celestial longitude oor Esperanto

celestial longitude

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(astronomy) the equatorial coordinate specifying the angle, measured eastward along the celestial equator, from the vernal equinox to the intersection of the hour circle that passes through an object in the sky; usually expressed in hours and minutes and seconds; used with declination to specify positions on the celestial sphere; "one hour of right ascension equals fifteen degrees"

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ekliptika longitudo

eo
Angulo, mezurata elde centro de ĉielsfero horloĝdirekte laŭlonge de ekliptiko, inter la orta projekcio de punkto de la ĉielsfero sur la ekliptiko kaj la printempa punkto.
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It begins when the Sun reaches the celestial longitude of 30° and ends when it reaches the longitude of 45°.
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It more often refers in particular to the day when the Sun is exactly at the celestial longitude of 105°.
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An armillary sphere (variations are known as spherical astrolabe, armilla, or armil) is a model of objects in the sky (on the celestial sphere), consisting of a spherical framework of rings, centred on Earth or the Sun, that represent lines of celestial longitude and latitude and other astronomically important features, such as the ecliptic.
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3 sinne gevind in 2 ms. Hulle kom uit baie bronne en word nie nagegaan nie.