Now I'm going to rotate this about this axis-- - it's going around like this-- with an angular velocity omega R and this is at a distance, R.
然后我将使其绕轴旋转-,像这样旋转-,为角速度,这个距离记为。
Your velocity is in this direction R and there is a certain distance to the center, R.
是这个方向的,离中心的距离为。
R And the track has a radius R, and at this moment in time the angle equals theta, and here is the object.
轨道半径是,在这个时刻,角度等于θ,这是物体。
That was the song "Discoverer." Like many R.E.M.songs, this one is poetic with a meaning that is not always clear.
VOA: special.2011.03.18
In an orbital is remember that this area right here at r equals zerio, that is not a node.
例如对于1s轨道,记住这里r等于0处不是一个节点。
And we can simplify this expression as saying negative e squared over 4 pi, epsilon nought r squared. Epsilon nought is a constant, it's something you might see in physics as well.
也会遇到它,在这里,你可以就把它,理解为一个转换系数,我们需要做的。
应用推荐