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सिद्धान्तशिरोमणि: गणिताध्याय (भास्कराचार्य - ग्रहगणित, मध्यमाधिकार व स्पष्टाधिकार सटीक)

सिद्धान्तशिरोमणि: गणिताध्याय (भास्कराचार्य - ग्रहगणित, मध्यमाधिकार व स्पष्टाधिकार सटीक)

Siddhanta Shiromani Ganitadhyaya of Bhaskaracharya with Commentary

भास्कराचार्य द्वितीय द्वारा

DevanagariHindipublished573 पृष्ठ

पृष्ठ 105, कुल 573 में से

संदर्भ में पढ़ें
पृष्ठ 105

85
through the locality (hereafter called the rectified circum-
ference). Also the primary terrestrial meridian is that
longitudinal line passing through the places (1) Lanka (2)
Ujjain (3) Kurukshetra and (4) the north pole.
Fig. 4
Comm. (Ref. fig. 4) Let ABC be the terrestrial Equa-
tor, and QST be a circle parallel to this terrestrial equator
and passing through the locality S. This QST is called the
rectified circumference of the earth at the place S. The
terrestrial equator is defined as follows. It is known that
the earth rotates about herself about the axis P₁ P₂ where
P₁ P₂ is called the polar axis or Dhruvayashti. In other
words the entire heavens appear to revolve round the earth
in such a way that any star will appear to be revolving in
a circle called its diurnal circle which is parallel to the
circle ABC. The points P₁ and P₂ are called the north and