[1] Emily M. Levesque1 et al 2005. "The effective temperature scale of galactic red supergiants: cool, but not as cool as we thought" Astrophysical Journal 628, 2. [1]

[1]

Mu Cephei

Related pages[change | change source]

References[change | change source]

Navigation menu

Personal tools

Namespaces

Variants

Views

More

Search

Getting around

In other projects

Print/export

Tools

In other languages