Calculus[edit]
His work, theSiddhānta Shiromani, is an astronomical treatise and contains many theories not found in earlier works.[citation needed]Preliminary concepts ofinfinitesimal calculusandmathematical analysis, along with a number of results intrigonometry,differential calculusandintegral calculusthat are found in the work are of particular interest.
His work, theSiddhānta Shiromani, is an astronomical treatise and contains many theories not found in earlier works.[citation needed]Preliminary concepts ofinfinitesimal calculusandmathematical analysis, along with a number of results intrigonometry,differential calculusandintegral calculusthat are found in the work are of particular interest.
Evidence suggests Bhaskara was acquainted with some ideas of differential calculus.[17]It seems, however, that he did not understand the utility of his researches, and thus historians of mathematics generally neglect this achievement.[citation needed]Bhaskara also goes deeper into the 'differential calculus' and suggests the differential coefficient vanishes at an extremum value of the function, indicating knowledge of the concept of 'infinitesimals'.[18]
- There is evidence of an early form ofRolle's theoremin his work
- If
- Bhaskara uses this result to work out the position angle of theecliptic, a quantity required for accurately predicting the time of an eclipse.
- In computing the instantaneous motion of a planet, the time interval between successive positions of the planets was no greater than atruti, or a1⁄33750of a second, and his measure of velocity was expressed in this infinitesimal unit of time.
- He was aware that when a variable attains the maximum value, itsdifferentialvanishes.
- He also showed that when a planet is at its farthest from the earth, or at its closest, the equation of the centre (measure of how far a planet is from the position in which it is predicted to be, by assuming it is to move uniformly) vanishes. He therefore concluded that for some intermediate position the differential of the equation of the centre is equal to zero.[citation needed]In this result, there are traces of the generalmean value theorem, one of the most important theorems in analysis, which today is usually derived from Rolle's theorem. The mean value theorem was later found byParameshvarain the 15th century in theLilavati Bhasya, a commentary on Bhaskara'sLilavati.
- If
- Astronomy[edit]
Using an astronomical model developed byBrahmaguptain the 7th century, Bhaskara accurately defined many astronomical quantities, including, for example, the length of thesidereal year, the time that is required for the Earth to orbit the Sun, as 365.2588 days which is the same as in Suryasiddhanta.[citation needed]The modern accepted measurement is 365.2563 days, a difference of just 3.5 minutes.[citation needed]
- His mathematical astronomy textSiddhanta Shiromaniis written in two parts: the first part on mathematical astronomy and the second part on thesphere.
- The twelve chapters of the first part cover topics such as:
- Meanlongitudesof theplanets.
- True longitudes of the planets.
- The three problems ofdiurnal rotation.
- Syzygies.
- Lunar eclipses.
- Solar eclipses.
- Latitudesof the planets.
- Sunrise equation
- TheMoon'screscent.
- Conjunctionsof the planets with each other.
- Conjunctions of the planets with the fixedstars.
- The paths of the Sun and Moon.
- Praise of study of the sphere.
- Nature of the sphere.
- Cosmographyandgeography.
- Planetarymean motion.
- Eccentricepicyclicmodel of the planets.
- Thearmillary sphere.
- Spherical trigonometry.
- Ellipsecalculations.[citation needed]
- First visibilities of the planets.
- Calculating the lunar crescent.
- Astronomical instruments.
- Theseasons.
- Problems of astronomical calculations.
The earliest reference to aperpetual motionmachine date back to 1150, when Bhāskara II described awheelthat he claimed would run forever.[20]
- Bhāskara II used a measuring device known asYasti-yantra. This device could vary from a simple stick to V-shaped staffs designed specifically for determining angles with the help of a calibrated scale.[21]
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