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Web1086 M. NAGASAWA et al.: ORIGIN OF HIGH ORBITAL ECCENTRICITY AND INCLINATION OF ASTEROIDS 0 5 10 15 20 2 3 4 (e 2 +i 2) 1 / 2 V kep (km/s) semi-major axis (AU) ν16 ν6 3:1 5:2 7:3 2:1 3:2 Fig. 1. The random velocities ((e 2+ i )1/ Vkep) versus semi-major axes of the present asteroids.Above the dotted line, orbits of asteroids with i = 0 cross Jovian orbit, … WebThey all different. So, it depend on what you look for, in order apply the properly formula. One example is: sin of 1 angle (in the right triangle) = opposite over hypotenuse. So, if you know sin of that angle, and you also know the length of the opposite. Then apply the formula of sin, you can find hypotenuse. how has technology shrunk the world
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