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ascensions

ascensions Sentence Examples

  • The photographic right ascensions gave the values 8.80" -}- 0.007" -}- 0.0027" (Hinks) and 8.80" + 0 .

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  • Rambert, Ascensions et fldneries (2 vols., 1888); G.

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  • It is easily seen that if the mirror be rotated at the same angular velocity as the sun the right ascensions will remain equal throughout the day, and therefore this device reflects the rays in the direction of the earth's axis; a second fixed mirror reflects them in any other fixed direction.

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  • Since the transit circle is preferable to the equatorial for such observations wherein great accuracy is required, the declination and hour circles of an equatorial are employed, not for the determination of the right ascensions and declinations of celestial objects, but for directing the telescope with ease and certainty to any object situated in an approximately known position, and which may or may not be visible to the naked eye, or to define approximately the position of an unknown object.

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  • A pair of stars of known declination are selected such that their zenith distances, when on the meridian, are nearly equal and opposite, and whose right ascensions differ by five or ten minutes of time.

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  • Formerly attempts were made to determine parallaxes by measuring changes in the absolute right ascensions and declinations of the stars from observations with the meridian circle.

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  • The latter motion leads to the use, in astronomical practice, of time instead of angle, as the unit in which the right ascensions are to be expressed.

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  • Right ascensions are now determined, not by measuring the angle between one star and another, but, by noting the time between the transits of successive stars over the meridian.

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  • The difference between these times, when reduced to an angle, is the difference of the right ascensions of the stars.

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  • We have already mentioned that in astronomical practice right ascensions are expressed in time, so that no multiplication by 15 is necessary.

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  • This instrument moves only in the plane of the meridian on a horizontal east and west axis, and is used to determine the right ascensions and declinations of stars.

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  • Christoph Rothmann and Joost Biirgi (1552-1632) became his assistants in 1577 and 1579 respectively; and through the skill of Biirgi, time-determinations were made available for measuring right ascensions.

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  • Flamsteed's mode of determining right ascensions.

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  • The photographic right ascensions gave the values 8.80" -}- 0.007" -}- 0.0027" (Hinks) and 8.80" + 0 .

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  • Rambert, Ascensions et fldneries (2 vols., 1888); G.

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  • It is easily seen that if the mirror be rotated at the same angular velocity as the sun the right ascensions will remain equal throughout the day, and therefore this device reflects the rays in the direction of the earth's axis; a second fixed mirror reflects them in any other fixed direction.

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  • Since the transit circle is preferable to the equatorial for such observations wherein great accuracy is required, the declination and hour circles of an equatorial are employed, not for the determination of the right ascensions and declinations of celestial objects, but for directing the telescope with ease and certainty to any object situated in an approximately known position, and which may or may not be visible to the naked eye, or to define approximately the position of an unknown object.

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  • A pair of stars of known declination are selected such that their zenith distances, when on the meridian, are nearly equal and opposite, and whose right ascensions differ by five or ten minutes of time.

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    0
  • Formerly attempts were made to determine parallaxes by measuring changes in the absolute right ascensions and declinations of the stars from observations with the meridian circle.

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  • The vernal equinox is the initial point from which the right ascensions and the longitudes of the heavenly bodies are measured (see Astronomy: Spherical).

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  • The latter motion leads to the use, in astronomical practice, of time instead of angle, as the unit in which the right ascensions are to be expressed.

    0
    0
  • Right ascensions are now determined, not by measuring the angle between one star and another, but, by noting the time between the transits of successive stars over the meridian.

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    0
  • The difference between these times, when reduced to an angle, is the difference of the right ascensions of the stars.

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    0
  • We have already mentioned that in astronomical practice right ascensions are expressed in time, so that no multiplication by 15 is necessary.

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    0
  • This instrument moves only in the plane of the meridian on a horizontal east and west axis, and is used to determine the right ascensions and declinations of stars.

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    0
  • Christoph Rothmann and Joost Biirgi (1552-1632) became his assistants in 1577 and 1579 respectively; and through the skill of Biirgi, time-determinations were made available for measuring right ascensions.

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  • Flamsteed's mode of determining right ascensions.

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  • Also I began to make balloon ascensions.

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