The description and use of the globes and the orrery: To which is prefix'd, by way of introduction, a brief account of the solar systemHarris, Joseph
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The description and use of the globes and the orrery: To which is prefix'd, by way of introduction, a brief account of the solar system
Harris, Joseph
Astronomical models; Globes
The following Problems are peculiar to the _Celestial Globe_.
PROB. XXXIV. _To find the Right Ascension and
Declination of the Sun, or any Fixed Star._
Bring the Sun’s place in the ecliptic to the meridian; then that degree
of the equator, which is cut by the meridian, will be the _Sun’s Right
Ascension_; and that degree of the meridian, which is exactly over the
Sun’s place, is the _Sun’s Declination_.
After the same manner, bring the place of any Fixed Star to the
meridian, and you will find its Right Ascension in the equinoctial, and
Declination of the meridian.
Thus, the right ascension and declination is found, after the same
manner as the longitude and latitude of a place upon the _Terrestrial
Globe_.
_Note_, The right ascension and declination of the Sun vary every
day; but the right ascension, _&c._ of the Fixed Stars is the same
throughout the year[6].
The Sun’s Right Ascension. Declin.
_Deg._ _Deg._
{ _January_ 31 314 17⅓ S.
{ _April_ 5 14¼ 6 N.
Thus on { _July_ 21 120¼ 20½ N.
{ _November_ 26 242¼ 21 S.
R. Asc. Dcl.
_Deg._ _Deg._
_Aldebaran_ 65 16 N.
_Spica Virginis_ 197¾ 9¾ S.
_Capella_ 74 45⅔ N.
_Syrius, or the Dog-Star_ 98¼ 16⅓ S.
_Note_, The declination of the Sun may be found after the same manner
by the _Terrestrial Globe_, and also his right ascension, when the
equinoctial is numbered into 360 degrees, commencing at the equinoctial
point ♈: But as the equinoctial is not always numbered so, and this
being properly a Problem in _Astronomy_, we choose rather to place it
here.
By the converse of this problem, having the right ascension and
declination of any point given, that point itself may be easily found
upon the globe.
PROB. XXXV. _To find the Longitude and
Latitude of a given Star._
Having brought the solstitial colure to the meridian, fix the quadrant
of altitude over the proper Pole of the ecliptic, whether it be North
or South; then turn the quadrant over the given Star, and the arch
contained betwixt the Star and the ecliptic, will be the latitude, and
the degree cut on the ecliptic will be the Star’s longitude.
Thus the latitude of _Arcturus_ will be found to be 31 degrees North,
and the longitude 200 degrees from ♈, or 20 degrees from ♎: The
latitude of _Fomalhaut_ in the Southern Fish, 21 degrees South, and
longitude 299½ degrees, or ♑ 29½ degrees. By the converse of this
method, having the latitude and longitude of a Star given, it will be
easy to find the Star upon the globe.
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