Mesarthim

Gamma Arietis (γ Arietis, abbreviated Gamma Ari, γ Ari) is a binary star (possibly trinary) in the northern constellation of Aries. The two components are designated γ1 Arietis or Gamma Arietis B and γ2 Arietis or Gamma Arietis A (formally named Mesarthim , the traditional name for the Gamma Arietis system). γ1 Arietis may itself be a spectroscopic binary with a low mass companion. The combined apparent visual magnitude of the stars is 3.86, which is readily visible to the naked eye and makes this the fourth-brightest member of Aries. Based upon parallax measurements obtained during the Hipparcos mission, the distance to Gamma Arietis from the Sun is approximately 164 light-years (50 parsecs).

Arrival - 2023-05-26T00:00:00.000000Z

Clg J02182-05102 - 2021-04-21T00:00:00.000000Z

Vacuum Solution - 2021-03-10T00:00:00.000000Z

The Degenerate Era - 2020-09-30T00:00:00.000000Z

The Density Parameter - 2018-03-10T00:00:00.000000Z

Absence - 2016-03-10T00:00:00.000000Z

Isolate - 2016-03-10T00:00:00.000000Z

Planet Nine - 2020-12-11T00:00:00.000000Z

Planet 9 - 2020-09-30T00:00:00.000000Z

Coma Wall - 2020-04-07T00:00:00.000000Z

Ghost Condensate - 2019-03-10T00:00:00.000000Z

The Great Filter / Type III - 2017-03-10T00:00:00.000000Z

Pillars - 2016-03-10T00:00:00.000000Z

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