例文・使い方で印象づける「galactic」の覚え方


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...It may be, as some astronomers hold, that most of the galactic stars are much smaller than the sun, so that their faintness is not due entirely to the effect of distance...   It may be, as some astronomers hold, that most of the galactic stars are much smaller than the sun, so that their faintness is not due entirely to the effect of distanceの読み方
Garrett Serviss 「Curiosities of the Sky」

...Instead of all moving one way, the galactic stars, as far as their movements can be inferred, are governed by local influences and conditions...   Instead of all moving one way, the galactic stars, as far as their movements can be inferred, are governed by local influences and conditionsの読み方
Garrett Serviss 「Curiosities of the Sky」

...Taking into account theapparent distribution of the stars in space, it is, however, more practicalto characterize the position of a star by its galactic longitude (l) andits galactic latitude (b)...   Taking into account theapparent distribution of the stars in space, it is, however, more practicalto characterize the position of a star by its galactic longitude (l) andits galactic latitude (b)の読み方
Carl Vilhelm Ludvig Charlier 「Lectures on Stellar Statistics」

...The galactic coordinates l and b are referred to the Milky Way(the Galaxy) as plane of reference...   The galactic coordinates l and b are referred to the Milky Way(the Galaxy) as plane of referenceの読み方
Carl Vilhelm Ludvig Charlier 「Lectures on Stellar Statistics」

...But having ascertained later thatthe real position of the galactic plane requires a greater number of starsfor an accurate determination of its value...   But having ascertained later thatthe real position of the galactic plane requires a greater number of starsfor an accurate determination of its valueの読み方
Carl Vilhelm Ludvig Charlier 「Lectures on Stellar Statistics」

...The galactic longitude (l) is reckoned from the ascending node ofthe Milky Way on the equator, which is situated in the constellationAquila...   The galactic longitude (l) is reckoned from the ascending node ofthe Milky Way on the equator, which is situated in the constellationAquilaの読み方
Carl Vilhelm Ludvig Charlier 「Lectures on Stellar Statistics」

...The galactic latitude (b) gives the angular distance of the starfrom the Galaxy...   The galactic latitude (b) gives the angular distance of the starfrom the Galaxyの読み方
Carl Vilhelm Ludvig Charlier 「Lectures on Stellar Statistics」

...It lies in the square GD7 and its galactic coordinates are seenin the 5th and 6th columns...   It lies in the square GD7 and its galactic coordinates are seenin the 5th and 6th columnsの読み方
Carl Vilhelm Ludvig Charlier 「Lectures on Stellar Statistics」

...Let us next count the number of stars visible in a powerful telescopein the region of the heavens around the galactic pole, now our zenith,and find the average number per square degree...   Let us next count the number of stars visible in a powerful telescopein the region of the heavens around the galactic pole, now our zenith,and find the average number per square degreeの読み方
Simon Newcomb 「Side-lights on Astronomy and Kindred Fields of Popular Science」

...They are just as thick around the south galactic poles as around thenorth one...   They are just as thick around the south galactic poles as around thenorth oneの読み方
Simon Newcomb 「Side-lights on Astronomy and Kindred Fields of Popular Science」

...This difference of coloralso is the same on the two sides of the galactic plane...   This difference of coloralso is the same on the two sides of the galactic planeの読み方
Simon Newcomb 「Side-lights on Astronomy and Kindred Fields of Popular Science」

...The corresponding squares southof the galactic equator (the plane of the Galaxy) are called GD1, GD2, ...   The corresponding squares southof the galactic equator (the plane of the Galaxy) are called GD1, GD2, の読み方
Carl Vilhelm Ludvig Charlier 「Lectures on Stellar Statistics」

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