Full text: [Theoretischer astronomischer Nachlass] (7. Band)

DETERMINATIO ORBITAE E TRIBUS OBSERVATIONIBUS COMPLETIS. 
221 
p, prodibunt valores approximati sequentes; 
•p rsin^' — u) 4 r' 1 sin a (i;'— v) sin-|-(ij"— v'] 
r" sin [v"— v') ’ ^ p cos %{v ,r — v) 
His itaque hypothesis prima superstruetur, paullulumque ad libitum immutatis 
secunda et tertia: haud enim e re esset, P' et Q' hic pro novis valoribus 
adoptare (uti supra fecimus), quum hos valores magis exactos evadere haud 
amplius supponere liceat. Hac ratione omnes tres hypotheses commodissime 
simul absolvi poterunt: quarta dein secundum praecepta art. 120 formabitur. 
Ceterum haud abnuemus, si quis unam alteramve decem methodorum in artt. 
124 —129 expositarum in tali casu si non magis tamen aeque fere expeditam 
existimet, ideoque in usum vocare malit.
	        
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