| 1. | Celestial coordinate systems most commonly used in astronomy are ecliptic coordinates.
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| 2. | In ecliptic coordinates the Sun is at latitude zero, so that
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| 3. | In November 2011, American amateur astronomer ecliptic coordinates, respectively ( ).
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| 4. | "' ecliptic coordinates used in astrology.
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| 5. | This defined an ecliptic coordinate system which was used throughout the medieval period and into the 18th century.
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| 6. | Earth-centered "'ecliptic coordinates "'as seen from outside the celestial sphere.
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| 7. | The ecliptic coordinate system specifies positions relative to the Earth's orbit, using celestial longitude and latitude.
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| 8. | In April 2005, a rotational lightcurve of " Crimea " was obtained by American astronomer ecliptic coordinates ( ).
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| 9. | In August 2008, a rotational light-curve of this asteroid was obtained by French amateur astronomer ecliptic coordinates, respectively ( ).
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| 10. | It gave it a well-defined rotation period of 4.32 hours with a brightness variation of 0.15 ecliptic coordinates.
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