). Others are Rho Cassiopeiae (40 Failed to parse (Missing texvc executable; please see math/README to configure.): \begin{smallmatrix}M_\odot\end{smallmatrix} ), Betelgeuse (20 Failed to parse (Missing texvc executable; please see math/README to configure.): \begin{smallmatrix}M_\odot\end{smallmatrix} ), and VY Canis Majoris (30-40 Failed to parse (Missing texvc executable; please see math/README to configure.): \begin{smallmatrix}M_\odot\end{smallmatrix} ). (The Sun (1 Failed to parse (Missing texvc executable; please see math/README to configure.): \begin{smallmatrix}M_\odot\end{smallmatrix}
) which is not visible in this thumbnail is included to illustrate the scale of example stars. Earth's orbit (grey), Jupiter's orbit (red), and Neptune's orbit (blue) are also given.)
The solar mass (Failed to parse (Missing texvc executable; please see math/README to configure.): \begin{smallmatrix}M_\odot\end{smallmatrix} ) is a standard unit of mass in astronomy, used to indicate the masses of other stars, as well as clusters, nebulae and galaxies. It is equal to the mass of the Sun, about two nonillion kilograms:
This is about 332,950 times the mass of the Earth or 1,048 times the mass of Jupiter.