太阳系模拟
几何画板及绘图内容加载中,请稍等……
①这个范例演示了地球和任意行星X在黄道平面内绕太阳公转的3D图形;②涉及的核心数学概念包括椭圆、平面图形、向量、旋转、轨迹等;③作图要点提炼自构造摘要,使用了椭圆、旋转、角度、射线、交点、圆、线、点、向量、平移、线段、球体、切线、平面、正交线、交点路径等GeoGebra命令和对象;④适合高中及以上学生学习和理解天体运动与几何图形的关系。
GeoGebra 命令及参数
Ellipse(A, B, C) → cRotate(C, α, A) → C'Angle(C, A, C') → βRay(A, C') → aIntersect(c, a) → D,Circle(A, Segment[A, E]) → dRotate(E, γ, A) → E'Angle(E, A, E') → δLine(A, E') → bPoint(b) → GRotate(G, ε, E') → G'Angle(G, E', G') → ζRay(E', G') → gRotate(C, 257.1*°, A) → C'_1Angle(C, A, C'_1) → ηLine(A, C'_1) → hRotate(C, 83.4*°, A) → C'_2Vector(D, A) → uTranslate(D, u) → D'Point(Circle[A, k]) → JSegment(A, J) → lRotate(J, γ, A) → J'Angle(J, A, J') → ιPoint(Circle[A, m]) → KSegment(A, K) → nRotate(K, γ, A) → K'Angle(K, A, K') → κEllipse(A, K', J') → pRotate(C, θ, A) → C'_3Angle(C, A, C'_3) → ξLine(A, C'_3) → iRotate(A, ε, K') → A'Angle(A, K', A') → μRay(K', A') → qRotate(p, Tilt, i) → p'Rotate(K', Tilt, i) → K''Rotate(A', Tilt, i) → A''Ray(K'', A'') → q'Intersect(q', p') → M, NSegment(D, M) → rVector(D, A) → vTranslate(D, v) → D'_1Translate(M, v) → M'Segment(D'_1, M') → r'Sphere(D'_1, k) → oRay(D'_1, M') → sIntersect(s, o) → O, PTangent(D, p') → t, a_1Intersect(t, p') → Q, RIntersect(a_1, p') → S, TIntersect(c, xAxis, 1) → UIntersect(c, xAxis, 2) → VPoint(c) → WPoint(c) → ZPoint(c) → Z_1Point(c) → C_1Point(c) → E_1Intersect(c, h, 2) → A_1Point(c) → B_1Point(c) → D_1Point(c) → F_1Point(c) → G_1Point(c) → H_1Point(c) → I_1Point(c) → J_1Point(c) → K_1Plane(F_1, B_1, J_1) → wRotate(w, 23.4*°, h) → w'OrthogonalLine(D'_1, w') → b_1IntersectPath(w', o) → c_1Intersect(q, q') → HIntersect(q, q') → IIntersect(q, q') → FIntersect(q, q') → LIntersectIntersect(p, p') → L_1, O_1, ,Intersect(p, q) → M_1, N_1Rotate(b, Tilt, i) → b'Intersect(zAxis, b') → R_1Point(h) → U_1Ray(R_1, U_1) → h_1Point(h_1) → V_1Vector(U_1, V_1) → u_1Intersect(h_1, c, 1) → W_1
AI 绘图提示语参考
绘制一个太阳系的3D模拟,包括太阳、地球和一个任意行星X绕太阳公转。首先画出太阳和地球的椭圆轨道,然后旋转地球和行星X,计算角度并绘制它们的轨迹。接着画出太阳系中的其他天体,如地球的卫星,最后将所有天体和轨道组合在一起,形成一个完整的太阳系模型。
以上提示语为根据原始绘图命令整理而来,仅供参考。