光多普勒频移计算器

Optical Doppler Shift Calculator (f′ = f·(1 + v/c))

Compute the observed frequency from source frequency, relative velocity and the speed of light, using the non-relativistic approximation.

📐 工作原理与说明
光学多普勒效应:观测频率 f prime = f*(1 + v/c),v 为光源与观察者的相对速度(远离为正、接近为负),c 为光速;频移量 Δf = f prime − f = f*v/c;相对频移 Δf/f = v/c,用于激光测速与天体红移测量。

Formula Reference

Item Formula / Note Source / Standard
Optical Doppler shift (non-relativistic)f' = f (1 ± v/c), first-order approximation for v << cClassical Doppler effect (Doppler, 1842)
Relativistic exact formf' = f·sqrt((1−β)/(1+β)) for recession, β=v/cSpecial relativity (Einstein, 1905)
📌 计算说明
  • v 取正为靠近(蓝移)。
  • 5×10¹⁴,3×10⁵,3×10⁸ → 5.005×10¹⁴。

📐 Physical Constants

Constants used on this page and their authoritative sources, for verification and citation

Constant Value Unit Source
Speed of light in vacuum c 299 792 458 m·s⁻¹ SI defining constant (exact; this page uses 3×10⁸ as an approximation)

Note: this page uses the classical longitudinal approximation f′ = f·(1 ± v/c), valid only for v ≪ c. At high speeds use the relativistic form f′ = f·√((1+β)/(1−β)) with β = v/c; transverse motion gives rise to the transverse Doppler effect.

📚 深度解析:光多普勒频移

💡 常见使用场景

光源远离 300km/s
f′=f(1+v/c)=5e14×(1+3e5/3e8)=5e14×1.001=5.005e14 Hz,Δf=5e11 Hz(红移)。
趋近 0.01c
v/c=0.01:f′=5e14×1.01=5.05e14 Hz,蓝移。

❓ 常见问题(FAQ)

接近光速为何用此近似?
v≪c 时用经典近似 f′=f(1+v/c);高速须用相对论纵向多普勒公式。
红移蓝移怎么区分?
远离(v>0 背离)频率降低为红移,趋近频率升高为蓝移。