Mu Arietis
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Please note that the content of this book primarily consists of articles available from Wikipedia or other free sources online. Mu Arietis is a star system in the constellation Aries. It is approximately 338 light years from Earth. It consists of a spectroscopic binary and a third component. The binary is classified as a white A-type main sequence dwarf with an apparent magnitude of +5.74. The two components are separated by 0.05 arcseconds and have an orbital period of 8.8 years. The third component is 19.1 arcseconds distant and has an apparent magnitude of +12.1.

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Please note that the content of this book primarily consists of articles available from Wikipedia or other free sources online. Mu Arietis is a star system in the constellation Aries. It is approximately 338 light years from Earth. It consists of a spectroscopic binary and a third component. The binary is classified as a white A-type main sequence dwarf with an apparent magnitude of +5.74. The two components are separated by 0.05 arcseconds and have an orbital period of 8.8 years. The third component is 19.1 arcseconds distant and has an apparent magnitude of +12.1.