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・ Iowa Commission for the Blind Building
・ Iota Phoenicis
・ Iota Pictoris
・ Iota Piscis Austrini
・ Iota Piscium
・ Iota Reticuli
・ Iota Sagittarii
・ Iota Scorpii
・ Iota Sculptoris
・ Iota Serpentis
・ Iota Sigma Pi
・ Iota subscript
・ Iota Tauri
・ Iota Telescopii
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Iota Trianguli Australis
・ Iota Tucanae
・ Iota Ursae Majoris
・ Iota Virginis
・ Iota Volantis
・ Iota, Louisiana
・ Iota-carrageenase
・ Iota1 Cygni
・ Iota1 Librae
・ Iota1 Muscae
・ Iota1 Normae
・ Iota1 Scorpii
・ Iota2 Cygni
・ Iota2 Muscae
・ Iota2 Scorpii


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Iota Trianguli Australis : ウィキペディア英語版
Iota Trianguli Australis

Iota Trianguli Australis (ι TrA, ι Trianguli Australis) is a triple star system in the constellation Triangulum Australe. It is approximately 132 light years from Earth.
It shows itself to be composed of a yellow and a white star when seen though a 7.5 cm telescope.
The primary component, Iota Trianguli Australis A, is a spectroscopic binary with a mean apparent magnitude of +5.28. Both components of the binary star are yellow-white F-type stars and they have an orbital period of 39.8 days. One of the components of the binary is also classified as a Gamma Doradus type variable star, and the binary's brightness varies by 0.12 magnitudes over a period of 1.45 days. The third component of the star system, Iota Trianguli Australis B, is a 10th magnitude star, 20 arcseconds away from the primary.
==References==




抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)
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