Tau Arietis (τ Ari / τ Arietis) is a triple star system in the constellation Aries. It is approximately 462 light years from Earth. The primary component, τ¹ Arietis A, is an eclipsing binary which is classified as a blue-white B-type subgiant. The two components have apparent magnitudes of +5.4 and +7.9 and are separated by 0.15 arcseconds. At 0.67 arcseconds from A is τ¹ Arietis B, which has an apparent magnitude of +8.4.
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- Tau Arietis (τ Ari / τ Arietis) is a triple star system in the constellation Aries. It is approximately 462 light years from Earth. The primary component, τ¹ Arietis A, is an eclipsing binary which is classified as a blue-white B-type subgiant. The two components have apparent magnitudes of +5.4 and +7.9 and are separated by 0.15 arcseconds. At 0.67 arcseconds from A is τ¹ Arietis B, which has an apparent magnitude of +8.4. The combined mean apparent magnitude of the system is +5.27, but due to eclipsing of the binary components, the brightness varies from magnitude +5.26 to +5.32.
- Tau Arietis (τ Ari / τ Arietis) és un sistema estel·lar triple de la constel·lació d'Àries. Està aproximadament a 462 anys-llum de la Terra. La component primària, τ¹ Arietis A, és una binària eclipsant classificada com a subgegant blanca-blava del tipus B. Les dues components són de la magnitud aparent +5,4 i +7,9 i estan separades 0,15 segons d'arc. A 0,67 segons d'arc d'A hi trobam τ¹ Arietis B, que és de la magnitud aparent +8,4. La magnitud combinada mitjana del sistema és +5,27, però degut als eclipses de les components, la lluentor varia de la magnitud +5,26 a +5,32.
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- Tau Arietis (τ Ari / τ Arietis) is a triple star system in the constellation Aries. It is approximately 462 light years from Earth. The primary component, τ¹ Arietis A, is an eclipsing binary which is classified as a blue-white B-type subgiant. The two components have apparent magnitudes of +5.4 and +7.9 and are separated by 0.15 arcseconds. At 0.67 arcseconds from A is τ¹ Arietis B, which has an apparent magnitude of +8.4.
- Tau Arietis (τ Ari / τ Arietis) és un sistema estel·lar triple de la constel·lació d'Àries. Està aproximadament a 462 anys-llum de la Terra. La component primària, τ¹ Arietis A, és una binària eclipsant classificada com a subgegant blanca-blava del tipus B. Les dues components són de la magnitud aparent +5,4 i +7,9 i estan separades 0,15 segons d'arc. A 0,67 segons d'arc d'A hi trobam τ¹ Arietis B, que és de la magnitud aparent +8,4.
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- Tau¹ Arietis
- Tau¹ Arietis
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